DARTS Astro

total 229

No.
target_name
center_ra
center_dec
center_ra_b1950
center_dec_b1950
center_ecliptic_lon
center_ecliptic_lat
center_galactic_lon
center_galactic_lat
roll_angle
observation_start_time_mjd
observation_start_time
observation_end_time_mjd
observation_end_time
observation_id
exposure
proposal_exposure
xis0_exposure
xis1_exposure
xis2_exposure
xis3_exposure
xis0_observation_mode
xis1_observation_mode
xis2_observation_mode
xis3_observation_mode
hxd_observation_mode
hxd_coarse_clock_rate_exposure
hxd_first_clock_rate_exposure
hxd_normal_clock_rate_exposure
hxd_all_clock_rate_exposure
hxd_wam_exposure
hxd_burst_num
processing_status
processing_end_time_mjd
processing_end_time
public_date_mjd
public_date
distribute_start_date_mjd
distribute_start_date
processing_version
processing_quantity
processing_software
proposal_id
proposal_abstract
proposal_category
proposal_category_code
proposal_priority
pi_name
co_pi_name
proposal_affiliated_country
proposal_cycle_count
observation_type
proposal_title
main_detector
xis_injection_flag
data_access_url
ql_access_url
ql_image_url
1 Crab Nebula 83.6449 22.0152 82.892626 21.982571 84.11016 -1.295832 184.56274906 -5.77473152 84.9987 53614.1083449074 2005-09-01 02:36:01 53614.1771759259 2005-09-01 04:15:08 100015030 2.1 5 2.1 2.1 2.1 2.1 1 1 1 1 1 0 0 2.3074 2.3074 5.9439 0 PROCESSED 57527.235150463 2016-05-19 05:38:37 54247 2007-05-27 00:00:00 54109.3966782407 2007-01-09 09:31:13 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000015 CALIBRATION 1 A SWG JAP 0 SWG HXD boresight check with Crab N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100015030/
2 E0102-72 15.9884 -72.0403 15.58329 -72.308299 314.593543 -65.036118 301.56673438 -45.05476105 119.5512 53595.2489236111 2005-08-13 05:58:27 53595.4618518518 2005-08-13 11:05:04 100001020 4.1598 10 4.1598 4.1598 4.1598 4.1598 1 1 1 2 0 0 0 0 0 0 0 PROCESSED 57520.6779861111 2016-05-12 16:16:18 54247 2007-05-27 00:00:00 54035.6312731482 2006-10-27 15:09:02 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000001 XIS door open with a SMC SNR E0102-72 CALIBRATION 1 A SWG JAP 0 SWG XIS door open N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100001020/ Quick Look
3 N132D 81.2751 -69.6506 81.377584 -69.69262 312.405312 -85.522517 280.31335191 -32.77744994 53.3312 53598.2402777778 2005-08-16 05:46:00 53598.5140046296 2005-08-16 12:20:10 100002060 5.9635 7 5.9635 5.9635 5.9635 5.9635 1 1 1 1 0 0 0 0 0 0 0 PROCESSED 57520.6925115741 2016-05-12 16:37:13 54247 2007-05-27 00:00:00 54038.4700810185 2006-10-30 11:16:55 3.0.22.43 6 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000002 HXD HV ON WITH N132D, and 5 pointings with XIS CALIBRATION 1 A SWG JAP 0 SWG HXD HV ON WITH N132D N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100002060/ Quick Look
4 DEM_L71/N23 76.4474 -67.958 76.476582 -68.023213 338.826937 -84.59461 278.75859594 -34.83581885 70.5849 53598.5206365741 2005-08-16 12:29:43 53599.6042592593 2005-08-17 14:30:08 100003010 5.7897 40 5.7897 5.7897 5.7897 5.7897 2 2 2 2 0 0 0 0 0 93.6061 0 PROCESSED 57520.7098611111 2016-05-12 17:02:12 54247 2007-05-27 00:00:00 54035.7018171296 2006-10-27 16:50:37 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000003 LMC SNRs L71/N23 CALIBRATION 1 A SWG JAP 0 SWG LMC SNRs N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100003010/ Quick Look
5 A 2052 229.2779 6.8766 228.662841 7.059342 224.77082 24.150691 9.31339919 49.96215441 281.2328 53602.4238078704 2005-08-20 10:10:17 53602.743287037 2005-08-20 17:50:20 100006010 13.9021 20 13.9021 13.9021 13.9021 13.9021 1 1 1 1 1 0 0 13.4163 13.4163 27.5839 0 PROCESSED 57520.7207407407 2016-05-12 17:17:52 53705 2005-12-01 00:00:00 53905.4607523148 2006-06-19 11:03:29 3.0.22.43 11 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000006 CALIBRATION 1 A SWG JAP 0 SWG Outer region of A 2052 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006010/ Quick Look
6 A 2052 229.3237 7.1059 228.709513 7.288472 224.747048 24.38343 9.64711471 50.05514889 281.2373 53602.7440393518 2005-08-20 17:51:25 53603.3406944445 2005-08-21 08:10:36 100006020 25.7431 20 25.7431 25.7431 25.7431 25.7431 1 1 1 1 1 0 0 21.0642 21.0642 51.5199 0 PROCESSED 57520.7246527778 2016-05-12 17:23:30 53705 2005-12-01 00:00:00 53905.4610300926 2006-06-19 11:03:53 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000006 CALIBRATION 1 A SWG JAP 0 SWG Outer region of A 2052 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006020/ Quick Look
7 A 2052 229.0933 7.1516 228.479191 7.335016 224.492199 24.361996 9.50335527 50.26933049 281.2093 53603.3412615741 2005-08-21 08:11:25 53603.6114351852 2005-08-21 14:40:28 100006030 12.969 20 12.969 12.969 12.969 12.969 1 1 1 1 1 0 0 13.1413 13.1413 23.3279 0 PROCESSED 57520.7271527778 2016-05-12 17:27:06 53705 2005-12-01 00:00:00 53905.4613310185 2006-06-19 11:04:19 3.0.22.43 9 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000006 CALIBRATION 1 A SWG JAP 0 SWG Outer region of A 2052 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006030/ Quick Look
8 A 2052 229.3311 7.2632 228.717502 7.445744 224.705557 24.536292 9.85579143 50.13807877 91.2371 53762.482650463 2006-01-27 11:35:01 53762.9209953704 2006-01-27 22:06:14 100006050 22.366 20 22.366 22.366 22.366 22.366 2 2 2 2 1 0 0 20.388 20.388 37.8659 0 PROCESSED 57532.800162037 2016-05-24 19:12:14 54247 2007-05-27 00:00:00 54040.5318634259 2006-11-01 12:45:53 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000006 CALIBRATION 1 A SWG JAP 0 SWG Outer region of A 2052 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006050/ Quick Look
9 NGC 4945 196.3681 -49.4152 195.638243 -49.147517 216.98939 -38.593586 305.27752827 13.39262005 96.1296 53750.3365625 2006-01-15 08:04:39 53752.9655092593 2006-01-17 23:10:20 100008030 95.0663 10 95.0817 95.1297 95.0663 95.1063 2 2 2 2 1 0 0 84.9813 84.9813 227.1157 2 PROCESSED 57532.7353240741 2016-05-24 17:38:52 54247 2007-05-27 00:00:00 54040.3587615741 2006-11-01 08:36:37 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000008 CALIBRATION 1 A SWG JAP 0 SWG NGC 4945 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100008030/ Quick Look
10 PSR1509-58 228.4798 -59.0943 227.494741 -58.907902 243.862404 -39.360151 320.34145971 -1.12587132 287.6342 53605.36 2005-08-23 08:38:24 53606.8597569444 2005-08-24 20:38:03 100009010 65.1618 60 65.1618 65.3227 65.2427 65.2427 3 3 3 3 1 0 0 49.7357 49.7357 129.5298 4 PROCESSED 57526.9045486111 2016-05-18 21:42:33 53705 2005-12-01 00:00:00 53905.4622337963 2006-06-19 11:05:37 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000009 HXD spectrum and timing check CALIBRATION 1 A SWG JAP 0 SWG PSR1509-58 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100009010/ Quick Look
11 Crab Nebula 83.6267 22.0751 82.874095 22.042383 84.095945 -1.235244 184.50282132 -5.75691305 86.8655 53607.0070833333 2005-08-25 00:10:12 53607.1389814815 2005-08-25 03:20:08 100010010 2.9379 5 2.9379 2.9379 2.9379 2.9379 2 2 2 2 1 0 0 3.4387 3.4387 11.3819 0 PROCESSED 57526.8678703704 2016-05-18 20:49:44 54247 2007-05-27 00:00:00 54118.9886689815 2007-01-18 23:43:41 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010010/ Quick Look
12 Crab nebula 83.6336 21.9568 82.881657 21.924117 84.097114 -1.353715 184.60669551 -5.81484075 86.8687 53607.1394560185 2005-08-25 03:20:49 53607.2779282407 2005-08-25 06:40:13 100010020 3.6533 5 3.6533 3.6533 3.6533 3.6533 1 1 1 1 1 0 0 3.8067 3.8067 11.934 0 PROCESSED 57526.8772337963 2016-05-18 21:03:13 54247 2007-05-27 00:00:00 54118.9337615741 2007-01-18 22:24:37 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010020/ Quick Look
13 Crab nebula 83.6511 21.6763 82.900722 21.643705 84.100986 -1.634666 184.85366771 -5.95118505 86.8795 53607.5153125 2005-08-25 12:22:03 53607.7153472222 2005-08-25 17:10:06 100010040 9.5806 5 9.5806 9.5806 9.5806 9.5806 1 1 1 1 1 0 0 8.1783 8.1783 17.248 0 PROCESSED 57526.8981828704 2016-05-18 21:33:23 54247 2007-05-27 00:00:00 54118.943125 2007-01-18 22:38:06 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010040/ Quick Look
14 Crab nebula 83.5677 22.0135 82.815455 21.980499 84.038563 -1.294359 184.52566905 -5.83608695 86.8444 53607.9175810185 2005-08-25 22:01:19 53608.0695023148 2005-08-26 01:40:05 100010060 4.8779 5 4.8779 4.8779 4.8779 4.8779 1 1 1 1 1 0 0 5.0217 5.0217 13.076 0 PROCESSED 57526.9066087963 2016-05-18 21:45:31 54247 2007-05-27 00:00:00 54122.4195486111 2007-01-22 10:04:09 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010060/ Quick Look
15 Crab nebula 83.6922 22.0221 82.939876 21.989699 84.154283 -1.290862 184.58047361 -5.73399538 86.8671 53608.0699768518 2005-08-26 01:40:46 53608.2084027778 2005-08-26 05:00:06 100010070 4.0899 5 4.0899 4.0899 4.0899 4.0899 1 1 1 1 1 0 0 4.2283 4.2283 11.9259 0 PROCESSED 57526.9072222222 2016-05-18 21:46:24 54247 2007-05-27 00:00:00 54119.0149074074 2007-01-19 00:21:28 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010070/ Quick Look
16 Crab nebula 83.5807 22.8483 82.82374 22.81535 84.087744 -0.460898 183.82410841 -5.37832099 86.8677 53608.3175810185 2005-08-26 07:37:19 53608.5139583333 2005-08-26 12:20:06 100010090 6.716 5 6.716 6.716 6.716 6.716 1 1 1 1 1 0 0 6.3768 6.3768 16.9501 0 PROCESSED 57526.9164699074 2016-05-18 21:59:43 54247 2007-05-27 00:00:00 54119.0235648148 2007-01-19 00:33:56 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010090/ Quick Look
17 Crab nebula 83.5122 24.0135 82.748583 23.980205 84.077056 0.70598 182.80375415 -4.80497322 86.8675 53608.7179976852 2005-08-26 17:13:55 53608.930625 2005-08-26 22:20:06 100010110 9.4805 5 9.4805 9.4805 9.4805 9.4805 1 1 1 1 1 0 0 7.363 7.363 18.336 0 PROCESSED 57526.9265162037 2016-05-18 22:14:11 54247 2007-05-27 00:00:00 54118.98625 2007-01-18 23:40:12 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010110/ Quick Look
18 Crab nebula 83.6374 21.9009 82.885769 21.868236 84.09817 -1.409717 184.65605757 -5.84178049 86.8664 53608.9333217593 2005-08-26 22:23:59 53609.069525463 2005-08-27 01:40:07 100010120 4.7456 5 4.7456 4.7456 4.7456 4.7456 2 2 2 2 1 0 0 5.1787 5.1787 11.7579 1 PROCESSED 57526.9343287037 2016-05-18 22:25:26 54247 2007-05-27 00:00:00 54118.9946180556 2007-01-18 23:52:15 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010120/ Quick Look
19 Crab nebula 83.5044 22.0116 82.752181 21.978293 83.979835 -1.293628 184.49566519 -5.88665136 86.8658 53609.0701388889 2005-08-27 01:41:00 53609.2014583333 2005-08-27 04:50:06 100010130 4.222 5 4.222 4.222 4.222 4.222 1 1 1 1 1 0 0 4.3724 4.3724 11.3359 0 PROCESSED 57526.9346180556 2016-05-18 22:25:51 54247 2007-05-27 00:00:00 54119.0454282407 2007-01-19 01:05:25 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010130/ Quick Look
20 Galactic bulge 236.4313 -31.7013 235.648361 -31.545749 241.296308 -11.543137 340.99994533 17.99808229 283.5446 53609.4365856482 2005-08-27 10:28:41 53611.060625 2005-08-29 01:27:18 100011010 61.133 70 61.133 61.133 61.133 61.133 1 1 1 1 1 0 0 47.9834 47.9834 140.282 2 PROCESSED 57526.962037037 2016-05-18 23:05:20 54247 2007-05-27 00:00:00 54034.8288310185 2006-10-26 19:53:31 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000011 CALIBRATION 1 A SWG JAP 0 SWG Galactic bulge N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100011010/ Quick Look
21 Eta Carinae 161.281 -59.6845 160.794333 -59.421136 202.162077 -58.916082 287.6040589 -0.62575348 343.8621 53611.0750347222 2005-08-29 01:48:03 53612.0627546296 2005-08-30 01:30:22 100012010 49.782 40 49.79 49.782 49.782 49.798 2 2 2 2 1 0 0 55.9607 55.9607 85.2529 0 PROCESSED 57526.9773032407 2016-05-18 23:27:19 53705 2005-12-01 00:00:00 53905.4648842593 2006-06-19 11:09:26 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000012 CALIBRATION 1 A SWG JAP 0 SWG Eta Carinae N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100012010/ Quick Look
22 N103B 77.2315 -68.7507 77.290508 -68.812132 329.838884 -84.691105 279.61119012 -34.36730962 73.8586 53612.0740162037 2005-08-30 01:46:35 53613.0626273148 2005-08-31 01:30:11 100013010 33.0646 40 33.0646 33.0646 33.0646 33.0646 2 2 2 2 1 0 0 37.2814 37.2814 85.4059 1 PROCESSED 57526.9730324074 2016-05-18 23:21:10 54247 2007-05-27 00:00:00 54034.8733449074 2006-10-26 20:57:37 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000013 CALIBRATION 1 A SWG JAP 0 SWG N103B N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100013010/ Quick Look
23 E0102-72 15.9813 -72.0378 15.57605 -72.305808 314.596715 -65.033076 301.56958331 -45.05740554 140.1798 53613.0710648148 2005-08-31 01:42:20 53613.7640509259 2005-08-31 18:20:14 100014010 24.3339 20 24.3339 24.3339 24.3339 24.3339 2 2 2 2 1 0 0 24.5144 24.5144 59.8639 2 PROCESSED 57511.5174884259 2016-05-03 12:25:11 53705 2005-12-01 00:00:00 53905.4615740741 2006-06-19 11:04:40 3.0.22.43 13 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000014 CALIBRATION 1 A SWG JAP 0 SWG XIS monitor with E0102-72 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100014010/ Quick Look
24 Crab Nebula 83.6296 22.1792 82.876409 22.146495 84.103227 -1.131361 184.41590928 -5.69889955 84.9998 53613.9762152778 2005-08-31 23:25:45 53614.1077314815 2005-09-01 02:35:08 100015020 4.95 5 4.95 4.95 4.95 4.95 1 1 1 1 1 0 0 5.1178 5.1178 11.3599 0 PROCESSED 57527.2276388889 2016-05-19 05:27:48 54247 2007-05-27 00:00:00 54109.1090972222 2007-01-09 02:37:06 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000015 CALIBRATION 1 A SWG JAP 0 SWG HXD boresight check with Crab N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100015020/ Quick Look
25 SN1006 SW BG 224.655 -42.4005 223.837497 -42.201017 234.783022 -24.341132 326.632731 14.54333558 310.4886 53624.9999189815 2005-09-11 23:59:53 53626.0071643518 2005-09-13 00:10:19 100019040 32.3334 50 32.3334 32.3494 32.3414 32.3414 2 2 2 2 1 0 0 24.6736 24.6736 87.0159 5 PROCESSED 57527.3647453704 2016-05-19 08:45:14 54247 2007-05-27 00:00:00 54035.4482638889 2006-10-27 10:45:30 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000019 CALIBRATION 1 A SWG JAP 0 SWG SN1006 observation with XIS and HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019040/ Quick Look
26 SN1006 SW BG 224.6468 -42.4025 223.829311 -42.202989 234.777387 -24.344913 326.62625739 14.54451897 100.3489 53761.7199652778 2006-01-26 17:16:45 53762.4752777778 2006-01-27 11:24:24 100019060 27.9813 50 27.9813 27.9893 27.9973 27.9973 2 2 2 2 1 0 0 29.5504 29.5504 65.2499 2 PROCESSED 57532.7989814815 2016-05-24 19:10:32 54247 2007-05-27 00:00:00 54040.5663541667 2006-11-01 13:35:33 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000019 CALIBRATION 1 A SWG JAP 0 SWG SN1006 observation with XIS and HXD XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019060/ Quick Look
27 Fornax Cluster 54.6395 -35.4918 54.160816 -35.653913 38.755932 -52.830853 236.7850293 -53.61976834 103.5002 53626.0756018518 2005-09-13 01:48:52 53627.5002662037 2005-09-14 12:00:23 100020010 76.0782 100 76.0782 76.0782 76.0782 76.0782 2 2 2 2 1 0 0 71.1128 71.1128 123.0639 3 PROCESSED 57527.3377430556 2016-05-19 08:06:21 54247 2007-05-27 00:00:00 54035.4442013889 2006-10-27 10:39:39 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000020 CALIBRATION 1 A SWG JAP 0 SWG Fornax Cluster N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100020010/ Quick Look
28 Crab Nebula 82.7325 21.9883 81.980613 21.951274 83.263643 -1.282782 184.12771921 -6.50224239 88.0978 53628.3006828704 2005-09-15 07:12:59 53628.5835416667 2005-09-15 14:00:18 100022020 10.9198 10 10.9198 10.9198 10.9198 10.9198 1 1 1 1 1 0 0 6.3401 6.3401 24.4 2 PROCESSED 57527.3262615741 2016-05-19 07:49:49 54247 2007-05-27 00:00:00 54109.1486342593 2007-01-09 03:34:02 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000022 Crab at 50arcmin off from the XIS aimpoint to study stray light. CALIBRATION 1 A SWG JAP 0 SWG Crab at 50 arcmin off N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100022020/ Quick Look
29 Crab Nebula 84.5289 22.0469 83.776247 22.018539 84.930453 -1.297747 184.974122 -5.06424795 87.5879 53629.0921759259 2005-09-16 02:12:44 53629.368275463 2005-09-16 08:50:19 100022030 12.8244 10 12.8404 12.8324 12.8244 12.8484 2 2 2 2 1 0 0 10.3518 10.3518 23.824 1 PROCESSED 57527.3478009259 2016-05-19 08:20:50 54247 2007-05-27 00:00:00 54109.1621527778 2007-01-09 03:53:30 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000022 Crab at 50arcmin off from the XIS aimpoint to study stray light. CALIBRATION 1 A SWG JAP 0 SWG Crab at 50 arcmin off N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100022030/ Quick Look
30 Crab Nebula 83.6282 22.0761 82.875589 22.04339 84.097378 -1.234306 184.5027205 -5.75520363 87.79 53628.5852199074 2005-09-15 14:02:43 53628.8265393518 2005-09-15 19:50:13 100023010 11.9978 10 11.9978 11.9978 11.9978 11.9978 1 1 1 1 1 0 0 10.5132 10.5132 20.8239 0 PROCESSED 57527.3355902778 2016-05-19 08:03:15 54247 2007-05-27 00:00:00 54109.2268287037 2007-01-09 05:26:38 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000023 Calibration of detector response at both of XIS/HXD nominal positions, together with an absolute flux confirmation with differnt hit-pattern widths. CALIBRATION 1 A SWG JAP 0 SWG Crab at nominal positions N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100023010/ Quick Look
31 BD +30 3639 293.6887 30.5051 293.198078 30.394341 303.540216 51.224252 64.77556877 5.01383279 277.8713 53634.3814930556 2005-09-21 09:09:21 53635.2473842593 2005-09-22 05:56:14 100025010 35.2146 40 35.2306 35.2306 35.2146 35.2226 2 2 2 2 1 0 0 33.3728 33.3728 74.8039 1 PROCESSED 57527.3931597222 2016-05-19 09:26:09 54247 2007-05-27 00:00:00 54035.4664583333 2006-10-27 11:11:42 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000025 The proposed target, BD +30 3639, is a prototypical planetary nebula which emit diffuse X-rays; planetary nebulae represent the final evolutionary stage of low mass stars, and contain very rich information on the stellar nucleosynthesis. The Chandra ACIS spectrum of BD +30 3639 bears an amazingly strong Ne-K line, most certainly because the X-ray emitting material directly reflect the "onion-like structure" of elements insied evolved stars. However, the ACIS was not able to resolve C, N, O lines, which are of vital importance. The XMM RGS and Chandra LETG could do, but we need very long exposure. Using the Suzaku XIS-BI with the excellent low-energy performance, we can for the first time measure the C/N/O/Mg abundance ratios of this important object in a short time. CALIBRATION 1 A SWG JAP 0 SWG Observation of planetary nebula BD +30 3639 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100025010/ Quick Look
32 RXJ1713-3946-BKGD2 257.2742 -41.0338 256.397744 -40.970376 259.926088 -18.035902 345.80577047 -0.54060643 270.0033 53641.2980671296 2005-09-28 07:09:13 53642.1843055556 2005-09-29 04:25:24 100026030 37.5132 40 37.5372 37.5292 37.5132 37.5132 2 2 2 2 1 0 0 31.8982 31.8982 76.5659 0 PROCESSED 57527.4461574074 2016-05-19 10:42:28 54247 2007-05-27 00:00:00 54035.6187268518 2006-10-27 14:50:58 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000026 RXJ1713 is very important sources in which we can study particle accelerator in the universe. X-ray synchrotron spectrum suggest the existence of distribution of high energy electron. Very similar TeV and ASCA morphologies show close connection between these energy bands. The interaction with molecular cloud suggests that proton accelerator resides in this object. The photon index of RXJ1713 seems to be difficult in the frame work of standard diffusive shock scenario. To obtain precise spectrum in the hard X-ray region is therefore very important to determine the energy cut off and to study the mechanism that produce such high energy electrons. CALIBRATION 1 A SWG JAP 0 SWG Observation of RXJ1713.7-3946 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100026030/ Quick Look
33 M82-Wind 148.8893 69.7655 147.850184 70.002482 118.869306 52.161633 141.33880284 40.49464345 137.7608 53647.5072800926 2005-10-04 12:10:29 53648.1418287037 2005-10-05 03:24:14 100033010 32.3274 100 32.3274 32.3274 32.3274 32.3274 2 2 2 2 1 0 0 30.2224 30.2224 54.8021 0 PROCESSED 57527.5155092593 2016-05-19 12:22:20 54247 2007-05-27 00:00:00 54037.0057175926 2006-10-29 00:08:14 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000033 We propose to observe the largely extened emission with the size of about 12kpc around M82 with Suzaku for 100ksec. CALIBRATION 1 A SWG JAP 0 SWG Largely Extended Emission (~12kpc) around M82 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100033010/ Quick Look
34 Sgr_A_west 266.3057 -29.1697 265.509983 -29.149828 266.748763 -5.770252 359.75546849 -0.04768885 264.9601 53637.5953356482 2005-09-24 14:17:17 53638.7273032407 2005-09-25 17:27:19 100027020 42.8148 50 42.8148 42.8148 42.8148 42.8148 2 2 2 2 1 0 0 36.091 36.091 97.8 0 PROCESSED 57527.4293865741 2016-05-19 10:18:19 54247 2007-05-27 00:00:00 54035.5135532407 2006-10-27 12:19:31 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000027 We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. CALIBRATION 1 A SWG JAP 0 SWG Suzaku Observation of Galactic Center Region N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027020/ Quick Look
35 E0102-72 16.139 -72.1205 15.73725 -72.388297 314.467235 -65.111919 301.50933431 -44.97149935 119.4064 53593.3086458333 2005-08-11 07:24:27 53595.2485069444 2005-08-13 05:57:51 100001010 2.4068 70 2.4068 2.4068 2.4068 2.4068 1 1 1 1 0 0 0 0 0 0 0 PROCESSED 57520.6843287037 2016-05-12 16:25:26 54247 2007-05-27 00:00:00 54035.5925115741 2006-10-27 14:13:13 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000001 XIS door open with a SMC SNR E0102-72 CALIBRATION 1 A SWG JAP 0 SWG XIS door open N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100001010/ Quick Look
36 1E1743.1-2843(GC_BGD_3) 266.592 -28.6516 265.799503 -28.633124 266.987582 -5.246121 0.32828705 0.00813221 264.88 53638.7286111111 2005-09-25 17:29:12 53638.793275463 2005-09-25 19:02:19 100027050 1.9846 5 1.9846 1.9846 1.9846 1.9846 1 1 1 1 1 0 0 1.7934 1.7934 5.5679 0 PROCESSED 57527.4093055556 2016-05-19 09:49:24 54247 2007-05-27 00:00:00 53905.6343055556 2006-06-19 15:13:24 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000027 We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. CALIBRATION 1 A SWG JAP 0 SWG Suzaku Observation of Galactic Center Region N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027050/ Quick Look
37 HESS J1616-508 244.1248 -50.8971 243.177731 -50.773494 251.629905 -29.09136 332.40352084 -0.15000913 282.8476 53632.5000231482 2005-09-19 12:00:02 53633.8183333333 2005-09-20 19:38:24 100028010 41.352 50 41.352 41.376 41.352 41.368 2 2 2 2 1 0 0 35.3731 35.3731 113.8899 0 PROCESSED 57527.3838194444 2016-05-19 09:12:42 54247 2007-05-27 00:00:00 54035.4361111111 2006-10-27 10:28:00 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000028 CALIBRATION 1 A SWG JAP 0 SWG New HESS sources and the Galactic ridge Background N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100028010/ Quick Look
38 HESS J1616-508_BGD1 243.666 -51.1742 242.717138 -51.048595 251.369654 -29.420684 332.00349288 -0.15039556 283.0062 53631.9497222222 2005-09-18 22:47:36 53632.4990856482 2005-09-19 11:58:41 100028020 19.3277 25 19.3277 20.63 19.36 19.6323 1 1 1 1 1 0 0 16.6426 16.6426 47.4479 0 PROCESSED 57527.3573148148 2016-05-19 08:34:32 54247 2007-05-27 00:00:00 54035.1692476852 2006-10-27 04:03:43 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000028 CALIBRATION 1 A SWG JAP 0 SWG New HESS sources and the Galactic ridge Background N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100028020/ Quick Look
39 GRO J1655-40 253.5027 -39.8455 252.639975 -39.764411 256.800671 -17.156383 344.98315976 2.45489032 268.0237 53635.3140625 2005-09-22 07:32:15 53636.2968055556 2005-09-23 07:07:24 100029010 35.2228 40 0 35.2336 35.2228 35.2308 0 1 2 2 1 0 0 28.7315 28.7315 84.9019 1 PROCESSED 57527.3997337963 2016-05-19 09:35:37 54247 2007-05-27 00:00:00 54035.4940625 2006-10-27 11:51:27 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000029 We propose to observe GRO J1655-40, a transient galactic black hole candidate. With M=~7 Msolar and distinct radio lobes, GRO J1655-40 has been classified as a microquasar. It was highly variable during the first few years after its discovery while showing irregular flaring and a wide range of continuum states. Discrete Fe K absorption structure was observed with ASCA. In the summer of 1997 it entered an extended quiescence that lasted for ~8 years. In March 2005 it became active again and XMM & Chandra have observed it since. Only Suzaku can provide the broadband sensitivity required to map the Fe K structure and the continuum as they change. GRO J1655-40 is rapidly declining and must be observed soon before it reenters quiescence. CALIBRATION 1 A SWG JAP 0 SWG GRO J1655-40 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100029010/ Quick Look
40 NGC3516 166.7299 72.5779 165.877553 72.848305 123.367172 57.997458 133.2179652 42.40001774 148.9366 53655.5813541667 2005-10-12 13:57:09 53658.3801388889 2005-10-15 09:07:24 100031010 134.4696 150 134.5096 134.5956 134.5096 134.4696 2 2 2 2 1 0 0 122.818 122.818 241.6848 0 PROCESSED 57527.6243634259 2016-05-19 14:59:05 54247 2007-05-27 00:00:00 54036.4704976852 2006-10-28 11:17:31 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000031 NGC 3516 is one of the brightest Seyfert 1s seen in BAT currently visible to Suzaku. Recent BAT and RXTE observations show that this source is ~2-3 mCrb in the 2-10 keV band and ~4-5 mCrb in 15-100 keV. NGC 3516 is currently much brighter than when XMM observed it in 2000 (e.g., it has since returned to "typical" flux). This source's Fe K line and Compton reflection hump are both quite strong (e.g., as seen with SAX; R is ~1.8 in SAX data). CALIBRATION 1 A SWG JAP 0 SWG NGC 3516 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100031010/ Quick Look
41 M82-Wind 148.894 69.7643 147.854963 70.001295 118.872596 52.161537 141.33883884 40.49666381 146.246 53662.0401273148 2005-10-19 00:57:47 53662.9390393518 2005-10-19 22:32:13 100033020 40.3586 100 40.3586 40.3826 40.3586 40.3666 2 2 2 2 1 0 0 38.3533 38.3533 77.658 0 PROCESSED 57527.6127546296 2016-05-19 14:42:22 54247 2007-05-27 00:00:00 54036.4196296296 2006-10-28 10:04:16 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000033 We propose to observe the largely extened emission with the size of about 12kpc around M82 with Suzaku for 100ksec. CALIBRATION 1 A SWG JAP 0 SWG Largely Extended Emission (~12kpc) around M82 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100033020/ Quick Look
42 M82-Wind 148.8885 69.7652 147.849381 70.00218 118.869202 52.16123 141.33933547 40.4945935 137.7608 53670.4681134259 2005-10-27 11:14:05 53671.1002199074 2005-10-28 02:24:19 100033030 28.3638 100 28.3798 28.3798 28.3718 28.3638 2 2 2 2 1 0 0 25.8121 25.8121 54.604 1 PROCESSED 57527.6784606482 2016-05-19 16:16:59 54247 2007-05-27 00:00:00 54036.8639467593 2006-10-28 20:44:05 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000033 We propose to observe the largely extened emission with the size of about 12kpc around M82 with Suzaku for 100ksec. CALIBRATION 1 A SWG JAP 0 SWG Largely Extended Emission (~12kpc) around M82 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100033030/ Quick Look
43 Her X-1 254.465 35.3306 254.01442 35.406187 246.002276 57.482156 58.13562438 37.51514805 249.5714 53648.6450462963 2005-10-05 15:28:52 53649.4341898148 2005-10-06 10:25:14 100035010 36.1235 40 36.9235 36.1235 36.9235 36.9235 2 1 2 2 1 0 0 33.3229 33.3229 68.178 0 PROCESSED 57527.5593518518 2016-05-19 13:25:28 54247 2007-05-27 00:00:00 54036.0084375 2006-10-28 00:12:09 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000035 CALIBRATION 1 A SWG JAP 0 SWG HXD Performance Verification using Her X-1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100035010/ Quick Look
44 Sgr_A_west 266.3063 -29.1685 265.51059 -29.148631 266.749258 -5.769039 359.75676556 -0.04750971 264.9604 53642.1914467593 2005-09-29 04:35:41 53643.187025463 2005-09-30 04:29:19 100037010 43.7412 50 43.7412 43.7492 43.7492 43.7492 2 2 2 2 1 0 0 39.3941 39.3941 86.0139 0 PROCESSED 57527.4581828704 2016-05-19 10:59:47 54247 2007-05-27 00:00:00 54035.6663310185 2006-10-27 15:59:31 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000037 CALIBRATION 1 A SWG JAP 0 SWG Suzaku Obseration of Galactic Center region 2 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100037010/ Quick Look
45 GRS1915+105 288.8014 10.9368 288.21144 10.848425 292.141211 32.943669 45.35928754 -0.22611181 260.5762 53659.6951967593 2005-10-16 16:41:05 53661.9724305556 2005-10-18 23:20:18 100039010 84.7777 80 85.0631 86.4305 85.0711 84.7777 3 3 3 3 1 0 0 68.8623 68.8623 196.7338 2 PROCESSED 57527.9188541667 2016-05-19 22:03:09 54247 2007-05-27 00:00:00 54043.8117476852 2006-11-04 19:28:55 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000039 This observation will be performed as a part of the big multiwavelength campain including Suzaku, VLA, Integral, RXTE, and Spitzer. CALIBRATION 1 A SWG JAP 0 SWG Campaign of coordinated observation of GRS 1915+105 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100039010/ Quick Look
46 RXJ1856.5-3754 284.1433 -37.91 283.291633 -37.976029 281.504649 -15.032837 358.59722216 -17.21146697 84.0127 53817.9388078704 2006-03-23 22:31:53 53819.4433217593 2006-03-25 10:38:23 100041020 79.169 80 79.177 79.169 79.177 79.177 2 2 2 2 1 0 0 53.2099 53.2099 129.9759 1 PROCESSED 57533.3325231482 2016-05-25 07:58:50 54247 2007-05-27 00:00:00 54042.2967824074 2006-11-03 07:07:22 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000041 We propose Suzaku observation of a nearby isolated neuron star RXJ1856.5-3754 for the low energy QE calibration of the XIS. Our main purpose is, however, using this source as a soft X-ray QE calibrator on the sky. We hope this source will be observed again in future to check possible contamination on the filter surface etc. Note that the calibration is not only for the BI-CCD(XIS1), but also for FI-CCDs or relative QE among them. CALIBRATION 1 A SWG JAP 0 SWG LOW ENERGY QE CALIBRATION OF XIS XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100041020/ Quick Look
47 Crab nebula 83.6399 21.8519 82.888543 21.819249 84.098328 -1.458773 184.69891686 -5.86604099 86.8683 53604.3898263889 2005-08-22 09:21:21 53604.4890972222 2005-08-22 11:44:18 100007030 2.7861 5 2.7861 2.7861 2.7901 2.7861 1 1 1 1 1 0 0 2.1927 2.1927 8.5541 0 PROCESSED 57520.7416203704 2016-05-12 17:47:56 54247 2007-05-27 00:00:00 54105.2865393518 2007-01-05 06:52:37 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000007 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Nebula N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100007030/ Quick Look
48 E0102-72 15.9926 -72.0236 15.587314 -72.291594 314.630688 -65.030221 301.56327722 -45.07133229 226.8326 53720.0716203704 2005-12-16 01:43:08 53723.4377199074 2005-12-19 10:30:19 100044010 59.731 20 59.735 125.9195 59.731 59.737 3 3 3 3 1 0 0 115.3302 115.3302 290.8037 1 PROCESSED 57532.5803935185 2016-05-24 13:55:46 54247 2007-05-27 00:00:00 54119.7612615741 2007-01-19 18:16:13 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001097 We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip CALIBRATION 1 A HIRONORI MATSUMOTO JAP 0 SWG XIS FLIGHT CAIBRATION PLAN N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100044010/ Quick Look
49 CYGNUS LOOP 314.0345 31.9311 313.518544 31.738505 329.353732 46.719144 75.67403832 -8.61676541 64.2261 53884.1556018518 2006-05-29 03:44:04 53884.3793865741 2006-05-29 09:06:19 100049010 8.3805 10 8.3805 8.3805 8.3805 8.3805 1 1 1 1 1 0 0 6.0211 6.0211 19.304 0 PROCESSED 57534.4628240741 2016-05-26 11:06:28 54258 2007-06-07 00:00:00 54059.411099537 2006-11-20 09:51:59 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 015007 Here is the list of the calibration sources in the AO-1 round: 1) E0102.2-7219 20ks x 2 2) PKS2155-304 30ks (simultaneous observation with CXO and XMM) 3) Galactic Center Plasma 50ks 4) Cygnus Loop 40ks (=10ks x 4), and 5) RXJ1856.5-3754 40ks CALIBRATION 1 A HIRONORI MATSUMOTO JAP 1 SWG XIS FLIGHT CALIBRATION PLAN SPE N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100049010/ Quick Look
50 CYGNUS LOOP 314.0785 32.0438 313.563 31.85105 329.470002 46.807189 75.78588033 -8.57358243 64.2263 53884.3796759259 2006-05-29 09:06:44 53884.6086342593 2006-05-29 14:36:26 100049020 7.8928 10 7.8928 7.8928 7.8928 7.8928 2 2 2 2 1 0 0 7.452 7.452 19.7699 0 PROCESSED 57534.4674884259 2016-05-26 11:13:11 54258 2007-06-07 00:00:00 54088.8429513889 2006-12-19 20:13:51 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 015007 Here is the list of the calibration sources in the AO-1 round: 1) E0102.2-7219 20ks x 2 2) PKS2155-304 30ks (simultaneous observation with CXO and XMM) 3) Galactic Center Plasma 50ks 4) Cygnus Loop 40ks (=10ks x 4), and 5) RXJ1856.5-3754 40ks CALIBRATION 1 A HIRONORI MATSUMOTO JAP 1 SWG XIS FLIGHT CALIBRATION PLAN SPE N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100049020/ Quick Look
51 CYGNUS LOOP 313.9494 32.0818 313.434356 31.889502 329.346118 46.886158 75.74490282 -8.46508453 64.2292 53884.6089236111 2006-05-29 14:36:51 53884.8377777778 2006-05-29 20:06:24 100049030 11.6971 10 11.7051 11.6971 11.7051 11.7051 2 2 2 2 1 0 0 12.2688 12.2688 19.772 0 PROCESSED 57534.4722800926 2016-05-26 11:20:05 54258 2007-06-07 00:00:00 54052.4915046296 2006-11-13 11:47:46 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 015007 Here is the list of the calibration sources in the AO-1 round: 1) E0102.2-7219 20ks x 2 2) PKS2155-304 30ks (simultaneous observation with CXO and XMM) 3) Galactic Center Plasma 50ks 4) Cygnus Loop 40ks (=10ks x 4), and 5) RXJ1856.5-3754 40ks CALIBRATION 1 A HIRONORI MATSUMOTO JAP 1 SWG XIS FLIGHT CALIBRATION PLAN SPE N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100049030/ Quick Look
52 Crab nebula 83.9887 22.0345 83.236236 22.00353 84.429494 -1.290207 184.71743044 -5.49499441 86.8666 53608.5155902778 2005-08-26 12:22:27 53608.7153472222 2005-08-26 17:10:06 100010100 9.694 5 9.694 9.694 9.694 9.694 1 1 1 1 1 0 0 7.5812 7.5812 17.2479 0 PROCESSED 57526.9259606482 2016-05-18 22:13:23 54247 2007-05-27 00:00:00 54122.4242939815 2007-01-22 10:10:59 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010100/ Quick Look
53 Vega 279.2264 38.7699 278.806278 38.72626 285.283614 61.72204 67.43212753 19.23869014 301.7896 53615.367349537 2005-09-02 08:48:59 53615.603587963 2005-09-02 14:29:10 100017010 11.3985 10 11.4065 11.4065 11.4065 11.3985 2 2 2 2 1 0 0 11.5751 11.5751 20.4039 0 PROCESSED 57527.2607407407 2016-05-19 06:15:28 54247 2007-05-27 00:00:00 53906.0764814815 2006-06-20 01:50:08 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000017 CALIBRATION 1 A SWG JAP 0 SWG XIS OBF check with Vega N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100017010/ Quick Look
54 A0535+026 84.7243 26.3189 83.946776 26.291426 85.267864 2.964757 181.44092218 -2.64422146 83.608 53627.5694907407 2005-09-14 13:40:04 53628.0418865741 2005-09-15 01:00:19 100021010 21.761 20 21.761 21.761 21.761 21.761 2 2 2 2 1 0 0 21.2572 21.2572 40.7839 1 PROCESSED 57527.3122337963 2016-05-19 07:29:37 54247 2007-05-27 00:00:00 54035.0644444444 2006-10-27 01:32:48 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000021 We propose to observe the X-ray binary pulsar A0535+26. The main objectives is measuring changes in the cyclotron resonance energy in an outburst decay.It is known from another X-ray pulsar 4U0115+63 that the cyclotron resonance energy increased from 11 keV to 16 keV, as the luminosity decreased across a threshold luminosity of 4x10^37 erg/s. The flare of A0535+26 is a chance to know whether this behavior is the RULE among binary pulsars or an EXCEPTION. A0535+26 is fading down and will reach 30mCrab (5-100keV) on September 17, which is 5x10^36 erg/s. It is better to be observed as soon as possible, before it fades out. CALIBRATION 1 A SWG JAP 0 SWG TOO Observation of A0535+026 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100021010/ Quick Look
55 Crab nebula 83.7552 22.0249 83.002845 21.992803 84.212769 -1.290605 184.60948321 -5.68314749 86.8656 53609.2022106482 2005-08-27 04:51:11 53609.3125810185 2005-08-27 07:30:07 100010140 3.419 5 3.419 3.419 3.419 3.419 1 1 1 1 1 0 0 3.7554 3.7554 9.5319 0 PROCESSED 57526.9383217593 2016-05-18 22:31:11 54247 2007-05-27 00:00:00 54118.9983796296 2007-01-18 23:57:40 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010140/ Quick Look
56 Crab Nebula 83.6309 22.0151 82.87863 21.982404 84.097185 -1.295359 184.55585082 -5.78574816 87.8466 53628.8269212963 2005-09-15 19:50:46 53629.0904976852 2005-09-16 02:10:19 100023020 12.5271 10 12.5311 12.5271 12.5364 12.5351 2 2 2 2 1 0 0 13.3529 13.3529 22.764 1 PROCESSED 57527.3409143518 2016-05-19 08:10:55 54247 2007-05-27 00:00:00 54109.193599537 2007-01-09 04:38:47 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000023 Calibration of detector response at both of XIS/HXD nominal positions, together with an absolute flux confirmation with differnt hit-pattern widths. CALIBRATION 1 A SWG JAP 0 SWG Crab at nominal positions N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100023020/ Quick Look
57 NGC 2110 88.0444 -7.458 87.440268 -7.468978 87.743148 -30.884192 212.92660512 -16.54877043 103.4188 53629.3796296296 2005-09-16 09:06:40 53631.8308333333 2005-09-18 19:56:24 100024010 101.7487 100 101.9265 103.7601 101.7487 102.1483 2 2 2 2 1 0 0 86.0433 86.0433 211.7558 4 PROCESSED 57527.4030324074 2016-05-19 09:40:22 54247 2007-05-27 00:00:00 54035.4624189815 2006-10-27 11:05:53 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000024 The Narrow Emission Line Galaxy NGC 2110 was the brightest AGN in the initial BAT survey release (BAT flux of 2.1E-10 erg/cm2/sec) visible to Suzaku during Sept./Oct., and is still currently bright in BAT. A 2003 RXTE observation yielded F_2-10 keV = 4E-11 erg/cm2/sec. The source is currently almost 3 times brighter than during the SAX observations. The main goals are to measure the high energy cutoff and to place a strong limit on the presence of reflection. The Compton reflection hump is weak in SAX data (suggesting that the Fe K line originates in Compton-thin material). Determining the strength of the reflection component is critical for constraining the geometry of the accreting material. CALIBRATION 1 A SWG JAP 0 SWG Narrow Emission Line Galaxy NGC 2110 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100024010/ Quick Look
58 GX 349+2 256.427 -36.366 255.587548 -36.298664 258.786235 -13.451096 349.14511841 2.78820606 85.6584 53808.5453240741 2006-03-14 13:05:16 53809.2216782407 2006-03-15 05:19:13 400003010 25.2308 50 25.2308 25.2332 25.2308 25.2308 1 1 1 1 1 0 0 20.0507 20.0507 58.434 2 PROCESSED 57533.2006365741 2016-05-25 04:48:55 54247 2007-05-27 00:00:00 54041.9132060185 2006-11-02 21:55:01 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001026 We propose Suzaku observations of two luminous low-mass X-ray binaries (Z sources), GX 349+2 and Cyg X-2, to investigate the origin of the hard tails of Z sources, of which the spectral photon indices are reported to become occasionally less than unity. With the high sensitivity of the HXD, we detect the spectral shape up to several 100 keV and reveal existence of particle acceleration caused by high radiation pressure. GALACTIC POINT SOURCES 4 A HIROMITSU TAKAHASHI JAP 0 SWG SUZAKU OBSERVATIONS OF THE HARD TAILS OF LUMINOUS LOW-MASS X-RAY BINARIES (Z SOURCES) HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400003010/ Quick Look
59 SS CYG 325.6789 43.5736 325.187819 43.344381 350.451149 52.649921 90.55119171 -7.12024619 276.5788 53676.0503703704 2005-11-02 01:12:32 53676.9856944444 2005-11-02 23:39:24 400006010 39.4512 40 39.4512 39.4512 39.4512 39.4512 2 2 2 2 1 0 0 32.0472 32.0472 80.81 1 PROCESSED 57527.7175925926 2016-05-19 17:13:20 54247 2007-05-27 00:00:00 54036.9898148148 2006-10-28 23:45:20 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001043 Although the boundary layer that is formed between the rapidly rotating inner accretion disk and the white dwarf surface has been known as a hard-X-ray emitter, its geometry and structure has not been well understood yet. We aim to investigate the boundary layer structure with SS Cyg, the brightest dwarf nova, by means of a soft X-ray component with the BI CCD, a fluorescent Fe K-alpha line with the FI CCDs, and a continuum reflection by the white dwarf surface with the HXD PIN. It is of great use to observe states of a different mass accretion rate, and hence we propose to observe both in quiescence and in outburst. GALACTIC POINT SOURCES 4 A MANABU ISHIDA JAP 0 SWG SS CYG OBSERVATION IN QUIESCENCE N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400006010/ Quick Look
60 X1630-472 248.4706 -47.343 247.550146 -47.238721 254.054156 -25.085181 336.93140696 0.30212129 69.0657 53781.9791087963 2006-02-15 23:29:55 53782.5474305556 2006-02-16 13:08:18 400010020 21.429 200 21.429 21.485 21.429 21.429 2 2 2 2 1 0 0 17.0223 17.0223 49.1019 0 PROCESSED 57533.0117592593 2016-05-25 00:16:56 54247 2007-05-27 00:00:00 54041.4892013889 2006-11-02 11:44:27 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001058 We propose to monitor a transient black hole binary in outburst through a series of 20 ks observations. Our goal is to map the physical conditions in the accretion disk as the source evolves through the various continuum states using the spectral diagnostics available in the Fe K fluorescence emission. Measurements of the Fe K emission will allow us to quantify the thermal, kinematic, and geometric conditions in both the disk and the surrounding material. Correlating the Fe K diagnostics with sensitive measurements of the direct and reprocessed continuum emission will allow us to map the evolving conditions and constrain models of the dynamic accretion processes in black hole binaries. We will monitor 7 targets with the RXTE. This observation will be triggered when one becomes active. GALACTIC POINT SOURCES 4 A JEAN COTTAM JAP 0 SWG-TOO FE K SPECTROSCOPY OF TRANSIENT BLACK HOLE BINARIES HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400010020/ Quick Look
61 NGC 4051 180.8556 44.5807 180.217538 44.859022 159.275193 40.404023 148.68917976 70.06918189 135.3482 53684.8015509259 2005-11-10 19:14:14 53687.4315277778 2005-11-13 10:21:24 700004010 119.578 150 119.61 119.61 119.586 119.578 2 2 2 2 1 0 0 120.0047 120.0047 227.1918 3 PROCESSED 57528.0225810185 2016-05-20 00:32:31 54247 2007-05-27 00:00:00 54037.5713078704 2006-10-29 13:42:41 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001012 We propose to obtain a broad band spectrum of the narrow-line Seyfert 1 (NLS1) NGC 4051. NLS1s are often presumed that they host a relatively small black hole with a very high accretion rate. Such a class would have played an important role in the growth of black holes in a cosmological context. We will measure the intrinsic photon index, amount of reflection, and high energy cutoff for the first time to investigate an accretion disk under a high accretion rate and compare them with conventional broad-line Seyferts. EXTRAGALACTIC COMPACT SOURCES 7 A YUICHI TERASHIMA JAP 0 SWG THE ACCRETION IN THE NARROW-LINE SEYFERT 1 NGC 4051 PROBED BY A BROAD BAND SPECTRUM HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700004010/ Quick Look
62 SN1006 SW-Rim 225.5051 -42.0698 224.686984 -41.873221 235.327536 -23.832864 327.36692545 14.52303039 297.2712 53623.5862962963 2005-09-10 14:04:16 53624.993287037 2005-09-11 23:50:20 100019030 28.5245 50 28.5325 28.5245 28.5409 28.5405 2 2 2 2 1 0 0 27.0082 27.0082 121.5519 5 PROCESSED 57527.3126967593 2016-05-19 07:30:17 54247 2007-05-27 00:00:00 54034.9697453704 2006-10-26 23:16:26 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000019 CALIBRATION 1 A SWG JAP 0 SWG SN1006 observation with XIS and HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019030/ Quick Look
63 BD +30 3639 293.6993 30.5065 293.208675 30.395694 303.554886 51.223276 64.78119899 5.00649051 237.7342 53676.9934837963 2005-11-02 23:50:37 53677.8230324074 2005-11-03 19:45:10 100025020 31.1384 40 31.1384 31.1624 31.1464 31.1544 2 2 2 2 1 0 0 27.1258 27.1258 71.638 1 PROCESSED 57527.9315509259 2016-05-19 22:21:26 54247 2007-05-27 00:00:00 54037.1080902778 2006-10-29 02:35:39 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000025 The proposed target, BD +30 3639, is a prototypical planetary nebula which emit diffuse X-rays; planetary nebulae represent the final evolutionary stage of low mass stars, and contain very rich information on the stellar nucleosynthesis. The Chandra ACIS spectrum of BD +30 3639 bears an amazingly strong Ne-K line, most certainly because the X-ray emitting material directly reflect the "onion-like structure" of elements insied evolved stars. However, the ACIS was not able to resolve C, N, O lines, which are of vital importance. The XMM RGS and Chandra LETG could do, but we need very long exposure. Using the Suzaku XIS-BI with the excellent low-energy performance, we can for the first time measure the C/N/O/Mg abundance ratios of this important object in a short time. CALIBRATION 1 A SWG JAP 0 SWG Observation of planetary nebula BD +30 3639 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100025020/ Quick Look
64 KS1741-293(GC_BGD_2) 266.2069 -29.3515 265.410046 -29.331146 266.666918 -5.954235 359.55541243 -0.06909433 265.0174 53637.5288541667 2005-09-24 12:41:33 53637.5946296296 2005-09-24 14:16:16 100027040 1.937 5 1.937 1.937 1.937 1.937 1 1 1 1 1 0 0 1.7637 1.7637 5.68 0 PROCESSED 57527.404525463 2016-05-19 09:42:31 54247 2007-05-27 00:00:00 53907.393275463 2006-06-21 09:26:19 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000027 We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. CALIBRATION 1 A SWG JAP 0 SWG Suzaku Observation of Galactic Center Region N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027040/ Quick Look
65 HESS J1616-508_BGD2 244.4656 -50.6883 243.5199 -50.566183 251.824242 -28.844194 332.70353325 -0.14997577 283.1793 53633.8196412037 2005-09-20 19:40:17 53634.3120833333 2005-09-21 07:29:24 100028030 21.8735 25 21.8895 21.8895 21.8815 21.8735 1 1 1 1 1 0 0 18.2063 18.2063 42.5359 0 PROCESSED 57527.3722800926 2016-05-19 08:56:05 54247 2007-05-27 00:00:00 54035.4698842593 2006-10-27 11:16:38 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000028 CALIBRATION 1 A SWG JAP 0 SWG New HESS sources and the Galactic ridge Background N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100028030/ Quick Look
66 ULXs in NGC 1313 49.5245 -66.5352 49.373425 -66.716272 341.380796 -74.178462 283.41323765 -44.63106544 172.6337 53658.556400463 2005-10-15 13:21:13 53659.6252777778 2005-10-16 15:00:24 100032010 32.878 40 32.878 32.878 32.878 32.878 1 1 1 1 1 0 0 30.38 30.38 92.3439 1 PROCESSED 57527.587349537 2016-05-19 14:05:47 54247 2007-05-27 00:00:00 54036.1929398148 2006-10-28 04:37:50 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000032 We propose Suzaku observation of a nearby (4.5 Mpc) galaxy NGC 1313 hosting two prototypical ULXs. These ASCA specta of many ULXs were described with a "high temperature diskbb" model, spectra obtained with XMM (and Chandra) prefer a "power-law plus low-temperature disk" modeling. The superior 5-10 keV sensitivity of Suzaku allows us to examine whether the spectra of luminous ULXs indeed exhibit a turn-over around 5 keV or extend up to 10 keV. CALIBRATION 1 A SWG JAP 0 SWG ULXs in NGC 1313 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100032010/ Quick Look
67 A 3376 90.5561 -39.9584 90.148808 -39.956705 90.960808 -63.398292 246.50686261 -25.98989573 107.6124 53649.6153703704 2005-10-06 14:46:08 53653.4495833333 2005-10-10 10:47:24 100034010 118.7792 150 118.7792 121.7373 118.8498 119.3357 2 2 2 2 1 0 0 100.5401 100.5401 331.2537 3 PROCESSED 57527.6218171296 2016-05-19 14:55:25 54247 2007-05-27 00:00:00 54109.6396990741 2007-01-09 15:21:10 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000034 Abell 3376 (z=0.046) is a merging cluster with a T=4 keV (*3) hosting a pair of strong radio halos (see figure). It is one of the few clusters from which BeppoSAX positively detected excess hard X-rays (Nevalainen et al. ApJ 608, 166, 2004). Because of the relatively low temperature, the HXD-PIN energy band is expected to be relatively free from thermal emission, making this object ideal to the search for non-thermal signals. We expect the non-thermal flux to be 4-5% of the PIN background at 20 keV, and a 150 ksec on-source exposure would be needed to securely detect this. To know the current background over the full COR range, an off-source exposure for one day or a ~40 ksec exposure onto a very soft source, would be required immediately before or after the on-source data acquisition. CALIBRATION 1 A SWG JAP 0 SWG Diffuse Hard X-rays from Clusters N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100034010/ Quick Look
68 1E1743.1-2843 GCBGD3 266.5944 -28.6526 265.801896 -28.634135 266.98972 -5.247071 0.32852719 0.00581314 264.8798 53644.2657523148 2005-10-01 06:22:41 53644.3162268518 2005-10-01 07:35:22 100037050 2.4 5 2.4 2.4 2.4 2.4 2 2 2 2 1 0 0 2.2329 2.2329 4.3539 0 PROCESSED 57527.4530902778 2016-05-19 10:52:27 54247 2007-05-27 00:00:00 54056.1970833333 2006-11-17 04:43:48 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000037 CALIBRATION 1 A SWG JAP 0 SWG Suzaku Obseration of Galactic Center region 2 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100037050/ Quick Look
69 NORTH POLAR SPUR 260.5905 4.7489 259.972652 4.795886 259.371969 27.842624 26.83412197 21.95376599 264.1143 53646.4785763889 2005-10-03 11:29:09 53647.4515277778 2005-10-04 10:50:12 100038010 43.0689 50 43.1489 44.2129 43.0689 43.2929 2 2 2 2 1 0 0 40.7715 40.7715 84.0019 0 PROCESSED 57527.5342824074 2016-05-19 12:49:22 54247 2007-05-27 00:00:00 54035.8928009259 2006-10-27 21:25:38 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000038 We propose to observe the North Polar Spur for 100 ksec. The main objectives are below (1) Search for emission lines of N and C that originates from low kT emission (2) Precisely determine the abundance of the NPS The measurement of N and C lines will be the first for XIS. This is also the first for extended sources. The first trial to measure the emission from the C-band (below 0.3keV) by using BI. This will be a guide line how to use the C-band data. Since the C-band intensity is already known, this will be the first calibration of the BI at low energy. The scientific objectives are already given in the mail distributed in the swg. CALIBRATION 1 A SWG JAP 0 SWG North Polar Spur N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100038010/ Quick Look
70 CAS A 350.8761 58.8091 350.310124 58.534509 27.390357 54.841399 111.74552355 -2.13963884 214.5537 53783.6003472222 2006-02-17 14:24:30 53783.9218055556 2006-02-17 22:07:24 100043020 14.155 10 14.155 14.155 14.155 14.155 1 1 1 1 1 0 0 17.3713 17.3713 27.768 0 PROCESSED 57533.0311805556 2016-05-25 00:44:54 54247 2007-05-27 00:00:00 54041.4627893518 2006-11-02 11:06:25 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001097 We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip CALIBRATION 1 A HIRONORI MATSUMOTO JAP 0 SWG XIS FLIGHT CAIBRATION PLAN XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100043020/ Quick Look
71 Crab Nebula 83.6372 22.097 82.884469 22.064333 84.106634 -1.213794 184.48946706 -5.73697 84.9994 53613.8323032407 2005-08-31 19:58:31 53613.975787037 2005-08-31 23:25:08 100015010 5.6587 5 5.6587 5.6587 5.6587 5.6587 1 1 1 1 1 0 0 5.7907 5.7907 12.3879 0 PROCESSED 57527.2296412037 2016-05-19 05:30:41 54247 2007-05-27 00:00:00 54109.1053240741 2007-01-09 02:31:40 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000015 CALIBRATION 1 A SWG JAP 0 SWG HXD boresight check with Crab N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100015010/ Quick Look
72 Crab nebula 83.6105 22.3483 82.856361 22.315501 84.093042 -0.96164 184.26290563 -5.62323625 86.8596 53607.2790509259 2005-08-25 06:41:50 53607.5139583333 2005-08-25 12:20:06 100010030 8.1129 5 8.1129 8.1129 8.1129 8.1129 2 2 2 2 1 0 0 7.8359 7.8359 20.264 1 PROCESSED 57526.8876388889 2016-05-18 21:18:12 54247 2007-05-27 00:00:00 54118.9698958333 2007-01-18 23:16:39 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010030/ Quick Look
73 N132D 81.2794 -69.6524 81.381964 -69.694399 312.375338 -85.522525 280.31514531 -32.77566051 53.3291 53595.4703125 2005-08-13 11:17:15 53597.5313541667 2005-08-15 12:45:09 100002010 7.4066 80 7.4066 7.4066 7.4066 7.4066 2 2 2 2 0 0 0 0 0 0 0 PROCESSED 57520.7109606482 2016-05-12 17:03:47 54247 2007-05-27 00:00:00 54038.5875925926 2006-10-30 14:06:08 3.0.22.43 6 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000002 HXD HV ON WITH N132D, and 5 pointings with XIS CALIBRATION 1 A SWG JAP 0 SWG HXD HV ON WITH N132D N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100002010/ Quick Look
74 TYCHO SNR HXD BKGD 9.2173 64.3076 8.488109 64.032592 44.61366 53.051862 121.35322514 1.48051733 84.2005 53915.6541782407 2006-06-29 15:42:01 53916.7606944444 2006-06-30 18:15:24 500025010 51.0088 50 51.0088 51.0088 51.0088 51.0088 2 2 2 2 1 0 0 48.7224 48.7224 95.5939 2 PROCESSED 57534.8010300926 2016-05-26 19:13:29 54302 2007-07-21 00:00:00 54052.5940509259 2006-11-13 14:15:26 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001099 We propose to observe Tycho's Supernova Remnant with Suzaku. The proposal has two main goals: (1) to measure the energy spectrum of the entire remnant above 10 keV with the HXD, and (2) to study the 0.5-10 keV band spectrum as a function of position with the XIS. GALACTIC DIFFUSE EMISSION 5 A JOHN HUGHES JAP 0 SWG SUZAKU STUDY OF TYCHO'S SUPERNOVA REMNANT HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500025010/ Quick Look
75 Crab nebula 83.6222 22.1365 82.869251 22.10376 84.094492 -1.173718 184.44846107 -5.72755512 86.8666 53608.2089236111 2005-08-26 05:00:51 53608.316087963 2005-08-26 07:35:10 100010080 3.382 5 3.382 3.382 3.382 3.382 1 1 1 1 1 0 0 3.7003 3.7003 9.2539 0 PROCESSED 57526.9140856482 2016-05-18 21:56:17 54247 2007-05-27 00:00:00 54119.0056134259 2007-01-19 00:08:05 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000010 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Offset 1 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100010080/ Quick Look
76 BULGE 2 270.6176 -29.5847 269.818763 -29.585758 270.530563 -6.144879 1.30042786 -3.49803376 83.2679 53801.7493981482 2006-03-07 17:59:08 53802.0689699074 2006-03-08 01:39:19 500002010 13.028 10 13.052 13.044 13.036 13.028 1 1 1 1 1 0 0 10.6741 10.6741 27.5999 1 PROCESSED 57533.1394444444 2016-05-25 03:20:48 54247 2007-05-27 00:00:00 54041.664525463 2006-11-02 15:56:55 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001014 Leading . GALACTIC DIFFUSE EMISSION 5 A DAN MCCAMMON JAP 0 SWG THE SOFT GALACTIC BULGE XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500002010/ Quick Look
77 CYGNUS LOOP 313.9037 31.9696 313.388205 31.777464 329.228113 46.799115 75.63250703 -8.50670526 64.2245 53884.8380671296 2006-05-29 20:06:49 53885.0891666667 2006-05-30 02:08:24 100049040 11.7656 10 11.7816 11.7816 11.7736 11.7656 1 1 1 1 1 0 0 9.788 9.788 21.6879 0 PROCESSED 57534.4771296296 2016-05-26 11:27:04 54258 2007-06-07 00:00:00 54052.5201157407 2006-11-13 12:28:58 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 015007 Here is the list of the calibration sources in the AO-1 round: 1) E0102.2-7219 20ks x 2 2) PKS2155-304 30ks (simultaneous observation with CXO and XMM) 3) Galactic Center Plasma 50ks 4) Cygnus Loop 40ks (=10ks x 4), and 5) RXJ1856.5-3754 40ks CALIBRATION 1 A HIRONORI MATSUMOTO JAP 1 SWG XIS FLIGHT CALIBRATION PLAN SPE N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100049040/ Quick Look
78 A3376 WEST RELIC 90.0363 -39.9917 89.629297 -39.992531 90.071049 -63.433501 246.43145562 -26.38385089 126.3601 54034.3950231482 2006-10-26 09:28:50 54035.9176388889 2006-10-27 22:01:24 800011020 62.2648 60 62.2648 62.2648 62.2648 62.2648 2 2 2 2 1 0 0 55.5629 55.5629 131.5378 2 PROCESSED 57535.9705902778 2016-05-27 23:17:39 54694 2008-08-16 00:00:00 54090.2671643518 2006-12-21 06:24:43 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001039 We propose a 150 ks observation of the giant radio relic in the west of the A3376 cluster. A3376 is a low temperature (4.5 keV) cluster with possible excess hard X-ray emission in 2.7 sigma significance by Beppo-SAX, and also with a pair of giant radio relics. This target is best suited for cluster hard excess survey with HXD. Following the first observation planned around October 2005 located near the east relic, the observation of the west relic 23 arcmin away can bring us the first spacial information on cluster excess hard X-rays. EXTRAGALACTIC DIFFUSE SOURCES 8 A KAZUHIRO NAKAZAWA JAP 0 SWG SEARCH FOR EXCESS HARD X-RAY EMISSION FROM ABELL 3376 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800011020/ Quick Look
79 GRB060105 297.6095 46.3384 297.227077 46.210211 319.460988 65.110067 80.2506255 9.98748628 191.1906 53740.5089351852 2006-01-05 12:12:52 53741.5002083333 2006-01-06 12:00:18 900001010 42.2208 40 42.2208 42.2208 42.2208 42.2208 2 2 2 2 1 0 0 37.718 37.718 85.6419 2 PROCESSED 57532.6415856482 2016-05-24 15:23:53 54247 2007-05-27 00:00:00 54039.776712963 2006-10-31 18:38:28 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001008 (i) Early break in lightcurve of X-ray afterglows using HXD. Recent Swift/XRT observations reveal that early X-ray afterglows of GRB has flat portion with very shallow decay. It may suggest continuous energy input from the central engine. The transition from its phase to general afterglow may display hard-to-soft evolution reflecting the cooling frequency. Thus multi wavelength observation will provide a key to the physics of central engine activity. (ii) Emission lines in the afterglows. The confirmation of line existence should be a matter of great importance because there remains unanswered questions. Some data may indicate a prominent iron line but others seem to suggest significant lower energy lines instead without iron lines. EXTRAGALACTIC COMPACT SOURCES 9 A TOSHIO MURAKAMI JAP 0 SWG-TOO TOO OBSERVATIONS OF GAMMA-RAY BURSTS HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/900001010/ Quick Look
80 A2218_offset 244.4769 65.4468 244.387309 65.566901 174.329918 79.629039 97.72059475 40.11912915 237.1965 53645.3474537037 2005-10-02 08:20:20 53646.32375 2005-10-03 07:46:12 100030020 44.8592 50 44.8592 46.1907 44.9141 45.3747 2 2 2 2 1 0 0 42.5366 42.5366 84.3439 0 PROCESSED 57527.5203125 2016-05-19 12:29:15 54247 2007-05-27 00:00:00 54036.969224537 2006-10-28 23:15:41 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000030 Search of redshifted (z=0.171) OVII emission line from warm-hot intergalactic matter around a cluster which shows a merger feature in the line of sight, with no central cool component. The depth of the structure can be ~20 Mpc, and the redshift allows a clear separation of the lines from the Galactic hot gas. The low background and the superior resolution of XIS in the soft X-ray energy range will allow the best measurement of the WHIM emission so far. CALIBRATION 1 A SWG JAP 0 SWG A2218 and its offset observation N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100030020/ Quick Look
81 ABELL 1795 Far North 207.223 26.9995 206.646903 27.247656 193.71055 35.352954 35.63943573 77.21561208 130.4264 53715.3208796296 2005-12-11 07:42:04 53715.9730092593 2005-12-11 23:21:08 800012030 30.6406 30 30.6486 30.6406 30.6639 30.6566 2 2 2 2 1 0 0 27.8833 27.8833 56.3379 1 PROCESSED 57532.4195833333 2016-05-24 10:04:12 54247 2007-05-27 00:00:00 54039.1003703704 2006-10-31 02:24:32 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001056 We propose a 120 ks Suzaku observation of Abell 1795. Five overlapping XIS pointings will: i) map the temperature to the virial radius for the first time; ii) check for the presence of soft excess emission and, if found, possibly determine whether the excess is associated with the cluster or our Galaxy; and iii) determine the run of abundance with radius in detail at r< 500. This observation will demonstrate the scientific value of the low-background and good spectral resolution of the Suzaku XIS in cluster studies. EXTRAGALACTIC DIFFUSE SOURCES 8 A MARK BAUTZ JAP 0 SWG TEMPERATURE, MASS AND SOFT-EXCESS MAPS TO THE VIRIAL RADIUS IN ABELL 1795 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800012030/ Quick Look
82 SN 1006 SW-Rim 225.4961 -42.0706 224.678007 -41.87399 235.320846 -23.835662 327.36052248 14.52564865 117.2713 53761.0914930556 2006-01-26 02:11:45 53761.7155555556 2006-01-26 17:10:24 100019050 28.4186 50 28.4186 28.4186 28.4186 28.4186 2 2 2 2 1 0 0 24.7444 24.7444 53.91 0 PROCESSED 57532.7834375 2016-05-24 18:48:09 54247 2007-05-27 00:00:00 54040.4586689815 2006-11-01 11:00:29 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000019 CALIBRATION 1 A SWG JAP 0 SWG SN1006 observation with XIS and HXD XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019050/ Quick Look
83 BULGE 3 274.7046 -31.4846 273.893726 -31.505472 274.041648 -8.109784 1.3002625 -7.49777303 80.4025 53800.3437962963 2006-03-06 08:15:04 53801.7474421296 2006-03-07 17:56:19 500001010 51.8468 50 51.8548 51.8548 51.8548 51.8468 2 2 2 2 1 0 0 45.0783 45.0783 121.2459 0 PROCESSED 57533.1540972222 2016-05-25 03:41:54 54247 2007-05-27 00:00:00 54041.7128703704 2006-11-02 17:06:32 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001014 Leading . GALACTIC DIFFUSE EMISSION 5 A DAN MCCAMMON JAP 0 SWG THE SOFT GALACTIC BULGE XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500001010/ Quick Look
84 SN1006 NW 225.6364 -41.8003 224.819551 -41.604176 235.339658 -23.546444 327.59294648 14.70833496 115.0008 53766.4881365741 2006-01-31 11:42:55 53767.55375 2006-02-01 13:17:24 500017010 53.0194 50 53.0194 53.0277 53.0273 53.0273 2 2 2 2 1 0 0 60.4123 60.4123 92.0679 0 PROCESSED 57532.8347685185 2016-05-24 20:02:04 54247 2007-05-27 00:00:00 54040.7669675926 2006-11-01 18:24:26 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001062 We propose two Suzaku pointings of the Galactic supernova remnant (SNR) that exploded as a supernova in 1006. The main goal of the project is to use the XIS measure the abundances of low-Z elements in the ejecta. GALACTIC DIFFUSE EMISSION 5 A JOHN HUGHES JAP 0 SWG THE EJECTA IN SN1006 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500017010/ Quick Look
85 A 2218 OFFSETB 249.9091 65.2119 249.835523 65.307656 180.044789 81.713752 96.37864193 38.09205953 233.3309 53670.1916319444 2005-10-27 04:35:57 53670.4620833333 2005-10-27 11:05:24 800020010 14.9215 15 14.9375 14.9335 14.9215 14.9415 2 2 2 2 1 0 0 14.1931 14.1931 23.3561 0 PROCESSED 57527.6596180556 2016-05-19 15:49:51 54247 2007-05-27 00:00:00 54036.8343981482 2006-10-28 20:01:32 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001096 To confirm the presence of redshifted oxygen lines from the WHIM surrounding A2218, we propose observations of 2 positions. One is a 35 ksec pointing on A2218 to raise the photon statistics of the oxygen feature, and the other is a 15 ksec pointing at about 1 degree west of the cluster to know the amplitude of the intensity variation of the Galactic oxygen lines. EXTRAGALACTIC DIFFUSE SOURCES 8 A TAKAYA OHASHI JAP 0 SWG SEARCH FOR OXYGEN LINES FROM WARM IGM N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800020010/ Quick Look
86 CAS A 350.8729 58.8094 350.30695 58.534812 27.388607 54.842749 111.74406014 -2.13880346 214.7372 53768.5363657407 2006-02-02 12:52:22 53768.833599537 2006-02-02 20:00:23 100043010 0 10 0 0 0 0 0 0 0 0 1 0 0 10.3268 10.3268 25.6739 1 PROCESSED 57532.8451736111 2016-05-24 20:17:03 54247 2007-05-27 00:00:00 54040.7488888889 2006-11-01 17:58:24 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001097 We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip CALIBRATION 1 A HIRONORI MATSUMOTO JAP 0 SWG XIS FLIGHT CAIBRATION PLAN XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100043010/ Quick Look
87 A 2218 CENTER 249.0052 66.205 248.955095 66.304813 172.75657 81.615548 97.72589248 38.11630228 233.3294 53669.4904050926 2005-10-26 11:46:11 53670.1905555556 2005-10-27 04:34:24 800019010 31.9354 35 31.9434 31.9434 31.9354 31.9434 2 2 2 2 1 0 0 28.9371 28.9371 60.4879 1 PROCESSED 57527.6471990741 2016-05-19 15:31:58 54247 2007-05-27 00:00:00 54036.9596990741 2006-10-28 23:01:58 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001096 To confirm the presence of redshifted oxygen lines from the WHIM surrounding A2218, we propose observations of 2 positions. One is a 35 ksec pointing on A2218 to raise the photon statistics of the oxygen feature, and the other is a 15 ksec pointing at about 1 degree west of the cluster to know the amplitude of the intensity variation of the Galactic oxygen lines. EXTRAGALACTIC DIFFUSE SOURCES 8 A TAKAYA OHASHI JAP 0 SWG SEARCH FOR OXYGEN LINES FROM WARM IGM N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800019010/ Quick Look
88 A 2052 229.0471 6.9211 228.432118 7.104686 224.516271 24.128025 9.16646689 50.17566284 281.2031 53603.6121875 2005-08-21 14:41:33 53603.9938425926 2005-08-21 23:51:08 100006040 16.7443 20 16.7443 16.7443 16.7443 16.7443 1 1 1 1 1 0 0 12.8395 12.8395 32.9519 0 PROCESSED 57520.7325810185 2016-05-12 17:34:55 53705 2005-12-01 00:00:00 53905.4634143518 2006-06-19 11:07:19 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000006 CALIBRATION 1 A SWG JAP 0 SWG Outer region of A 2052 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100006040/ Quick Look
89 Crab Nebula 83.5484 22.0881 82.795741 22.055005 84.024019 -1.219032 184.45272098 -5.81121698 85.0004 53614.9103009259 2005-09-01 21:50:50 53615.0418518518 2005-09-02 01:00:16 100015050 5.3447 5 5.3447 5.3447 5.3447 5.3447 1 1 1 1 1 0 0 5.4859 5.4859 11.356 0 PROCESSED 57527.2511342593 2016-05-19 06:01:38 54247 2007-05-27 00:00:00 54109.1357986111 2007-01-09 03:15:33 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000015 CALIBRATION 1 A SWG JAP 0 SWG HXD boresight check with Crab N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100015050/ Quick Look
90 NGC 2992 146.4207 -14.2696 145.81924 -14.038457 154.003817 -26.061971 249.65504756 28.81616071 88.7924 53693.8781597222 2005-11-19 21:04:33 53694.9759722222 2005-11-20 23:25:24 700005020 37.4935 120 37.6565 39.6915 37.4935 37.8205 1 1 1 1 1 0 0 33.8991 33.8991 94.8479 1 PROCESSED 57528.0334490741 2016-05-20 00:48:10 54247 2007-05-27 00:00:00 54037.7316087963 2006-10-29 17:33:31 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001013 NGC 2992 is a nearby Seyfert 1.9 galaxy showing long-term (20 yrs) large amplitude (factor of 20) variability. This object showed switching between Compton-thick and -thin. Recent RXTE monitoring has shown that this object is highly variable on shorter time scales (2 weeks). We propose three Suzaku observations to monitor the variability of absorption column, broad band continuum shape, and Fe line intensity to understand the cause of the remarkable variability. EXTRAGALACTIC COMPACT SOURCES 7 A YUICHI TERASHIMA JAP 0 SWG THE SPECTRAL VARIABILITY IN NGC 2992: FE-LINE, REFLECTION, AND COMPTON-THIN/THICK SWITCHING HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700005020/ Quick Look
91 Cas A 350.8254 58.8156 350.259841 58.54105 27.364711 54.864063 111.72292809 -2.12474901 12.9937 53614.2486458333 2005-09-01 05:58:03 53614.7640509259 2005-09-01 18:20:14 100016010 27.965 20 27.973 27.973 27.973 27.965 2 2 2 2 1 0 0 24.13 24.13 44.4959 2 PROCESSED 57527.2832175926 2016-05-19 06:47:50 53705 2005-12-01 00:00:00 53905.4659606482 2006-06-19 11:10:59 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000016 CALIBRATION 1 A SWG JAP 0 SWG Cas A N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100016010/ Quick Look
92 NEP 272.7884 65.9814 272.771336 65.967881 333.879188 88.742697 95.75202722 28.67554678 290.9299 53615.6136921296 2005-09-02 14:43:43 53617.625162037 2005-09-04 15:00:14 100018010 106.2015 100 106.2015 106.2175 106.2495 106.2255 2 2 2 2 1 0 0 106.125 106.125 173.5718 3 PROCESSED 57527.2880092593 2016-05-19 06:54:44 53705 2005-12-01 00:00:00 53905.4636921296 2006-06-19 11:07:43 3.0.22.43 6 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000018 CALIBRATION 1 A SWG JAP 0 SWG HXD background at North Ecliptic Pole N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100018010/ Quick Look
93 A3376 WEST RELIC 90.0415 -39.9946 89.634521 -39.995405 90.079962 -63.436398 246.43569548 -26.38071178 132.0018 53681.5938078704 2005-11-07 14:15:05 53684.7883912037 2005-11-10 18:55:17 800011010 126.9969 150 126.9969 127.1809 127.0769 127.0289 2 2 2 2 1 0 0 112.9113 112.9113 230.9397 3 PROCESSED 57528.0013541667 2016-05-20 00:01:57 54247 2007-05-27 00:00:00 54037.6050231482 2006-10-29 14:31:14 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001039 We propose a 150 ks observation of the giant radio relic in the west of the A3376 cluster. A3376 is a low temperature (4.5 keV) cluster with possible excess hard X-ray emission in 2.7 sigma significance by Beppo-SAX, and also with a pair of giant radio relics. This target is best suited for cluster hard excess survey with HXD. Following the first observation planned around October 2005 located near the east relic, the observation of the west relic 23 arcmin away can bring us the first spacial information on cluster excess hard X-rays. EXTRAGALACTIC DIFFUSE SOURCES 8 A KAZUHIRO NAKAZAWA JAP 0 SWG SEARCH FOR EXCESS HARD X-RAY EMISSION FROM ABELL 3376 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/800011010/ Quick Look
94 Crab Nebula 83.6274 22.0192 82.875108 21.986487 84.094124 -1.29112 184.55062413 -5.78629385 86.8663 53604.1571412037 2005-08-22 03:46:17 53604.2501273148 2005-08-22 06:00:11 100007010 1.7229 5 1.7229 1.7229 1.7229 1.7229 1 1 1 1 1 0 0 1.808 1.808 8.034 0 PROCESSED 57520.7330324074 2016-05-12 17:35:34 54247 2007-05-27 00:00:00 54105.2758912037 2007-01-05 06:37:17 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000007 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Nebula N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100007010/ Quick Look
95 Crab nebula 83.6201 22.1854 82.866876 22.152649 84.094711 -1.124779 184.40591259 -5.70300776 86.8631 53604.2507175926 2005-08-22 06:01:02 53604.3889351852 2005-08-22 09:20:04 100007020 3.0531 5 3.0571 3.0531 3.0531 3.0531 1 1 1 1 1 0 0 3.1343 3.1343 11.94 1 PROCESSED 57520.7416782407 2016-05-12 17:48:01 54247 2007-05-27 00:00:00 54105.2987268518 2007-01-05 07:10:10 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000007 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Nebula N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100007020/ Quick Look
96 Crab nebula 83.4512 22.0082 82.699013 21.974637 83.930395 -1.294795 184.47195778 -5.93010486 86.7989 53604.489849537 2005-08-22 11:45:23 53604.5835416667 2005-08-22 14:00:18 100007040 4.2682 5 4.2682 4.2682 4.2682 4.2682 1 1 1 1 1 0 0 4.1392 4.1392 8.056 0 PROCESSED 57520.7454513889 2016-05-12 17:53:27 54247 2007-05-27 00:00:00 54105.3073726852 2007-01-05 07:22:37 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000007 Crab nebula multi pointings CALIBRATION 1 A SWG JAP 0 SWG Crab Nebula N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100007040/ Quick Look
97 NGC 4945 196.3733 -49.4666 195.643253 -49.198924 217.025297 -38.636782 305.27803835 13.34111135 313.9078 53605.101087963 2005-08-23 02:25:34 53605.1034490741 2005-08-23 02:28:58 100008020 0.1776 10 0.1815 0.1815 0.1796 0.1776 1 1 1 1 1 0 0 0.2001 0.2001 0.202 0 PROCESSED 57526.8486574074 2016-05-18 20:22:04 54247 2007-05-27 00:00:00 54034.6891435185 2006-10-26 16:32:22 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000008 CALIBRATION 1 A SWG JAP 0 SWG NGC 4945 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100008020/ Quick Look
98 CYG X-1 299.5907 35.1892 299.120596 35.052727 313.656273 54.237702 71.32454904 3.06010347 276.9898 53648.2025347222 2005-10-05 04:51:39 53648.6335532407 2005-10-05 15:12:19 100036010 18.213 20 18.213 18.213 18.213 18.213 1 1 1 1 1 0 0 18.1457 18.1457 37.2299 0 PROCESSED 57527.5598726852 2016-05-19 13:26:13 54247 2007-05-27 00:00:00 54037.7278819444 2006-10-29 17:28:09 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000036 We propose to probe the geometry of optically-thick accretion disks which should exist around a BH even in the hard state and to verify the HXD performance to thermal cut-off in hard X-rays expected from AGN. The 1st may be done by measuring the cool disk emission with the XIS-BI, resolving the fluorescent Fe-K line with the XIS-FI and detecting the reflection continuum with the HXD. Since these features are thought to come from the optically-thick disk a simultaneous measurement will for the 1st time allow for self-consistent constraining of the disk geometry in the hard state. Cyg X-1 is the best & most secure object for this stufy and is now in the low/hard state. A 20 ks Suzaku obs. is sufficient to get a fine spectrum up to 300 keV & to determine the cutoff with a high significance. CALIBRATION 1 A SWG JAP 0 SWG Cyg X-1 in the low state N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100036010/ Quick Look
99 Sgr_B2 266.8775 -28.4435 266.086257 -28.426412 267.234561 -5.032377 0.63628385 -0.09835114 265.3727 53653.5194560185 2005-10-10 12:28:01 53655.2954050926 2005-10-12 07:05:23 100037060 76.5966 100 76.6286 76.6446 76.5966 76.6286 2 2 2 2 1 0 0 70.8192 70.8192 153.4319 0 PROCESSED 57527.5776041667 2016-05-19 13:51:45 54247 2007-05-27 00:00:00 54036.2262731482 2006-10-28 05:25:50 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000037 CALIBRATION 1 A SWG JAP 0 SWG Suzaku Obseration of Galactic Center region 2 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100037060/ Quick Look
100 Sgr_B2_BGD 267.0943 -28.1356 266.304946 -28.119568 267.419629 -4.720546 0.99854005 -0.10262599 269.0208 53655.2988888889 2005-10-12 07:10:24 53655.4620833333 2005-10-12 11:05:24 100037070 9.1612 10 9.1612 9.1643 9.1643 9.1632 2 2 2 2 1 0 0 9.5364 9.5364 14.092 0 PROCESSED 57527.5688078704 2016-05-19 13:39:05 54247 2007-05-27 00:00:00 54036.0749884259 2006-10-28 01:47:59 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000037 CALIBRATION 1 A SWG JAP 0 SWG Suzaku Obseration of Galactic Center region 2 N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100037070/ Quick Look
101 MKN 3 93.8839 71.0477 92.433649 71.063052 91.875357 47.63268 143.2836301 22.71631463 71.8326 53665.0848263889 2005-10-22 02:02:09 53667.2682175926 2005-10-24 06:26:14 100040010 95.0265 100 95.0265 95.0772 95.0452 95.0345 2 2 2 2 1 0 0 91.3441 91.3441 188.6299 0 PROCESSED 57527.6643055556 2016-05-19 15:56:36 54247 2007-05-27 00:00:00 53906.4896759259 2006-06-20 11:45:08 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000040 Mkn 3 is the second brightest Compton-thick Sy 2 currently visible with Suzaku. The broadband spectrum of Mkn 3, as probed by previous SAX and Chandra observations, is dominated by a reflection component (Compton hump strength R is near 1), but there is also evidence for a strongly absorbed hard X-ray power law that may be direct emission from the obscured nucleus, filtering through Compton-thick material (such as the molecular torus). CALIBRATION 1 A SWG JAP 0 SWG MKN 3 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100040010/ Quick Look
102 RXJ1856.5-3754 284.1498 -37.9103 283.298136 -37.976359 281.509901 -15.033652 358.59888263 -17.21635309 269.4259 53667.2829976852 2005-10-24 06:47:31 53669.4793287037 2005-10-26 11:30:14 100041010 76.2548 80 0 76.2548 0 0 0 2 0 0 1 0 0 62.6217 62.6217 189.72 3 PROCESSED 57527.6811111111 2016-05-19 16:20:48 54247 2007-05-27 00:00:00 54037.2294791667 2006-10-29 05:30:27 3.0.22.43 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000041 We propose Suzaku observation of a nearby isolated neuron star RXJ1856.5-3754 for the low energy QE calibration of the XIS. Our main purpose is, however, using this source as a soft X-ray QE calibrator on the sky. We hope this source will be observed again in future to check possible contamination on the filter surface etc. Note that the calibration is not only for the BI-CCD(XIS1), but also for FI-CCDs or relative QE among them. CALIBRATION 1 A SWG JAP 0 SWG LOW ENERGY QE CALIBRATION OF XIS XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100041010/ Quick Look
103 E0102-72 16.027 -72.0223 15.622199 -72.290248 314.64413 -65.039289 301.54815221 -45.07189388 294.0751 53768.8467592593 2006-02-02 20:19:20 53769.4065393518 2006-02-03 09:45:25 100044030 20.8277 20 20.8357 20.8437 20.8437 20.8277 2 2 2 2 1 0 0 20.2688 20.2688 48.36 1 PROCESSED 57532.8615740741 2016-05-24 20:40:40 54247 2007-05-27 00:00:00 53905.6764351852 2006-06-19 16:14:04 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001097 We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip CALIBRATION 1 A HIRONORI MATSUMOTO JAP 0 SWG XIS FLIGHT CAIBRATION PLAN XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100044030/ Quick Look
104 ETA CARINAE 161.248 -59.6859 160.761598 -59.422588 202.142 -58.929196 287.58997588 -0.63475906 156.124 53769.4163194444 2006-02-03 09:59:30 53769.9481944444 2006-02-03 22:45:24 100045010 21.3678 20 21.3678 21.3678 21.3678 21.3678 2 2 2 2 1 0 0 18.1458 18.1458 45.9459 1 PROCESSED 57532.9369907407 2016-05-24 22:29:16 54247 2007-05-27 00:00:00 54040.9846643518 2006-11-01 23:37:55 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001097 We propose the calibration observations for XIS: E0102-72 ... Gain and QE in the low energy band Cas A ... Gain and QE in the high energy band Eta Carinae ... Contamination of the BI chip CALIBRATION 1 A HIRONORI MATSUMOTO JAP 0 SWG XIS FLIGHT CAIBRATION PLAN XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100045010/ Quick Look
105 BULGE 6 282.6839 -33.8925 281.860158 -33.951684 280.687841 -10.9215 1.99857856 -14.59644221 88.3467 53802.7373032407 2006-03-08 17:41:43 53803.0466087963 2006-03-09 01:07:07 500003010 14.2617 10 14.2617 14.2617 14.2617 14.2617 2 2 2 2 1 0 0 11.414 11.414 26.7159 1 PROCESSED 57533.1570833333 2016-05-25 03:46:12 54247 2007-05-27 00:00:00 54041.7424305556 2006-11-02 17:49:06 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001014 Leading . GALACTIC DIFFUSE EMISSION 5 A DAN MCCAMMON JAP 0 SWG THE SOFT GALACTIC BULGE XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500003010/ Quick Look
106 X1630-472 248.4772 -47.3405 247.556757 -47.236251 254.058584 -25.081993 336.93627828 0.30053306 75.5959 53794.9708333333 2006-02-28 23:18:00 53795.6968055556 2006-03-01 16:43:24 400010030 21.5216 200 21.5216 21.5216 21.5216 21.5216 2 2 2 2 1 0 0 19.0328 19.0328 62.718 0 PROCESSED 57533.1079050926 2016-05-25 02:35:23 54247 2007-05-27 00:00:00 54041.5956018518 2006-11-02 14:17:40 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001058 We propose to monitor a transient black hole binary in outburst through a series of 20 ks observations. Our goal is to map the physical conditions in the accretion disk as the source evolves through the various continuum states using the spectral diagnostics available in the Fe K fluorescence emission. Measurements of the Fe K emission will allow us to quantify the thermal, kinematic, and geometric conditions in both the disk and the surrounding material. Correlating the Fe K diagnostics with sensitive measurements of the direct and reprocessed continuum emission will allow us to map the evolving conditions and constrain models of the dynamic accretion processes in black hole binaries. We will monitor 7 targets with the RXTE. This observation will be triggered when one becomes active. GALACTIC POINT SOURCES 4 A JEAN COTTAM JAP 0 SWG-TOO FE K SPECTROSCOPY OF TRANSIENT BLACK HOLE BINARIES HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400010030/ Quick Look
107 LOCKMANHOLE 163.4063 57.6108 162.636897 57.876997 137.149157 45.549363 148.98193179 53.14624927 119.611 53688.2372337963 2005-11-14 05:41:37 53689.8300694444 2005-11-15 19:55:18 100046010 76.9806 100 76.9806 77.0446 77.0126 77.0206 2 2 2 2 1 0 0 94.5107 94.5107 137.6079 3 PROCESSED 57528.0048148148 2016-05-20 00:06:56 54247 2007-05-27 00:00:00 54037.5889814815 2006-10-29 14:08:08 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001098 We propose a 100 ks observation of LockmanHole with Suzaku. The main purpose is to obtain a template dataset of HXD background. CALIBRATION 1 A MOTOHIDE KOKUBUN JAP 0 SWG BACKGROUND ESTABLISHMENT OF HXD XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100046010/ Quick Look
108 AE AQUARII 310.0612 -0.931 309.416636 -1.108991 312.236832 16.82972 45.23545862 -24.46836188 250.6241 54033.2319907407 2006-10-25 05:34:04 54034.3829282407 2006-10-26 09:11:25 400001020 47.9743 50 47.9743 48.5956 48.1316 48.3103 2 2 2 2 1 0 0 45.5384 45.5384 99.4239 1 PROCESSED 57526.8238773148 2016-05-18 19:46:23 54526 2008-03-01 00:00:00 54109.7083449074 2007-01-09 17:00:01 3.0.22.43 9 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001004 We have a new idea that a magnetized white dwarf can be a particle-acceleration cite to emit non thermal emission. In order to understand the particle acceleration process in rotation-powered objects, it is important to measure the hard X-ray emission from magnetized white dwarfs, in addition to that from well-known neutron stars. Here, we propose a 100ksec observation of a magnetic cataclysmic valiable, AE Aqurii. It is difficult for INTEGRAL mission, and is challenging even for the HXD, but it will be a ``first detection'' of the non-thermal emission in the hard X-ray band from a white dwarf with Suzaku. GALACTIC POINT SOURCES 4 A YUKIKATSU TERADA JAP 0 SWG SEARCH FOR THE NON-THERMAL EMISSION FROM MAGNETIZED WHITE DWARF WITH SUZAKU HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400001020/ Quick Look
109 GX 349+2 256.4194 -36.3657 255.579957 -36.298328 258.779942 -13.451385 349.14166441 2.79326977 78.9359 53813.9267708333 2006-03-19 22:14:33 53814.6043402778 2006-03-20 14:30:15 400003020 28.1177 50 28.1177 28.1317 28.1204 28.1204 2 2 2 2 1 0 0 25.6573 25.6573 58.538 0 PROCESSED 57533.2767939815 2016-05-25 06:38:35 54247 2007-05-27 00:00:00 54042.1657407407 2006-11-03 03:58:40 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001026 We propose Suzaku observations of two luminous low-mass X-ray binaries (Z sources), GX 349+2 and Cyg X-2, to investigate the origin of the hard tails of Z sources, of which the spectral photon indices are reported to become occasionally less than unity. With the high sensitivity of the HXD, we detect the spectral shape up to several 100 keV and reveal existence of particle acceleration caused by high radiation pressure. GALACTIC POINT SOURCES 4 A HIROMITSU TAKAHASHI JAP 0 SWG SUZAKU OBSERVATIONS OF THE HARD TAILS OF LUMINOUS LOW-MASS X-RAY BINARIES (Z SOURCES) HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400003020/ Quick Look
110 SN1006 NE BG 226.7036 -41.3998 225.886024 -41.207391 236.037501 -22.925171 328.51405135 14.65073262 293.6503 53617.7018865741 2005-09-04 16:50:43 53622.1668287037 2005-09-09 04:00:14 100019010 44.7503 50 44.7543 44.7543 44.7543 44.7503 2 2 2 2 1 0 0 37.3883 37.3883 385.6018 5 PROCESSED 57527.2923148148 2016-05-19 07:00:56 54247 2007-05-27 00:00:00 54035.4224768518 2006-10-27 10:08:22 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 000019 CALIBRATION 1 A SWG JAP 0 SWG SN1006 observation with XIS and HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100019010/ Quick Look
111 X1630-472 248.4828 -47.3401 247.56235 -47.235876 254.062648 -25.080987 336.93914719 0.29801709 78.3341 53774.6318981482 2006-02-08 15:09:56 53775.1390972222 2006-02-09 03:20:18 400010010 22.1902 200 22.1902 22.1902 22.1902 22.1902 1 1 1 1 1 0 0 22.247 22.247 43.816 0 PROCESSED 57532.9380787037 2016-05-24 22:30:50 54247 2007-05-27 00:00:00 54040.9540856482 2006-11-01 22:53:53 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001058 We propose to monitor a transient black hole binary in outburst through a series of 20 ks observations. Our goal is to map the physical conditions in the accretion disk as the source evolves through the various continuum states using the spectral diagnostics available in the Fe K fluorescence emission. Measurements of the Fe K emission will allow us to quantify the thermal, kinematic, and geometric conditions in both the disk and the surrounding material. Correlating the Fe K diagnostics with sensitive measurements of the direct and reprocessed continuum emission will allow us to map the evolving conditions and constrain models of the dynamic accretion processes in black hole binaries. We will monitor 7 targets with the RXTE. This observation will be triggered when one becomes active. GALACTIC POINT SOURCES 4 A JEAN COTTAM JAP 0 SWG-TOO FE K SPECTROSCOPY OF TRANSIENT BLACK HOLE BINARIES HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/400010010/ Quick Look
112 73P/SW3 279.6627 33.4734 279.203358 33.427762 284.650097 56.423756 62.35168426 17.03145652 46.5564 53862.4804282407 2006-05-07 11:31:49 53862.5419444444 2006-05-07 13:00:24 500012020 3.248 5 3.248 3.248 3.248 3.248 1 1 1 1 1 0 0 2.1119 2.1119 5.2799 0 PROCESSED 57533.7332407407 2016-05-25 17:35:52 54256 2007-06-05 00:00:00 54042.2282175926 2006-11-03 05:28:38 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001050 Cometary X-ray emission is likely the result of charge exchange interactions between the highly charged solar wind and neutral material ablated from the nucleus. Recent measurements using Chandra coupled with precise laboratory measurements at EBIT lend support for this hypothesis. In fact we have successfully deconvolved the Chandra/ACIS observation of comet C/Linear using direct observations of charge exchanging plasmas at EBIT using a flight spare XRS detector system. Here, we propose to observe a magnitude 1 comet, 73P/SW 3, the brightest comet of the decade during May 2006 within only 0.08 AU of the earth using the XIS1 (BI) instrument on Suzaku. The exceptional low energy response of the XIS will allow us to unambiguously identify the x-ray emission mechanism in comets. GALACTIC DIFFUSE EMISSION 5 A FREDERICK PORTER JAP 0 SWG AN XIS OBSERVATION OF THE BRIGHTEST COMET OF THE DECADE: 73P/SCHWASSMANN-WACHMANN 3 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500012020/ Quick Look
113 73P/SW3 316.717 24.6807 316.164001 24.478965 328.484877 39.12074 71.53645371 -15.07849931 72.7087 53868.1752314815 2006-05-13 04:12:20 53868.2085532407 2006-05-13 05:00:19 500013010 2.353 20 2.353 2.353 2.353 2.353 1 1 1 1 1 0 0 2.595 2.595 2.8719 0 PROCESSED 57534.2831597222 2016-05-26 06:47:45 54256 2007-06-05 00:00:00 54042.2312268518 2006-11-03 05:32:58 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 001050 Cometary X-ray emission is likely the result of charge exchange interactions between the highly charged solar wind and neutral material ablated from the nucleus. Recent measurements using Chandra coupled with precise laboratory measurements at EBIT lend support for this hypothesis. In fact we have successfully deconvolved the Chandra/ACIS observation of comet C/Linear using direct observations of charge exchanging plasmas at EBIT using a flight spare XRS detector system. Here, we propose to observe a magnitude 1 comet, 73P/SW 3, the brightest comet of the decade during May 2006 within only 0.08 AU of the earth using the XIS1 (BI) instrument on Suzaku. The exceptional low energy response of the XIS will allow us to unambiguously identify the x-ray emission mechanism in comets. GALACTIC DIFFUSE EMISSION