DARTS Astro

total 38

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 A1914_OFFSET4 216.4138 37.6152 215.900162 37.839927 196.47734 48.33006 66.75628519 67.60183749 330.9949 55365.2958333333 2010-06-18 07:06:00 55366.115462963 2010-06-19 02:46:16 805094010 27.2904 40 27.2904 27.3001 0 27.2944 2 2 0 2 1 0 0 25.4203 25.4203 70.816 0 PROCESSED 57552.407037037 2016-06-13 09:46:08 55769 2011-07-27 00:00:00 55403.4672106482 2010-07-26 11:12:47 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA ERIC MILLER JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805094010/ Quick Look
2 A1750S 202.5548 -2.1063 201.910476 -1.848597 201.643103 6.819901 322.18359807 59.30814244 293.521 55751.0328009259 2011-07-09 00:47:14 55753.0002314815 2011-07-11 00:00:20 806097010 80.1668 80 80.1668 80.1668 0 80.1668 2 2 0 2 1 0 0 67.0448 67.0448 169.9618 3 PROCESSED 57602.5725578704 2016-08-02 13:44:29 56148 2012-08-09 00:00:00 55778.4321412037 2011-08-05 10:22:17 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 063019 We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA SCOTT RANDALL JUS 6 AO6 SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806097010/ Quick Look
3 A1914_OFFSET1 216.5507 38.0175 216.039339 38.24183 196.32687 48.734523 67.63121502 67.35438204 324.9943 55362.5248148148 2010-06-15 12:35:44 55363.4724768518 2010-06-16 11:20:22 805091010 32.2034 40 32.2034 32.2034 0 32.2034 2 2 0 2 1 0 0 27.5086 27.5086 81.876 1 PROCESSED 57552.3572569445 2016-06-13 08:34:27 55766 2011-07-24 00:00:00 55399.2609722222 2010-07-22 06:15:48 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA ERIC MILLER JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805091010/ Quick Look
4 A262 E3 29.2513 35.7586 28.51426 35.514871 40.102333 22.236821 137.59731231 -25.23895106 250.0003 56701.0116319444 2014-02-13 00:16:45 56701.8717939815 2014-02-13 20:55:23 808114010 38.5681 40 38.5761 38.5681 0 38.5761 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57613.8129861111 2016-08-13 19:30:42 57080 2015-02-27 00:00:00 56714.7407986111 2014-02-26 17:46:45 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 083002 We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy. EXTRAGALACTIC DIFFUSE SOURCES 8 B KYOKO MATSUSHITA NORBERT WERNER JUS 8 AO8 OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808114010/ Quick Look
5 M106 184.7117 47.2376 184.094273 47.515109 160.404745 44.085185 138.43381178 68.89762168 287.1938 53896.5413078704 2006-06-10 12:59:29 53898.7113425926 2006-06-12 17:04:20 701095010 99.8175 100 99.8815 99.8175 99.8815 99.8815 2 2 2 2 1 0 0 97.5229 97.5229 187.4839 1 PROCESSED 57534.6515393518 2016-05-26 15:38:13 54401 2007-10-28 00:00:00 53927.2308449074 2006-07-11 05:32:25 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 013151 We propose observations of the nearby Low Luminosity AGN, M81 and M106, for 100 ks for each target. We aim to detect both targets up to ~200 keV for the first time. We will determine the photon indices of the hard X-ray power-law continuum, with searching for other possible characteristics such as Compton hump around 10-20 keV and cutoff around 100-200 keV which would lead major discoveries. We will study the shape of Fe-K line(s) around 6-7 keV and their time variances. Our goal is to compare their hard X-ray spectra with those of SWG seyfert galaxies, with unprecedented accuracy, to study the accresion mechanism of LLAGN. EXTRAGALACTIC COMPACT SOURCES 7 A TAKESHI ITOH CHRISTOPHER REYNOLDS JUS 1 AO1 OBSERVATIONS OF HARD X-RAYS FROM LOW LUMINOSITY ACTIVE GALACTIC NUCLEI HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701095010/ Quick Look
6 A1914_OFFSET1 216.5784 38.0421 216.067238 38.26635 196.337734 48.766613 67.66951456 67.3249966 134.001 55565.4188194445 2011-01-04 10:03:06 55565.728599537 2011-01-04 17:29:11 805091020 11.393 10 11.401 11.393 0 11.401 2 2 0 2 1 0 0 11.3763 11.3763 25.4979 0 PROCESSED 57600.5573263889 2016-07-31 13:22:33 55995 2012-03-09 00:00:00 55627.1165625 2011-03-07 02:47:51 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA RYO NAGINO JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805091020/ Quick Look
7 A1914_OFFSET3 216.2252 37.8719 215.712166 38.097165 196.093912 48.482824 67.5271644 67.6467927 330.9949 55364.3811805556 2010-06-17 09:08:54 55365.2953587963 2010-06-18 07:05:19 805093010 28.5066 40 28.5066 28.5066 0 28.5066 2 2 0 2 1 0 0 26.3813 26.3813 78.9679 1 PROCESSED 57552.3531018518 2016-06-13 08:28:28 55769 2011-07-27 00:00:00 55400.3084375 2010-07-23 07:24:09 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA ERIC MILLER JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805093010/ Quick Look
8 A262 E4 29.5568 35.6351 28.819272 35.392091 40.300853 22.029449 137.89892988 -25.28797491 250 56701.8723148148 2014-02-13 20:56:08 56702.5974652778 2014-02-14 14:20:21 808115010 31.9389 30 31.9469 31.9389 0 31.9549 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57613.8117361111 2016-08-13 19:28:54 57080 2015-02-27 00:00:00 56714.739525463 2014-02-26 17:44:55 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 083002 We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy. EXTRAGALACTIC DIFFUSE SOURCES 8 B KYOKO MATSUSHITA NORBERT WERNER JUS 8 AO8 OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808115010/ Quick Look
9 G156.2+5.7 CENTER 74.723 51.7342 73.743251 51.658579 79.264036 28.862327 156.21466687 5.62934315 273.4473 54148.7568171296 2007-02-17 18:09:49 54149.9169444444 2007-02-18 22:00:24 501106010 51.2142 50 51.2222 51.2302 0 51.2142 1 1 0 1 1 0 0 46.482 46.482 100.1999 0 PROCESSED 57537.3992824074 2016-05-29 09:34:58 54695 2008-08-17 00:00:00 54158.4264351852 2007-02-27 10:14:04 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 013079 Recent observations revealed that about 10 shell-like supernova remnants (SNRs) exhibit power-law X-ray spectra with no emission line which are considered to be synchrotron radiation from high-energy electrons (larger than 1 TeV). However, all those samples are young SNRs (ages about 300-2000 yr). G156.2+5.7 is an old SNR (age about 10^4 year), but emits hard X-rays in addition to usual thin thermal emission (about 0.5 keV temperature). We propose a Suzaku observation on a center region of this SNR, where diffuse hard X-rays were detected with ASCA and XMM. Our primary objective is to determine whether or not the hard tail is synchrotron X-rays, and study cosmic-ray acceleration in this old SNR. GALACTIC DIFFUSE EMISSION 5 B MASARU UENO ROBERT PETRE JUS 1 AO1 REVEALING THE ORIGIN OF HARD X-RAY EMISSION FROM AN OLD SNR, G156.2+5.7 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501106010/ Quick Look
10 KEPLER 262.6698 -21.4886 261.920525 -21.451271 263.169114 1.778808 4.51918955 6.82146946 98.2145 54514.1665393518 2008-02-18 03:59:49 54516.9793287037 2008-02-20 23:30:14 502078010 116.9636 100 116.9636 116.9636 0 116.9636 2 2 0 2 1 0 0 98.9551 98.9551 242.9956 3 PROCESSED 57541.7751388889 2016-06-02 18:36:12 54894 2009-03-04 00:00:00 54525.6176851852 2008-02-29 14:49:28 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 023074 We propose to observe the Kepler's SNR in which evidence of particle acceleration will be found. Aim of the observation is to determine power-law contribution in the hard-tail spectrum above 10 keV with HXD-PIN. If we also find the Fe-Kb and Ni-K emission lines with XIS which have not observed in any previous missions, temperature and nt parameter of a NEI model will be fixed. The determination will help to distinguish the power-law component from the thermal one. We also memtioned that the amount of Fe and Ni will be a good estimator to determine the type of Kepler's SNR. GALACTIC DIFFUSE EMISSION 5 B TORU TAMAGAWA Sangwook Park JUS 2 AO2 SEARCH FOR EVIDENCE OF COSMIC-RAY ACCELERATION IN THE KEPLER'S SNR XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502078010/ Quick Look
11 K3/PSR J1420-6048 215.0274 -60.7627 214.105774 -60.533369 236.492647 -43.553641 313.55205119 0.26755801 90.771 54842.5598263889 2009-01-11 13:26:09 54843.8801388889 2009-01-12 21:07:24 503110010 50.269 50 50.269 50.269 0 50.269 1 1 0 1 1 0 0 50.0618 50.0618 114.0639 2 PROCESSED 57545.1792013889 2016-06-06 04:18:03 55328 2010-05-12 00:00:00 54854.3728703704 2009-01-23 08:56:56 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 033076 K3/PSR J1420-6048 is one of the TeV gamma-ray pulsar wind nebulae detected by HESS, which are thought to be main particle accelerators to the Galactic Cosmic rays. It was also detected by EGRET and its X-ray spectrum is very hard. In order to reveal the radiation mechanism, we propose to observe the extended source for 50 ksec on HXD nominal position and contamination source for 20 ksec on XIS nominal position. The main purpose of this observation is to obtain the hard X-ray spectrum up to about 40 keV. GALACTIC DIFFUSE EMISSION 5 C TETSUICHI KISHISHITA ROGER ROMANI JUS 3 AO3 SUZAKU OBSERVATION OF TEV GAMMA-RAY PWN K3/PSR J1420-6048 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503110010/ Quick Look
12 A3667_CENTER 303.141 -56.7974 302.14092 -56.947599 291.656641 -35.82366 340.90266514 -33.39955413 74.263 53861.7363078704 2006-05-06 17:40:17 53862.3843055556 2006-05-07 09:13:24 801096010 20.8805 20 20.8885 20.8885 20.8965 20.8805 1 1 1 1 1 0 0 8.425 8.425 55.9439 1 PROCESSED 57533.6497337963 2016-05-25 15:35:37 54394 2007-10-21 00:00:00 53913.7840509259 2006-06-27 18:49:02 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 013080 We propose to observe along the north west relic of Abell 3667 cluster. The aim of this observation is to obtain a high quality hard X-ray spectra of the NW relic, utlizing the high sensitivity and norrow field of view of the HXD detector, as well as the high sensitivity of the XIS to widely diffuse souces. EXTRAGALACTIC DIFFUSE SOURCES 8 A KAZUHIRO NAKAZAWA CRAIG SARAZIN JUS 1 AO1 SUZAKU OBSERVATION OF A MERGING CLUSTER ABELL 3667 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801096010/ Quick Look
13 ABELL 262 OFFSET1 28.5344 36.2686 27.797773 36.023209 39.729024 22.927942 136.82832457 -24.90547123 69.9996 54318.8941898148 2007-08-06 21:27:38 54320.0772337963 2007-08-08 01:51:13 802079010 54.5894 48 54.5974 54.5894 0 54.6029 2 2 0 2 1 0 0 50.9123 50.9123 102.2038 1 PROCESSED 57539.4485416667 2016-05-31 10:45:54 54730 2008-09-21 00:00:00 54347.4244791667 2007-09-04 10:11:15 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 023004 We propose to observe Abell 262. The temperature of the intracluster mediums of the cluster is 2 keV and therefore this cluster is between groups of galaxies and clusters of galaxies. The purpuse of the observation is to determine the distribution of O, Mg, Si and Fe f the intracluster medium upto 0.3 r180. The exposures are 30 ks for the central pointing and 40 ks for two offset pointings and the total exposure is 110ks. EXTRAGALACTIC DIFFUSE SOURCES 8 A KYOKO MATSUSHITA Fabio Gastaldello JUS 2 AO2 O AND MG ABUNDANCES OF THE INTRACLUSTER MEDIUMS OF ABELL 262 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802079010/ Quick Look
14 A262 E2 28.9415 35.8688 28.205018 35.624348 39.895398 22.433371 137.29682221 -25.20210685 249.9999 56695.375625 2014-02-07 09:00:54 56696.1043518518 2014-02-08 02:30:16 808113010 33.0569 32 33.0609 33.0569 0 33.0649 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57613.8024884259 2016-08-13 19:15:35 57074 2015-02-21 00:00:00 56709.7139814815 2014-02-21 17:08:08 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 083002 We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy. EXTRAGALACTIC DIFFUSE SOURCES 8 B KYOKO MATSUSHITA NORBERT WERNER JUS 8 AO8 OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808113010/ Quick Look
15 1FGL J1018.6-5856 154.7461 -58.9386 154.30337 -58.687202 196.560422 -60.861111 284.35392298 -1.67969789 308.622 56105.7124189815 2012-06-27 17:05:53 56106.6523611111 2012-06-28 15:39:24 407096010 60.4324 60 60.4324 60.4324 0 60.4324 2 2 0 2 1 0 0 53.5978 53.5978 81.2059 1 PROCESSED 57606.5124768518 2016-08-06 12:17:58 56484 2013-07-11 00:00:00 56118.0496527778 2012-07-10 01:11:30 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 073113 Recently, a modulated signal has been detected with the Fermi from the source 1FGL J1018.6-5856. The presence of a O-type star in this source, and the variable character of the signal suggested that the source is a new gamma-ray binary system. Since it is expected that X-rays in these sources has the synchrotron origin, detailed X-ray observations are very important for understanding of the processes occurring in the system. However, sensitive observations of source in the X-ray energy bands are still missing. Therefore, we propose to observe the source with Suzaku. Since a long observational campaign is planned for 2012 by the HESS collaboration, the obtained X-ray, together with TeV, data will allow a proper modeling of the physical processes behind the non-thermal emission in system. GALACTIC POINT SOURCES 4 B HIROKAZU ODAKA TAKAAKI TANAKA JUS 7 AO7 X-RAY OBSERVATION OF GAMMA-RAY BINARY 1FGL J1018.6-5856 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407096010/ Quick Look
16 A1750C 202.6943 -1.8873 202.05036 -1.629855 201.691973 7.074913 322.57262201 59.47596371 293.5241 55766.9371064815 2011-07-24 22:29:26 55767.8814814815 2011-07-25 21:09:20 806095010 41.4893 40 41.5049 41.4893 0 41.5049 2 2 0 2 1 0 0 41.0991 41.0991 81.5778 0 PROCESSED 57602.6723148148 2016-08-02 16:08:08 56219 2012-10-19 00:00:00 55851.4572106482 2011-10-17 10:58:23 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 063019 We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA SCOTT RANDALL JUS 6 AO6 SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806095010/ Quick Look
17 PKS 1510-089 228.2108 -9.1043 227.537329 -8.917552 228.287746 8.492539 351.2856545 40.1353659 286.8003 53949.3968634259 2006-08-02 09:31:29 53952.2544444445 2006-08-05 06:06:24 701094010 119.1577 120 119.1577 119.1577 119.1657 119.1657 2 2 2 2 1 0 0 106.2588 106.2588 246.8638 5 PROCESSED 57535.1605208333 2016-05-27 03:51:09 54394 2007-10-21 00:00:00 54018.7363194444 2006-10-10 17:40:18 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 013016 It has been a long mystery (i) how the relativistic jets are formed, and (ii) what is the composition of a jet. In the theoretical view, strong magnetic field (u_B >> u_e) is necessary to produce such outflows with baryonic matters, but observations favor opposite scenario, namely particle dominated (u_e >> u_B), leptonic jet. Such discrepancies can be resolved if moderate numbers of protons (n_e/n_p > 50) are mixed in the non-tnermal pair populations. This can be easily tested if we can observe characteristic "soft X-ray bump" produced by the bulk-Comptonization of UV photons emitted from an accretion disk. We propose a deep observation (40ksec x3) of an EGRET quasar PKS 1510-089, which shows a clear sign of soft X-ray bump in BeppoSAX, ROSAT and ASCA observations. EXTRAGALACTIC COMPACT SOURCES 7 B JUN KATAOKA GRZEGORZ MADEJSKI JUS 1 AO1 DIRECT TESTING THE JET COMPOSITION IN A POWERFUL EGRET QUASAR PKS 1510-089 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701094010/ Quick Look
18 A1914_OFFSET2 216.7383 37.763 216.226328 37.986791 196.709268 48.583272 66.87630822 67.3091462 329.9943 55363.4747569444 2010-06-16 11:23:39 55364.3800115741 2010-06-17 09:07:13 805092010 28.5462 40 28.5542 28.5542 0 28.5462 2 2 0 2 1 0 0 25.8343 25.8343 78.204 0 PROCESSED 57552.3515856482 2016-06-13 08:26:17 55766 2011-07-24 00:00:00 55399.3275231482 2010-07-22 07:51:38 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA ERIC MILLER JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805092010/ Quick Look
19 A1914_OFFSET4 216.4424 37.6372 215.928949 37.861845 196.491265 48.360248 66.78881215 67.57279807 134.0011 55566.4311574074 2011-01-05 10:20:52 55566.8258912037 2011-01-05 19:49:17 805094020 17.3531 12 17.3531 17.3611 0 17.3691 2 2 0 2 1 0 0 16.0606 16.0606 34.1 0 PROCESSED 57600.564375 2016-07-31 13:32:42 55995 2012-03-09 00:00:00 55627.1583333333 2011-03-07 03:48:00 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA ERIC MILLER JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805094020/ Quick Look
20 A3667_NW_17OFF 302.8177 -56.56 301.819585 -56.708877 291.523842 -35.547493 341.18808838 -33.22347241 74.1682 53861.293912037 2006-05-06 07:03:14 53861.7356944444 2006-05-06 17:39:24 801095010 17.2586 20 17.2826 17.2746 17.2666 17.2586 1 1 1 1 1 0 0 14.2555 14.2555 38.1519 1 PROCESSED 57533.636099537 2016-05-25 15:15:59 54735 2008-09-26 00:00:00 53913.7593518518 2006-06-27 18:13:28 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 013080 We propose to observe along the north west relic of Abell 3667 cluster. The aim of this observation is to obtain a high quality hard X-ray spectra of the NW relic, utlizing the high sensitivity and norrow field of view of the HXD detector, as well as the high sensitivity of the XIS to widely diffuse souces. EXTRAGALACTIC DIFFUSE SOURCES 8 A KAZUHIRO NAKAZAWA CRAIG SARAZIN JUS 1 AO1 SUZAKU OBSERVATION OF A MERGING CLUSTER ABELL 3667 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801095010/ Quick Look
21 A3667_NW_17OFF 302.869 -56.6666 301.869632 -56.815685 291.522519 -35.657764 341.06051648 -33.2513141 258.9342 54038.8325578704 2006-10-30 19:58:53 54039.0106944444 2006-10-31 00:15:24 801095020 11.9634 10 11.9794 11.9794 11.9634 11.9714 1 1 1 1 1 0 0 8.724 8.724 15.3839 0 PROCESSED 57535.9848032407 2016-05-27 23:38:07 54735 2008-09-26 00:00:00 54056.1858796296 2006-11-17 04:27:40 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 013080 We propose to observe along the north west relic of Abell 3667 cluster. The aim of this observation is to obtain a high quality hard X-ray spectra of the NW relic, utlizing the high sensitivity and norrow field of view of the HXD detector, as well as the high sensitivity of the XIS to widely diffuse souces. EXTRAGALACTIC DIFFUSE SOURCES 8 A KAZUHIRO NAKAZAWA CRAIG SARAZIN JUS 1 AO1 SUZAKU OBSERVATION OF A MERGING CLUSTER ABELL 3667 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801095020/ Quick Look
22 A3667_NW_RELIC 302.5617 -56.3599 301.565299 -56.507728 291.421165 -35.317169 341.42703548 -33.08195751 74.7123 53858.7409837963 2006-05-03 17:47:01 53861.2933449074 2006-05-06 07:02:25 801094010 94.3946 95 94.4026 94.3946 94.3946 94.4026 3 3 3 3 1 0 0 56.2506 56.2506 220.489 4 PROCESSED 57533.7274074074 2016-05-25 17:27:28 54394 2007-10-21 00:00:00 53913.7574189815 2006-06-27 18:10:41 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 013080 We propose to observe along the north west relic of Abell 3667 cluster. The aim of this observation is to obtain a high quality hard X-ray spectra of the NW relic, utlizing the high sensitivity and norrow field of view of the HXD detector, as well as the high sensitivity of the XIS to widely diffuse souces. EXTRAGALACTIC DIFFUSE SOURCES 8 A KAZUHIRO NAKAZAWA CRAIG SARAZIN JUS 1 AO1 SUZAKU OBSERVATION OF A MERGING CLUSTER ABELL 3667 HXD N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801094010/ Quick Look
23 MRK 110 141.3383 52.3497 140.469294 52.565715 125.649662 35.070751 164.91808924 44.3703784 110.1475 54406.3443055556 2007-11-02 08:15:48 54408.31625 2007-11-04 07:35:24 702124010 90.8712 100 90.8712 90.8792 0 90.8792 2 2 0 2 1 0 0 86.5231 86.5231 170.3558 2 PROCESSED 57540.442037037 2016-06-01 10:36:32 54786 2008-11-16 00:00:00 54417.3880092593 2007-11-13 09:18:44 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 023012 We request a 100 ks SUZAKU observation of Mrk 110 to quantify the accretion disk geometry in this high luminosity narrow line Seyfert 1 galaxy. This is an unique low mass AGN which shows an almost featureless X-ray continuum described by a two component Comptonization model. It has shown, based on an XMM-Newton data, energy dependent delays which are consistent with the idea of a Comptonized plasma confined within 10 Schwartzschild radius of the central black hole. The proposed long observation will provide high signal-to-noise hard X-ray data, thus allowing us to extend the observed delay to higher energies and also to quantify the high energy spectral parameters like cut-off energy and reflection parameters. This will help us to identify the accretion disk geometry in this source. EXTRAGALACTIC COMPACT SOURCES 7 C ARIKKALA RAO Gulab Dewangan EUS 2 AO2 PROBING THE ACCRETION DISK GEOMETRY IN THE TYPE I SEYFERT GALAXY MRK 110 HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702124010/ Quick Look
24 A1914_OFFSET2 216.77 37.7885 216.258243 38.012199 196.723878 48.617689 66.91478771 67.27662817 134.0016 55565.7291203704 2011-01-04 17:29:56 55566.0216550926 2011-01-05 00:31:11 805092020 17.0912 12 17.0992 17.0912 0 17.1072 1 1 0 1 1 0 0 13.2058 13.2058 25.2719 0 PROCESSED 57600.5511689815 2016-07-31 13:13:41 56037 2012-04-20 00:00:00 55670.1137384259 2011-04-19 02:43:47 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA ERIC MILLER JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805092020/ Quick Look
25 A262 NE2 28.537 36.7219 27.798764 36.476514 39.918494 23.346467 136.69850182 -24.46778258 249.9995 56703.1881712963 2014-02-15 04:30:58 56703.8821643518 2014-02-15 21:10:19 808109010 32.9447 32 32.9527 32.9607 0 32.9447 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57613.8208564815 2016-08-13 19:42:02 57080 2015-02-27 00:00:00 56714.743275463 2014-02-26 17:50:19 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 083002 We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy. EXTRAGALACTIC DIFFUSE SOURCES 8 A KYOKO MATSUSHITA NORBERT WERNER JUS 8 AO8 OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808109010/ Quick Look
26 SWIFT J1322.2-1641 200.5819 -16.7858 199.912392 -16.524578 205.294799 -7.530887 313.4989766 45.45121448 290.037 55013.9738310185 2009-07-01 23:22:19 55014.9981365741 2009-07-02 23:57:19 704022010 41.3487 40 41.3487 41.6207 0 41.6127 2 2 0 2 1 0 0 36.2368 36.2368 88.4858 7 PROCESSED 57547.7444097222 2016-06-08 17:51:57 55393 2010-07-16 00:00:00 55027.0523148148 2009-07-15 01:15:20 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 043059 The number of Compton thick AGNs is the biggest issue in the origin of the X-ray background and AGN evolution. According to the latetest population synthesis model, its estimate is strongly coupled with the broad band spectral shape of moderately absorbed AGNs, which is only poorly understood. Recently, Swift/BAT has provided the first unbiased AGN sample above 15 keV, which includes many hard X-ray bright, absorbed AGNs that can be best followed-up with Suzaku. Here we propose to observe three of them to measure the amount of reflection component with unpreceded accuracy, a key parameter to determine the total contribution of Compton thick AGNs to the X-ray background. With these observations we can make the spectral survey of bright absorbed Swift/BAT AGNs complete. EXTRAGALACTIC COMPACT SOURCES 7 A YOSHIHIRO UEDA MAURO DADINA JEU 4 AO4 SPECTRAL SURVEY OF A COMPLETE SAMPLE OF SWIFT/BAT SELECTED AGNS AND THE ORIGIN OF THE X-RAY BACKGROUND HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704022010/ Quick Look
27 A262 NE1 28.4051 36.5019 27.66806 36.256213 39.720751 23.183318 136.64990456 -24.70790073 250 56702.5986342593 2014-02-14 14:22:02 56703.187662037 2014-02-15 04:30:14 808108010 25.6102 24 25.6102 25.6102 0 25.6102 2 2 0 2 0 0 0 0 0 0 0 PROCESSED 57613.8178472222 2016-08-13 19:37:42 57080 2015-02-27 00:00:00 56714.742037037 2014-02-26 17:48:32 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 083002 We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy. EXTRAGALACTIC DIFFUSE SOURCES 8 A KYOKO MATSUSHITA NORBERT WERNER JUS 8 AO8 OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808108010/ Quick Look
28 A1914_OFFSET3 216.2544 37.895 215.741562 38.120181 196.10746 48.514193 67.56094175 67.61680074 134.0009 55566.0223148148 2011-01-05 00:32:08 55566.4306365741 2011-01-05 10:20:07 805093020 12.8294 12 12.8294 12.8294 0 12.8294 2 2 0 2 1 0 0 13.721 13.721 35.2699 0 PROCESSED 57600.553599537 2016-07-31 13:17:11 55995 2012-03-09 00:00:00 55627.1328009259 2011-03-07 03:11:14 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 053087 We propose four pointing observations of the merging cluster Abell 1914 with exposure of 160 ks (40 ks each). We measure temperature, electron density, and entropy distributions of the ICM out to the virial radius to study the merging history of this cluster. We determine the supra-thermal component expected by the merger with a wide-band spectroscopy using XIS and HXD-PIN, and quantify heat input to the ICM by a joint analysis with weak lensing data of Subaru telescope. Then, we aim to estimate the energy ratio of the heat input to total delivered energy through the merger. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA ERIC MILLER JUS 5 AO5 THERMODYNAMICS OF INTRACLUSTER MEDIUM IN THE MERGING CLUSTER ABELL 1914 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805093020/ Quick Look
29 ABELL 262 OFFSET2 28.0598 36.4356 27.324082 36.18913 39.413922 23.227924 136.37355079 -24.84408055 69.9996 54320.0778935185 2007-08-08 01:52:10 54321.2405555556 2007-08-09 05:46:24 802080010 54.7081 48 54.7241 54.7081 0 54.7241 2 2 0 2 1 0 0 50.1788 50.1788 100.3968 1 PROCESSED 57539.4536226852 2016-05-31 10:53:13 54730 2008-09-21 00:00:00 54347.6730671296 2007-09-04 16:09:13 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 023004 We propose to observe Abell 262. The temperature of the intracluster mediums of the cluster is 2 keV and therefore this cluster is between groups of galaxies and clusters of galaxies. The purpuse of the observation is to determine the distribution of O, Mg, Si and Fe f the intracluster medium upto 0.3 r180. The exposures are 30 ks for the central pointing and 40 ks for two offset pointings and the total exposure is 110ks. EXTRAGALACTIC DIFFUSE SOURCES 8 A KYOKO MATSUSHITA Fabio Gastaldello JUS 2 AO2 O AND MG ABUNDANCES OF THE INTRACLUSTER MEDIUMS OF ABELL 262 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802080010/ Quick Look
30 A1750N 202.8147 -1.6537 202.171177 -1.396479 201.71761 7.336429 322.93839507 59.66232121 293.5219 55744.8544444444 2011-07-02 20:30:24 55746.9911111111 2011-07-04 23:47:12 806096010 74.7134 80 74.7294 74.7134 0 74.7294 2 2 0 2 1 0 0 61.6402 61.6402 184.5979 1 PROCESSED 57602.5091435185 2016-08-02 12:13:10 56144 2012-08-05 00:00:00 55775.4134027778 2011-08-02 09:55:18 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 063019 We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA SCOTT RANDALL JUS 6 AO6 SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806096010/ Quick Look
31 A3558 WEST OFF 201.4503 -31.5856 200.748303 -31.325817 211.928183 -20.890972 311.44383739 30.71755895 288.4754 54657.5304513889 2008-07-10 12:43:51 54660.0225 2008-07-13 00:32:24 803072010 81.8162 80 81.8162 81.8162 0 81.8162 2 2 0 2 1 0 0 67.3941 67.3941 215.2857 1 PROCESSED 57543.1016898148 2016-06-04 02:26:26 55037 2009-07-25 00:00:00 54670.5540162037 2008-07-23 13:17:47 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 033089 We aim at the first significant detection of redshifted OVII and OVIII lines from the warm-hot intergalactic medium (WHIM) in the Shapley Supercluster. The system, located at z = 0.048, shows the richest concentration of X-ray clusters in the nearby universe. Previous ROSAT observation showed enhanced soft X-ray emission along the cluster connection. We propose to observe for 80 ksec a region between A3558 (the brightest central cluster) and A3556, separated by 0.9 virial radius from both clusters and along the line of cluster connection. A 40 ksec observation is also proposed at a 2-degree offest region to measure the foreground Galactic spectrum. Based on the ROSAT flux, we expect to detect redshifted OVII and OVII lines at more than 7 sigma confidence. EXTRAGALACTIC DIFFUSE SOURCES 8 A TAKAYA OHASHI MASSIMILIANO GALEAZZAI JUS 3 AO3 SEARCH FOR WHIM IN THE SHAPLEY SUPERCLUSTER XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803072010/ Quick Look
32 G306.3-0.9 200.4753 -63.5602 199.643661 -63.298602 230.10249 -49.420915 306.31531317 -0.88874973 306.5675 56889.7845833333 2014-08-20 18:49:48 56894.0099768518 2014-08-25 00:14:22 509072010 190.0114 200 190.0181 190.0114 0 190.0114 2 2 0 2 1 0 0 14.4515 14.4515 20.22 0 PROCESSED 57616.5396759259 2016-08-16 12:57:08 57305 2015-10-10 00:00:00 56938.2302777778 2014-10-08 05:31:36 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 093109 The origin of the distorted, inhomogeneous structure of mixed-morphology SNRs (MM SNRs) is a mystery. Recently we have discovered recombining plasma from MM SNRs. The existence of recombining plasma implies rapid cooling process in past. Recombining plasma, together with the peculiar morphologies, would indicate a new SNR evolution scenario. Our systematic analysis of recombining SNRs shows that the recombination ages are almost the same, although their dynamical ages range over an order of magnitude. Such a trend can be explained by past rapid rarefaction. This hypothesis can be tested by measuring a recombination age of a dynamically young recombining SNR. We thus propose a 100-ks Suzaku observation of G306.3-0.9, a candidate of the youngest recombining SNR ever. GALACTIC DIFFUSE EMISSION 5 A MAKOTO SAWADA Reynolds,Matsumura JUS 9 AO9 THE DYNAMICS OF MIXED-MORPHOLOGY SNRS PROBED BY THE YOUNGEST RECOMBINING PLASMA XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/509072010/ Quick Look
33 GK PER 52.8202 43.8404 51.968435 43.670553 61.500851 24.010688 151.00566373 -10.1477205 257.5144 54875.4415277778 2009-02-13 10:35:48 54876.0899884259 2009-02-14 02:09:35 403081010 30.3888 30 30.3888 30.3888 0 30.3888 2 2 0 2 1 0 0 27.3999 27.3999 55.9979 2 PROCESSED 57545.5260648148 2016-06-06 12:37:32 55330 2010-05-14 00:00:00 54893.4257407407 2009-03-03 10:13:04 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 033107 We propose observations of 5 Intermediate Polars, a subcategory of magnetic CVs, as the first step toward establishment of an averaged hard X-ray spectrum of IPs that exist near the Solar system.The averaged spectrum should be compared with that of the Galactic Diffese X-ray Emssion (GDXE), to investigate the claimed spectral resemblance between them in energies above 10 keV. If the averaged IP spectrum shows any discrepancy with that of the GDXE, the "point-source origin" explanation for the GDXE would face a lack of appropriate hard X-ray source populations. This in turn is expected to strengthen the competing "truly diffuse origin"explanation, which attributes the GDXE hard X-rays to non thermal emission from electrons being accelerated in the interstellar space. GALACTIC POINT SOURCES 4 C TAKAYUKI YUASA THOMAS HARRISON JUS 3 AO3 SURVEY OBSERVATION OF INTERMEDIATE POLARS HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403081010/ Quick Look
34 A262 E1 28.6322 35.9862 27.896259 35.741034 39.692258 22.636644 136.99532529 -25.15665513 249.9998 56694.7928935185 2014-02-06 19:01:46 56695.3750694444 2014-02-07 09:00:06 808112010 25.9466 24 25.9546 25.9466 0 25.9626 3 3 0 3 0 0 0 0 0 0 0 PROCESSED 57613.7986226852 2016-08-13 19:10:01 57074 2015-02-21 00:00:00 56709.7127893518 2014-02-21 17:06:25 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 083002 We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy. EXTRAGALACTIC DIFFUSE SOURCES 8 B KYOKO MATSUSHITA NORBERT WERNER JUS 8 AO8 OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808112010/ Quick Look
35 A262 NE4 28.8115 37.1901 28.070704 36.945344 40.33412 23.695949 136.79382783 -23.95810874 249.9999 56704.7992476852 2014-02-16 19:10:55 56705.5321064815 2014-02-17 12:46:14 808111010 30.9305 30 30.9625 30.9305 0 30.9625 1 1 0 1 1 0 0 27.8027 27.8027 63.3119 2 PROCESSED 57613.8474652778 2016-08-13 20:20:21 57085 2015-03-04 00:00:00 56719.7343981482 2014-03-03 17:37:32 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 083002 We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy. EXTRAGALACTIC DIFFUSE SOURCES 8 A KYOKO MATSUSHITA NORBERT WERNER JUS 8 AO8 OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808111010/ Quick Look
36 A262 NE3 28.6712 36.9514 27.931716 36.706321 40.12197 23.517818 136.74540455 -24.21802206 250.0003 56703.8826388889 2014-02-15 21:11:00 56704.7987731482 2014-02-16 19:10:14 808110010 40.4903 40 40.5134 40.4903 0 40.4966 2 2 0 2 1 0 0 34.2624 34.2624 69.899 1 PROCESSED 57613.8476041667 2016-08-13 20:20:33 57081 2015-02-28 00:00:00 56715.76 2014-02-27 18:14:24 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 083002 We propose to observe a poor cluster, Abell 262 (kT=2.2 keV, z=0.017), out to 0.9 r180 toward directions of a filament and void. The objectives are to derive gas-mass and fe-mass-to-light ratios and entropy profiles out the virial radius and study their dependence of the system mass, and to study azimuthal dependence of the temperature, density and entropy. EXTRAGALACTIC DIFFUSE SOURCES 8 A KYOKO MATSUSHITA NORBERT WERNER JUS 8 AO8 OBSERVATIONS OF AN POOR CLUSTER OUT TO THE VIRIAL RADIUS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808110010/ Quick Look
37 A1750R 202.8691 -2.0415 202.224847 -1.784379 201.912931 6.996197 322.80853082 59.27632496 111.4517 55918.5150810185 2011-12-23 12:21:43 55918.843912037 2011-12-23 20:15:14 806098020 16.062 13 16.062 16.062 0 16.062 1 1 0 1 1 0 0 11.964 11.964 28.4079 0 PROCESSED 57604.214375 2016-08-04 05:08:42 56311 2013-01-19 00:00:00 55972.6764236111 2012-02-15 16:14:03 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 063019 We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA JUS 6 AO6 SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806098020/ Quick Look
38 A1750R 202.8633 -2.0722 202.218991 -1.815068 201.918925 6.965529 322.77954726 59.24881782 293.5198 55748.0658796296 2011-07-06 01:34:52 55750.0419097222 2011-07-08 01:00:21 806098010 66.5035 80 66.5115 66.5035 0 66.5115 3 2 0 2 1 0 0 54.7821 54.7821 170.7128 3 PROCESSED 57602.5535763889 2016-08-02 13:17:09 56311 2013-01-19 00:00:00 55795.163912037 2011-08-22 03:56:02 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 063019 We observe Abell 1750 which has three clusters of galaxies in a filamentary structure of the large-scale structure, with 4 pointing observations (80 x 3 + 40 ks). We reveal global spatial structures of temperature, density, and entropy in Abell 1750 for the first time. By a correlation with a galaxy map obtained from SDSS, and a comparison between thermal pressure and total pressure required by the total mass derived from weal lensing analysis, we explore the inflow of matter and evolutionary process in this system. EXTRAGALACTIC DIFFUSE SOURCES 8 A MADOKA KAWAHARADA SCOTT RANDALL JUS 6 AO6 SUZAKU OBSERVATION OF ABELL 1750 IN THE LARGE-SCALE STRUCTURE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806098010/ Quick Look

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SELECT * FROM suzaku_master_data WHERE SUBSTRING(proposal_id,3,1) = '3'

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