DARTS Astro

total 1

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 IGRJ16479-4514 252.0242 -45.1934 251.117904 -45.10536 256.364901 -22.598296 340.16807688 -0.11668459 91.5317 55980.9438194444 2012-02-23 22:39:06 55983.5363541667 2012-02-26 12:52:21 406078010 149.7785 150 149.7865 149.7785 0 149.7865 2 2 0 2 1 0 0 154.7295 154.7295 223.9819 0 PROCESSED 57604.8063888889 2016-08-04 19:21:12 56429 2013-05-17 00:00:00 56062.2788425926 2012-05-15 06:41:32 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 068014 We propose a 100 ks observation of the Supergiant Fast X-ray Transient (SFXT) with the shortest orbital period, the eclipsing IGRJ16479-4514 (3.3 d), with the main aim of probing its X-ray properties along one entire orbital phase with unprecedented sensitivity. The requested net exposure time indeed translates into an observation almost continuously spanning the whole binary system orbit, allowing for the first time an orbital phase resolved investigation of the X-ray emission properties, which will allow us to study the structure of the supergiant companion (its density and ionization state) and to cast light on the outburst mechanism at work in this new class of transients. GALACTIC POINT SOURCES 4 A LARA SIDOLI ARASH BODAGHEE EUS 6 AO6 UNVEILING THE MYSTERY OF THE SUPERGIANT FAST X-RAY TRANSIENT WITH THE SHORTEST ORBITAL PERIOD XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406078010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE SUBSTRING(proposal_id,3,1) = '8'

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