DARTS Astro
total 1
Show the used SQL Download WgetScript
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 |
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1 | GX 339-4 | 255.7297 | -48.7352 | 254.782436 | -48.66432 | 259.586148 | -25.80756 | 338.99220289 | -4.30584956 | 108.3513 | 54920.4773958333 | 2009-03-30 11:27:27 | 54921.5216435185 | 2009-03-31 12:31:10 | 403011030 | 39.6384 | 40 | 39.6633 | 39.6384 | 0 | 39.6633 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 35.0686 | 35.0686 | 90.186 | 0 | PROCESSED | 57545.9795601852 | 2016-06-06 23:30:34 | 55330 | 2010-05-14 00:00:00 | 54931.0610416667 | 2009-04-10 01:27:54 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030046 | Growing evidence indicates that a relativistic jet from a black hole is produced during its transition from the "hard state" to the "soft state" through the "very high state". We propose to make TOO observations of a Galactic black hole binary in the early phase of ourburst with Suzaku in order to reveal the evolution of the accretion disk structure during ejection events. We will trigger a TOO observation upon the RXTE ASM. At the same time we organize multiwavelength observations in radio and infrared/optical bands to examine the exact relation between the ejection and state transition. | GALACTIC POINT SOURCES | 4 | A | YOSHIHIRO UEDA | JAP | 3 | AO3-TOO | MULTIWAVELENGH OBSERVATIONS OF A GALACTIC BLACK HOLE IN EARLY PHASE OF OUTBURST | HXD | Y | https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403011030/ | Quick Look | ![]() |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403011030'
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