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 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://darts.isas.jaxa.jp/pub/suzaku/ver3.0/100021010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '100021010'

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