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 SGR 1806-20 272.1687 -20.4711 271.424026 -20.47983 272.024767 2.954425 9.94559743 -0.27498509 268.1397 54387.2332060185 2007-10-14 05:35:49 54388.333599537 2007-10-15 08:00:23 402094010 52.2477 50 52.2477 52.2717 0 52.2637 2 2 0 2 1 0 0 50.0895 50.0895 95.0599 1 PROCESSED 57540.2839583333 2016-06-01 06:48:54 54771 2008-11-01 00:00:00 54403.9548611111 2007-10-30 22:55:00 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 022016 Among magnetars, SGR 1806-20 is particularly interesting since it emitted two years ago the most powerful giant flare ever observed. We are performing a long term monitoring in the soft X-rays with XMM-Newton and hard X-rays with INTEGRAL to study how the source evolves back to quiescence. We obtained in AO-1 a Suzaku observation that was carried out simultaneously with XMM-Newton and provided for the first time a broad band spectrum of SGR 1806-20 on a short timescale. A new observation is required to study the spectral variability in the hard X-ray range and possibly the properties of bursts. GALACTIC POINT SOURCES 4 C SANDRO MEREGHETTI EUR 2 AO2 CONTINUED MONITORING OF SGR 1806-20 AFTER THE GIANT FLARE WITH SUZAKU AND XMM-NEWTON HXD Y https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/402094010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402094010'

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