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 |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
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'
Your request has been accepted.
The download will start soon automatically.