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 | Sgr_A_East | 266.5146 | -28.9267 | 265.720381 | -28.907844 | 266.926105 | -5.522764 | 0.05802898 | -0.07696746 | 264.7152 | 53636.3044560185 | 2005-09-23 07:18:25 | 53637.462025463 | 2005-09-24 11:05:19 | 100027010 | 44.785 | 50 | 44.801 | 44.8523 | 44.785 | 44.8283 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 37.8543 | 37.8543 | 100.0139 | 1 | PROCESSED | 57527.4188657407 | 2016-05-19 10:03:10 | 54247 | 2007-05-27 00:00:00 | 54035.502662037 | 2006-10-27 12:03:50 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000027 | We propose to obtain high quality spectra from 6 positions near the GC. The objective is to resolve 6.4 , 6.7 and 6.9 keV line and determine the high energy tail from each positions and/or from the sub-structures in each position. Combining all the results, we can see which sub-sub-structure is X-ray reflection from Sgr A* ( 6.4 keV line+ 7.1 keV edge + high energy tail), thermal plasma (6.7+6.9 keV lines, with no hard X-ray tail), non thermal emission (e.g. line but hard X-ray tail). Unexpected spectral feature could be also found, depending on the real origin. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Suzaku Observation of Galactic Center Region | N | https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/100027010/ | Quick Look | ![]() |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100027010'
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