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 | MKN 3 | 93.8839 | 71.0477 | 92.433649 | 71.063052 | 91.875357 | 47.63268 | 143.2836301 | 22.71631463 | 71.8326 | 53665.0848263889 | 2005-10-22 02:02:09 | 53667.2682175926 | 2005-10-24 06:26:14 | 100040010 | 95.0265 | 100 | 95.0265 | 95.0772 | 95.0452 | 95.0345 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 91.3441 | 91.3441 | 188.6299 | 0 | PROCESSED | 57527.6643055556 | 2016-05-19 15:56:36 | 54247 | 2007-05-27 00:00:00 | 53906.4896759259 | 2006-06-20 11:45:08 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000040 | Mkn 3 is the second brightest Compton-thick Sy 2 currently visible with Suzaku. The broadband spectrum of Mkn 3, as probed by previous SAX and Chandra observations, is dominated by a reflection component (Compton hump strength R is near 1), but there is also evidence for a strongly absorbed hard X-ray power law that may be direct emission from the obscured nucleus, filtering through Compton-thick material (such as the molecular torus). | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | MKN 3 | HXD | N | https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/100040010/ | Quick Look | ![]() |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100040010'
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