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 | ARCHES CLUSTER | 266.4808 | -28.778 | 265.687528 | -28.758983 | 266.892731 | -5.374834 | 0.16960578 | 0.02569084 | 109.9998 | 54911.0857407407 | 2009-03-21 02:03:28 | 54913.7681712963 | 2009-03-23 18:26:10 | 403009010 | 110.7933 | 100 | 110.7933 | 110.7933 | 0 | 110.7933 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 91.6578 | 91.6578 | 231.7417 | 3 | PROCESSED | 57545.9555787037 | 2016-06-06 22:56:02 | 55330 | 2010-05-14 00:00:00 | 54924.3822106482 | 2009-04-03 09:10:23 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030029 | We propose to observe a hard X-ray ring which has an emission line around 6.4 keV, located at the north of the Arches cluster. The ring is probably produced by an energetic jet or a supernova explosion. We aim to determine the continuum shape, the center energy of the emission line, and the absorption column to figure out the origin of the ring. | GALACTIC POINT SOURCES | 4 | B | MASAHIRO TSUJIMOTO | JAP | 3 | AO3 | A 6.4 KEV RING AT THE NORTH OF THE ARCHES CLUSTER | XIS | Y | https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/403009010/ | Quick Look | ![]() |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403009010'
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