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 | A 2218 | 249.0001 | 66.203 | 248.949919 | 66.302836 | 172.76704 | 81.613118 | 97.724401 | 38.11892096 | 242.3617 | 53644.3643402778 | 2005-10-01 08:44:39 | 53645.3446643518 | 2005-10-02 08:16:19 | 100030010 | 43.3629 | 50 | 43.3629 | 44.7173 | 43.4253 | 43.8248 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 41.4918 | 41.4918 | 84.678 | 1 | PROCESSED | 57527.4791898148 | 2016-05-19 11:30:02 | 54247 | 2007-05-27 00:00:00 | 54035.7677314815 | 2006-10-27 18:25:32 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000030 | Search of redshifted (z=0.171) OVII emission line from warm-hot intergalactic matter around a cluster which shows a merger feature in the line of sight, with no central cool component. The depth of the structure can be ~20 Mpc, and the redshift allows a clear separation of the lines from the Galactic hot gas. The low background and the superior resolution of XIS in the soft X-ray energy range will allow the best measurement of the WHIM emission so far. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | A2218 and its offset observation | N | https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/100030010/ | Quick Look | ![]() |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100030010'
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