DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_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
|
awarded_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
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | A2218_offset | 244.4769 | 65.4468 | 244.387309 | 65.566901 | 174.329918 | 79.629039 | 97.72059475 | 40.11912915 | 237.1965 | 53645.3474537037 | 2005-10-02 08:20:20 | 53646.32375 | 2005-10-03 07:46:12 | 100030020 | 44.8592 | 50 | 44.8592 | 46.1907 | 44.9141 | 45.3747 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 42.5366 | 42.5366 | 84.3439 | 0 | PROCESSED | 57527.5203125 | 2016-05-19 12:29:15 | 54247 | 2007-05-27 00:00:00 | 54036.969224537 | 2006-10-28 23:15:41 | 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://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/100030020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100030020'
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