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
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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