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 ABELL 3571 206.8624 -32.8524 206.14186 -32.603207 216.960537 -20.284209 316.31343933 28.55973438 103.8412 56666.0275 2014-01-09 00:39:36 56666.7772453704 2014-01-09 18:39:14 808094010 38.279 60 38.279 38.279 0 38.279 2 2 0 2 1 0 0 39.0047 39.0047 64.776 0 PROCESSED 57613.7763425926 2016-08-13 18:37:56 57096 2015-03-15 00:00:00 56730.4916435185 2014-03-14 11:47:58 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 081531 Abell 3571 is one of the brightest cluster in the X-ray sky and one of the main clusters in the Shapley supercluster. We have recently found evidence that it may be passing through a violent (~2000 km/s) merger in the line of sight (los). If corroborated it would be the closest template for the systems of this kind allowing us to study and characterize los mergers. We request a short observation of 60 ksec to corroborate the velocity gradients found with Chandra for this cluster, using the improved spectral resolution and gain stability of Suzaku s XISs. EXTRAGALACTIC DIFFUSE SOURCES 8 C RENATO DUPKE USA 8 AO8 ABELL 3571. THE CLOSEST LINE OF SIGHT MERGER? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808094010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '808094010'

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