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 | 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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