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 | A496 P-OUT | 68.2513 | -13.0087 | 67.67058 | -13.113188 | 64.018052 | -34.510238 | 209.22191803 | -36.52315476 | 62.0525 | 54674.5225347222 | 2008-07-27 12:32:27 | 54675.6050231482 | 2008-07-28 14:31:14 | 803048010 | 37.5516 | 35 | 37.5516 | 37.5596 | 0 | 37.5596 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 33.1599 | 33.1599 | 93.4939 | 1 | PROCESSED | 57543.1577314815 | 2016-06-04 03:47:08 | 55055 | 2009-08-12 00:00:00 | 54689.4360416667 | 2008-08-11 10:27:54 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031424 | A496 is a "normal" nearby cluster that has been the testbed for metal enrichment models in clusters and, more recently, of different mechanisms to generate cold fronts. Suzaku's excellent spectral resolution, low background and high effective area, combined with the moderate temperatures of this cluster allows us to probe, with two short exposures, into the large scale metal enrichment processes through determination of elemental abundance ratios out to half the virial radius for the first time. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | RENATO DUPKE | USA | 3 | AO3 | LARGE SCALE METAL ENRICHMENT MECHANISMS IN ABELL 496 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/803048010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '803048010'
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