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 | A133_S | 15.6819 | -22.1029 | 15.071421 | -22.371383 | 5.125588 | -26.4157 | 150.58121257 | -84.35810156 | 44.9946 | 55355.2966203704 | 2010-06-08 07:07:08 | 55356.727974537 | 2010-06-09 17:28:17 | 805022010 | 51.128 | 50 | 51.128 | 51.128 | 0 | 51.128 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 42.8599 | 42.8599 | 123.6558 | 1 | PROCESSED | 57551.9312962963 | 2016-06-12 22:21:04 | 55737 | 2011-06-25 00:00:00 | 55370.2538310185 | 2010-06-23 06:05:31 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050019 | We propose a mapping observation of Abell 133 to study temperature and metal abundance distributions up to ~0.8 times of virial radius. A good energy resolution, and a low and stable background level of the XIS instrument are crucial for this study. This data allow us to put constraints on the metal enrichment processes in the intergalactic space. We also investigate the magnetic field in the central region associated with the radio relic of Abell 133. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | KOSUKE SATO | JAP | 5 | AO5 | METALLICITY OF ABELL 133 FOR INVESTIGATING OF THE METAL ENRICHMENT PROCESS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805022010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '805022010'
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