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 | CENTAURUS CLUSTER N | 192.2138 | -40.9141 | 191.523743 | -40.64159 | 208.863601 | -32.495572 | 302.40583252 | 21.95501054 | 115.2417 | 55961.0060763889 | 2012-02-04 00:08:45 | 55962.6667939815 | 2012-02-05 16:00:11 | 806011010 | 54.0496 | 50 | 54.0496 | 54.0496 | 0 | 54.0496 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 48.6109 | 48.6109 | 143.4758 | 2 | PROCESSED | 57604.5565972222 | 2016-08-04 13:21:30 | 56360 | 2013-03-09 00:00:00 | 55992.1577546296 | 2012-03-06 03:47:10 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060035 | We propose to observe two fields at 0.1-0.2r180 of the Centaurus cluster for total 90 ks exposures with Suzaku. The purpose of the observations is to determine Mg and Fe distributions of the intracluster medium up to 0.2 r180 and to study origin of metals in the intracluster medium. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | KYOKO MATSUSHITA | JAP | 6 | AO6 | MG AND FE ABUNDANCES OF THE ICM IN THE CENTAURUS CLUSTER UP TO 0.2R180 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806011010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '806011010'
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