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 A1246_CENTER 170.9992 21.4865 170.340675 21.761183 163.096496 16.147963 224.00399917 69.32667171 120.0006 55151.2043981482 2009-11-16 04:54:20 55152.274525463 2009-11-17 06:35:19 804028010 48.4564 40 48.4724 48.4564 0 48.4724 2 2 0 2 1 0 0 37.2156 37.2156 92.4339 0 PROCESSED 57549.4081018518 2016-06-10 09:47:40 55531 2010-12-01 00:00:00 55162.1616319445 2009-11-27 03:52:45 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040053 We propose 40 and 80 ksec observations of the central and offset regions of Abell 1246, respectively, to study the temperature and mass profiles out to the virial radius. This cluster is moderately distant (z=0.1902), and relaxed system (kT=5.7 keV), with a diameter of about 20'. The low background of the XIS instrument will enable us to observe the region around the virial radius. The dentity and temperature of ICM around the virial radius should directly reflect the process of gas infall and heating. The correct temperature curve is also vital to determine the gravitational mass distribution. EXTRAGALACTIC DIFFUSE SOURCES 8 B KOSUKE SATO JAP 4 AO4 MASS AND TEMPERATURE PROFILES OF THE RELAXED CLUSTER A1246 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804028010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '804028010'

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