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 | A1246_OFF | 171.128 | 21.4191 | 170.469781 | 21.693883 | 163.239064 | 16.135503 | 224.30142226 | 69.41574013 | 120.0005 | 55163.0212152778 | 2009-11-28 00:30:33 | 55164.9606365741 | 2009-11-29 23:03:19 | 804029010 | 80.3804 | 80 | 80.3964 | 80.3804 | 0 | 80.391 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 55.158 | 55.158 | 167.5558 | 1 | PROCESSED | 57549.6578472222 | 2016-06-10 15:47:18 | 55549 | 2010-12-19 00:00:00 | 55181.239849537 | 2009-12-16 05:45:23 | 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/ver3.0/804029010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '804029010'
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