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 PKS 0745-191 116.6543 -19.2063 116.100315 -19.082609 123.362638 -39.608686 236.25768919 2.88874721 294.0002 54231.8221180556 2007-05-11 19:43:51 54232.5001041667 2007-05-12 12:00:09 802062020 31.2266 30 31.2266 31.2266 0 31.2266 2 2 0 2 1 0 0 25.967 25.967 58.5739 1 PROCESSED 57538.6330208333 2016-05-30 15:11:33 54695 2008-08-17 00:00:00 54238.8889814815 2007-05-18 21:20:08 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021440 PKS 0745-191 is the X-ray brightest galaxy cluster beyond a redshift of 0.1. It has a smooth surface brightness profile and appears relaxed. Using the low background of Suzaku we will measure the temperature of the intracluster medium to the virial radius of the cluster. Its high temperature means that we will be unaffected by any loss of effective area at low energies. In addition the cluster is bright enough so that the bremsstrahlung emission will be easily detected using the PIN detector. This will allow us to search for any nonthermal component as well as accurately determining the high temperature components in the cluster. EXTRAGALACTIC DIFFUSE SOURCES 8 A ANDREW YOUNG USA 2 AO2 PKS 0745-191: THE BRIGHTEST CLUSTER BEYOND Z=0.1 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802062020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '802062020'

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