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 RXCJ0013.2-4905 3.3206 -49.1017 2.696864 -49.379799 337.855034 -45.122753 318.93482177 -66.82406097 263.5597 55565.2569328704 2011-01-04 06:09:59 55565.4036689815 2011-01-04 09:41:17 805023010 8.432 10 8.432 8.432 0 8.432 1 1 0 1 0 0 0 0 0 0 0 PROCESSED 57600.5421875 2016-07-31 13:00:45 56016 2012-03-30 00:00:00 55627.5157638889 2011-03-07 12:22:42 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 050021 We propose Suzaku observations of 5 X-ray luminous clusters of galaxies at z~0.4 that were discovered in the flux-limited REFLEX2 survey. Since some of the targets are to be observed in the AO4, we request an additional exposure for the remaining clusters to complete the program. With a short exposure time of 10 ks per cluster, we can determine the temperature of each cluster with 10% accuracy. This significantly improves the determination of the evolution of the luminosity-temperature relation, and will also have an impact on conducting precision cosmology with cluster observations. Thanks to the high sensitivity and low background, this study is carried out most efficiently by Suzaku. EXTRAGALACTIC DIFFUSE SOURCES 8 C NAOMI OTA JAP 5 AO5 LUMINOSITY-TEMPERATURE RELATION OF GALAXY CLUSTERS AT Z~0.4 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805023010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805023010'

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