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 HCG62_W 192.9973 -9.0837 192.347013 -8.812069 195.480643 -3.238715 303.16227701 53.78780217 292.9782 55405.1509953704 2010-07-28 03:37:26 55406.9773611111 2010-07-29 23:27:24 805031010 66.947 60 66.955 66.955 0 66.947 2 2 0 2 1 0 0 52.9972 52.9972 157.7758 1 PROCESSED 57552.8094675926 2016-06-13 19:25:38 55808 2011-09-04 00:00:00 55441.3150925926 2010-09-02 07:33:44 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 050034 We propose offset observations of groups of galaxies to study the metal distributions up to ~0.5 times of the virial radius. Metal mass to galaxy light ratios (MLRs) for groups are much smaller than those for clusters of galaxies. In order to solve the problem which is important to understand the chemical history of the universe, we need much information of the metal abundance and distributions to the outer region of the groups. Suzaku firstly enable us to measure the metals to such an outer region of groups. EXTRAGALACTIC DIFFUSE SOURCES 8 B KOSUKE SATO JAP 5 AO5 SEARCH FOR THE METAL DISTRIBUTIONS OF GROUPS OF GALAXIES TO 0.5 R180 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805031010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805031010'

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