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 NGC 5044 NORTH 30' 199.0992 -15.8941 198.433238 -15.630477 203.627041 -7.241957 311.67530339 46.55349501 110.0017 55220.5889814815 2010-01-24 14:08:08 55222.2571064815 2010-01-26 06:10:14 804013010 62.8482 60 62.8562 62.8482 0 62.8562 2 2 0 2 1 0 0 44.5926 44.5926 144.0998 1 PROCESSED 57550.396099537 2016-06-11 09:30:23 55602 2011-02-10 00:00:00 55235.338587963 2010-02-08 08:07:34 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040013 Why groups of galaxies contain smaller amount of metals than clusters of galaxies? To study metal sysnthesis history of galaxies in groups, we propose to observe two offset pointings of the NGC 5044 group and HCG 62 to derive metal distribution of intragroup medium up to 0.5 r180. Due to its low background, Suzaku enables us to study regions at low surface brightness. EXTRAGALACTIC DIFFUSE SOURCES 8 C KYOKO MATSUSHITA JAP 4 AO4 METAL MASS TO LIGHT RATIOS OF GROUPS OF GALAXIES UP TO 0.5R180 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/804013010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '804013010'

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