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 | 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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