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 ESO3060170 OFFSET 85.0343 -41.2366 84.63691 -41.261684 81.30371 -64.529199 246.8664627 -30.36071331 321.0164 55326.497025463 2010-05-10 11:55:43 55327.7204166667 2010-05-11 17:17:24 805076010 78.6782 80 78.6782 78.6862 0 78.6862 2 2 0 2 1 0 0 69.7827 69.7827 105.6858 1 PROCESSED 57551.4828240741 2016-06-12 11:35:16 55707 2011-05-26 00:00:00 55341.5427893518 2010-05-25 13:01:37 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051513 We propose 30 and 80 ksec observations of the X-ray brightest fossil group, ESO 3060170. The target pointings will reach to 75% of the virial radius from the center of the galaxy, in order to determine the temperature and metal abundances of group gas at large radii. This will allow us to determine the radial profiles of the gaseous iron mass to stellar light ratio, the relative distributions of ejecta from SN Ia and SN II, the entropy, the total mass to light ratio, and the dark matter concentration for this fossil group. The energy resolution and low background of the XIS instrument are crucial for this study, which will help constrain the evolutional history of this fossil group and tell us how fossil groups relate to normal groups and clusters. EXTRAGALACTIC DIFFUSE SOURCES 8 B YUANYUAN SU USA 5 AO5 HOW DO FOSSIL GROUPS OF GALAXIES DIFFER FROM NORMAL GROUPS? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/805076010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '805076010'

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