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 | 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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