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 | FG25 | 234.9579 | 30.7058 | 234.452539 | 30.866616 | 221.876556 | 48.458584 | 48.772653 | 53.18955534 | 294.6599 | 56136.7541898148 | 2012-07-28 18:06:02 | 56137.0821875 | 2012-07-29 01:58:21 | 807049010 | 10.6393 | 10 | 10.6393 | 10.6393 | 0 | 10.6393 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 11.074 | 11.074 | 28.3281 | 0 | PROCESSED | 57606.6807523148 | 2016-08-06 16:20:17 | 56527 | 2013-08-23 00:00:00 | 56161.2376736111 | 2012-08-22 05:42:15 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 071511 | Optical and X-ray measurements of fossil groups/clusters (FGs) suggest that they are old and relaxed systems. If FGs are assembled at higher redshift, there is enough time for intermediate-luminosity galaxies to merge, resulting in the formation of the brightest system galaxy. We carry out the first, systematic study of a large sample of FGs, the ``FOssil Group Origins'' (FOGO) based on an International Time Project at the Roque de los Muchachos Observatory. For ten FOGO FGs we propose to measure the temperature of the hot intracluster gas (ICM) and to evaluate Lx-Tx, Lopt-Tx, and sigmaV-Tx relations as compared to the non fossil systems. By combining these observations with hydrodynamical simulations we will open a new window into the study of the ICM and the nature of fossil systems. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | ELENA D'ONGHIA | USA | 7 | AO7 | SCALING RELATIONS OF FOSSIL GALAXY SYSTEMS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807049010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807049010'
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