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 | A3391&A3395 FILAMENT | 96.6913 | -54.1225 | 96.432969 | -54.090694 | 107.900065 | -77.146986 | 262.85175229 | -25.18315788 | 316.4875 | 56791.0860532407 | 2014-05-14 02:03:55 | 56792.4794328704 | 2014-05-15 11:30:23 | 809033010 | 88.6134 | 92 | 88.6134 | 88.6134 | 0 | 88.6134 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 15.2448 | 15.2448 | 23.346 | 0 | PROCESSED | 57615.0916319445 | 2016-08-15 02:11:57 | 57227 | 2015-07-24 00:00:00 | 56861.4967361111 | 2014-07-23 11:55:18 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 090082 | To investigate hot gas properties of a large scale filament, we propose Suzaku observation (92 ks) of a filamentary structure between Abell 3391 and Abell 3395. A3391 and A3395 are located in Horologium supercluster and expected to be in an initial phase of a cluster merger. With Suzaku fs high sensitivity observation, we will (i) determine the physical conditions of IntraCluster Medium by measuring the temperature and density distribution, (ii) unveil the origin of the filamentary structure from distribution of abundance, pressure and entropy. Our study will reveal the formation history of the filament and provide a useful information for the future Sunyaev-Zeldovich effect observations. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | B | YOSHITAKA ISHISAKI | JAP | 9 | AO9 | INVESTIGATION OF THE ORIGIN OF THE FILAMENTARY STRUCTURE BETWEEN ABELL 3391 AND ABELL 3395 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/809033010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '809033010'
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