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 | ABELL 3395 N | 96.6064 | -54.3394 | 96.351199 | -54.307997 | 107.885857 | -77.369468 | 263.07484149 | -25.27687082 | 220.9999 | 56329.4933449074 | 2013-02-06 11:50:25 | 56330.7758564815 | 2013-02-07 18:37:14 | 807031010 | 46.9751 | 45 | 46.98 | 46.9751 | 0 | 46.9861 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 42.0083 | 42.0083 | 110.7998 | 2 | PROCESSED | 57610.5772337963 | 2016-08-10 13:51:13 | 56715 | 2014-02-27 00:00:00 | 56349.5329398148 | 2013-02-26 12:47:26 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070072 | We propose observations of north and south regions of merging cluster Abell 3395 (A3395), which have high temperature intracluster gas, with each exposure time of 45 ks in order to obtain a detailed temperature distribution in these regions. A3395 is a very complex system, which is composed of three subclusters (A3395 NE, SW and NW) and a bridge structure which joining the A3395 NE and NW subclusters. We can obtain the information of the merging direction and the structure formation in A3395 from the detailed high-accuracy temperature distribution. In addition, it might be possible to get from this observations some information of the hot gas filling the supercluster which includes A3395. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | NOBUHIRO TANAKA | JAP | 7 | AO7 | INVESTIGATION OF TEMPERATURE DISTRIBUTION OF OUTER REGIONS IN MERGING CLUSTER ABELL 3395 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807031010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807031010'
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