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 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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