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 A2256 256.0138 78.7112 256.73222 78.776756 102.386288 77.234603 111.08264828 31.72462704 207.9671 54049.8560069445 2006-11-10 20:32:39 54052.0834722222 2006-11-13 02:00:12 801061010 95.5111 100 95.5111 95.5111 0 95.5111 2 2 0 2 1 0 0 103.5789 103.5789 192.4418 4 PROCESSED 57536.1203009259 2016-05-28 02:53:14 54456 2007-12-22 00:00:00 54089.4338425926 2006-12-20 10:24:44 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010139 A2256 is a nearby (z=0.058) rich cluster with strong X-ray emission. The cluster has variety of indications of a on-going merger; two peaks separated by 3.5 arcmin are clearly visible near the center of X-ray emission, gas temperature map show sub structure and a cold front etc. The velocity distribution of member galaxies also exhibits two or three sub groups in this cluster. We measure the bulk motion of the hot gas using Suzaku XIS, in particular, about 2000km/s velocity difference between the main-cluster and the sub-cluster is the target. We also aim to search for hard X-ray emission claimed by previous missions with Suzaku HXD. EXTRAGALACTIC DIFFUSE SOURCES 8 C KIYOSHI HAYASHIDA JAP 1 AO1 BULK MOTION AND NON THERMAL PROCESS IN THE MERGING CLUSTER A2256 XIS N https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801061010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801061010'

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