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 A2255_NW 258.0206 64.3236 257.946874 64.381524 198.635574 84.547798 94.26240936 34.95584628 200.0017 56613.0157060185 2013-11-17 00:22:37 56613.9467476852 2013-11-17 22:43:19 808039010 43.7688 40 43.7688 43.7688 0 43.7688 2 2 0 2 1 0 0 41.8557 41.8557 80.4121 0 PROCESSED 57613.3414814815 2016-08-13 08:11:44 56991 2014-11-30 00:00:00 56625.6806481482 2013-11-29 16:20:08 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080047 We propose to obtain high-quality X-ray spectra of two subcluster regions in A2255 aiming at detection of supersonic motion of the intracluster gas. Previous optical and X-ray observations suggest that A2255 is indeed in the process of merging and subclusters have high velocities relative to the main cluster. Utilizing the high-sensitivity Suzaku spectroscopy, the line-of-sight velocity of the X-ray emitting gas can be measured from the Doppler shift of iron-K lines. With additional 40ks/80ks observations of the NW/SE subclusters, we expect to detect significant bulk velocities for the first time in this cluster. This will enhance our understanding of the 3-dimensional structure of the object including line-of-sight gas velocities and the cluster dynamical evolution. EXTRAGALACTIC DIFFUSE SOURCES 8 C HIROKO YOSHIDA JAP 8 AO8 MAPPING GAS MOTIONS IN THE MERGING CLUSTER A2255 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808039010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '808039010'

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