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_SE 258.2963 63.8192 258.210545 63.875842 203.735886 84.382935 93.63129587 34.92006939 200.0025 56613.9474537037 2013-11-17 22:44:20 56615.3084953704 2013-11-19 07:24:14 808040010 64.733 60 64.741 64.741 0 64.733 2 2 0 2 1 0 0 64.8865 64.8865 117.5879 1 PROCESSED 57613.3519097222 2016-08-13 08:26:45 57029 2015-01-07 00:00:00 56653.6890046296 2013-12-27 16:32:10 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/ver3.0/808040010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '808040010'

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