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 | 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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