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 | COMA OUTSKIRTS4 | 193.3444 | 28.9037 | 192.738609 | 29.174872 | 179.533604 | 31.586326 | 109.48887466 | 88.17367696 | 116.0002 | 55902.7178125 | 2011-12-07 17:13:39 | 55903.9105324074 | 2011-12-08 21:51:10 | 806023010 | 51.6563 | 50 | 51.6643 | 51.6563 | 0 | 51.6713 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 49.0198 | 49.0198 | 103.0419 | 1 | PROCESSED | 57604.0840972222 | 2016-08-04 02:01:06 | 56284 | 2012-12-23 00:00:00 | 55915.2433449074 | 2011-12-20 05:50:25 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060099 | In order to search cluster evolutions, we propose to observe high temperature cluster(about 8 keV), Coma cluster(z = 0.0231) with six pointings. Three of the field lie in the direction of the large-scale filament, and others are in the perpendicular direction, with their total exposure is 200 ks from 0.5r_180 to virial radius. Thanks to its low background, we can derive the anisotropy of temperature and density profile up to virial radius in detail, and we will search thermalization process in the cluster outskirts region. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | C | TAKUYA SATO | JAP | 6 | AO6 | STUDY OF CLUSTER EVOLUTION IN THE COMA CLUSTER OUTSKIRTS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/806023010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '806023010'
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