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 COMA OUTSKIRTS2 195.8535 28.5112 195.253601 28.779358 182.053697 32.234375 61.20140467 87.01280614 116.0004 55901.4349189815 2011-12-06 10:26:17 55901.9223842593 2011-12-06 22:08:14 806021010 20.3577 20 20.3617 20.3577 0 20.3648 2 2 0 2 1 0 0 19.1946 19.1946 42.114 0 PROCESSED 57604.0414351852 2016-08-04 00:59:40 56282 2012-12-21 00:00:00 55914.2609375 2011-12-19 06:15:45 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/ver3.0/806021010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '806021010'

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