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 ABELL 2199 CENTER 247.1922 39.484 246.76294 39.592842 233.179095 60.039777 62.84241749 43.66620611 252.3681 54009.2972222222 2006-10-01 07:08:00 54009.8967361111 2006-10-01 21:31:18 801056010 24.9282 25 25.4799 24.9282 25.4799 25.4799 2 2 2 2 1 0 0 20.519 20.519 51.7939 1 PROCESSED 57535.7247453704 2016-05-27 17:23:38 54735 2008-09-26 00:00:00 54021.2246990741 2006-10-13 05:23:34 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010138 Detection of hard X-ray emission from clusters of Galaxies is one of the top goals of Suzaku. For this purpose, we propose 5 pointing observations of Abell 2199 each of which is 25 ks. Abell 2199 is one of objects from which significant hard X-ray emission have been detected by BeppoSAX PDS with 2 sigma significance level. Among them, Abell 2199 is unique in that it neither have a signature of cluster merger nor significant AGN activities. The HXD PIN detector can just covers the whole X-ray emission from Abell 2199, and determine photon index and flux of the hard component. The detection of hard X-ray emission from a relaxed cluster opens a new field of study in which particle accelerations occur generally in clusters even without energetic events like sub-cluster mergers. EXTRAGALACTIC DIFFUSE SOURCES 8 B MADOKA KAWAHARADA JAP 1 AO1 PROBING HARD X-RAY EMISSION FROM A RELAXED CLUSTER OF GALAXIES HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/801056010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801056010'

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