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 OFFSET 3 247.3596 39.3165 246.92934 39.424595 233.528009 59.920137 62.61707687 43.53145251 252.4737 54012.1589351852 2006-10-04 03:48:52 54012.6786921296 2006-10-04 16:17:19 801059010 25.2467 25 25.2467 25.2467 25.2467 25.2467 1 1 1 1 1 0 0 20.505 20.505 44.8879 1 PROCESSED 57535.7507291667 2016-05-27 18:01:03 54735 2008-09-26 00:00:00 54025.4730092593 2006-10-17 11:21:08 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/ver3.0/801059010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '801059010'

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