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 A2052_GALACTIC_1 225.6293 8.2927 225.017778 8.488428 220.521255 24.436359 7.81905694 53.73503279 292.5625 54295.7150810185 2007-07-14 17:09:43 54296.5765509259 2007-07-15 13:50:14 802038010 33.7334 30 33.7334 33.7334 0 33.7334 1 1 0 1 1 0 0 30.5272 30.5272 74.4239 1 PROCESSED 57539.2674305556 2016-05-31 06:25:06 54709 2008-08-31 00:00:00 54339.4114583333 2007-08-27 09:52:30 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 020119 We propose observations of Galactic foreground emission around clusters of galaxies observed in the SWG or AO1 phase. Since the Galactic emission level is comparable to the cluster one in the cluster outskirts, spatial fluctuation of the Galactic emission would lead to a large systematic uncertainty in determining the cluster emission. To exclude the uncertainty, offset-pointing observations of the clusters are useful. We selected six clusters, with priority order, for which the offset-pointing is essential. Note that each 20--40 ks observation can sufficiently determine the Galactic emission level. EXTRAGALACTIC DIFFUSE SOURCES 8 B YOH TAKEI JAP 2 AO2 DETERMINING ACCURATE FOREGROUND GALACTIC EMISSION AROUND CLUSTERS OF GALAXIES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/802038010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '802038010'

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