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 3C390.3_VICINITY_1 276.9861 79.7253 277.865171 79.689308 84.608267 76.703493 111.37115096 27.70478895 240.0064 56607.4234953704 2013-11-11 10:09:50 56608.4910648148 2013-11-12 11:47:08 808046010 57.71 50 57.71 57.72 0 57.7141 2 2 0 2 1 0 0 52.9408 52.9408 92.2319 1 PROCESSED 57613.2938425926 2016-08-13 07:03:08 56991 2014-11-30 00:00:00 56625.6961458333 2013-11-29 16:42:27 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080060 We propose for observations of the vicinities of 3C 390.3 and Fairall 9, in order to constrain the origins of 'excess' emission in the soft X-ray diffuse background observed with Suzaku and to confirm its possible relation to high velocity clouds (HVCs). We have been observing blank-skies in many directions and studying a oxygen emission from the Galactic halo. Intensities of the emission show a uniform value in most of directions; however in some directions we can see an excess, which possibly originate to a blob-like high density gas and/or a distribution of HVCs. By conducting a joint analysis of absorption and emission lines, we can characterize the roots of the excess emission. Moreover, the joint analysis even constraints a density of the origins, which has never been done until now. EXTRAGALACTIC DIFFUSE SOURCES 8 C KAZUHIRO SAKAI JAP 8 AO8 DO HIGH VELOCITY CLOUDS HEAT THE HALO OF OUR GALAXY? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/808046010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '808046010'

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