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 GALACTIC_BULGE3 267.9488 -29.7963 267.148788 -29.784389 268.199437 -6.368042 359.95634845 -1.5962466 107.1729 55624.8013310185 2011-03-04 19:13:55 55626.2292939815 2011-03-06 05:30:11 505078010 51.2756 50 51.2756 51.2756 0 51.2756 2 2 0 2 1 0 0 39.3124 39.3124 123.3618 0 PROCESSED 57601.0957407407 2016-08-01 02:17:52 55287 2010-04-01 00:00:00 55642.1205787037 2011-03-22 02:53:38 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 056001 We propose to observe three classes of objects, which seem independent subjects, but are closely related with each others. These subjects are the Galactic center and the ridge diffuse X-rays (GCDX & GRDX), Unidentified sources (UIDHESS) found with HESS and the hard X-rays from radio faint supernova remnants (Hard SNR) found with ASCA. Our objectives are to study individual science on each subject, combined the results, and to finally approach to a unified picture on the diffuse high energy aspects in our Galaxy. GALACTIC DIFFUSE EMISSION 5 A KATSUJI KOYAMA JAP 5 AO5 SYSTEMATIC STUDY OF THE DIFFUSE HIGH ENERGY OBJECTS IN OUR GALAXY XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505078010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '505078010'

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