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 GALACTICDISC3-2 16.1096 72.7817 15.228315 72.513728 58.016186 57.534015 123.90816526 9.93459858 241.5401 55216.0250115741 2010-01-20 00:36:01 55217.5772685185 2010-01-21 13:51:16 504039010 73.5282 70 73.5282 73.5282 0 73.5282 2 2 0 2 1 0 0 54.648 54.648 134.1058 1 PROCESSED 57550.3049884259 2016-06-11 07:19:11 55602 2011-02-10 00:00:00 55236.1178240741 2010-02-09 02:49:40 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 040097 To elucidate the vertical structure of the yet-not-understood excess soft X-ray emission from the galactic disk, we propose to observe two offset directions from the plane along l = 123 degree. We expect the spectra contains the 0.75 keV emission component which we discovered in the energy spectra of two midplane observations. The proposed observations will strongly constrain the nature of the sources which are responsible for the excess emission, in particular the vertical distribution in the Galaxy. GALACTIC DIFFUSE EMISSION 5 C SHUNSUKE KIMURA JAP 4 AO4 STUDY OF SOFT X-RAY DIFFUSE EMISSION FROM THE GALACTIC DISK: VERTICAL STRUCTURE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504039010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '504039010'

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