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 RADIO_ARC_SOUTH 266.9853 -29.0688 266.190093 -29.052225 267.342882 -5.6555 0.15000746 -0.5026703 267.1998 56186.0290509259 2012-09-16 00:41:50 56188.8203472222 2012-09-18 19:41:18 507016010 103.472 100 103.472 103.472 0 103.472 2 2 0 2 1 0 0 89.1906 89.1906 241.1319 4 PROCESSED 57607.146875 2016-08-07 03:31:30 56668 2014-01-11 00:00:00 56303.6234490741 2013-01-11 14:57:46 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070016 The 6.4 keV emission associated with giant molecular clouds is the most prominent feature in the Galactic center region. So far, the origin has only been found and discussed in the X-ray reflection process. We propose deep observation at the Radio Arc to discover the 6.4 keV emission in the particle origin, which would open the window to study the nature of the Galactic cosmic ray. GALACTIC DIFFUSE EMISSION 5 A SYUKYO RYU JAP 7 AO7 X-RAY OBSERVATION OF THE RADIO ARC -- DISCOVERY OF THE GALACTIC 6.4 KEV EMISSION IN PARTICLE ORIGIN -- XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507016010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '507016010'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏