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
|
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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'
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