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 | L139_B-32 | 28.093 | 28.6837 | 27.38183 | 28.437322 | 36.368533 | 16.024453 | 138.75887563 | -32.3084393 | 253.9538 | 55569.4091319444 | 2011-01-08 09:49:09 | 55571.3188541667 | 2011-01-10 07:39:09 | 505044010 | 84.0041 | 80 | 84.0041 | 84.0041 | 0 | 84.0041 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 79.0377 | 79.0377 | 164.9839 | 0 | PROCESSED | 57600.6057175926 | 2016-07-31 14:32:14 | 55962 | 2012-02-05 00:00:00 | 55595.2037615741 | 2011-02-03 04:53:25 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050064 | Suzaku measurements of the large scale variation of the Halo emission surrounding our Galaxy are proposed. To minimize the local emission and absorption structure, we selected three pointings toward the anti-center region (l=140) of the Galactic latitude between-20 and -40. | GALACTIC DIFFUSE EMISSION | 5 | C | NORIKO YAMASAKI | JAP | 5 | AO5 | STRUCTURE OF THE GALACTIC HALO EMISSION TOWARD THE ANTI-CENTER REGION | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505044010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505044010'
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