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 | LOOP 2 L=356.33 | 263.4562 | -31.667 | 262.645073 | -31.633306 | 264.364444 | -8.35361 | 356.33349006 | 0.70266893 | 94.2779 | 54916.2757060185 | 2009-03-26 06:37:01 | 54917.0786921296 | 2009-03-27 01:53:19 | 503023010 | 31.1527 | 40 | 31.1527 | 31.1527 | 0 | 31.1527 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 28.2346 | 28.2346 | 69.3699 | 0 | PROCESSED | 57545.9012615741 | 2016-06-06 21:37:49 | 55330 | 2010-05-14 00:00:00 | 54930.234849537 | 2009-04-09 05:38:11 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030023 | NANTEN telescope discovered huge molecular loops in the galactic center region. The model that the huge loops is due to magnetic buoyancy caused by the Parkey instability is proposed. The loops size is 12 order of magnitude larger than the solar loops, but the physics would be common. X-ray emission from shock heated and/or accelerated particles would be expected at the foot point of the loops. We propose an X-ray observation at the foot point of the molecular loop with Suzaku and investigate the magnetic activity in the galactic scale. | GALACTIC DIFFUSE EMISSION | 5 | C | SHIGEO YAMAUCHI | JAP | 3 | AO3 | SUZAKU OBSERVATION OF MOLECULAR LOOPS IN THE GALACTIC CENTER | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503023010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503023010'
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