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 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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