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 | ARC_BACKGROUND | 39.2055 | -35.7283 | 38.691278 | -35.944876 | 20.761341 | -47.725244 | 240.48717091 | -66.02341726 | 233.8071 | 54830.2554861111 | 2008-12-30 06:07:54 | 54835.3468055556 | 2009-01-04 08:19:24 | 503104010 | 201.8775 | 140 | 201.9575 | 201.8775 | 0 | 201.9815 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 5.5028 | 5.5028 | 14.506 | 0 | PROCESSED | 57545.0672685185 | 2016-06-06 01:36:52 | 55328 | 2010-05-12 00:00:00 | 54851.4354166667 | 2009-01-20 10:27:00 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031235 | Aside from the lengthy bright arcs in the northern sky, few X-ray bright, high latitude regions are understood. Yet, studying this gas is important for understanding the Galactic halo. Here, we propose to study a medium-sized (~7 degree) bright feature in the southern sky. The feature is arc-shaped, suspiciously like the edge of a hot bubble. We propose to make Suzaku observations of the arc and nearby background. With them and an existing Suzaku observation, we will be able to determine the thermal properties of the arc plasma and if the arc is the bright limb of a hot bubble. | GALACTIC DIFFUSE EMISSION | 5 | B | ROBIN SHELTON | USA | 3 | AO3 | A CLOSER LOOT AT HOT HALO GAS: A SUZAKU STUDY OF AN X-RAY BRIGHT ARC | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503104010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503104010'
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