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 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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