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 | ARC1 | 40.8605 | -42.0069 | 40.383748 | -42.218277 | 17.737941 | -53.844666 | 253.28744097 | -62.75503946 | 235.1247 | 54480.7980787037 | 2008-01-15 19:09:14 | 54482.7640509259 | 2008-01-17 18:20:14 | 502070010 | 104.3694 | 100 | 104.3774 | 104.3854 | 0 | 104.3694 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 115.4202 | 115.4202 | 169.8377 | 3 | PROCESSED | 57541.3640277778 | 2016-06-02 08:44:12 | 54860 | 2009-01-29 00:00:00 | 54490.7270717593 | 2008-01-25 17:26:59 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021222 | Outside of the largest loops in the northern sky, few X-ray bright regions in the Galactic halo are understood. Here, we propose to study of a medium sized (~10 degree) bright feature in the southern sky. The feature is arc-shaped, suspiciously like the edge of a hot bubble. We propose to make three Suzaku observations along a radial line through the arc. With them, we will be able to determine the thermal properties of the region and whether or not the plasma temperature decreases with radius from the projected center, as expected for middle aged supernova remnants. | GALACTIC DIFFUSE EMISSION | 5 | C | ROBIN SHELTON | USA | 2 | AO2 | A CLOSER LOOK AT HOT HALO GAS: AN EXAMINATION OF AN X-RAY BRIGHT ARC | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/502070010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '502070010'
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