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 | SMC DIFFUSE 1 | 13.0188 | -72.8206 | 12.579325 | -73.092182 | 312.037754 | -64.558836 | 302.86615918 | -44.30756989 | 221.6864 | 53687.4452893518 | 2005-11-13 10:41:13 | 53688.2231944445 | 2005-11-14 05:21:24 | 500011010 | 46.7789 | 50 | 46.7789 | 46.7869 | 46.7869 | 46.7869 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 47.8684 | 47.8684 | 67.1999 | 0 | PROCESSED | 57527.967337963 | 2016-05-19 23:12:58 | 54247 | 2007-05-27 00:00:00 | 54038.3531712963 | 2006-10-30 08:28:34 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001049 | We propose to use Suzaku XIS to observe regions of diffuse emission in the Magellanic Clouds. The diffuse component was identified by ROSAT PSPC observations, but has never been studied with a true spectroscopic instrument. Suzaku is well-matched to the angular size and expected temperature of the regions of diffuse emission in the LMC. Not only will such observations give a clear view of the temperature structure of this gas, they will provide a direct measurement of ambient abundances in the Clouds. | GALACTIC DIFFUSE EMISSION | 5 | A | UNA HWANG | JAP | 0 | SWG | DIFFUSE EMISSION IN THE MAGELLANIC CLOUDS | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500011010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '500011010'
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