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 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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