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 CYGNUS_LOOP_P19 311.8094 30.0818 311.288879 29.89716 325.768852 45.764417 73.00862935 -8.2918477 237.4997 54087.3411805556 2006-12-18 08:11:18 54087.8245833333 2006-12-18 19:47:24 501036010 18.595 17 18.595 18.595 0 18.595 2 2 0 2 1 0 0 18.355 18.355 41.7559 0 PROCESSED 57536.3627199074 2016-05-28 08:42:19 54744 2008-10-05 00:00:00 54096.1443171296 2006-12-27 03:27:49 3.0.22.43 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 010052 We propose to observe a large part of the Cygnus Loop. The objective is to study the plasma of C and N that can not be measured without the BI of the XIS. The limb regoin showing C and N lines as well as O line. The central part showing strong Si and S lines is believed to be a fossil of the explosion. The fossil contains quite a lot of metal with relatively low density. Studying the C and N lines, we can evaluate O lines from the central part of the Loop. The observation should be done as soon as possible before C and N lines can not be seen due to the degradation of the XIS. GALACTIC DIFFUSE EMISSION 5 A HIROSHI TSUNEMI JAP 1 AO1 OBSERVATION OF THE CYGNUS LOOP XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501036010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501036010'

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