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_P5 312.5567 31.1701 312.040041 30.982753 327.230821 46.520779 74.2739834 -8.12038976 239.9995 54419.3201388889 2007-11-15 07:41:00 54420.0627777778 2007-11-16 01:30:24 501016010 28.4062 22 28.4062 28.4062 0 28.4062 2 2 0 2 1 0 0 25.37 25.37 64.1559 1 PROCESSED 57540.538900463 2016-06-01 12:56:01 54798 2008-11-28 00:00:00 54430.4318865741 2007-11-26 10:21:55 3.0.22.43 2 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/ver3.0/501016010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501016010'

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