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 | CYGNUS_LOOP_P17 | 312.199 | 30.014 | 311.677424 | 29.82795 | 326.178147 | 45.573278 | 73.16561663 | -8.59879153 | 61.9999 | 53877.7613657407 | 2006-05-22 18:16:22 | 53878.0446064815 | 2006-05-23 01:04:14 | 501034010 | 14.1953 | 14 | 14.1993 | 14.2033 | 14.1993 | 14.1953 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 14.8231 | 14.8231 | 24.464 | 0 | PROCESSED | 57534.3944328704 | 2016-05-26 09:27:59 | 54394 | 2007-10-21 00:00:00 | 53926.1395833333 | 2006-07-10 03:21:00 | 3.0.22.43 | 4 | 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 | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501034010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '501034010'
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