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 | G7.6+2.0 | 268.7973 | -21.391 | 268.047539 | -21.383335 | 268.869887 | 2.045161 | 7.58937554 | 2.00788461 | 270.4016 | 56194.0843865741 | 2012-09-24 02:01:31 | 56194.4237037037 | 2012-09-24 10:10:08 | 507065010 | 16.521 | 10 | 16.529 | 16.521 | 0 | 16.5347 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 12.1603 | 12.1603 | 29.3139 | 2 | PROCESSED | 57607.1654050926 | 2016-08-07 03:58:11 | 56676 | 2014-01-19 00:00:00 | 56315.5110069444 | 2013-01-23 12:15:51 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 072014 | We propose to investigate the four brightest and most-promising RASS-detected SNR candidates. With the observations we will be able to determine if the objects are supernova remnants, and if so, measure their spectral characteristics (temperature, abundance), details of their morphology (angular size) and their expansion velocity. This study will complete previous surveys of SNR in other wavelength and provide insight into the structure and composition of the ISM. Follow-up radio continuum and linear polarization observations, and optical studies will be performed. | GALACTIC DIFFUSE EMISSION | 5 | A | TOBIAS PRINZ | EUR | 7 | AO7 | IDENTIFICATION OF X-RAY SELECTED SUPERNOVA REMNANTS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507065010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '507065010'
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