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 G278.0+12.4 158.151 -43.7043 157.610146 -43.446336 182.388463 -47.807278 278.01040448 12.3478226 304.0284 56102.6152199074 2012-06-24 14:45:55 56102.9842476852 2012-06-24 23:37:19 507067010 18.996 17.5 19.004 18.996 0 19.004 1 1 0 1 1 0 0 16.442 16.442 31.8799 0 PROCESSED 57605.7438078704 2016-08-05 17:51:05 56582 2013-10-17 00:00:00 56219.6572916667 2012-10-19 15:46:30 3.0.22.44 3 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/ver3.0/507067010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '507067010'

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