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 | G18.8+0.3 | 275.9435 | -12.3781 | 275.241856 | -12.405238 | 275.902948 | 10.940788 | 18.78460262 | 0.39706413 | 83.4994 | 55994.9180324074 | 2012-03-08 22:01:58 | 55996.1598958333 | 2012-03-10 03:50:15 | 506051010 | 52.0205 | 50 | 52.0205 | 52.0285 | 0 | 52.0365 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 44.882 | 44.882 | 107.2639 | 1 | PROCESSED | 57604.8541435185 | 2016-08-04 20:29:58 | 56382 | 2013-03-31 00:00:00 | 56016.6717708333 | 2012-03-30 16:07:21 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 061311 | We propose a 50 ks exploratory observation of an interesting first-quadrant supernova remnant, G18.8+0.3, for which radio-continuum and CO data indicate interaction with a molecular cloud. Prior X-ray studies are limited to a 14 ks ROSAT PSPC observation producing about 500 counts. We expect about 12,000 counts with Suzaku, which should permit basic characterization of the spectrum and morphology of X-rays: shell-type, mixed-morphology (central thermal emission) or even composite (central PWN). Spectral analysis will allow us to determine or estimate shock speed, age, ambient density, and swept-up mass. As more middle-aged remnants are found to have unusual properties such as GeV-TeV emission, the study of objects like G18.8+0.3 assumes greater importance. | GALACTIC DIFFUSE EMISSION | 5 | C | STEPHEN REYNOLDS | USA | 6 | AO6 | G18.8+0.3: A SUPERNOVA REMNANT WITH STRONG MOLECULAR INTERACTION | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506051010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506051010'
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