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 W63 304.8117 45.7821 304.405742 45.623994 328.881818 62.294552 82.4091518 5.43831098 57.9996 57171.5134837963 2015-05-29 12:19:25 57172.616712963 2015-05-30 14:48:04 510025010 42.7003 150 44.302 44.606 0 42.7003 2 2 0 2 1 0 0 13.7747 13.7747 92.7739 0 PROCESSED 57618.8028703704 2016-08-18 19:16:08 57636 2016-09-05 00:00:00 57260.7216898148 2015-08-26 17:19:14 3.0.22.44 5 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 101315 We propose to conduct a deep Suzaku observation of the X-ray bright central portion of the Galactic supernova remnant (SNR) W63 (G82.2+5.3). This SNR belongs to a class of objects known as mixed-morphology SNRs (MMSNRs) that feature a shell-like radio morphology with a center-filled thermal X-ray morphology: the origin of these contrasting morphologies for these SNRs remains unknown. Our proposed Suzaku observation of this SNR will investigate the putative overabundances of such elements as magnesium, silicon and sulfur (as reported in a previous analysis of an ASCA observation of W63) as well as search for evidence of over-ionization conditions in the X-ray emitting plasma, as has been reported for other MMSNRs. GALACTIC DIFFUSE EMISSION 5 C THOMAS PANNUTI USA 10 AO10 A SUZAKU OBSERVATION OF THE GALACTIC SUPERNOVA REMNANT W63 (G82.2+5.3) XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/510025010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '510025010'

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