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 VELA FRAGMENT C 136.2696 -44.691 135.819541 -44.490549 161.57955 -57.213344 266.51473212 1.58715492 269.3614 54580.6978703704 2008-04-24 16:44:56 54582.3056481482 2008-04-26 07:20:08 503095010 84.1167 70 84.1167 84.1167 0 84.1167 2 2 0 2 1 0 0 91.3547 91.3547 138.9018 2 PROCESSED 57542.4305439815 2016-06-03 10:19:59 54960 2009-05-09 00:00:00 54594.2480324074 2008-05-08 05:57:10 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031212 Ejecta fragments projecting from the nearby Vela supernova remnant provide a unique opportunity to examine supernova ejecta as they shock and finally merge into the interstellar medium (ISM). Fragments "A" and "D", observed with Chandra and XMM, and Fragment "B", observed with Suzaku, show strongly enhanced (but very different) abundances. These fragments are indeed ejecta, but originating in different layers of the precursor. We propose to observe two of the remaining ejecta fragments. In combination with the existing observations of Fragments A, B, and D, these data will provide a much more complete picture of the variation in ejecta fragment abundances and their interactions with the remnant shell and the surrounding ISM. GALACTIC DIFFUSE EMISSION 5 B TERRANCE GAETZ USA 3 AO3 SEARCHING FOR EJECTA IN THE VELA SUPERNOVA REMNANT FRAGMENTS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/503095010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '503095010'

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