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 | VELA FRAGMENT E | 119.9016 | -44.3755 | 119.497107 | -44.237549 | 140.837519 | -62.635644 | 259.34445053 | -7.61175769 | 281.1138 | 54582.309224537 | 2008-04-26 07:25:17 | 54583.7849421296 | 2008-04-27 18:50:19 | 503096010 | 79.2004 | 70 | 79.2189 | 79.2004 | 0 | 79.2324 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 84.2529 | 84.2529 | 127.4899 | 1 | PROCESSED | 57542.4144212963 | 2016-06-03 09:56:46 | 54960 | 2009-05-09 00:00:00 | 54594.2098842593 | 2008-05-08 05:02:14 | 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/ver3.0/503096010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '503096010'
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