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 | PUP A : INTERIOR | 125.5916 | -42.8951 | 125.161363 | -42.733897 | 147.106586 | -59.478577 | 260.333956 | -3.34905821 | 276.8883 | 53842.5813541667 | 2006-04-17 13:57:09 | 53842.9127199074 | 2006-04-17 21:54:19 | 501088010 | 20.2709 | 20 | 20.2924 | 20.2949 | 20.2789 | 20.2709 | 1 | 1 | 1 | 1 | 1 | 0 | 0 | 19.9519 | 19.9519 | 28.6239 | 0 | PROCESSED | 57533.5042476852 | 2016-05-25 12:06:07 | 54401 | 2007-10-28 00:00:00 | 53906.8948611111 | 2006-06-20 21:28:36 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 011246 | We propose to use Suzaku XIS to locate X-ray emitting oxygen ejecta in Puppis A, a middle-aged oxygen-rich supernova remnant. The ejecta are seen in optical emission, and enhanced X-ray oxygen line emission is detected but not localized. Puppis A has never been surveyed with an adequate combination of bandpass and spectral resolution, and Suzaku offers a unique capability for providing such observations. The line emission will also provide diagnostics of plasma conditions throughout the remnant through their intensity ratios in addition to conventional broadband spectral fits. We propose five fields to cover the eastern portion of the remnant where the oxygen ejecta are expected to be present. | GALACTIC DIFFUSE EMISSION | 5 | A | UNA HWANG | USA | 1 | AO1 | MAPPING OXYGEN IN PUPPIS A | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501088010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '501088010'
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