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 PUP A : BEK 125.942 -42.9405 125.511174 -42.777913 147.596211 -59.401563 260.51799115 -3.16426215 276.3687 53842.2933449074 2006-04-17 07:02:25 53842.5807407407 2006-04-17 13:56:16 501086010 16.0913 15 16.0913 16.0993 16.0913 16.0913 1 1 1 1 1 0 0 9.6985 9.6985 24.797 0 PROCESSED 57533.4850115741 2016-05-25 11:38:25 54401 2007-10-28 00:00:00 53906.8467708333 2006-06-20 20:19:21 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/ver3.0/501086010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '501086010'

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