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 | TYCHO SNR HXD BKGD | 9.2173 | 64.3076 | 8.488109 | 64.032592 | 44.61366 | 53.051862 | 121.35322514 | 1.48051733 | 84.2005 | 53915.6541782407 | 2006-06-29 15:42:01 | 53916.7606944444 | 2006-06-30 18:15:24 | 500025010 | 51.0088 | 50 | 51.0088 | 51.0088 | 51.0088 | 51.0088 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 48.7224 | 48.7224 | 95.5939 | 2 | PROCESSED | 57534.8010300926 | 2016-05-26 19:13:29 | 54302 | 2007-07-21 00:00:00 | 54052.5940509259 | 2006-11-13 14:15:26 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001099 | We propose to observe Tycho's Supernova Remnant with Suzaku. The proposal has two main goals: (1) to measure the energy spectrum of the entire remnant above 10 keV with the HXD, and (2) to study the 0.5-10 keV band spectrum as a function of position with the XIS. | GALACTIC DIFFUSE EMISSION | 5 | A | JOHN HUGHES | JAP | 0 | SWG | SUZAKU STUDY OF TYCHO'S SUPERNOVA REMNANT | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/500025010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '500025010'
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