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 SOUTHWEST 1 | 126.2671 | -48.2152 | 125.877652 | -48.051248 | 153.532268 | -63.870386 | 264.99036518 | -5.99332729 | 119.5649 | 55164.9700925926 | 2009-11-29 23:16:56 | 55165.818900463 | 2009-11-30 19:39:13 | 504063010 | 32.7331 | 30 | 32.7492 | 32.7331 | 0 | 32.7411 | 3 | 2 | 0 | 2 | 1 | 0 | 0 | 23.7674 | 23.7674 | 73.3099 | 0 | PROCESSED | 57549.6219791667 | 2016-06-10 14:55:39 | 55546 | 2010-12-16 00:00:00 | 55179.268587963 | 2009-12-14 06:26:46 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040121 | We propose 2 pointing-observations of south western part of Vela supernova remnant. Vela SNR has the largest angular size of 8 degree in diameter, so it is suitable to carry out spatial resolved spectroscopy with Suzaku. | GALACTIC DIFFUSE EMISSION | 5 | C | JUNKO HIRAGA | JAP | 4 | AO4 | X-RAY STUDY ON THE NEAREST SUPERNOVA REMNANT, VELA | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504063010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '504063010'
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