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 PULSAR/PWN 1 | 128.7701 | -45.1981 | 128.348103 | -45.024538 | 153.316878 | -60.401286 | 263.5414959 | -2.83747227 | 337.9628 | 53926.0492592593 | 2006-07-10 01:10:56 | 53927.7841782407 | 2006-07-11 18:49:13 | 501109010 | 60.2913 | 60 | 60.3446 | 60.2913 | 60.3313 | 60.3233 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 52.6899 | 52.6899 | 149.8659 | 1 | PROCESSED | 57534.9239699074 | 2016-05-26 22:10:31 | 54401 | 2007-10-28 00:00:00 | 53942.4588078704 | 2006-07-26 11:00:41 | 3.0.22.43 | 5 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 014211 | The nature of Vela X, the radio-bright central region of the Vela SNR, has remained a mystery for three decades. Particulary puzzling is the brightest filament of Vela X. It has an apparent X-ray counterpart which was thought to be the jet of the Vela pulsar energizing the Vela X complex. This seemingly straightforward interpretation has been ruled out by the Chandra discovery of the true pulsar jets. To elucidate the nature of the filament and the Vela X complex and their connection to the Vela pulsar, we propose spatially-resolved spectroscopy of the radio/X-ray filament with XIS. Simultaneously, we will measure the spectra of the Vela pulsar and PWN between 10 and 600 keV and perform phase-resolved spectroscopy of the pulsar in the 20-50 keV band. | GALACTIC DIFFUSE EMISSION | 5 | B | OLEG KARGALTSEV | KOJI MORI | USJ | 1 | AO1 | THE ORIGIN OF VELA X: CONNECTION TO THE PULSAR | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/501109010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '501109010'
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