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 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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