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 X-1 135.5377 -40.5514 135.064105 -40.353478 157.048654 -53.915556 263.06039339 3.93722667 314.5441 54634.1981134259 2008-06-17 04:45:17 54635.9043287037 2008-06-18 21:42:14 403045010 104.7096 100 104.7234 104.7096 0 104.7154 2 2 0 2 1 0 0 96.0089 96.0089 147.3899 1 PROCESSED 57542.8859375 2016-06-03 21:15:45 55010 2009-06-28 00:00:00 54644.4687847222 2008-06-27 11:15:03 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031153 We propose to observe the well-known X-ray pulsar Vela X-1 (4U0900-40) using Suzaku in order to test models for the circumstellar environment by measuring teh spectrum and searching for variability in the iron line. The line is expected to exhibit changes in intensity and centroid energy as the X-ray beam sweeps around the wind an illuminates material with varying column density, ionization state, and vleocity. In addition we will study the variability in the cyclotron feature. We will compare our observations with detailed hydrodynamical simulations of the stellar wind and its interaction with the compact object. GALACTIC POINT SOURCES 4 A TIMOTHY KALLMAN USA 3 AO3 SPECTROSCOPY OF VELA X-1 (4U0900-40) AND SEARCHES FOR PULSE PHASE VARIABILITY XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403045010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '403045010'

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