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 GK PER 52.8052 43.8974 51.953057 43.727495 61.505862 24.068527 150.96310366 -10.10758836 250.0842 57086.777037037 2015-03-05 18:38:56 57090.7709606482 2015-03-09 18:30:11 409018020 182.886 140 0 0 0 182.886 0 0 0 2 1 0 0 134.9166 134.9166 344.9376 0 PROCESSED 57617.786712963 2016-08-17 18:52:52 57468 2016-03-21 00:00:00 57101.0913657407 2015-03-20 02:11:34 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090055 A 140-ks observation of the magnetic cataclysmic variable GK Per is proposed. By fitting Suzaku broadband spectra using our multitemperature spectral model of the accretion column, we estimate a white dwarf mass with statistical fitting errors smaller than 5%. The estimated mass will be compared with one obtained from the optical lightcurve fitting method developed and applied by Hachisu and Kato in a series of papers. GK Per is the only known magnetic cataclysmic variable which underwent classical nova explosion (in 1901), and both the mass estimation methods can be applied. Cross-validated WD mass estimation methods will be of importance in studying massive white dwarfs in accretion systems, in relation with the progenitor of type Ia supernovae. GALACTIC POINT SOURCES 4 A TAKAYUKI YUASA JAP 9 AO9 CROSS VALIDATION OF WHITE DWARF MASS ESTIMATION METHODS XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/409018020/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '409018020'

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