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".

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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 HEN 3-1591 271.8863 -25.8981 271.110376 -25.90538 271.688765 -2.468309 5.07192211 -2.68044312 269.6421 56203.7249537037 2012-10-03 17:23:56 56204.7793981482 2012-10-04 18:42:20 407042010 51.3876 50 51.3877 51.3876 0 51.4036 4 3 0 3 1 0 0 52.3681 52.3681 91.0959 1 PROCESSED 57607.2899884259 2016-08-07 06:57:35 56592 2013-10-27 00:00:00 56226.5545601852 2012-10-26 13:18:34 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 071211 The number of symbiotic stars known to be medium energy (2-10 keV) X-ray emitters has increased markedly in the last several years. These are white dwarfs accreting from a giant mass donor, unlike the less common class of symbiotic X-ray binaries in which the accretor is a neutron star. The X-ray spectra of the white dwarf symbiotics can be used to constrain the white dwarf mass and accretion rate. Here we focus on one object, Hen 3-1591, which belongs to a rare subclass of d'-type yellow symbiotic, commonly thought to harbor a young white dwarf. Hen 3-1591 is the first of this subclass to show medium energy X-ray emission, and hence we propose a moderately deep Suzaku observation to characterize its white dwarf and the circum-binary environment. GALACTIC POINT SOURCES 4 B KOJI MUKAI USA 7 AO7 THE X-RAY EMISSION OF THE YELLOW SYMBIOTIC STAR, HEN 3-1591 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407042010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407042010'

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