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 | 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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