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 4U 0614+091 94.2788 9.1363 93.59351 9.155405 94.360649 -14.24001 200.87717258 -3.36522944 89.7995 56579.4227314815 2013-10-14 10:08:44 56580.8314351852 2013-10-15 19:57:16 408009010 33.687 60 33.687 34.6474 0 34.9366 3 4 0 4 1 0 0 57.7016 57.7016 121.6639 0 PROCESSED 57612.9715393518 2016-08-12 23:19:01 57144 2015-05-02 00:00:00 56601.6144791667 2013-11-05 14:44:51 3.0.22.44 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080028 We propose an Suzaku observation of LMXB 4U 0614+091 for the study of Neutron Star Binary (NSB) in the low/hard state. An aim of this observation is to reveal a physical model of the NSB low/hard state in a same analogy of Black-Hole Binary (BHB) low/hard state. In the BHB Cyg X-1, the spectra in low/hard state radiate from a cool accretion disk and a hot comptonizing corona. A spectra of NS in low/hard state would have the same structure as Cyg X-1, but it is hard to study the fine structure of the spectra because of low luminosity. Suzaku can determine the low temperature of the disk and the high temperature of the corona, thanks to wide-band and high sensitivity detectors: XIS/BI and HXD. This observation is important for an unified model between BHB and NSB. GALACTIC POINT SOURCES 4 B SATOSHI SUGITA JAP 8 AO8 THE SPECTRAL STUDY OF LMXB 4U 0614+091 IN THE LOW/HARD STATE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/408009010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '408009010'

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