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 | AQL X-1 | 287.8182 | 0.5791 | 287.179926 | 0.495378 | 289.379323 | 22.828874 | 35.71383379 | -4.14703266 | 264.9589 | 54382.2112384259 | 2007-10-09 05:04:11 | 54382.6877893518 | 2007-10-09 16:30:25 | 402053030 | 19.7117 | 15 | 19.7197 | 19.7277 | 0 | 19.7117 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 17.5522 | 17.5522 | 41.162 | 0 | PROCESSED | 57540.2157291667 | 2016-06-01 05:10:39 | 54770 | 2008-10-31 00:00:00 | 54402.5719328704 | 2007-10-29 13:43:35 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021114 | We recently proposed a solution to the problem of model ambiguity for the X-ray spectra of atoll-type neutron stars. Our preferred model involves a resurrection of the double-thermal model for the soft state. The results have ramifications for such issues as neutron star ISCOs, the structure of the accretion boundary layer, and the radiative efficiency of the hard state (jets). Suzaku instruments can test and refine the model directly, with a focus on spectral fits rather than a reliance on model performance arguments. This proposal requests a TOO program for monitoring observations of one of the two atoll-type transients that were used to develop our spectral model with RXTE data. | GALACTIC POINT SOURCES | 4 | A | RONALD REMILLARD | USA | 2 | AO2-TOO | X-RAY SPECTRA OF NEUTRON-STAR X-RAY TRANSIENTS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402053030/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402053030'
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