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 AQL X-1 287.8217 0.5796 287.183429 0.495861 289.383158 22.828908 35.71588636 -4.14991498 243.6715 54403.2743171296 2007-10-30 06:35:01 54403.66 2007-10-30 15:50:24 402053070 17.5362 15 17.5842 17.604 0 17.5362 1 1 0 1 1 0 0 14.3322 14.3322 33.3199 0 PROCESSED 57540.3767824074 2016-06-01 09:02:34 54776 2008-11-06 00:00:00 54409.1320138889 2007-11-05 03:10:06 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/ver3.0/402053070/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '402053070'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏