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 | HETEJ1900.1-2455 | 285.0506 | -24.9802 | 284.284146 | -25.050704 | 283.615122 | -2.248458 | 11.25454685 | -12.90928139 | 259.4192 | 54389.5913425926 | 2007-10-16 14:11:32 | 54390.5071064815 | 2007-10-17 12:10:14 | 402016010 | 41.7591 | 40 | 41.7788 | 41.7591 | 0 | 41.7751 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 39.9063 | 39.9063 | 79.1058 | 1 | PROCESSED | 57540.3158564815 | 2016-06-01 07:34:50 | 54771 | 2008-11-01 00:00:00 | 54403.1292708333 | 2007-10-30 03:06:09 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 020068 | We propose a 40 ks observation of the accreting millisecond pulsar HETE J1900.1-2455, which was discovered by HETE-2 only recently. Good sensitivity in 10-100keV and enough timing resolution of HXD on Suzaku allow us to measure the light curve and the phase resolved spectra of its hard X-ray pulsation, with which we study the physical parameters of the Comptonizing plasma that is considered as the source of the hard X-ray emission of accreting millisecond pulsars. With XIS, we study the radiation from the accretion disk and the neutron star surface, and search for spectral features such as emission lines or absorption edges, which will provide information on the binary environment. | GALACTIC POINT SOURCES | 4 | B | MOTOKO SUZUKI | JAP | 2 | AO2 | HARD X-RAY PULSATION OF ACCRETION-DRIVEN MILLISECOND PULSAR HETE J1900.1-2455 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402016010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402016010'
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