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 0142+61 26.5838 61.7628 25.715895 61.512967 52.16359 46.394147 129.37704782 -0.4200572 82.997 56504.4205902778 2013-07-31 10:05:39 56506.6252430556 2013-08-02 15:00:21 408011010 101.1678 100 101.1678 101.1828 0 101.1828 2 2 0 2 1 0 0 102.4739 102.4739 190.4637 1 PROCESSED 57612.1558680556 2016-08-12 03:44:27 56953 2014-10-23 00:00:00 56587.5059606482 2013-10-22 12:08:35 3.0.22.44 3 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 080035 A toroidal magnetic field is thought to be formed in neutron star interior after core-collapse supernovae and become an energy source with recently observed X-ray outbursts from magnetars. Since the toroidal field is hidden in the stellar interior, it was thought to be undetectable via the well-known p-pdot method and the cyclotron resonance scattering features. However, a magnetic stress of the magnetar toroidal field is strong enough to distort the stellar shape and produce a free precession in its X-ray pulse timing if the emission pattern deviates from its axis of symmetry. From our analyses of magnetar 4U 0142+61, we found an evidence on the free precession in the hard X-ray component. To confirm and establish this evidence, we propose an additional 100 ks observation of 4U 0142+61. GALACTIC POINT SOURCES 4 A TERUAKI ENOTO JAP 8 AO8 TOROIDAL FIELD INSIDE MAGNETARS OBSERVED WITH SUZAKU TIMING ANALYSES OF ITS FREE PRECESSION XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/408011010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '408011010'

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