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 PSR J0726-2612 111.531 -26.2114 111.017873 -26.110384 119.169713 -47.49417 240.07877209 -4.64696128 117.9984 55881.5691782407 2011-11-16 13:39:37 55882.6252546296 2011-11-17 15:00:22 406012010 43.757 100 43.757 43.792 0 43.792 2 2 0 2 1 0 0 39.7288 39.7288 91.2278 0 PROCESSED 57603.8172685185 2016-08-03 19:36:52 56264 2012-12-03 00:00:00 55895.2388078704 2011-11-30 05:43:53 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 060041 To study the origin of magnetars, a unique opportunity is provided by detecting an excess of thermal radiation in the radio pulsars which has dipolar magnetic fields as high as magnetars. The excess is caused by field decay as seen in magnetars. A question is raised whether the rotation powered pulsars can have active magnetic flux similar to magnetars. PSR J0726-2612 is a nearby (3kpc) radio pulsar with magnetic field as high as 10^13.5 G, and therefore is an ideal target. We propose 100ksec observation of this pulsar to discover magnetar-like thermal radiation, and determine the structure of the active magnetic flux tubes by phase alignment of rotational modulation of the X-ray radiation with radio pulses. GALACTIC POINT SOURCES 4 C SHINPEI SHIBATA JAP 6 AO6 CAN HIGH MAGNETIC FIELD RADIO PULSARS BE THE MAGNETAR ? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406012010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '406012010'

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