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 AX J1445.7-5931 221.4519 -59.5275 220.50216 -59.317243 239.705831 -41.083897 316.97780419 0.18867801 281.526 56143.2829513889 2012-08-04 06:47:27 56144.2918865741 2012-08-05 07:00:19 407021010 40.0525 40 41.0682 41.0602 0 40.0525 2 1 0 2 1 0 0 36.8089 36.8089 87.1579 1 PROCESSED 57606.7459722222 2016-08-06 17:54:12 56533 2013-08-29 00:00:00 56167.2116319444 2012-08-28 05:04:45 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 070043 Through studies of magnetars and supernova remnants associated to them, we have arrived at a possibility that magnetars are in fact much younger than their characteristic ages, and hence are born with a much higher rate than was considered previously. This predicts a large population of aged magnetars to lurk in the Galactic plane as slowly rotating soft X-ray sources. From the X-ray source catalog with the ASCA Galactic plane survey, we have selected four candidates for such aged magnetars, and propose to observe them for 40 ksec each. We expect them to appear as faint soft X-ray sources with blackbody temperatures of 0.5 keV or so, possibly pulsating at periods of about 10 seconds. One FI CCD of the XIS is set in the 1/8-window option to achieve a sufficient time resolution. GALACTIC POINT SOURCES 4 A KAZUO MAKISHIMA JAP 7 AO7 ARE A LARGE FRACTION OF NEUTRON STARS BORN AS MAGNETARS? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407021010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407021010'

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