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 | 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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