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 | SGR 0501+4516 | 75.2795 | 45.3414 | 74.367379 | 45.268539 | 78.857896 | 22.469212 | 161.49568149 | 1.98976538 | 93.3341 | 55060.8485069445 | 2009-08-17 20:21:51 | 55061.8348842593 | 2009-08-18 20:02:14 | 404078010 | 42.6753 | 40 | 42.6753 | 42.9553 | 0 | 42.8913 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 27.4878 | 27.4878 | 85.1858 | 0 | PROCESSED | 57548.1780092593 | 2016-06-09 04:16:20 | 54922 | 2009-04-01 00:00:00 | 55071.2594328704 | 2009-08-28 06:13:35 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 046002 | We propose a comprehensive study of magnetars and associated objects in order to resolve strong magnetism of neutron stars. Magnetars are estimated to have an ultra strong magnetic filed as 1E+15 Gauss, and have been attracted growing wide attention recent years. These classes are extreme case of magnetars and have excellent clues to complete our scientific goal, including magnetism and ultrahigh magnetic-field physics. This proposal carries a sense of future potential to become "Suzaku Legacy" Key Project and to break the new ground of "Magnetar Physics". | GALACTIC POINT SOURCES | 4 | A | KAZUO MAKISHIMA | JAP | 4 | AO4 | A SUZAKU STUDY OF MAGNETARS AND THE NEUTRON-STAR MAGNETISM | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/404078010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '404078010'
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