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 | 1FGL J2339.7-0531 | 354.9077 | -5.5469 | 354.264388 | -5.824081 | 353.120926 | -3.069352 | 81.34836456 | -62.4702773 | 67.4026 | 55741.5915625 | 2011-06-29 14:11:51 | 55743.8092361111 | 2011-07-01 19:25:18 | 406007010 | 104.0914 | 100 | 104.0914 | 104.0914 | 0 | 104.0994 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 92.9022 | 92.9022 | 191.5837 | 2 | PROCESSED | 57602.4861805556 | 2016-08-02 11:40:06 | 56144 | 2012-08-05 00:00:00 | 55775.4025925926 | 2011-08-02 09:39:44 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060007 | We propose to observe an unidentified Fermi source (1FGL J2339.7-0531) in the first-year Fermi catalog to search for the first ``radio-quiet'' Gamma-ray emitting millisecond pulsar. The Fermi source has a candidate X-ray counterpart from Chandra data and its X-ray and Gamma-ray properties are consistent with known Gamma-ray pulsars. This system is likely in a low-mass X-ray binary system based on optical observations. Both X-ray and optical observations show clear variability. We propose to observe the Chandra source with Suzaku to search for the possible orbital period and to study its X-ray spectrum in detail. The results will provide a better insight into the high-energy emission processes in the magnetosphere of millisecond pulsars. | GALACTIC POINT SOURCES | 4 | A | ALBERT KONG | JUN KATAOKA | JAP | 6 | AO6 | REVEALING THE NATURE OF AN UNIDENTIFIED FERMI SOURCE | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/406007010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '406007010'
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