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 J1018.6-5856 | 154.7461 | -58.9386 | 154.30337 | -58.687202 | 196.560422 | -60.861111 | 284.35392298 | -1.67969789 | 308.622 | 56105.7124189815 | 2012-06-27 17:05:53 | 56106.6523611111 | 2012-06-28 15:39:24 | 407096010 | 60.4324 | 60 | 60.4324 | 60.4324 | 0 | 60.4324 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 53.5978 | 53.5978 | 81.2059 | 1 | PROCESSED | 57606.5124768518 | 2016-08-06 12:17:58 | 56484 | 2013-07-11 00:00:00 | 56118.0496527778 | 2012-07-10 01:11:30 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 073113 | Recently, a modulated signal has been detected with the Fermi from the source 1FGL J1018.6-5856. The presence of a O-type star in this source, and the variable character of the signal suggested that the source is a new gamma-ray binary system. Since it is expected that X-rays in these sources has the synchrotron origin, detailed X-ray observations are very important for understanding of the processes occurring in the system. However, sensitive observations of source in the X-ray energy bands are still missing. Therefore, we propose to observe the source with Suzaku. Since a long observational campaign is planned for 2012 by the HESS collaboration, the obtained X-ray, together with TeV, data will allow a proper modeling of the physical processes behind the non-thermal emission in system. | GALACTIC POINT SOURCES | 4 | B | HIROKAZU ODAKA | TAKAAKI TANAKA | JUS | 7 | AO7 | X-RAY OBSERVATION OF GAMMA-RAY BINARY 1FGL J1018.6-5856 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407096010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '407096010'
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