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 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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