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 154.7377 -58.9433 154.295067 -58.691919 196.56156 -60.86748 284.35288518 -1.68600623 306.342 56102.9882407407 2012-06-24 23:43:04 56103.3696875 2012-06-25 08:52:21 407070010 17.4473 20 17.4645 17.4633 0 17.4473 2 2 0 2 1 0 0 14.4474 14.4474 32.9499 2 PROCESSED 57606.4834722222 2016-08-06 11:36:12 56480 2013-07-07 00:00:00 56114.1719328704 2012-07-06 04:07:35 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 071234 We propose Suzaku observations of a newly discovered gamma-ray binary 1FGL J1018.6-5856. Recent observations by the Fermi Gamma-ray Space Telescope and follow-up observations in other wavelengths revealed that the gamma-ray source is a new member of the rare gamma-ray binary class with an orbital period of 16 days. We propose two types of observations with Suzaku. One is a continuous observation of a sharp X-ray peak found in the lightcurve by the Swift XRT. Another is a series of snap shot observations in orbital phase between the peaks. We aim to perform phase-resolved spectral analysis which is not possible with the Swift XRT data. We also compare the Swift XRT lightcurve with new lightcurves taken by Suzaku in order to test the repeatability of the X-ray orbital modulation. GALACTIC POINT SOURCES 4 B TAKAAKI TANAKA USA 7 AO7 SUZAKU OBSERVATIONS OF A NEWLY DISCOVERED GAMMA-RAY BINARY: 1FGL J1018.6-5856 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/407070010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '407070010'

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