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 | LS I+61 303_3 | 40.2018 | 61.1949 | 39.239095 | 60.980826 | 59.865781 | 42.86376 | 135.72005286 | 1.06843757 | 246.2753 | 54872.1842592593 | 2009-02-10 04:25:20 | 54873.7252199074 | 2009-02-11 17:24:19 | 403017010 | 68.6273 | 60 | 68.6273 | 68.6273 | 0 | 68.6273 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 65.0685 | 65.0685 | 133.1218 | 1 | PROCESSED | 57545.5290856482 | 2016-06-06 12:41:53 | 55330 | 2010-05-14 00:00:00 | 54893.4210300926 | 2009-03-03 10:06:17 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 030077 | We propose to observe a gamma-ray binary LS I+61 303 simultaneously with the GeV/TeV gamma-ray (GLAST/VERITAS), radio, and optical, in order to ob tain the orbital-phase dependent multi-wavelength spectra (SED) in the early 2009. This observation will give us information of the relation between the binary geometry and the emission to understand the gamma-ray emissio n mechanism. Suzaku data also will enable us to probe the material distribution in the binary system by searching the Fe-K emission or absorption line, edge, an d so on. This observation will open a new window to study gamma-ray binaries, which are expected to be found with GLAST. | GALACTIC POINT SOURCES | 4 | A | YASUSHI FUKAZAWA | JAP | 3 | AO3 | X-RAY SPECTRAL VARIABILITY OF THE GAMMA-RAY BINARY LS I+61 303 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/403017010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '403017010'
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