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 | 4U2206+54 | 331.9811 | 54.5897 | 331.524827 | 54.344502 | 8.281106 | 58.879755 | 100.6432606 | -1.04691755 | 90.2357 | 54236.1620949074 | 2007-05-16 03:53:25 | 54237.812662037 | 2007-05-17 19:30:14 | 402069010 | 103.9768 | 100 | 103.9848 | 103.9906 | 0 | 103.9768 | 3 | 3 | 0 | 3 | 1 | 0 | 0 | 99.7842 | 99.7842 | 142.5819 | 1 | PROCESSED | 57538.7118402778 | 2016-05-30 17:05:03 | 54695 | 2008-08-17 00:00:00 | 54242.76625 | 2007-05-22 18:23:24 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021125 | 4U 2206+54 is a high mass X-ray binary which is suspected to contain a neutron star accreting from the wind of its companion BD +53 2790. However, there has been no confirmed detection of X-ray pulsations, and while several authors have reported hints of a cyclotron line in the energy spectra near 30 keV, none have reported significant detections. We propose Suzaku observations to search for long-period pulsations with the XIS, and possible confirmation of the cyclotron line using HXD/PIN. | GALACTIC POINT SOURCES | 4 | A | MARK FINGER | USA | 2 | AO2 | SUZAKU OBSERVATIONS OF THE PECULIAR HMXB 4U 2206+54 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402069010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402069010'
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