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 | XB1916-053 | 289.7015 | -5.2503 | 289.036388 | -5.342643 | 290.518339 | 16.797779 | 31.34764946 | -8.47089453 | 261.8034 | 56948.5140856482 | 2014-10-18 12:20:17 | 56952.1112152778 | 2014-10-22 02:40:09 | 409032020 | 140.4495 | 300 | 140.4575 | 140.4655 | 0 | 140.4495 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 6.8873 | 6.8873 | 14.636 | 0 | PROCESSED | 57616.6738773148 | 2016-08-16 16:10:23 | 56748 | 2014-04-01 00:00:00 | 57000.2058680556 | 2014-12-09 04:56:27 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 091221 | XB1916-053 is a prototypical dipping low mass X-ray binary (LMXB) with a dip recurrence period of 3000.6+-0.2s. However, extensive optical observations also show a longer stable period of 3027s. The former is most likely the orbital period, and the latter the superhump period caused by the precession of an elliptical accretion disk at a period of 3.9 days, representing the beat period between optical and X-ray periods. The morphology of the X-ray dips does indeed change dramatically over several days, but existing data suggest a somewhat longer period for the dip morphology cycle of 4.7 days. Here we propose a 300ks Suzaku observation of XB1916-053 with as few interruptions as possible, to conduct a definitive timing and spectroscopic study of its disk emission and dipping activity. | GALACTIC POINT SOURCES | 4 | B | ALAN SMALE | USA | 9 | AO9 | THE PRECESSING DISK IN THE DIPPING X-RAY BINARY XB1916-053 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/409032020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '409032020'
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