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 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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