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 | PDS 456 | 262.0805 | -14.2617 | 261.369811 | -14.221632 | 262.221115 | 8.965551 | 10.39443055 | 11.16720212 | 96.2512 | 56354.8215972222 | 2013-03-03 19:43:06 | 56359.5001388889 | 2013-03-08 12:00:12 | 707035020 | 164.8107 | 450 | 164.8267 | 164.8107 | 0 | 164.8291 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 147.4496 | 147.4496 | 404.1815 | 2 | PROCESSED | 57610.8342824074 | 2016-08-10 20:01:22 | 56018 | 2012-04-01 00:00:00 | 56373.6804166667 | 2013-03-22 16:19:48 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 071431 | PDS 456 is the most luminous nearby (z=0.184) AGN, more typical of quasars at high redshift. A 2007 Suzaku observation resolved iron K absorption at 9 keV in the QSO frame, moving at near relativistic velocities (0.25c). A follow-up 2011 observation was highly absorbed and showed a direct response of the iron K absorber to a decrease in the ionizing flux, while the harder photons lag behind the soft, by 10^4 secs. We propose to monitor the remarkable spectral variability and outflow from PDS 456, through a deep 450ks Suzaku observation. We wish to:- (i) quantify the time lags and determine the location of the reprocessor, (ii) determine the origin and timescale of the absorber variability and (iii) measure the hard X-ray variability from a Compton thick absorber in PDS 456. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | JAMES REEVES | USA | 7 | AO7 | VARIABILITY AND REVERBERATION OF THE QUASAR WIND IN PDS 456 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/707035020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '707035020'
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