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 PDS 456 262.0807 -14.2604 261.370018 -14.220332 262.221238 8.96686 10.39565911 11.16772638 98.239 54155.7486574074 2007-02-24 17:58:04 54160.0355787037 2007-03-01 00:51:14 701056010 190.6002 188 190.6082 190.6002 0 190.6142 2 2 0 2 1 0 0 176.4708 176.4708 370.3428 4 PROCESSED 57537.5850578704 2016-05-29 14:02:29 54757 2008-10-18 00:00:00 54168.6244560185 2007-03-09 14:59:13 3.0.22.43 4 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 011351 A long 150ks Suzaku observation of the most luminous nearby quasar, PDS 456, is proposed. In the X-ray band, PDS 456 shows a deep iron K absorption trough. One possibility is that the absorption arises from a massive 0.1c outflow, of column density 10^24 cm^-2. Such an outflow would represent a significant fraction of the quasar energy budget. A deep Suzaku observation is proposed to test this outflow model, in particular the high energy bandpass of Suzaku is essential for measuring the profile of the absorption feature and determining the kinematics of the outflow. It is also possible to differentiate between competing models for the iron K feature, most notably between an outflow and a strong reflection component from the innermost radii around a Kerr black hole. EXTRAGALACTIC COMPACT SOURCES 7 A JAMES REEVES USA 1 AO1 SOLVING THE ORIGIN OF THE DEEP IRON K ABSORPTION IN PDS 456 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701056010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '701056010'

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