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 456 262.0809 -14.2537 261.370252 -14.213634 262.221057 8.97356 10.4015562 11.17111116 96.1694 55636.625462963 2011-03-16 15:00:40 55639.3564930556 2011-03-19 08:33:21 705041010 125.5272 130 125.5352 125.5272 0 125.5327 2 2 0 2 1 0 0 100.875 100.875 235.9276 2 PROCESSED 57601.2862615741 2016-08-01 06:52:13 56050 2012-05-03 00:00:00 55677.3183564815 2011-04-26 07:38:26 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 051421 PDS 456 is the most luminous nearby AGN and a recent Suzaku observation revealed a powerful ionized outflow moving at 0.25c with kinetic output matching the quasar bolometric luminosity. Above 10 keV the HXD appears to show a factor 3 rise in flux over the XIS, implying that a high column density absorber (>10^24 cm^-2) is located close to the X-ray source in order to partially covers its emission. We propose to study the remarkable X-ray absorption towards PDS 456 through two further 130 ks Suzaku observations. This will:-i) confirm the nature of the hard excess, ii) determine whether spectral variability can be explained by variable partial covering and iii) enable us to measure the imprint of the ionized outflow at Fe K with unprecedented accuracy. EXTRAGALACTIC COMPACT SOURCES 7 B TRACEY TURNER USA 5 AO5 THE COMPTON-THICK OUTFLOW IN THE TYPE I QSO PDS 456 XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705041010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '705041010'

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