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 | 262.0809 | -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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