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 | NGC 7469 | 345.7842 | 8.9301 | 345.154297 | 8.660604 | 350.460681 | 13.82437 | 83.10914575 | -45.403242 | 63.4793 | 54641.7015856482 | 2008-06-24 16:50:17 | 54644.683599537 | 2008-06-27 16:24:23 | 703028010 | 112.1128 | 100 | 112.1251 | 112.1331 | 0 | 112.1128 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 91.5571 | 91.5571 | 257.6126 | 2 | PROCESSED | 57542.968125 | 2016-06-03 23:14:06 | 55027 | 2009-07-15 00:00:00 | 54658.7891319444 | 2008-07-11 18:56:21 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 031311 | We propose a 100 ksec observation of the X-ray bright Seyfert 1 AGN NGC 7469, a strong candidate for having ionized reflection from the accretion disk. Only the broad bandpass provided by Suzaku, including >12 keV coverage via the HXD, will allow us to deconvolve the broadband emitting components, including the strong Compton reflection hump, broad Fe K line, and soft excess. With the XIS, we will study in detail the Fe K emission complex, including the narrow 6.4 keV Fe K core and in particular the prominent ``blue wing'' near 6.9 keV. Our proposed observation will thus be an example of how broad bandpass X-ray observations can critically test blurred, ionized disk reflection model in Seyfert 1s. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | ALEX MARKOWITZ | USA | 3 | AO3 | IONIZED DISK REFLECTION IN THE SEYFERT AGN NGC 7469 | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703028010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703028010'
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