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 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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