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 3998 179.4698 55.4443 178.823114 55.722594 149.626555 48.892783 138.19460038 60.06850959 319.2188 56780.8797569445 2014-05-03 21:06:51 56782.5966898148 2014-05-05 14:19:14 709002010 80.6754 80 80.6754 80.6754 0 80.6754 2 2 0 2 1 0 0 76.8901 76.8901 148.2858 0 PROCESSED 57615.0693981482 2016-08-15 01:39:56 57159 2015-05-17 00:00:00 56793.5775 2014-05-16 13:51:36 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 090017 The number of Compton thick AGNs is the biggest issue in the origin of the X-ray background and AGN evolution. According to population synthesis models, its estimate is strongly coupled with the broad band spectral shape of Compton thin AGNs. Swift/BAT has provided the first unbiased AGN sample above 15 keV, which includes many hard X-ray bright AGNs that can be best followed-up with Suzaku. Here we propose to observe two of the lowest luminosity BAT AGNs to measure the amount of the reflection component with unpreceded accuracy, a key parameter to determine the contribution of Compton thick AGNs to the X-ray background. We will also study how the torus structure of low luminosity AGNs differs from that of more luminous AGNs. EXTRAGALACTIC COMPACT SOURCES 7 A YOSHIHIRO UEDA JAP 9 AO9 BROAD BAND SPECTRA OF HARD X-RAY SELECTED VERY LOW LUMINOSITY AGNS AND THEIR TORUS STRUCTURE XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/709002010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '709002010'

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