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 NGC5929 231.5229 41.6989 231.07632 41.872918 210.309469 57.436696 67.89643134 55.30533508 120.4869 56651.8033217593 2013-12-25 19:16:47 56652.6042824074 2013-12-26 14:30:10 708022010 24.649 30 24.649 24.6689 0 24.6565 2 2 0 2 1 0 0 25.1767 25.1767 69.1919 0 PROCESSED 57613.6825925926 2016-08-13 16:22:56 56383 2013-04-01 00:00:00 56700.6301388889 2014-02-12 15:07:24 3.0.22.44 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 081418 Using Suzaku's sensitivity in the 2-50keV range, we propose to obtain broad-band spectral fits to the X-ray emission from five Seyfert galaxies which have nuclei that are likely to be Compton-thick. We will thereby derive estimates of their absorbing column densities (hitherto unknown), Fe line widths and equivalent widths, absorption-corrected nuclear X-ray emission and the reprocessed components. With these new estimates we will have complete measurements for a rigorously selected sample of 20 Seyferts that are matched in orientation-independent parameters. The sample selection enables us to account for orientation effects which dominate in them, and investigate the AGN evolution, AGN-star burst connection, and host galaxy evolution. EXTRAGALACTIC COMPACT SOURCES 7 C PRAJVAL SHASTRI USA 8 AO8 COMPTON-THICK SEYFERT NUCLEI AND SEYFERT UNIFICATION XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708022010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '708022010'

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