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 | MRK533 | 351.9889 | 8.7759 | 351.354325 | 8.500435 | 356.155514 | 11.232339 | 90.62800693 | -48.78900326 | 248.1747 | 56634.8830671296 | 2013-12-08 21:11:37 | 56636.0847569444 | 2013-12-10 02:02:03 | 708023010 | 52.194 | 50 | 52.194 | 52.194 | 0 | 52.194 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 48.5617 | 48.5617 | 103.8059 | 0 | PROCESSED | 57613.5724421296 | 2016-08-13 13:44:19 | 56383 | 2013-04-01 00:00:00 | 56646.7358449074 | 2013-12-20 17:39:37 | 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/ver3.0/708023010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '708023010'
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