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 ESO 103- G 035 279.5941 -65.4238 278.351287 -65.467222 275.354112 -42.161198 329.78379096 -23.17817546 291.5832 54761.6331597222 2008-10-22 15:11:45 54764.1717476852 2008-10-25 04:07:19 703031010 91.442 80 91.442 91.45 0 91.45 2 2 0 2 1 0 0 81.0096 81.0096 219.282 2 PROCESSED 57544.3339467593 2016-06-05 08:00:53 55148 2009-11-13 00:00:00 54782.4220023148 2008-11-12 10:07:41 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031322 X-ray observations of Seyfert 2 have shown that the distribution and ionization state of the circumnuclear material is more complex than the simple homogeneous torus predicted by the AGN Unification Scheme. To investigate the nature of this material, high sensitivity is needed to detect relatively faint emission lines, while broad bandpass is required to constrain the primary X-ray continuum. We propose Suzaku observations (80 ksec each) of three bright Compton-thin Seyfert 2 galaxies, selected from the Swift/BAT survey, with a hard X-ray flux exceeding 9e-11cgs, to form a flux-limited sample. The unprecedented bandpass of Suzaku offers a unique tool to investigate the X-ray emission of these sources, allowing us to put strong constraints on the reprocessing matter in Seyfert 2s. EXTRAGALACTIC COMPACT SOURCES 7 B VALENTINA BRAITO USA 3 AO3 THE NATURE OF THE X-RAY ABSORBER IN SEYFERT 2 GALAXIES XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703031010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '703031010'

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