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 3C 105 61.8399 3.6518 61.183972 3.519003 60.504157 -16.952891 187.66746701 -33.63397375 251.3728 54501.5363078704 2008-02-05 12:52:17 54503.0833912037 2008-02-07 02:00:05 702074010 38.319 53 38.319 38.319 0 38.319 2 2 0 2 1 0 0 48.8811 48.8811 133.6558 2 PROCESSED 57541.5364351852 2016-06-02 12:52:28 54883 2009-02-21 00:00:00 54515.7678819444 2008-02-19 18:25:45 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 021372 The nature and even the existence of type II quasars is highly controversial. Due to their highly obscured nature, very hard (> 15 keV) observations are needed to probe their properties. With the 9-month SWIFT BAT all-sky AGN survey, detection of heavily obscured sources is now possible. Indeed, 6 type II quasars have been identified. Their properties, however, are a challenge to standard AGN models e.g., all but one of these sources are strong radio sources and several have optical spectra indicative of an un-absorbed source. We propose Suzaku observations of the 5 without broadband high signal to noise x-ray data to perform a detailed analysis of their x-ray properties and to understand their relationship to the lower luminosity well studied Seyfert IIs. EXTRAGALACTIC COMPACT SOURCES 7 B RICHARD MUSHOTZKY USA 2 AO2 SUZAKU OBSERVATIONS OF SWIFT BAT TYPE II QUASARS HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702074010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702074010'

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