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 SWIFT J0318.7+6828 49.4315 68.5395 48.26024 68.35635 69.167768 48.016071 135.6962435 9.37350025 42.3301 54365.4488078704 2007-09-22 10:46:17 54367.125162037 2007-09-24 03:00:14 702075010 77.1156 53 77.1396 77.1156 0 77.1396 2 2 0 2 1 0 0 70.6855 70.6855 144.7978 1 PROCESSED 57540.0779513889 2016-06-01 01:52:15 54770 2008-10-31 00:00:00 54403.1984490741 2007-10-30 04:45:46 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/ver3.0/702075010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '702075010'

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