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 MCG-03-58-007 342.3795 -19.2152 341.708645 -19.480081 336.393592 -10.851288 42.20057234 -60.96689333 68.5139 55350.7016203704 2010-06-03 16:50:20 55352.8940046296 2010-06-05 21:27:22 705052010 99.0873 100 99.0873 99.0873 0 99.0873 2 2 0 2 1 0 0 81.42 81.42 189.406 1 PROCESSED 57551.8454513889 2016-06-12 20:17:27 55734 2011-06-22 00:00:00 55365.563912037 2010-06-18 13:32:02 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 052011 Despite their relevance, less than two dozens of confirmed Compton-thick (CT) AGN have been found so far. We have recently selected a well defined sample of CT AGN candidates using FX/Fir ratios and X-ray colors. Due to their heavy obscuration, good statistics at 6.4 keV and data above 10 keV are needed to assess the real nature of these sources. We propose deep Suzaku observations (100 and 150 ks) for two sources for which data above 10 keV are not available and the quality of XMM data is poor. This request is a continuation of an approved AO4 proposal. These observations will allow us to possibly unveil two more examples of CT AGN, provide a physical characterization of the relatively bright tail of our sample, and estimate the efficiency of our method in selecting CT AGN. EXTRAGALACTIC COMPACT SOURCES 7 A PAOLA SEVERGNINI EUR 5 AO5 SUZAKU OBSERVATIONS OF TWO COMPTON-THICK CANDIDATES HXD Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/705052010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '705052010'

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