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 | 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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