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 | IRAS 04507+0358 | 73.3635 | 4.1233 | 72.703908 | 4.042054 | 72.49644 | -18.313087 | 194.58361833 | -23.84576016 | 98.871 | 55075.0228356482 | 2009-09-01 00:32:53 | 55078.1356481482 | 2009-09-04 03:15:20 | 704058010 | 109.0524 | 100 | 109.0524 | 109.0524 | 0 | 109.0524 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 84.1098 | 84.1098 | 268.9118 | 3 | PROCESSED | 57548.5242939815 | 2016-06-09 12:34:59 | 55476 | 2010-10-07 00:00:00 | 55109.5623842593 | 2009-10-05 13:29:50 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 042022 | According to X-ray synthesis models, Compton-thick AGN (NH>1e24 cm-2) should represent 50% of the total absorbed AGN population. Despite their importance in the cosmological context, only a few of them have been found so far. We have selected a well-defined sample of 31 Compton-thick candidates on the basis on their FX/FIR and X-ray colors. Due to the heavy obscuration, data above 10 keV are fundamental to unveil these sources. We ask here deep Suzaku observations (100 ks on each source) for 2 sources of our sample for which data at energy >10keV are not available yet. These observations will allow to complete the physical characterization (NH and LX) of the bright tail (F(2-10 keV)>5e-12 cgs) of our sample and to add more information to test the prediction of the AGN synthesis model. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | PAOLA SEVERGNINI | EUR | 4 | AO4 | SUZAKU OBSERVATIONS OF COMPTON-THICK CANDIDATES | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/704058010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '704058010'
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