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 | IC 4518A | 224.419 | -43.1269 | 223.597719 | -42.926611 | 234.851401 | -25.085272 | 326.11466585 | 13.99053707 | 102.9822 | 55959.1723263889 | 2012-02-02 04:08:09 | 55961.0002777778 | 2012-02-04 00:00:24 | 706012010 | 64.3986 | 60 | 64.3986 | 64.3986 | 0 | 64.3986 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 57.2381 | 57.2381 | 157.9058 | 1 | PROCESSED | 57604.5692708333 | 2016-08-04 13:39:45 | 56434 | 2013-05-22 00:00:00 | 56068.6321064815 | 2012-05-21 15:10:14 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060040 | We propose to observe the Compton-thin AGN IC 4518A with a very small L_X/L_IR ratio, which has often been employed as an indicator of the presence of a Compton-thick AGN. Our aim is to examine the recent argument that L_X/L_IR is not a good measure of absorption column densities and that this ratio is more dependent on the covering fraction of absorber and intrinsic spectral shape. We measure the spectral slope, covering fraction, and NH, and compare them with the prediction of Monte-Carlo simulations to test the validity of L_X/L_IR as a measure of Compton thickness. | EXTRAGALACTIC COMPACT SOURCES | 7 | C | YOSHITAKA HIRATA | JAP | 6 | AO6 | BROAD-BAND SPECTRA OF THE COMPTON-THIN AGN IC 4518A WITH A SMALL L_X/L_IR: TESTING VALIDITY OF A COMPTON-THICK INDICATOR | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/706012010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '706012010'
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