1996A&AS..120C.683D


Query : 1996A&AS..120C.683D

1996A&AS..120C.683D - Astron. Astrophys., Suppl. Ser., 120C, 683-686 (1996/December-3)

Pixon-based deconvolution.

DIXON D.D., JOHNSON W.N., KURFESS J.D., PINA R.K., PUETTER R.C., PURCELL W.R., TUEMER T.O., WHEATON W.A. and ZYCH A.D.

Abstract (from CDS):

We describe a new technique, pixon-based deconvolution, for the reconstruction of images and spectra from low signal-to-noise data. In ``traditional'' techniques, such as Maximum Likelihood (ML) and Maximum Entropy (ME), the model parameters (e.g., pixel size) are considered ``nuisance parameters'', and generally held fixed in the course of deconvolution. Pixon techniques allow the model parameters to change according to the information contained in the data. The pixon model admits only that level of detail which is statistically justified by the data, thus greatly reducing the production of spurious sources and signal correlated residuals, common problems in ML and ME reconstructions. As a result, gains in sensitivity and spatial/energy resolution may be realized. Sample applications to data from OSSE and COMPTEL will be presented.

Abstract Copyright: ∼

Journal keyword(s): gamma rays: observations - methods: data analysis - techniques: image processing

CDS comments: Special Issue "3rd Compton Symposium"

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 QSO J0530+13 Bla 05 30 56.41674741 +13 31 55.1494688     20.00 19.35   ~ 1004 1
2 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
3 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
4 NGC 4388 Sy2 12 25 46.820 +12 39 43.45 11.91 11.76 11.02     ~ 1433 2
5 3C 273 BLL 12 29 06.6998257176 +02 03 08.597629980   13.05 14.830 14.11   ~ 6022 1

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