Details

Title

An efficient algorithm for determining positions of astronomical objects in the Deep Sky Object pictures

Journal title

Bulletin of the Polish Academy of Sciences: Technical Sciences

Yearbook

2015

Volume

63

Numer

No 3

Authors

Divisions of PAS

Nauki Techniczne

Coverage

679-684

Date

2015[2015.01.01 AD - 2015.12.31 AD]

References

Suszynski (2009), Convolution method for CCD images processing for DSO astrophotography nd Midwest Circuits and Systems, Proc IEEE Int Symp, 1. ; Suszynski (2011), image processing for auto - guiding system th Midwest on Circuits and Systems MWSCAS CD - ROM, Proc IEEE Int Symp, 1. ; Jeffs (1998), Blind bayesian restoration of adaptive optics telescope images using generalized gaussian markov random field models on Adaptive Optics and Telescope Systems SPIE CD - ROM, Proc Conf, 3353. ; McGuire (1998), Adaptive optics : neural networks wavefront sensing reconstruction and prediction th Seminar CD - ROM, Proc, 194. ; Vyas (2010), Cetroid detection by Gaussian pattern matching in adaptive optics Computer Applications, Int J, 1. ; Zhang (2012), Optical image simulation system for space surveillance th Parallel and Distributed Processing Symp CD - ROM, Proc IEEE Int. ; Li (2013), Implementing high - performance intensity model with blur effect on gpus for large - scale star image simulation on Image and Graphics CD - ROM, Proc Int Conf, 1. ; Berghi (2007), Atmospheric turbulence prediction : a pca approach th Decision and Control, Proc IEEE Conf, 1. ; Roesser (1975), A discrete state - space model for linear image processing, IEEE Trans Automat Contr, 20, 1, doi.org/10.1109/TAC.1975.1100844 ; Suszynski (2013), Rapid prototyping of algorithmic converters based on FPAA devices, Bull Pol Tech, 61, 691. ; Suszynski (2014), An improvement of stars centroid determination using PSF - fitting method Signals and Electronics Systems ICSES, Proc IEEE Int Conf, 1. ; Thomas (2006), Comparison of centroid computation algorithms in a Shack - Hartmann sensor Monthly Notices of the Royal, Astronomical Society, 371. ; Wawryn (2013), Low power bit pipelined - bit self - calibrated converters for a DSP system, Bull Pol Tech, 8, 979. ; Suszynski (2014), A stand - alone station and DSP method for deep sky objects astrophotography Electronics and Telecommunications, Int J, 157. ; Li (2006), The implement of high speed correlation tracking algorithm based on FPGA in space solar telescope th on Signal Processing CD - ROM, Proc Int Conf, 8, 1. ; Suszynski (2008), Digital processing of CCD images for auto - guiding astrophotography system th on Mixed Design of Integrated Circuits and Systems, Proc Int Conf, 15, 559. ; Baker (2007), Iteratively weighted centroid of Shack - Hartmann wave - front sensors, Opt Express, 15, 5147, doi.org/10.1364/OE.15.005147 ; Suszynski (2009), Stand - alone station for deep space objects astrophotography nd Midwest Symposium on Circuits and Systems, Proc IEEE Int, 1. ; Wawryn (2010), Implementation of finite impulse response systems using rotation structures Information Theory and Its Applications ISITA CD - ROM, Proc Int Symp, 20101.

DOI

10.1515/bpasts-2015-0079

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