Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/4816
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Vyas, A | - |
dc.contributor.author | Roopashree, M. B | - |
dc.contributor.author | Prasad, B. R | - |
dc.date.accessioned | 2009-09-11T16:29:58Z | - |
dc.date.available | 2009-09-11T16:29:58Z | - |
dc.date.issued | 2009 | - |
dc.identifier.citation | Proceeding of the National Conference on Innovative Computational Intelligence & Security Systems, Sona College of Technology, Salem. April 3 - 4, 2009. pp. 400 - 405 | en |
dc.identifier.uri | http://hdl.handle.net/2248/4816 | - |
dc.description.abstract | Three centroiding techniques to estimate the position of the spots in a Shack Hartmann sensor: Normalized Centre of Gravity (CoG), Iteratively Weighted Centre of Gravity (IWCoG) and Intensity Weighted (IWC) centroiding are studied in comparison. The spot pattern at the focal plane of a Shack Hartmann sensor was simulated by including the effect of a background noise. We present the results of optimization of the performance of each of the centroiding techniques as a function of Signal to Noise Ratio (SNR) at different experimental conditions. | en |
dc.language.iso | en | en |
dc.relation.uri | http://arxiv1.library.cornell.edu/abs/0908.4328 | en |
dc.subject | Shack Hartmann Sensor | en |
dc.subject | Centroiding Algorithms | en |
dc.subject | Centroid Estimation Error | en |
dc.subject | Astrophysics | en |
dc.subject | Instrumentation and Methods for Astrophysics | en |
dc.title | Optimization of existing centroiding algorithms for Shack Hartmann sensor | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Optimization of existing centroiding algorithms | 203.69 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.