dc.contributor.author |
Velusamy, T. |
|
dc.contributor.author |
Marsh, K. A. |
|
dc.contributor.author |
Ware, B. |
|
dc.date.accessioned |
2006-02-14 |
|
dc.date.available |
2006-02-14 |
|
dc.date.issued |
2005-10 |
|
dc.identifier.citation |
IAUC200 Direct Imaging of Exoplanets: Science & Techniques |
en |
dc.identifier.clearanceno |
05-3596 |
|
dc.identifier.uri |
http://hdl.handle.net/2014/38651 |
|
dc.description.abstract |
TPF-I capability for planetary signal extraction, including both detection and spectral characterization, can be optimized by taking proper account of instrumental characteristics and astrophysical prior information. We have developed the Point Process Algorithm, a Bayesian technique for estracting planetary signals using the sine/cosine chopped outputs of a dual nulling interferometer. |
en |
dc.description.sponsorship |
NASA |
en |
dc.format.extent |
327157 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
en |
dc.publisher |
asadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2005. |
en |
dc.subject |
methods |
en |
dc.subject |
data analysis |
en |
dc.subject |
techniques |
en |
dc.subject |
interferometric |
en |
dc.subject |
stars |
en |
dc.subject |
planetary systems |
en |
dc.title |
Point process algorithm: a new Bayesian approach for TPF-I planet signal extraction |
en |
dc.type |
Preprint |
en |