Visibility estimators and their performance are presented for use with the Palomar Testbed Interferometer (PTI). One operational mode of PTI is single-baseline visibility measurement using pathlength modulation with synchronous readout by a NICMOS-3 infrared array. Visibility is estimated from the fringe quadratures, either incoherently, or using source phase referencing to provide a longer coherent integration time. The visibility estimators differ those used with photon-counting detectors in order to account for biases attributable to detector offsets and read noise. The performance of these estimators is affected not only by photon noise, but also by the detector read noise and errors in estimating the bias corrections, which affect the ...
We describe the fringe-packet tracking system used to equalize the optical path lengths at the Infra...
Context. Long-baseline optical interferometry uses the power spectrum and bispectrum const...
Transient radio signals of astrophysical origin present an avenue for studying the dynamic universe....
The Palomar Testbed Interferometer (PTI) is an infrared, phase-tracking interferometer in operation ...
The Palomar Testbed Interferometer is a long-baseline near- infrared interferometer operating at Pal...
We discuss recent work from the Palomar Testbed Interferometer (PTI), including science results and ...
International audienceIn the near-infrared, where detectors are limited by readout noise, most inter...
In the near infrared where detectors are limited by read-out noise, most interferometers have been o...
I present in this paper a method to subtract the bias due to source photon noise from visibilities m...
We describe the fringe-packet tracking software installed at the infrared optical telescope array (I...
By construction, optical (and near-infrared) interferometers typically have resolutions designed to ...
The Palomar Testbed Interferometer (PTI) is a near-infrared, long-baseline interferometer located at...
The Palomar Testbed Interferometer (PTI) is a long-baseline infrared interferometer located at Palom...
The Palomar Testbed Interferometer (PTI) archive of observations between 1998 and 2005 is examined f...
The Palomar Testbed Interferometer (PTI) is a long-baseline, near-infrared interferometer located on...
We describe the fringe-packet tracking system used to equalize the optical path lengths at the Infra...
Context. Long-baseline optical interferometry uses the power spectrum and bispectrum const...
Transient radio signals of astrophysical origin present an avenue for studying the dynamic universe....
The Palomar Testbed Interferometer (PTI) is an infrared, phase-tracking interferometer in operation ...
The Palomar Testbed Interferometer is a long-baseline near- infrared interferometer operating at Pal...
We discuss recent work from the Palomar Testbed Interferometer (PTI), including science results and ...
International audienceIn the near-infrared, where detectors are limited by readout noise, most inter...
In the near infrared where detectors are limited by read-out noise, most interferometers have been o...
I present in this paper a method to subtract the bias due to source photon noise from visibilities m...
We describe the fringe-packet tracking software installed at the infrared optical telescope array (I...
By construction, optical (and near-infrared) interferometers typically have resolutions designed to ...
The Palomar Testbed Interferometer (PTI) is a near-infrared, long-baseline interferometer located at...
The Palomar Testbed Interferometer (PTI) is a long-baseline infrared interferometer located at Palom...
The Palomar Testbed Interferometer (PTI) archive of observations between 1998 and 2005 is examined f...
The Palomar Testbed Interferometer (PTI) is a long-baseline, near-infrared interferometer located on...
We describe the fringe-packet tracking system used to equalize the optical path lengths at the Infra...
Context. Long-baseline optical interferometry uses the power spectrum and bispectrum const...
Transient radio signals of astrophysical origin present an avenue for studying the dynamic universe....