Improvements for group delay fringe tracking

Details Improvements for group delay fringe tracking Improvements for group delay fringe tracking

2004-11-30

arxiv.org/abs/astro-ph/0411787v1

Mon.Not.Roy.Astron.Soc. 357 (2005) 656-668

Astronomy and Astrophysics

Astrophysics

15 pages, accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2005.08681.x

Group delay fringe tracking using spectrally-dispersed fringes is suitable for stabilising the optical path difference in ground-based astronomical optical interferometers in low light situations. We discuss the performance of group delay tracking algorithms when the effects of atmospheric dispersion, high-frequency atmospheric temporal phase variations, non-ideal path modulation, non-ideal spectral sampling, and the detection artifacts introduced by electron-multiplying CCDs (EMCCDs) are taken into account, and we present ways in which the tracking capability can be optimised in the presence of these effects.

Affiliated with

Also associated with

No associations

Rating

Improvements for group delay fringe tracking does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Improvements for group delay fringe tracking, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Improvements for group delay fringe tracking will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-13608