De-biasing interferometric visibilities in VLTI-AMBER data of low SNR observations

Abstract

AIMS: We have found that the interferometric visibilities of VLTI-AMBER observations, extracted via the standard reduction package, are significantly biased when faint targets are concerned. The visibility biases derive from a time variable fringing effect (correlated noise) appearing on the detector. METHODS: We have developed a method to correct this bias that consists in a subtraction of the extra power due to such correlated noise, so that the real power spectrum at the spatial frequencies of the fringing artifact can be restored. RESULTS: This pre-processing procedure is implemented in a software, called AMDC and available to the community, to be run before the standard reduction package. Results obtained on simulated and real observations are presented and discussed.

7 pages, 9 figures

References in corpus (1)

• Interferometric data reduction with AMBER/VLTI.Principle,estimators and illustration

Cited by in corpus (2)

• Spatially resolving the hot CO around the young Be star 51 Ophiuchi
• Resolving the ionized wind of the post-Red Supergiant IRC +10 420 with VLTI/AMBER