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Parasitic Interference in Nulling InterferometryNulling interferometry aims to detect faint objects close to bright stars. Its principle is to produce a destructive interference along the line of sight so that the stellar flux is rejected, while the flux of the off-axis source can be transmitted. In practice, various instrumental perturbations can degrade the nulling performance. Any imperfection in phase, amplitude or polarization produces a spurious flux that leaks to the interferometer output and corrupts the transmitted off-axis flux. One of these instrumental perturbations is the crosstalk phenomenon, which occurs because of multiple parasitic reflections inside transmitting optics, and/or diffraction effects related to beam propagation along finite size optics. It can include a crosstalk of a beam with itself, and a mutual crosstalk between different beams. This can create a parasitic interference pattern, which degrades the intrinsic transmission map - or intensity response - of the interferometer. In this context, we describe how this instrumental effect impairs the performance of a Bracewell interferometer. A simple formalism is developed to derive the corresponding modified intensity response of the interferometer, as a function of the two parameters of interest: the crosstalk level (or contamination rate) and the phase shift between the primary and secondary - parasitic - beams. We then apply our mathematical approach to a few scientific cases, both analytically and using the GENIESIM simulation software, adapted to handle coherent crosstalk. Our results show that a coherent crosstalk level of about 1 per cent implies a 20 per cent drop of the signal-to-noise ratio at most. Careful attention should thus be paid to reduce the crosstalk level inside an interferometric instrument and ensure an instrumental stability that provides the necessary sensitivity through calibration procedures.
Document ID
20180006092
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Matter, A.
(Max-Planck-Inst. fuer Radioastronomie Bonn, Germany)
Defrere, D.
(Max-Planck-Inst. fuer Radioastronomie Bonn, Germany)
Danchi, W. C.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lopez, B.
(Observatoire de la Cote d'Azur Nice, France)
Absil, O.
(Liege Univ. Belgium)
Date Acquired
October 4, 2018
Publication Date
March 6, 2013
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 431
Issue: 2
ISSN: 0035-8711
e-ISSN: 1365-2966
Subject Category
Astrophysics
Report/Patent Number
GSFC-E-DAA-TN8690
GSFC-E-DAA-TN8702
Report Number: GSFC-E-DAA-TN8690
Report Number: GSFC-E-DAA-TN8702
ISSN: 0035-8711
E-ISSN: 1365-2966
Distribution Limits
Public
Copyright
Other
Keywords
circumstellar matter
evolution stars
planetary systems

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