Characterizing closure-phase measurements at IOTA

S. Ragland; W.~A. Traub; J.-P. Berger; R. Millan-Gabet; J.~D. Monnier; E. Pedretti; F.~P. Schloerb; N.~P. Carleton; P. Haguenauer; P.~Y. Kern; P.~R. Labeye; M.~G. Lacasse; F. Malbet; K. Rousselet-Perraut

doi:10.1117/12.552447

Characterizing closure-phase measurements at IOTA

S. Ragland, W.~A. Traub, J.-P. Berger, R. Millan-Gabet, J.~D. Monnier, E. Pedretti, F.~P. Schloerb, N.~P. Carleton, P. Haguenauer, P.~Y. Kern, P.~R. Labeye, M.~G. Lacasse, F. Malbet, K. Rousselet-Perraut

School of Engineering & Physical Sciences

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

6 Citations (Scopus)

Abstract

We are working towards imaging the surfaces and circumstellar envelopes of Mira stars in the near-infrared, using the IOTA interferometer and the IONIC integrated-optics 3-beam combiner. In order to study atmospheric structures of these stars, we installed 3 narrow-band filters that subdivide H-band into 3 roughly equal-width sub-bands - a central one for continuum, and 2 adjacent ones to sample Mira star's (mostly water) absorption-bands. We present here our characterization of the IOTA 3-Telescope interferometer for closure-phase measurements with broad and narrow-band filters in the H atmospheric window. This includes characterizing the stability, chromaticity, and polarization effects of the present IOTA optics with the IONIC beam-combiner, and characterizing the accuracy of our closure phase measurements.

Original language	Undefined/Unknown
Title of host publication	New Frontiers in Stellar Interferometry
Editors	W.~A. Traub
Pages	1390
Number of pages	1
Volume	5491
DOIs	https://doi.org/10.1117/12.552447
Publication status	Published - 20 Oct 2004

Publication series

Name	Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

Access to Document

10.1117/12.552447

Cite this

Ragland, S., Traub, W. A., Berger, J.-P., Millan-Gabet, R., Monnier, J. D., Pedretti, E., Schloerb, F. P., Carleton, N. P., Haguenauer, P., Kern, P. Y., Labeye, P. R., Lacasse, M. G., Malbet, F., & Rousselet-Perraut, K. (2004). Characterizing closure-phase measurements at IOTA. In W. A. Traub (Ed.), New Frontiers in Stellar Interferometry (Vol. 5491, pp. 1390). (Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series). https://doi.org/10.1117/12.552447

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title = "Characterizing closure-phase measurements at IOTA",

abstract = "We are working towards imaging the surfaces and circumstellar envelopes of Mira stars in the near-infrared, using the IOTA interferometer and the IONIC integrated-optics 3-beam combiner. In order to study atmospheric structures of these stars, we installed 3 narrow-band filters that subdivide H-band into 3 roughly equal-width sub-bands - a central one for continuum, and 2 adjacent ones to sample Mira star's (mostly water) absorption-bands. We present here our characterization of the IOTA 3-Telescope interferometer for closure-phase measurements with broad and narrow-band filters in the H atmospheric window. This includes characterizing the stability, chromaticity, and polarization effects of the present IOTA optics with the IONIC beam-combiner, and characterizing the accuracy of our closure phase measurements.",

author = "S. Ragland and W.~A. Traub and J.-P. Berger and R. Millan-Gabet and J.~D. Monnier and E. Pedretti and F.~P. Schloerb and N.~P. Carleton and P. Haguenauer and P.~Y. Kern and P.~R. Labeye and M.~G. Lacasse and F. Malbet and K. Rousselet-Perraut",

year = "2004",

month = oct,

day = "20",

doi = "10.1117/12.552447",

language = "Undefined/Unknown",

volume = "5491",

series = "Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series",

pages = "1390",

editor = "W.~A. Traub",

booktitle = "New Frontiers in Stellar Interferometry",

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Ragland, S, Traub, WA, Berger, J-P, Millan-Gabet, R, Monnier, JD, Pedretti, E, Schloerb, FP, Carleton, NP, Haguenauer, P, Kern, PY, Labeye, PR, Lacasse, MG, Malbet, F & Rousselet-Perraut, K 2004, Characterizing closure-phase measurements at IOTA. in WA Traub (ed.), New Frontiers in Stellar Interferometry. vol. 5491, Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, pp. 1390. https://doi.org/10.1117/12.552447

TY - GEN

T1 - Characterizing closure-phase measurements at IOTA

AU - Ragland, S.

AU - Traub, W.~A.

AU - Berger, J.-P.

AU - Millan-Gabet, R.

AU - Monnier, J.~D.

AU - Pedretti, E.

AU - Schloerb, F.~P.

AU - Carleton, N.~P.

AU - Haguenauer, P.

AU - Kern, P.~Y.

AU - Labeye, P.~R.

AU - Lacasse, M.~G.

AU - Malbet, F.

AU - Rousselet-Perraut, K.

PY - 2004/10/20

Y1 - 2004/10/20

N2 - We are working towards imaging the surfaces and circumstellar envelopes of Mira stars in the near-infrared, using the IOTA interferometer and the IONIC integrated-optics 3-beam combiner. In order to study atmospheric structures of these stars, we installed 3 narrow-band filters that subdivide H-band into 3 roughly equal-width sub-bands - a central one for continuum, and 2 adjacent ones to sample Mira star's (mostly water) absorption-bands. We present here our characterization of the IOTA 3-Telescope interferometer for closure-phase measurements with broad and narrow-band filters in the H atmospheric window. This includes characterizing the stability, chromaticity, and polarization effects of the present IOTA optics with the IONIC beam-combiner, and characterizing the accuracy of our closure phase measurements.

AB - We are working towards imaging the surfaces and circumstellar envelopes of Mira stars in the near-infrared, using the IOTA interferometer and the IONIC integrated-optics 3-beam combiner. In order to study atmospheric structures of these stars, we installed 3 narrow-band filters that subdivide H-band into 3 roughly equal-width sub-bands - a central one for continuum, and 2 adjacent ones to sample Mira star's (mostly water) absorption-bands. We present here our characterization of the IOTA 3-Telescope interferometer for closure-phase measurements with broad and narrow-band filters in the H atmospheric window. This includes characterizing the stability, chromaticity, and polarization effects of the present IOTA optics with the IONIC beam-combiner, and characterizing the accuracy of our closure phase measurements.

U2 - 10.1117/12.552447

DO - 10.1117/12.552447

M3 - Conference contribution

VL - 5491

T3 - Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

SP - 1390

BT - New Frontiers in Stellar Interferometry

A2 - Traub, W.~A.

ER -