Characterizing closure-phase measurements at IOTA

Sam Ragland; Wesley A. Traub; Jean-Philippe Berger; Rafael Millan-Gabet; John D. Monnier; Ettore Pedretti; F. P. Schloerb; Nathaniel P. Carleton; Pierre Haguenauer; Pierre Y. Kern; Pierre R. Labeye; Marc G. Lacasse; Fabien Malbet; Karine Rousselet-Perraut

Characterizing closure-phase measurements at IOTA

Sam Ragland
, Wesley A. Traub
, Jean-Philippe Berger
, Rafael Millan-Gabet
, John D. Monnier
, Ettore Pedretti
, F. P. Schloerb
, Nathaniel P. Carleton
, Pierre Haguenauer
, Pierre Y. Kern
, Pierre R. Labeye
, Marc G. Lacasse
, Fabien Malbet
, Karine Rousselet-Perraut

SAMS UHI

Producción científica: Article › revisión exhaustiva

7 Citas (Scopus)

Resumen

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.

Idioma original	English
Páginas (desde-hasta)	1390
Publicación	New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The International Society for Optical Engineering, 2004., p.1390
Volumen	5491
Estado	Published - 1 oct 2004

Acceder al documento

http://adsabs.harvard.edu/abs/2004SPIE.5491.1390R

Citar esto

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. New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The International Society for Optical Engineering, 2004., p.1390, 5491, 1390. http://adsabs.harvard.edu/abs/2004SPIE.5491.1390R

@article{5ae0c0635769428a8d624370459d29b2,

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 = "Sam Ragland and Traub, \{Wesley A.\} and Jean-Philippe Berger and Rafael Millan-Gabet and Monnier, \{John D.\} and Ettore Pedretti and Schloerb, \{F. P.\} and Carleton, \{Nathaniel P.\} and Pierre Haguenauer and Kern, \{Pierre Y.\} and Labeye, \{Pierre R.\} and Lacasse, \{Marc G.\} and Fabien Malbet and Karine Rousselet-Perraut",

year = "2004",

month = oct,

day = "1",

language = "English",

volume = "5491",

pages = "1390",

journal = "New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The International Society for Optical Engineering, 2004., p.1390",

publisher = "SPIE",

}

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', New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The International Society for Optical Engineering, 2004., p.1390, vol. 5491, pp. 1390. <http://adsabs.harvard.edu/abs/2004SPIE.5491.1390R>

Characterizing closure-phase measurements at IOTA. / Ragland, Sam; Traub, Wesley A.; Berger, Jean-Philippe et al.
En: New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The International Society for Optical Engineering, 2004., p.1390, Vol. 5491, 01.10.2004, p. 1390.

Producción científica: Article › revisión exhaustiva

TY - JOUR

T1 - Characterizing closure-phase measurements at IOTA

AU - Ragland, Sam

AU - Traub, Wesley A.

AU - Berger, Jean-Philippe

AU - Millan-Gabet, Rafael

AU - Monnier, John D.

AU - Pedretti, Ettore

AU - Schloerb, F. P.

AU - Carleton, Nathaniel P.

AU - Haguenauer, Pierre

AU - Kern, Pierre Y.

AU - Labeye, Pierre R.

AU - Lacasse, Marc G.

AU - Malbet, Fabien

AU - Rousselet-Perraut, Karine

PY - 2004/10/1

Y1 - 2004/10/1

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.

M3 - Article

VL - 5491

SP - 1390

JO - New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The International Society for Optical Engineering, 2004., p.1390

JF - New Frontiers in Stellar Interferometry, Proceedings of SPIE Volume 5491. Edited by Wesley A. Traub. Bellingham, WA: The International Society for Optical Engineering, 2004., p.1390

ER -

Characterizing closure-phase measurements at IOTA

Resumen

Acceder al documento

Huella

Citar esto