MI-6: Michigan interferometry with six telescopes

John D. Monnier; M. Anderson; F. Baron; D. H. Berger; X. Che; T. Eckhause; S. Kraus; E. Pedretti; N. Thureau; R. Millan-Gabet; T. Ten Brummelaar; P. Irwin; M. Zhao

MI-6: Michigan interferometry with six telescopes

John D. Monnier
, M. Anderson
, F. Baron
, D. H. Berger
, X. Che
, T. Eckhause
, S. Kraus
, E. Pedretti
, N. Thureau
, R. Millan-Gabet
, T. Ten Brummelaar
, P. Irwin
, M. Zhao

SAMS UHI

Résultats de recherche: Conference contribution

Résumé

Based on the success of four-telescope imaging with the Michigan Infrared Combiner (MIRC) on the CHARA Array, our Michigan-based group will now upgrade our system to combine all six CHARA telescope simultaneously. In order to make this observationally efficient, we have had to improve a number of subsystems and commission new ones, including the new CHAMP fringe tracker, the introduction of photometric channels,the upgrading of the real time operating systems, and the obvious hardware and software upgrades of the control system and the data pipeline. Here we will discuss the advantages of six-telescope operation, outline our upgrade plans and discuss our current progress.

langue originale	English
titre	Optical and Infrared Interferometry II
Sous-titre	Proceedings of the SPIE
Editeur	SPIE
Pages	13
Volume	7734
état	Published - 1 juil. 2010

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http://adsabs.harvard.edu/abs/2010SPIE.7734E..13M

Contient cette citation

Monnier, J. D., Anderson, M., Baron, F., Berger, D. H., Che, X., Eckhause, T., Kraus, S., Pedretti, E., Thureau, N., Millan-Gabet, R., Ten Brummelaar, T., Irwin, P., & Zhao, M. (2010). MI-6: Michigan interferometry with six telescopes. Dans Optical and Infrared Interferometry II: Proceedings of the SPIE (Vol 7734, p. 13). SPIE. http://adsabs.harvard.edu/abs/2010SPIE.7734E..13M

@inproceedings{07ef454e752a4982a52ef6b6fec391d8,

title = "MI-6: Michigan interferometry with six telescopes",

abstract = "Based on the success of four-telescope imaging with the Michigan Infrared Combiner (MIRC) on the CHARA Array, our Michigan-based group will now upgrade our system to combine all six CHARA telescope simultaneously. In order to make this observationally efficient, we have had to improve a number of subsystems and commission new ones, including the new CHAMP fringe tracker, the introduction of photometric channels,the upgrading of the real time operating systems, and the obvious hardware and software upgrades of the control system and the data pipeline. Here we will discuss the advantages of six-telescope operation, outline our upgrade plans and discuss our current progress.",

author = "Monnier, \{John D.\} and M. Anderson and F. Baron and Berger, \{D. H.\} and X. Che and T. Eckhause and S. Kraus and E. Pedretti and N. Thureau and R. Millan-Gabet and \{Ten Brummelaar\}, T. and P. Irwin and M. Zhao",

year = "2010",

month = jul,

day = "1",

language = "English",

volume = "7734",

pages = "13",

booktitle = "Optical and Infrared Interferometry II",

publisher = "SPIE",

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TY - GEN

T1 - MI-6: Michigan interferometry with six telescopes

AU - Monnier, John D.

AU - Anderson, M.

AU - Baron, F.

AU - Berger, D. H.

AU - Che, X.

AU - Eckhause, T.

AU - Kraus, S.

AU - Pedretti, E.

AU - Thureau, N.

AU - Millan-Gabet, R.

AU - Ten Brummelaar, T.

AU - Irwin, P.

AU - Zhao, M.

PY - 2010/7/1

Y1 - 2010/7/1

N2 - Based on the success of four-telescope imaging with the Michigan Infrared Combiner (MIRC) on the CHARA Array, our Michigan-based group will now upgrade our system to combine all six CHARA telescope simultaneously. In order to make this observationally efficient, we have had to improve a number of subsystems and commission new ones, including the new CHAMP fringe tracker, the introduction of photometric channels,the upgrading of the real time operating systems, and the obvious hardware and software upgrades of the control system and the data pipeline. Here we will discuss the advantages of six-telescope operation, outline our upgrade plans and discuss our current progress.

AB - Based on the success of four-telescope imaging with the Michigan Infrared Combiner (MIRC) on the CHARA Array, our Michigan-based group will now upgrade our system to combine all six CHARA telescope simultaneously. In order to make this observationally efficient, we have had to improve a number of subsystems and commission new ones, including the new CHAMP fringe tracker, the introduction of photometric channels,the upgrading of the real time operating systems, and the obvious hardware and software upgrades of the control system and the data pipeline. Here we will discuss the advantages of six-telescope operation, outline our upgrade plans and discuss our current progress.

M3 - Conference contribution

VL - 7734

SP - 13

BT - Optical and Infrared Interferometry II

PB - SPIE

ER -

MI-6: Michigan interferometry with six telescopes

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