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  MATISSE: performance in laboratory, results of AIV in Paranal, and first results on sky

Robbe-Dubois, S., Lagarde, S., Antonelli, P., Lopez, B., Allouche, F., Bailet, C., et al. (2018). MATISSE: performance in laboratory, results of AIV in Paranal, and first results on sky.

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Robbe-Dubois, S.1, Author
Lagarde, S.1, Author
Antonelli, P.1, Author
Lopez, B.1, Author
Allouche, F.1, Author
Bailet, C.1, Author
Berio, Ph.1, Author
Bresson, Y.1, Author
Clausse, J. -M.1, Author
Cruzalèbes, P.1, Author
Fantei-Caujolle, Y.1, Author
Marcotto, A.1, Author
Matter, A.1, Author
Meilland, A.1, Author
Millour, F.1, Author
Morel, S.1, Author
Petrov, R. G.1, Author
Rousseau, S.1, Author
Soulain, A.1, Author
Zins, G.1, Author
Lehmitz, M.1, AuthorLaun, W.1, AuthorAdler, T.1, AuthorKlein, R.1, AuthorMaurer, T.1, AuthorBettonvil, F.1, AuthorEldswick, E.1, AuthorBeckmann, U.1, AuthorHeininger, M.1, AuthorBristow, P.1, AuthorGlindemann, A.1, AuthorHubin, N.1, AuthorJochum, L.1, AuthorRivinus, Th.1, AuthorSchoeller, M.1, AuthorBeltran, J.1, AuthorBourget, P.1, AuthorGallenne, A.1, AuthorGuerlet, Th.1, AuthorHaubois, X.1, AuthorIves, D.1, AuthorJakob, G.1, AuthorMeister, A.1, AuthorRiquelme, M.1, AuthorSchuhler, N.1, AuthorStephan, C.1, AuthorToledo, P.1, AuthorTristam, K.1, AuthorWoillez, J.1, AuthorNeumann, U.1, AuthorChelli, A.1, AuthorGuitton, F.1, AuthorMeisenheimer, K.1, AuthorPichon, B.1, AuthorSpang, A.1, AuthorVarga, J.1, AuthorHenning, Th.1, AuthorJaffe, W.1, AuthorPasquini, L.1, AuthorStee, Ph.1, AuthorWeigelt, G.1, Author more..
Affiliations:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

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 Abstract: MATISSE (Multi AperTure mid-Infrared SpectroScopic Experiment) is the spectro-interferometer for the VLTI of the European Southern Observatory (ESO), operating in the L-, M- and N- spectral bands, and combining up to four beams from the unit or the auxiliary telescopes (UTs or ATs). MATISSE will offer new breakthroughs in the study of circumstellar environments by allowing the mapping of the material distribution, the gas and essentially the dust. The instrument consists in a warm optical system (WOP) accepting four beams from the VLTI and relaying them after a spectral splitting to cold optical benches (COB) located in two separate cryostats, one in L-M- band, and one in N-band. The test plan of the complete instrument has been conducted at the Observatoire de la Côte d'Azur in order to confirm the compliance of the performance with the high-level requirements. MATISSE has successfully passed the Preliminary Acceptance in Europe the 12th September 2017. Following this result, ESO gave approval for the instrument to be shipped to Paranal. The Alignment, Integration and Verification phase was conducted until end of February 2018, at the end of which first observations on sky have been performed to test the operations with the VLTI and to obtain first stellar light. The two first runs of the commissioning followed, respectively in March and in May 2018. It has the goal to optimize the MATISSE-VLTI communication, the acquisition procedures and the interface parameters. The observations were performed on bright L-M- and N- stars, with four ATs located on short baselines and UTs. The limit magnitudes will be deduced. This paper reports on the performance of the instrument measured in laboratory (results of test plan in Nice and AIV in Paranal) in terms of spectral coverage, dispersion laws and spectral resolutions, and transfer function analysis: instrumental contrast, visibility accuracy, accuracy of the differential phase, of the closure-phase and of the differential visibility. It also provides results of the first tests on sky and the planning of the on-going commissioning.

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 Dates: 2018
 Publication Status: Issued
 Pages: -
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 Rev. Type: -
 Identifiers: ISBN: 9781510619555
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Title: Optical and Infrared Interferometry and Imaging VI
Place of Event: -
Start-/End Date: 2018

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