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Start Over Author "Meneux B." Journal publications of the astronomical society of the pacific
4 results on '"Meneux B."'

1. The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface

Author

Scodeggio, M., Franzetti, P., Garilli, B., Zanichelli, A., Paltani, S., Maccagni, D., Bottini, D., Le Brun, V., Contini, T., Scaramella, R., Adami, C., Bardelli, S., Zucca, E., Tresse, L., Ilbert, O., Foucaud, S., Iovino, A., Merighi, R., Zamorani, G., Gavignaud, I., Rizzo, D., McCracken, H. J., Le Fèvre, O., Picat, J. P., Vettolani, G., Arnaboldi, M., Arnouts, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Guzzo, L., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Pellò, R., Pollo, A., Pozzetti, L., and Radovich, M.

Published
2005
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2. The VIMOS Integral Field Unit: Data‐Reduction Methods and Quality Assessment

Author

Zanichelli, A., Garilli, B., Scodeggio, M., Franzetti, P., Rizzo, D., Maccagni, D., Merighi, R., Picat, J. P., Le Fèvre, O., Foucaud, S., Bottini, D., Le Brun, V., Scaramella, R., Tresse, L., Vettolani, G., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Gavignaud, I., Guzzo, L., Ilbert, O., Iovino, A., McCracken, H. J., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Paltani, S., Pellò, R., Pollo, A., Pozzetti, L., Radovich, M., Zamorani, G., and Zucca, E.

Published
2005
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3. The Very Large Telescope Visible Multi‐Object Spectrograph Mask Preparation Software

Author

Bottini, D., Garilli, B., Maccagni, D., Tresse, L., Le Brun, V., Le Fèvre, O., Picat, J. P., Scaramella, R., Scodeggio, M., Vettolani, G., Zanichelli, A., Adami, C., Arnaboldi, M., Arnouts, S., Bardelli, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., Foucaud, S., Franzetti, P., Guzzo, L., Ilbert, O., Iovino, A., McCracken, H. J., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Merighi, R., Paltani, S., Pollo, A., Pozzetti, L., Radovich, M., Zamorani, G., and Zucca, E.

Published
2005
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4. The Very Large Telescope Visible Multi‐Object Spectrograph Mask Preparation Software

Author

G. Mathez, G. Vettolani, Magda Arnaboldi, A. Pollo, C. Adami, Alain Mazure, S. Paltani, Roberto Scaramella, D. Maccagni, A. Cappi, B. Garilli, V. Le Brun, O. Ilbert, R. Merighi, T. Contini, E. Zucca, S. Bardelli, M. Bolzonella, Stephane Charlot, H. J. McCracken, A. Iovino, J. P. Picat, L. Tresse, D. Bottini, B. Meneux, Stephane Arnouts, Bruno Marano, Sylvie Foucaud, Lucia Pozzetti, Christian Marinoni, P. Franzetti, O. Le Fevre, Paolo Ciliegi, Mario Radovich, A. Zanichelli, Marco Scodeggio, Luigi Guzzo, G. Zamorani, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astronomico di Capodimonte (OAC), Istituto Nazionale di Astrofisica (INAF), Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Institut d'Astrophysique de Paris (IAP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Astrophysik (MPA), Max-Planck-Gesellschaft, Services communs OMP (UMS 831), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Università di Bologna, Dipartimento di Astronomia, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Bottini D., Garilli B., Maccagni D., Tresse L., Le Brun V., Le Fèvre O., Picat J. P., Scaramella R., Scodeggio M., Vettolani G., Zanichelli A., Adami C., Arnaboldi M., Arnouts S., Bardelli S., Bolzonella M., Cappi A., Charlot S., Ciliegi P., Contini T., Foucaud S., Franzetti P., Guzzo L., Ilbert O., Iovino A., McCracken H. J., Marano B., Marinoni C., Mathez G., Mazure A., Meneux B., Merighi R., Paltani S., Pollo A., Pozzetti L., Radovich M., Zamorani G., and Zucca E.

Subjects
Physics, Very Large Telescope, Single exposure, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, business.industry, Software tool, Instrumentation: Spectrographs, Techniques: Spectroscopic, Astronomy and Astrophysics, Object (computer science), 01 natural sciences, Multiplexing, Software, Optics, Space and Planetary Science, Observatory, Methods: Numerical, 0103 physical sciences, business, 010303 astronomy & astrophysics, Spectrograph, Remote sensing
Abstract

VIMOS (Visible Multi-Object Spectrograph) is a multiobject imaging spectrograph installed at the VLT (Very large Telescope) at the ESO (European Southern Observatory) Paranal Observatory that is especially suited for survey work. VIMOS is characterized by its very high multiplexing factor: it is possible to take up to 800 spectra with 10" long slits in a single exposure. To fully exploit its multiplexing potential, we designed and implemented a dedicated software tool: the VIMOS Mask Preparation Software (VMMPS), which allows the astronomer to select the objects to be spectroscopically observed, and provides for automatic slit positioning and slit number maximization within the instrumental constraints. The output of VMMPS is used to manufacture the slit masks to be mounted in the instrument for spectroscopic observations.

Published
2005
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