We introduce the 4-metre Multi-Object Spectroscopic Telescope (4MOST), a new high-multiplex, wide-field spectroscopic survey facility under development for the four-metre-class Visible and Infrared Survey Telescope for Astronomy (VISTA) at Paranal. Its key specifications are: a large field of view (FoV) of 4.2 square degrees and a high multiplex capability, with 1624 fibres feeding two low-resolution spectrographs (R = λ/Δλ 6500), and 812 fibres transferring light to the high-resolution spectrograph (R 20 000). After a description of the instrument and its expected performance, a short overview is given of its operational scheme and planned 4MOST Consortium science; these aspects are covered in more detail in other articles in this edition of The Messenger. Finally, the processes, schedules, and policies concerning the selection of ESO Community Surveys are presented, commencing with a singular opportunity to submit Letters of Intent for Public Surveys during the first five years of 4MOST operations.

4MOST: Project overview and information for the First Call for Proposals / Roelof S. De Jong, Oscar Agertz, Alex Agudo Berbel, James Aird, David A. Alexander, Anish Amarsi, Friedrich Anders, Rene Andrae, Behzad Ansarinejad, Wolfgang Ansorge, Pierre Antilogus, Heiko Anwand-Heerwart, Anke Arentsen, Anna Arnadottir, Martin Asplund, Matt Auger, Nicolas Azais, Dietrich Baade, Gabriella Baker, Sufyan Baker, et al.. - In: THE MESSENGER. - ISSN 0722-6691. - ELETTRONICO. - (2019), pp. 0-0. [10.18727/0722-6691/5117]

4MOST: Project overview and information for the First Call for Proposals

Cristina Chiappini;David Murphy;Thomas Schmidt;Asa Skuladottir;
2019

Abstract

We introduce the 4-metre Multi-Object Spectroscopic Telescope (4MOST), a new high-multiplex, wide-field spectroscopic survey facility under development for the four-metre-class Visible and Infrared Survey Telescope for Astronomy (VISTA) at Paranal. Its key specifications are: a large field of view (FoV) of 4.2 square degrees and a high multiplex capability, with 1624 fibres feeding two low-resolution spectrographs (R = λ/Δλ 6500), and 812 fibres transferring light to the high-resolution spectrograph (R 20 000). After a description of the instrument and its expected performance, a short overview is given of its operational scheme and planned 4MOST Consortium science; these aspects are covered in more detail in other articles in this edition of The Messenger. Finally, the processes, schedules, and policies concerning the selection of ESO Community Surveys are presented, commencing with a singular opportunity to submit Letters of Intent for Public Surveys during the first five years of 4MOST operations.
2019
0
0
Roelof S. De Jong; Oscar Agertz; Alex Agudo Berbel; James Aird; David A. Alexander; Anish Amarsi; Friedrich Anders; Rene Andrae; Behzad Ansarinejad; W...espandi
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/1313349
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