The 4MOST instrument concept overview

Roger Haynes; Sam Barden; Roelof de Jong; Olivier Schnurr; Olga Bellido; Jakob Walcher; Dionne Haynes; Roland Winkler; Svend-Marian Bauer; Frank Dionies; Allar Saviauk; Cristina Chiappini; Axel Schwope; Joar Brynnel; Matthias Steinmetz; Richard McMahon; Sofia Feltzing; Patrick Francois; Scott Trager; Ian Parry; Mike Irwin; Nicholas Walton; David King; David Sun; Eduaro Gonzalez-Solares; Ian Tosh; Gavin Dalton; Kevin Middleton; Piercarlo Bonifacio; Pascal Jagourel; Shan. Mignot; Mathieu Cohen; Jean-Philippe Amans; Frederic Royer; Paola Sartoretti; Johan Pragt; Gerrit Gerlofsma; Ronald Roelfsema; Ramon Navarro; Guido Thimm; Walter Seifert; Norbert Christleib; Holger Mandel; Trifon Trifonov; Wenli Xu; Florian Lang-Bardl; Bernard Muschielok; Jeorg Schlichter; Hans-Joachim Hess; Frank Grupp; Hans Boehringer; Thomas Boller; Tom Dwelly; Ralf Bender; Piero Rosati; Olaf Iwert; Gert Finger; Jean-Louis Lizon L'Allemand; Will Saunders; Andrew Sheinis; Gabriella Frost; Tony Farrell; Lew Waller; Eric Depagne; Florence Laurent; Patrick Caillier; Johan Kosmalski; Johan Richard; Roland Bacon; Wolfgang Ansorge

doi:10.1117/12.2057253

The 4MOST instrument concept overview

Roger Haynes, Sam Barden, Roelof de Jong, Olivier Schnurr, Olga Bellido, Jakob Walcher, Dionne Haynes, Roland Winkler, Svend-Marian Bauer, Frank Dionies, Allar Saviauk, Cristina Chiappini, Axel Schwope, Joar Brynnel, Matthias Steinmetz, Richard McMahon, Sofia Feltzing, Patrick Francois, Scott Trager, Ian ParryMike Irwin, Nicholas Walton, David King, David Sun, Eduaro Gonzalez-Solares, Ian Tosh, Gavin Dalton, Kevin Middleton, Piercarlo Bonifacio, Pascal Jagourel, Shan. Mignot, Mathieu Cohen, Jean-Philippe Amans, Frederic Royer, Paola Sartoretti, Johan Pragt, Gerrit Gerlofsma, Ronald Roelfsema, Ramon Navarro, Guido Thimm, Walter Seifert, Norbert Christleib, Holger Mandel, Trifon Trifonov, Wenli Xu, Florian Lang-Bardl, Bernard Muschielok, Jeorg Schlichter, Hans-Joachim Hess, Frank Grupp, Hans Boehringer, Thomas Boller, Tom Dwelly, Ralf Bender, Piero Rosati, Olaf Iwert, Gert Finger, Jean-Louis Lizon L'Allemand, Will Saunders, Andrew Sheinis, Gabriella Frost, Tony Farrell, Lew Waller, Eric Depagne, Florence Laurent, Patrick Caillier, Johan Kosmalski, Johan Richard, Roland Bacon, Wolfgang Ansorge

Astronomi - Genomgår omorganisation

Forskningsoutput: Kapitel i bok/rapport/Conference proceeding › Konferenspaper i proceeding › Peer review

Sammanfattning

The 4MOST([1]) instrument is a concept for a wide-field, fibre-fed high multiplex spectroscopic instrument facility on the ESO VISTA telescope designed to perform a massive (initially >25x10(6) spectra in 5 years) combined all-sky public survey. The main science drivers are: Gaia follow up of chemo-dynamical structure of the Milky Way, stellar radial velocities, parameters and abundances, chemical tagging; eROSITA follow up of cosmology with x-ray clusters of galaxies, X-ray AGN/galaxy evolution to z similar to 5, Galactic X-ray sources and resolving the Galactic edge; Euclid/LSST/SKA and other survey follow up of Dark Energy, Galaxy evolution and transients. The surveys will be undertaken simultaneously requiring: highly advanced targeting and scheduling software, also comprehensive data reduction and analysis tools to produce high-level data products. The instrument will allow simultaneous observations of similar to 1600 targets at R similar to 5,000 from 390-900nm and similar to 800 targets at R>18,000 in three channels between similar to 395-675nm (channel bandwidth: 45nm blue, 57nm green and 69nm red) over a hexagonal field of view of similar to 4.1 degrees2. The initial 5-year 4MOST survey is currently expect to start in 2020. We provide and overview of the 4MOST systems: opto-mechanical, control, data management and operations concepts; and initial performance estimates.

Originalspråk	engelska
Titel på värdpublikation	Ground-based and Airborne Instrumentation for Astronomy V
Förlag	SPIE
Sidor	91476I
Volym	9147
DOI	https://doi.org/10.1117/12.2057253
Status	Published - 2014
Evenemang	5th Conference on Ground-Based and Airborne Instrumentation for Astronomy - Montreal, Kanada Varaktighet: 2014 juni 22 → 2014 juni 26

Publikationsserier

Namn
Volym	9147
ISSN (tryckt)	1996-756X
ISSN (elektroniskt)	0277-786X

Konferens

Konferens	5th Conference on Ground-Based and Airborne Instrumentation for Astronomy
Land/Territorium	Kanada
Ort	Montreal
Period	2014/06/22 → 2014/06/26

Ämnesklassifikation (UKÄ)

Astronomi, astrofysik och kosmologi

Tillgång till dokument

10.1117/12.2057253

NMW: The New Milky Way
Feltzing, S., Bensby, T., Lindegren, L., Church, R., Hobbs, D., Ryde, N., Hartman, H., Mcmillan, P., Traven, G., Feuillet, D., Sahlholdt, C., Howes, L. & Stonkute, E.
Knut and Alice Wallenberg Foundation
2014/07/01 → 2027/06/30
Projekt: Forskning
4MOST: 4MOST - massive spectroscopic surveys of the Milky Way and the Universe
Feltzing, S., Church, R., Hobbs, D., Bensby, T., Ryde, N., Hartman, H., Mcmillan, P., Jönsson, H., Agertz, O., Howes, L., Kushniruk, I., Agertz, O., Traven, G. & Feuillet, D.
2011/01/01 → 2029/12/31
Projekt: Forskning

Citera det här

Haynes, R., Barden, S., de Jong, R., Schnurr, O., Bellido, O., Walcher, J., Haynes, D., Winkler, R., Bauer, S-M., Dionies, F., Saviauk, A., Chiappini, C., Schwope, A., Brynnel, J., Steinmetz, M., McMahon, R., Feltzing, S., Francois, P., Trager, S., ... Ansorge, W. (2014). The 4MOST instrument concept overview. I Ground-based and Airborne Instrumentation for Astronomy V (Vol. 9147, s. 91476I). SPIE. https://doi.org/10.1117/12.2057253

@inproceedings{b54e68073f4a4ff592caa220c1da5ab3,

title = "The 4MOST instrument concept overview",

abstract = "The 4MOST([1]) instrument is a concept for a wide-field, fibre-fed high multiplex spectroscopic instrument facility on the ESO VISTA telescope designed to perform a massive (initially >25x10(6) spectra in 5 years) combined all-sky public survey. The main science drivers are: Gaia follow up of chemo-dynamical structure of the Milky Way, stellar radial velocities, parameters and abundances, chemical tagging; eROSITA follow up of cosmology with x-ray clusters of galaxies, X-ray AGN/galaxy evolution to z similar to 5, Galactic X-ray sources and resolving the Galactic edge; Euclid/LSST/SKA and other survey follow up of Dark Energy, Galaxy evolution and transients. The surveys will be undertaken simultaneously requiring: highly advanced targeting and scheduling software, also comprehensive data reduction and analysis tools to produce high-level data products. The instrument will allow simultaneous observations of similar to 1600 targets at R similar to 5,000 from 390-900nm and similar to 800 targets at R>18,000 in three channels between similar to 395-675nm (channel bandwidth: 45nm blue, 57nm green and 69nm red) over a hexagonal field of view of similar to 4.1 degrees2. The initial 5-year 4MOST survey is currently expect to start in 2020. We provide and overview of the 4MOST systems: opto-mechanical, control, data management and operations concepts; and initial performance estimates.",

keywords = "4MOST, VISTA, spectroscopic facility, wide field MOS, multi-object, optical fibre, system design",

author = "Roger Haynes and Sam Barden and {de Jong}, Roelof and Olivier Schnurr and Olga Bellido and Jakob Walcher and Dionne Haynes and Roland Winkler and Svend-Marian Bauer and Frank Dionies and Allar Saviauk and Cristina Chiappini and Axel Schwope and Joar Brynnel and Matthias Steinmetz and Richard McMahon and Sofia Feltzing and Patrick Francois and Scott Trager and Ian Parry and Mike Irwin and Nicholas Walton and David King and David Sun and Eduaro Gonzalez-Solares and Ian Tosh and Gavin Dalton and Kevin Middleton and Piercarlo Bonifacio and Pascal Jagourel and Shan. Mignot and Mathieu Cohen and Jean-Philippe Amans and Frederic Royer and Paola Sartoretti and Johan Pragt and Gerrit Gerlofsma and Ronald Roelfsema and Ramon Navarro and Guido Thimm and Walter Seifert and Norbert Christleib and Holger Mandel and Trifon Trifonov and Wenli Xu and Florian Lang-Bardl and Bernard Muschielok and Jeorg Schlichter and Hans-Joachim Hess and Frank Grupp and Hans Boehringer and Thomas Boller and Tom Dwelly and Ralf Bender and Piero Rosati and Olaf Iwert and Gert Finger and L'Allemand, {Jean-Louis Lizon} and Will Saunders and Andrew Sheinis and Gabriella Frost and Tony Farrell and Lew Waller and Eric Depagne and Florence Laurent and Patrick Caillier and Johan Kosmalski and Johan Richard and Roland Bacon and Wolfgang Ansorge",

year = "2014",

doi = "10.1117/12.2057253",

language = "English",

volume = "9147",

publisher = "SPIE",

pages = "91476I",

booktitle = "Ground-based and Airborne Instrumentation for Astronomy V",

address = "United States",

note = "5th Conference on Ground-Based and Airborne Instrumentation for Astronomy ; Conference date: 22-06-2014 Through 26-06-2014",

}

Haynes, R, Barden, S, de Jong, R, Schnurr, O, Bellido, O, Walcher, J, Haynes, D, Winkler, R, Bauer, S-M, Dionies, F, Saviauk, A, Chiappini, C, Schwope, A, Brynnel, J, Steinmetz, M, McMahon, R, Feltzing, S, Francois, P, Trager, S, Parry, I, Irwin, M, Walton, N, King, D, Sun, D, Gonzalez-Solares, E, Tosh, I, Dalton, G, Middleton, K, Bonifacio, P, Jagourel, P, Mignot, S, Cohen, M, Amans, J-P, Royer, F, Sartoretti, P, Pragt, J, Gerlofsma, G, Roelfsema, R, Navarro, R, Thimm, G, Seifert, W, Christleib, N, Mandel, H, Trifonov, T, Xu, W, Lang-Bardl, F, Muschielok, B, Schlichter, J, Hess, H-J, Grupp, F, Boehringer, H, Boller, T, Dwelly, T, Bender, R, Rosati, P, Iwert, O, Finger, G, L'Allemand, J-LL, Saunders, W, Sheinis, A, Frost, G, Farrell, T, Waller, L, Depagne, E, Laurent, F, Caillier, P, Kosmalski, J, Richard, J, Bacon, R & Ansorge, W 2014, The 4MOST instrument concept overview. i Ground-based and Airborne Instrumentation for Astronomy V. vol. 9147, SPIE, s. 91476I, 5th Conference on Ground-Based and Airborne Instrumentation for Astronomy, Montreal, Kanada, 2014/06/22. https://doi.org/10.1117/12.2057253

TY - GEN

T1 - The 4MOST instrument concept overview

AU - Haynes, Roger

AU - Barden, Sam

AU - de Jong, Roelof

AU - Schnurr, Olivier

AU - Bellido, Olga

AU - Walcher, Jakob

AU - Haynes, Dionne

AU - Winkler, Roland

AU - Bauer, Svend-Marian

AU - Dionies, Frank

AU - Saviauk, Allar

AU - Chiappini, Cristina

AU - Schwope, Axel

AU - Brynnel, Joar

AU - Steinmetz, Matthias

AU - McMahon, Richard

AU - Feltzing, Sofia

AU - Francois, Patrick

AU - Trager, Scott

AU - Parry, Ian

AU - Irwin, Mike

AU - Walton, Nicholas

AU - King, David

AU - Sun, David

AU - Gonzalez-Solares, Eduaro

AU - Tosh, Ian

AU - Dalton, Gavin

AU - Middleton, Kevin

AU - Bonifacio, Piercarlo

AU - Jagourel, Pascal

AU - Mignot, Shan.

AU - Cohen, Mathieu

AU - Amans, Jean-Philippe

AU - Royer, Frederic

AU - Sartoretti, Paola

AU - Pragt, Johan

AU - Gerlofsma, Gerrit

AU - Roelfsema, Ronald

AU - Navarro, Ramon

AU - Thimm, Guido

AU - Seifert, Walter

AU - Christleib, Norbert

AU - Mandel, Holger

AU - Trifonov, Trifon

AU - Xu, Wenli

AU - Lang-Bardl, Florian

AU - Muschielok, Bernard

AU - Schlichter, Jeorg

AU - Hess, Hans-Joachim

AU - Grupp, Frank

AU - Boehringer, Hans

AU - Boller, Thomas

AU - Dwelly, Tom

AU - Bender, Ralf

AU - Rosati, Piero

AU - Iwert, Olaf

AU - Finger, Gert

AU - L'Allemand, Jean-Louis Lizon

AU - Saunders, Will

AU - Sheinis, Andrew

AU - Frost, Gabriella

AU - Farrell, Tony

AU - Waller, Lew

AU - Depagne, Eric

AU - Laurent, Florence

AU - Caillier, Patrick

AU - Kosmalski, Johan

AU - Richard, Johan

AU - Bacon, Roland

AU - Ansorge, Wolfgang

PY - 2014

Y1 - 2014

N2 - The 4MOST([1]) instrument is a concept for a wide-field, fibre-fed high multiplex spectroscopic instrument facility on the ESO VISTA telescope designed to perform a massive (initially >25x10(6) spectra in 5 years) combined all-sky public survey. The main science drivers are: Gaia follow up of chemo-dynamical structure of the Milky Way, stellar radial velocities, parameters and abundances, chemical tagging; eROSITA follow up of cosmology with x-ray clusters of galaxies, X-ray AGN/galaxy evolution to z similar to 5, Galactic X-ray sources and resolving the Galactic edge; Euclid/LSST/SKA and other survey follow up of Dark Energy, Galaxy evolution and transients. The surveys will be undertaken simultaneously requiring: highly advanced targeting and scheduling software, also comprehensive data reduction and analysis tools to produce high-level data products. The instrument will allow simultaneous observations of similar to 1600 targets at R similar to 5,000 from 390-900nm and similar to 800 targets at R>18,000 in three channels between similar to 395-675nm (channel bandwidth: 45nm blue, 57nm green and 69nm red) over a hexagonal field of view of similar to 4.1 degrees2. The initial 5-year 4MOST survey is currently expect to start in 2020. We provide and overview of the 4MOST systems: opto-mechanical, control, data management and operations concepts; and initial performance estimates.

AB - The 4MOST([1]) instrument is a concept for a wide-field, fibre-fed high multiplex spectroscopic instrument facility on the ESO VISTA telescope designed to perform a massive (initially >25x10(6) spectra in 5 years) combined all-sky public survey. The main science drivers are: Gaia follow up of chemo-dynamical structure of the Milky Way, stellar radial velocities, parameters and abundances, chemical tagging; eROSITA follow up of cosmology with x-ray clusters of galaxies, X-ray AGN/galaxy evolution to z similar to 5, Galactic X-ray sources and resolving the Galactic edge; Euclid/LSST/SKA and other survey follow up of Dark Energy, Galaxy evolution and transients. The surveys will be undertaken simultaneously requiring: highly advanced targeting and scheduling software, also comprehensive data reduction and analysis tools to produce high-level data products. The instrument will allow simultaneous observations of similar to 1600 targets at R similar to 5,000 from 390-900nm and similar to 800 targets at R>18,000 in three channels between similar to 395-675nm (channel bandwidth: 45nm blue, 57nm green and 69nm red) over a hexagonal field of view of similar to 4.1 degrees2. The initial 5-year 4MOST survey is currently expect to start in 2020. We provide and overview of the 4MOST systems: opto-mechanical, control, data management and operations concepts; and initial performance estimates.

KW - 4MOST

KW - VISTA

KW - spectroscopic facility

KW - wide field MOS

KW - multi-object

KW - optical fibre

KW - system design

U2 - 10.1117/12.2057253

DO - 10.1117/12.2057253

M3 - Paper in conference proceeding

VL - 9147

SP - 91476I

BT - Ground-based and Airborne Instrumentation for Astronomy V

PB - SPIE

T2 - 5th Conference on Ground-Based and Airborne Instrumentation for Astronomy

Y2 - 22 June 2014 through 26 June 2014

ER -

The 4MOST instrument concept overview

Sammanfattning

Publikationsserier

Konferens

Ämnesklassifikation (UKÄ)

Tillgång till dokument

Fingeravtryck

Projekt

NMW: The New Milky Way

4MOST: 4MOST - massive spectroscopic surveys of the Milky Way and the Universe

Citera det här