4MOST: Project overview and information for the First Call for Proposals
arXiv:1903.02464 · doi:10.18727/0722-6691/5117
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 (), and 812 fibres transferring light to the high-resolution spectrograph (). 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.
Part of the 4MOST issue of The Messenger, published in preparation of 4MOST Community Workshop, see http://www.eso.org/sci/meetings/2019/4MOST.html
Cited by in corpus (64)
- Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
- The Global Dynamical Atlas of the Milky Way mergers: Constraints from Gaia EDR3 based orbits of globular clusters, stellar streams and satellite galaxies
- Detection of the Milky Way reflex motion due to the Large Magellanic Cloud infall
- All-purpose, all-sky photometric redshifts for the Legacy Imaging Surveys Data Release 8
- Overview of the LAMOST survey in the first decade
- Galaxy And Mass Assembly (GAMA): Assimilation of KiDS into the GAMA database
- The 40 pc sample of white dwarfs from Gaia
- OzDES multi-object fibre spectroscopy for the Dark Energy Survey: Results and second data release
- white dwarfs within 40 pc I: spectroscopic observations of new candidates
- The Impact of Metallicity on the Evolution of Rotation and Magnetic Activity of Sun-Like Stars
- Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
- The Pristine Inner Galaxy Survey (PIGS) II: Uncovering the most metal-poor populations in the inner Milky Way
- IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
- Ultra-faint dwarf galaxies: unveiling the minimum mass of the first stars
- BACCHUS Analysis of Weak Lines in APOGEE Spectra (BAWLAS)
- white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere
- The VMC survey -- XLIV: Mapping metallicity trends in the Large Magellanic Cloud using near-infrared passbands
- Gaia EDR3 in 6D: Searching for unbound stars in the Galaxy
- The Pristine survey XIII: Uncovering the very metal-poor tail of the thin disc
- Metal line emission from galaxy haloes at z~1
- A local measurement of the growth rate from peculiar velocities and galaxy clustering correlations in the 6dF Galaxy Survey
- Features of Gaia DR3 Spectroscopic Binaries I. Tidal circularization of Main-Sequence Stars
- Evidence of First Stars-enriched Gas in High-redshift Absorbers
- Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
- Estimating AGN Black Hole Masses via Continuum Reverberation Mapping in the Era of LSST
- The Pristine survey -- XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations
- Extracting Photometric Redshift from Galaxy Flux and Image Data using Neural Networks in the CSST Survey
- PISN-explorer: hunting the descendants of very massive first stars
- Assessing the accuracy of cosmological parameters estimated from velocity -- density comparisons via simulations
- Origin of metals in old Milky Way halo stars based on GALAH and Gaia
- Constraining planet formation around 6-8 stars
- Detecting Globular Cluster Tidal Extensions with Bayesian Inference: I. Analysis of Centauri with Gaia EDR3
- On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
- Study of the departures from LTE in the unevolved stars infra-red spectra
- MUSE-ALMA Halos XI: Gas flows in the circumgalactic medium
- Uranium Abundances and Ages of -process Enhanced Stars with Novel U II Lines
- Constraining Cosmic Inflation with Observations: Prospects for 2030
- Stars in the Local Galactic Thick Disk and Halo in Gaia EDR3: A catalogue of Half a Million Local Main-sequence Stars with Photometric Metallicities
- Model-independent way to determine the Hubble constant and the curvature from phase shift of gravitational waves with DECIGO
- Quantifying kinematic substructure in star-forming regions with statistical tests of spatial autocorrelation
- Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
- Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
- Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models
- A machine learning approach to photometric metallicities of giant stars
- Emission Line Galaxies in the SHARDS Frontier Fields I: Candidate Selection and the Discovery of Bursty Hα Emitters
- An optimised tiling pattern for multi-object spectroscopic surveys: application to the 4MOST survey
- Tracing the 10K Warm-Hot Intergalactic Medium with UV absorption lines
- Fundamental effective temperature measurements for eclipsing binary stars -- II. The detached F-type eclipsing binary CPD-54 810
- Searching for ejected supernova companions in the era of precise proper motion and radial velocity measurements
- Forward and Back: Kinematics of the Palomar 5 Tidal Tails
- Kinematics of stellar substructures in the Small Magellanic Cloud
- Young stars raining through the Galactic Halo: the nature and orbit of Price-Whelan 1
- Efficient Analysis Routines for Single and Double Peaked Type 2 AGN Spectra
- A Ghost in Boötes: The Least Luminous Disrupted Dwarf Galaxy
- A Machine Learning Approach to Correct for Mass Resolution Effects in Simulated Halo Clustering Statistics
- AuriDESI: Mock Catalogues for the DESI Milky Way Survey
- Environmental effects on associations of dwarf galaxies
- Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
- Harvesting the Lyα forest with convolutional neural networks
- Radial velocities from far red spectra of Carina Arm O and early B stars
- XGAPS: a sub-arcsecond cross-match of Galactic Plane Surveys
- 3D intrinsic shapes of quiescent galaxies in observations and simulations
- Improving white dwarfs as chronometers with Gaia parallaxes and spectroscopic metallicities
- A new member of the Milky Way's family tree: Characterizing the Pontus merger of our Galaxy