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Matthew Smith

Researcher at Cardiff University

Publications -  400
Citations -  21259

Matthew Smith is an academic researcher from Cardiff University. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 78, co-authored 392 publications receiving 18599 citations. Previous affiliations of Matthew Smith include Heidelberg University & Stanford University.

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The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types

Ilse De Looze, +23 more
- 01 Aug 2014 - 
TL;DR: In this paper, the authors analyzed the applicability of far-infrared fine-structure lines [Cii] 158μm, [Oi] 63μm and [Oiii] 88μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and furthermore, extended the analysis to a broad sample of galaxies of various types and metallicities in the literature.
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The manga integral field unit fiber feed system for the sloan 2.5 m telescope

Niv Drory, +25 more
- 01 Feb 2015 - 
TL;DR: In this paper, the authors describe the design, manufacture, and performance of bare-fiber integral field units (IFUs) for the SDSS-IV survey Mapping Nearby Galaxies at Apache Point Observatory (MaNGA).
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The applicability of FIR fine-structure lines as Star Formation Rate tracers over wide ranges of metallicities and galaxy types

Ilse De Looze, +21 more
- 17 Feb 2014 - 
TL;DR: In this article, the authors analyzed the applicability of far-infrared fine-structure lines [CII] 158 micron, [OI] 63 micron and [OIII] 88 micron to reliably trace the star formation rate (SFR) in a sample of low-metallicity dwarf galaxies from the Herschel Dwarf Galaxy Survey and compare with a broad sample of galaxies of various types and metallicities in the literature.
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OBSERVATIONS OF Arp 220 USING HERSCHEL-SPIRE: AN UNPRECEDENTED VIEW OF THE MOLECULAR GAS IN AN EXTREME STAR FORMATION ENVIRONMENT

Naseem Rangwala, +22 more
- 10 Dec 2011 - 
TL;DR: In this paper, the Herschel Spectral and Photometric Imaging Receiver Fourier Transform Spectrometer (Herschel SPIRE-FTS) observations of Arp 220, a nearby ultra-luminous infrared galaxy, were presented.
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Search for new high-mass phenomena in the dilepton final state using 36 fb−1 of proton-proton collision data at √s=13 TeV with the ATLAS detector

Morad Aaboud, +2947 more
- 08 Jul 2017 - 
TL;DR: In this article, a search for new resonant and non-resonant high-mass phenomena in dielectron and dimuon fi nal states was conducted using 36 : 1 fb(-1) of proton-proton collision data.