How Accurately Can Obscured Galaxy Luminosities Be Measured Using Spectral Energy Distribution Fitting of Near- through Far-infrared Observations?
| Title: | How Accurately Can Obscured Galaxy Luminosities Be Measured Using Spectral Energy Distribution Fitting of Near- through Far-infrared Observations? |
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| Authors: | Farrah D; Ejercito K; Efstathiou A; Leisawitz D; Engholm A; Shivaei I; Bonato M; Clements DL; Petty S; Pitchford LK; Varnava C; Afonso J; Gruppioni C; Hatziminaoglou E; Hoffman A; Lacy M; Matthews BC; Nixon C; Pearson C; Ricketti BV; Rigopoulou D; Robinson L; Spencer LD; Wang L; Sanders DB; van Belle G |
| Publication Year: | 2026 |
| Collection: | Science & Technology Facilities Council: ePublication Archive |
| Document Type: | article in journal/newspaper |
| Language: | unknown |
| ISSN: | 1538-4357 |
| Relation: | urn:ISSN:1538-4357; Astrophys J; http://purl.org/net/epubs/series/1885; Science and Technology Facilities Council (2007- ); RAL Space (2010- ); http://purl.org/net/epubs/work/64310813 |
| Availability: | http://purl.org/net/epubs/work/64310813 |
| Rights: | https://creativecommons.org/licenses/by/4.0/ |
| Accession Number: | edsbas.9902B488 |
| Database: | BASE |