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http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1448| The detection of a population of submillimeter−bright, strongly-lensed galaxies | |
| ITZIAR ARETXAGA MENDEZ David Hughes | |
| Acceso Abierto | |
| Atribución-NoComercial-SinDerivadas | |
| Submillimeter wavelengths | |
| Gravitational lensing is a powerful astrophysical and cosmological probe and is particularly valuable at submillimeter wavelengths for the study of the statistical and individual properties of dusty starforming galaxies. However the identification of gravitational lenses is often time-intensive, involving the sifting of large volumes of imaging or spectroscopic data to find few candidates. We used early data from the Herschel Astrophysical Terahertz Large Area Survey to demonstrate that wide-area submillimeter surveys can simply and easily detect strong gravitational lensing events, with close to 100% efficiency. | |
| Science | |
| 2010 | |
| Artículo | |
| Inglés | |
| Estudiantes Investigadores Público en general | |
| Negrello, Mattia, et al., (2010). The detection of a population of submillimeter−bright, strongly-lensed galaxies, Science. Vol. 330(6005): 800-804 | |
| ASTRONOMÍA Y ASTROFÍSICA | |
| Versión aceptada | |
| acceptedVersion - Versión aceptada | |
| Aparece en las colecciones: | Artículos de Astrofísica |
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| Fichero | Tamaño | Formato | |
|---|---|---|---|
| 1-A.pdf | 1.3 MB | Adobe PDF | Visualizar/Abrir |