| dc.date.accessioned | 2020-03-11T20:34:14Z | |
| dc.date.accessioned | 2022-10-18T22:57:32Z | |
| dc.date.available | 2020-03-11T20:34:14Z | |
| dc.date.available | 2022-10-18T22:57:32Z | |
| dc.date.created | 2020-03-11T20:34:14Z | |
| dc.date.issued | 2010 | |
| dc.identifier | http://hdl.handle.net/10533/240193 | |
| dc.identifier | 15010003 | |
| dc.identifier | WOS:000276513700016 | |
| dc.identifier | no scielo | |
| dc.identifier | eid=2-s2.0-77950995856 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4471532 | |
| dc.description.abstract | Given an observed gravitational lens mirage produced by a foreground deflector (cf. galaxy, quasar, cluster,...), it is possible via numerical lens inversion to retrieve the real source image, taking full advantage of the magnifying power of the cosmic le | |
| dc.language | eng | |
| dc.relation | https://doi.org/10.1088/0004-6256/139/5/1935 | |
| dc.relation | 10.1088/0004-6256/139/5/1935 | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
| dc.title | The Optimal Gravitational Lens Telescope | |
| dc.type | Articulo | |
