Determining the abundance of extragalactic planets
| dc.creator | Dominik, M. | |
| dc.date | 2003-09-23 | |
| dc.date | 2003-10-23 | |
| dc.date.accessioned | 2026-07-25T12:04:10Z | |
| dc.description | Gravitational microlensing provides a unique technique to reveal information about extragalactic planets. A network of at least four 2m-class telescopes distributed around the northern hemisphere could probe 15-35 jupiters and 4-10 saturns around M31 stars per year. | |
| dc.description | 2 pages, LaTeX using newpasp.sty (supplied). To appear in the proceedings of the XIXth IAP colloquium "Extrasolar Planets: Today and Tomorrow" held in Paris, France, 2003 June 30 -- July 4, ASP Conf. Ser | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0309607 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0309607 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/7396 | |
| dc.subject | Astrophysics | |
| dc.title | Determining the abundance of extragalactic planets | |
| dc.type | text |