The Outer Cut-Off of the Giant Planet Population and the 6pc-Survey
| dc.creator | Apai, D. | |
| dc.creator | Meyer, M. R. | |
| dc.creator | Hinz, P. | |
| dc.creator | Kasper, M. | |
| dc.date | 2007-10-15 | |
| dc.date.accessioned | 2026-07-07T08:36:26Z | |
| dc.date.available | 2026-07-07T08:36:26Z | |
| dc.description | We present results from two high-contrast imaging surveys that exploit a novel technique, L-band angular differential imaging. Our first survey targeted 21 young stars in the Beta Pic and Tuc-Hor moving groups with VLT/NACO reaching typical sensitivities of <1 MJup at r > 20 AU. The statistical analysis of the null result demonstrates that the giant planet population is truncated at 30 AU or less (90% confidence level). Our second, on-going MMT/Clio survey utilizes the unique sensitivity achieved in the L-band for old planets to probe all M-dwarf stars within 6 pc. The proximity of these targets enables direct imaging of planets in orbits like Jupiter for the first time - a key step for directly imaging giant planets. | |
| dc.description | To appear in the Conference Proceedings "Extreme Solar Systems"; 3 pages, 1 figure | |
| dc.identifier | https://arxiv.org/abs/0710.2864 | |
| dc.identifier | http://arxiv.org/abs/0710.2864 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/140062 | |
| dc.subject | Astrophysics | |
| dc.title | The Outer Cut-Off of the Giant Planet Population and the 6pc-Survey | |
| dc.type | text |