| dc.creator | MARIJA STROJNIK POGACAR | |
| dc.date | 2014-06 | |
| dc.date | info:eu-repo/date/embargoEnd/2019-06-30 | |
| dc.date.accessioned | 2022-10-12T19:48:31Z | |
| dc.date.available | 2022-10-12T19:48:31Z | |
| dc.identifier | http://cio.repositorioinstitucional.mx/jspui/handle/1002/703 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4122433 | |
| dc.description | We define the simplest signal-to-noise ratio (SNR) to determine the optimal wavelength interval for extrasolar planet detection. We expand the width of the spectral region from infrared up to submillimeter range. For a nearby solar system similar to our own, we find that the SNR increases by about 100 in comparison to that considered previously. We propose the planet detection in a spectral interval around 0.3 mm (900 GHz), in which we evaluate the SNR to be 10–4. We perform trade-off analysis for alternative sites for the planet observatory, concluding that the far side of the moon offers a most favorable, atmosphere-free environment and a stable
base. | |
| dc.format | application/pdf | |
| dc.rights | info:eu-repo/semantics/embargoedAccess | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/4.0 | |
| dc.subject | info:eu-repo/classification/cti/1 | |
| dc.title | Extrasolar planet observatory on the far side of the moon | |
| dc.type | info:eu-repo/semantics/article | |
