2026-06-26T20:12:32Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/357682023-09-07T20:29:24Zcom_20.500.14352_14col_20.500.14352_21

Ocaña, Francisco Ponz, José Daniel Zamorano Calvo, Jaime 2023-06-19T15:54:51Z 2023-06-19T15:54:51Z 2014 978-83-232-2726-7 https://hdl.handle.net/20.500.14352/35768 http://adsabs.harvard.edu/abs/2014me13.conf..315O Meteor observing requires a huge field of view (FoV) as its appearance in the sky cannot be foreseen. In the new era of the time-domain astronomy many telescopes will cover the whole sky with a cadence of a few days. These requirements lead to fast large telescopes with wide FoVs, like the Schmidt cameras that were widely used for meteor observing in the past. Common general-purpose telescopes have small plate scale and employ large integration times, what plays against meteor detection. We present here an estimation of the number of meteors detected as a byproduct of these surveys, with the detailed example of the Test-Bed Telescopes, an ESA project for NEO and space debris surveillance. eng open access Meteor detection in wide-field survey telescopes book part