Ocaña, FranciscoPonz, José DanielZamorano Calvo, JaimeJopek, T. J.Rietmeijer, F. J. M.Watanabe, J.Williams, I. P.2023-06-192023-06-192014978-83-232-2726-7https://hdl.handle.net/20.500.14352/35768Meteoroids Conference (8ª. 2013. Poznań, Polonia)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.engbook parthttp://adsabs.harvard.edu/abs/2014me13.conf..315Oopen access52MeteorsVideo techniqueCCDSchmidtAstrofísicaAstronomía (Física)