New Variables Discovered by Data Mining Images Taken During Recent Asteroid Photometric Surveys at the Astronomical Observatory of the University of Siena: Results for the Year 2017

Volume 46 number 2 (2018)

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Alessandro Marchini
Astronomical Observatory, DSFTA, University of Siena (K54), Siena, Italy; alessandro.marchini@unisi.it
Riccardo Papini
AAVSO, UAI, Wild Boar Remote Observatory (K49), San Casciano in val di Pesa, Florence, Italy
Fabio Salvaggio
UAI, Wild Boar Remote Observatory (K49), Saronno, Italy; Gruppo Astrofili Catanesi, Catania, Italy
Claudio Arena
UAI, Private remote observatory, Catania, Italy; Gruppo Astrofili Catanesi, Catania, Italy
Davide Agnetti
UAI, Osservatorio Aldo Agnetti di Lomazzo, Como, Italy
Mauro Bachini
UAI, Osservatorio Astronomico di Tavolaia (A29), Santa Maria a Monte, Pisa, Italy
Giacomo Succi
UAI, Osservatorio Astronomico di Tavolaia (A29), Santa Maria a Monte, Pisa, Italy
Massimo Banfi
UAI, Osservatorio di Nova Milanese (A25), Nova Milanese, Italy; Osservatorio delle Prealpi orobiche (A36), Ganda di Aviatico, Italy

Abstract

This paper continues the publication of the list of the new variables discovered at Astronomical Observatory, DSFTA, University of Siena, while observing asteroids for determining their rotational periods. Further observations of these new variables are strongly encouraged in order to better characterize these stars, especially those showing non-ordinary light curves.