HISTORY
PAST AND PRESENT ACTIVITY
The Pianoro Observatory, designated observatory "610" by the Minor Planet Center, is a very active private facility. It is located in the town of Pianoro, about 17 km south of the city of Bologna in northern Italy. Latitude,longitude and elevation of the site are respectively +44ø 23' 29.6", 11ø 20' 35" East, 180 meters. Despite the vicinity of Bologna, the sky is a reasonably dark, especially towards the southern side. As retired Professor of high school Math and Phisics, I developed a keen interest in minor planets many years ago. In 1976 , I joined the asteroid observing program at San Vittore Observatory (code 552), the first such program in Italy. This activity, done with Tech Pan films hypered with hydrogen, kept me busy for about 15 years, and heightened my interest in photographic chemistry. From 1993 to 1994, more powerful developers than the classic D-19 were tested in the course of an asteroid search program with the 67-cm Schmidt telescope at the Asiago Astrophysical Observatory (with Andrea Boattini and Maura Tombelli). In 1995, I bought a 25-cm f/6.3 Schmidt-Cassegrain and equipped it with a HySIS22 CCD camera, with a matrix of 768 x 512 pixels,each pixel measuring 9 x 9 microns. This camera is equipped with a Kodak KAF-400 chip, with a quantum efficiency peak of 42%.In effect, this is my observatory. In October of the same year, I started my astrometric activity with the observations of (433) Eros. Since then , I have produced almost 10,000 astrometric positions of minor planets , becoming the most prolific Italian observer since 1997. I usually observe in binned mode , with pixels being of 18 microns. This gives me a scale of 3.4 arcsec/pixel when I observe with a focal reducer (25-cm f/4). This scale still allows me to get good astrometric data. There are the fields in which I have concentrated my efforts: a) Follow-up of Near-Earth Asteroids. b) Follow-up of numbered asteroids that have been poorly observed over the last few years. c) Follow-up of main-belt objects that are close to being numbered. d) Photometry of asteroids. When I started this program the limiting magnitude of my system was only about 17.0 V, giving me the opportunity to concentrate only on programs (b) and (c). In the following few months I improved my results, partly due to better telescope tracking, and partly due to a better image calibration procedure. Right now I can take exposures of 4 minutes without using guiding corrections and this allows me to reach magnitude 18.0 V routinely. Also I have discovered 32 main-belt asteroids ad nine of them already have permanent numbers. Astrometry of comets My activity involves 21 different comets, with 297 positions. At present, I collaborate with the Minor Planet Center and the Spaceguard Foundation for the follow-up of Near-Earth Asteroids brighter than magnitude 18.0 V. VITTORIO GORETTI
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