Lightcurve analysis of five main belt asteroids 339 Dorothea, 549 Jessonda, 2445 Blazhko, 4528 Berg and 5317 Vero-lacqua observed at Bulgarian National Astronomical Observatory (NAO) Rozhen since March to December 2014 is presented. The choice of the asteroids was made according to their visibility in allocated observing time on the 50/70cm Schmidt and 60cm Cassegrain telescope and in the frame of our long term photometry program for determining the shape and poles of asteroids.
REFERENCES
1.
M.
Buie
, CCDPHOT, An interactive tool for CCD Photometry in IDL
, 1998
, see http://www.boulder.swri.edu/∼buie/idl/ccdphot.html2.
3.
R.
Behrend
, Observatoire de Genève web site
, 2006
, see http://obswww.unige.ch/∼behrend/page_cou.html4.
5.
6.
D. A.
Klinglesmith
III, E.
Risley
, J.
Turk
, A.
Vargas
, C.
Warren
, A.
Ferrero
, Minor Planet Bul.
40
, 15
–16
(2013
).7.
G.
Apostolovska
, Z.
Donchev
, A.
Kostov
, V.
Ivanova
, G.
Borisov
and B.
Bilkina
, Serbian Astronomical Journal
189
, 79
–85
(2014
).8.
J.
Hanuš
, J.
Ďurech
, M.
Brož
, B. D.
Warner
, F.
Pilcher
, R.
Stephens
, J.
Oey
, L.
Bernasconi
, S.
Casulli
, R.
Behrend
, D.
Polishook
, T.
Henych
, M.
Lehký
, F.
Yoshida
, T.
Ito
, A&A
530
, 134
(2011
)
This content is only available via PDF.
© 2016 AIP Publishing LLC.
2016
AIP Publishing LLC
You do not currently have access to this content.