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20 October 2009 Institut d'Astrophysique et de Géophysique Université de Liège. Poznań Astronomical Observatory of Adam Mickiewicz University Poznań, Poland. Radial-velocity observations with a new Poznań Spectroscopic Telescope. Our team R. Baranowski, P. Bartczak, W. Borczyk,
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20 October 2009 Institut d'Astrophysique et de Géophysique Université de Liège Poznań Astronomical Observatory of Adam Mickiewicz University Poznań, Poland Radial-velocity observations with a newPoznań Spectroscopic Telescope
Our team R. Baranowski, P. Bartczak, W. Borczyk, W. Dimitrow, M. Fagas, R. Hirsch, K. Kamiński, A. Kruszewski, K. Kurzawa, T. Kwiatkowski, A. Przybyszewska, A. Rożek, A. Schwarzenberg-Czerny, N. Żywucka ...
The telescope Mirrors diameter – 0.5 m Focal length – 2.2 m Optical system – Newtonian Diameter of the fibers – 50 m
CCD camera: Andor DZ 436 5-stage peltier cooling Temp. –95°C 2048 x 2048 pix pixel size 13.5 x 13.5μm dark current <1el/h readout noise 2.1 el/pix Echellé spectrograph Spectral range: 4480 Å – 9250 Å Resolution: R=35000 (~8 km/s)
The echellé spectrograph Baudrand and Bohm (1992)
Echellé spectrum – 64 orders 4480 Å – 9250 Å blue range: 1pix = 0.04 Å order length = 80 Å every order adds 40 Å middle: 1pix = 0.05 Å ~2.5 km/s order length = 100 Åevery order adds 80 Å red range: 1pix = 0.08 Å order length = 160 Å every order adds 125 Å
ThAr calibration spectrum 1400 lines
Line profile Sp=B1 V=1m exp=250s Hβ 4861 Å
Limiting magnitude BD+39 3012C 11m.2 Sp=F5 exp=30min analysed by A. Rożek
V2080 Cyg Sodium NaD
V2080 Cyg detached binary Sp=F5 V=7m.4 exp=600s period=4.9d analysed by K. Kamiński
28 And δ Sct Sp=A7III V=5m.2 exp=600s analysed by T. Kwiatkowski, W. Borczyk and A. Rożek
V440 Per δ Cep Sp=F7Ib V=6m.3 exp=600s okres=7.57d σRV=136 m/s • --2 harmoniki • --1 harmonika analysed by M. Fagas, A.Schwarzenberg-Czerny, R. Smolec, published: MNRAS 396, 2194 - 2200
Bootis analysed by M. Fagas
γ Peg β Cep Sp=B2IV V=2m.8 exp=300s period=3.4h υ1=6.59 c/d analysed by W. Dimitrov
Quadruple system Rozhen PST
Iodine cell First tests 7 february 2009 RV = 20 m/s
Current statistics • 2 years of operation • 1650 spectra • 50 objects
Future perspectives • Spectroscopy on both mirrors • Simultaneus photometry and spectroscopy • Observing with iodine cell