Radial-velocity observations of pulsating stars with a new Poznań Spectroscopic Telescope

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Radial-velocity observations of pulsating stars with a new Poznań Spectroscopic Telescope 23 June 2008 Poznań Astronomical Observatory Adam Mickiewicz University Poznań, Poland

description

Poznań Astronomical Observatory Adam Mickiewicz University Poznań, Poland. Radial-velocity observations of pulsating stars with a new Poznań Spectroscopic Telescope. 23 June 2008. Our team R. Baranowski, P. Bartczak, W. Borczyk, W. Dimitrov, M. Fagas, K. Kamiński, T. Kwiatkowski, - PowerPoint PPT Presentation

Transcript of Radial-velocity observations of pulsating stars with a new Poznań Spectroscopic Telescope

Page 1: Radial-velocity observations of  pulsating stars with a new  Poznań Spectroscopic Telescope

Radial-velocity observations of pulsating stars with a new

Poznań Spectroscopic Telescope

23 June 2008

Poznań Astronomical ObservatoryAdam Mickiewicz University

Poznań, Poland

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Our team

R. Baranowski, P. Bartczak, W. Borczyk, W. Dimitrov, M. Fagas, K. Kamiński, T. Kwiatkowski, R. Ratajczak, A. Rożek, A. Schwarzenberg-Czerny

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The „dome”

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Mirors diameter – 0.4 m

Focal length – 1.8 m

Optical system – Newtonian

Diameter of the fibers – 50 m

Accesible altitudes h>24°

Mean. slewing rate 90°/min

Guiding cameras ST7

The telescope

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The echellé spectrograph

Baudrand and Bohm (1992)

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CCD camera:Andor DZ 4365-stage peltier cooling Temp. –95°C2048 x 2048 pix

pixel size 13.5 x 13.5μmdark current <1el/hreadout noise 2.1 el/pix

Echellé spectrograph

Spectral range:

4480 Å – 9250 Å

Resolution:

R=35000 (~8 km/s)

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Acquisition box

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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 Å every order adds 80 Å

red range: 1pix = 0.08 Å order length = 160 Å every order adds 125 Å

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ThAr calibration spectrum

1400 lines

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Flatfield and fringe effect

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Flatfield and fringe effect

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Telluric lines removal

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Flux calibration

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Line profiles

Sp=B1

V=1m

exp=250s

Hβ 4861 Å

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Limiting magnitude - BD+39 3012C 11m.2 Sp=F5 exp=30min

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28 And

δ Sct

Sp=A7III

V=5m.2

exp=600s

analysed by T. Kwiatkowski, W. Borczyk & A. Rożek

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γ Peg

β Cep

Sp=B2IV

V=2m.8

exp=600sor 300s

period=3.4h

υ1=6.59 c/d

analysed by W. Borczyk

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V440 Per

δ Cep

Sp=F7Ib

V=6m.3

exp=600s

analysed by A.Schwarzenberg-Czerny and M. Fagas

σpoz=136 m/s---2 harmonics---1 harmonic

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Polaris

analysed by M. Fagas and K. Kamiński

okres obs. P [d] 2K [km/s] ref.

1896 – 1950 ~5-6Campbell (1899),Roemer (1965)

1899 - 1923 3.96809 Moore (1924)

1944 – 1954 3.96961 Stebbius (1946)

1981 – 1982 3.971562 ± 1

2.8 ± 0.6Arellano Ferro (1983)Kamper et al. (1984)

1987 - 1988 3.9746 ± 0.0008 1.5 ± 0.08 Dinshaw et al. (1989)

1992.41993.2

3.97268 ± 0.00011

1.555 ± 0.0561.517 ± 0.047

Hatzes & Cochran (2000)

1994.261996.96

3.97211.66 ± 0.021.68 ± 0.08

Kamper & Fernie (1998)

2005.1832006.3602007.349

3.97208 ± 0.00013

2.210 ± 0.0482.080 ± 0.0422.406 ± 0.018

Lee et al. (2008)

20083.97792 ±

0.00152.52 ± 0.03 Borowiec (2008)

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Statistics

13 august 2007 - 30 may 2008

• 83 nights• 637 hours• 1080 science spectra

Colaborators

• Warsaw CAMK• Vienna Institute of Astronomy• Wrocław Astronomical Institute• Toruń Centre for Astronomy

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Future perspectives

Upgrade of the telescope:

• 2 x 0.5m mirrors• simultaneous exposure of two fibers• better automatisation and remote control

Upgrade of the calibration, some ideas:

• experiment - mixing the ThAr and stellar light• Vrad accuracy increase with a iodine cell• spectral resolution increase with the EDI

interferometer

Radial velocity measurements:

• broadening function• TODCOR• spectral disentangling

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