Telescopes
I used many telescopes for both visual and CCD observing. Following is the list of actual equipment of AO on Kolonica Saddle dedicated to variable stars .
Telescopes for CCD photometry
VNT | Main | Guide | Typical observing program |
Aperture/ Focal length [mm] | 1000 / 9000 | 300 / 1500 | Intermediate polars |
CCD, binning | FLI PL 1001E, 2×2 | WATEC 902H | |
Chip size [px], pixel size [μm] | 512 x 512, 48 x 48 | 320 x 240, 5.6 x 5.6 | |
Scale [arcsec/px] | 1.11 | 0.8 | |
FOV [arcmin] | 9.47 x 9.47 | 4.1 x 3.0 | |
readout noise [e-] / gain [e- per ADU] | 8.26 / 2.39 | – | |
Mount | Fork equatorial without GoTo | – | |
C14 – Celestron Edge HD, focal reducer 0.7x | Main | Guide | Typical observing program |
Aperture/ Focal length [mm] | 356 / 3000 | 50 / 300 | Superhumps of cataclysmic variables, |
CCD, binning | MII G2-1600, 2×2 | MII G1-800C | Multicolor long term light curves |
Chip size [px], pixel size [μm] | 768 x 512, 18 x 18 | 1032 x 778, 4.65 x 4.65 | |
Scale [arcsec/px] | 1.21 | 3.21 | |
FOV [arcmin] | 13.4 x 8.9 | 55.2 x 41.6 | |
readout noise [e-] / gain [e- per ADU] | 12 / 2.3 | – | |
Mount | CGE 1400, GoTo | – | |
ZIGA – Dall-Kirkham 16” | Main | Guide | Typical observing program |
Aperture/ Focal length [mm] | 500 / 3454 | off axis | Eclipsing binaries W UMa type, multicolor light curves, full phase |
CCD, binning | MII G4-16000, 2×2 | MII G1-800C | |
Chip size [px], pixel size [μm] | 2048 x 2048, 18 x 18 | 1032 x 778, 4.65 x 4.65 | |
Scale [arcsec/px] | 1.09 | 3.21 | |
FOV [arcmin] | 36.7 x 36.7 | 55.2 x 41.6 | |
readout noise [e-] / gain [e- per ADU] | 12 / 1.6 | – | |
Mount | Paramount | – | |
Púpava | Main | Guide | Typical observing program |
Aperture/ Focal length [mm] | 280 / 1500 | off axis | Superhumps of catalclysmic variables |
CCD, binning | DSI Pro II, 1×1 | SXVF-H9, 2×2 | |
Chip size [px], pixel size [μm] | 748 x 577, 8.6 x 8.3 | 1392 x 1040, 6.45 x 6.45 | |
Scale [arcsec/px] | 1.18 x 1.14 | – | |
FOV [arcmin] | 14.7 x 10.9 | – | |
readout noise [e-] / gain [e- per ADU] | 12 / 0.7 | – | |
Mount | German equatorial without GoTo | – |
Telescopes for spectroscopy
C11 – Celestron CGEM 1100, focal reducer 0.66x, spectrograph LISA | Main | Guide | Typical observing program |
Aperture/ Focal length [mm] | 280 / 1750 | off slit | Be stars |
CCD, binning | ATIK-460ex, 1×1 | ATIK-317 | Symbiotic stars |
Chip size [px], pixel size [μm] | 2450 x 600, 4.54 x 4.54 | – | |
Scale [arcsec/px] | – | – | |
FOV [arcmin] | – | – | |
Resolution power | 1000 | – | |
Mount | CGEM, GoTo | – |
Telescopes for visual observations
Meade LightBridge 14”, Newton with coma corrector | Main | Finder | Typical observing program |
Aperture/ Focal length [mm] | 405 / 1860 | 50 / 300 | Cataclysmic variables – monitoring for outbursts |
Eyepiece Celestron focal length/ FOV | 26 mm/ 80° | – | |
Eyepiece Televue focal length/ FOV | 8 mm/ 72° | – | |
Mount | Dobson | – | |
Bibinar – 2 binoculars on common mount | Somet | Artillery | Typical observing program |
Aperture x magnification | 100 x 25 | 60 x 12 | Semiregular and symbiotic variables – long term light curves |
Mount | Alt-acimuthal | – | – |
Chermelin 30cm Newtonian” | Main | Finder | Typical observing program |
Aperture/ Focal length [mm] | 300 / 1500 | 50 / 300 | Cataclysmic variables – visual monitoring for outbursts |
ZOOM Eyepiece focal length | 24 – 8 mm | – | The majority of visual estimates was done with this instrument in the observatory in Podbiel village |
Mount | Dobson | – |
Kamenicky 20cm Newtonian” | Main | Finder | Typical observing program |
Aperture/ Focal length [mm] | 200 / 1400 | 20 / 150 | Semiregular and Symbiotics + brighter Cataclysmic variables |
ZOOM Eyepiece focal length | 24 – 8 mm | – | The first telescope used for regular variable star observing. First light in 1999. Translated to Madeira in 2020. |
Mount | Dobson | – |
Zennox Newtonian | Main | Finder | Typical observing program |
Aperture/ Focal length [mm] | 76 / 700 | 10 / 150 | Semiregular and Symbiotics |
Televue Eyepiece focal length/FOV | 20 mm/ 52° | – | The first telescope used in Madeira. First light in 2018. |
Mount | Dobson | – |