Observatories

Visual Observatory at Telescope hosting site in Piconcillo, Andalusia, Spain

38˚10‘30.79“N, 05°27‘25.39“W

A new observing place connected with the new project. The visual observatory is at the same time the control room for managing the entire hosting facility. The telescope is the same model as Yogajtódo in Kolonica. 16″ Skywatcher GoTo Dobson. Aperture 400 mm, focal length 1800 mm, resulting in an F/4.5 focal ratio. Collapsible tube design. Here, a different name for the new telescope was chosen: “ARDILLA.” In Spanish, this means “squirrel.” Those familiar with the local realities know exactly why such a name was chosen.

Skywatcher 16”, Newton GoToMainFinder
Aperture/ Focal length [mm]405 / 186050 / 300
Eyepiece Explore scientific focal length/ FOV2″ 24 mm/ 82°
Eyepiece Explore scientific focal length/ FOV1.25″ 24 mm/ 68°
Eyepiece Explore scientific focal length/ FOV1.25″ 6.7 mm/ 82°
MountDobsonwith GoTo
Typical observing programDwarf novae outburstsSymbiotics and semiregular variables

Tramtarian National Observatory, Kolonica, Slovakia

48°56’10.6″N, 22°16’30.6″Е

The private, garden observatory where I moved with 12″ Dobsonian Chermelin after the end of the contract at the Vihorlat Observatory.

TNO
Chermelin 30cm NewtonianMainFinderTypical observing program
Aperture/ Focal length [mm]300 / 150050 / 300Cataclysmic variables – visual monitoring for outbursts
ZOOM Eyepiece focal length24 – 8 mmThe majority of visual estimates were done with this instrument in the observatory in Podbiel village
MountDobson

Astronomical Observatory on Kolonica Sadle, Slovakia

48°56’06.0″N, 22°16’26.0″Е

Observing site of the Vihorlat Observatory in Humenné. I have been working at this place since 2006 to 2025. More on http://www.astrokolonica.sk/

Telescopes for CCD and CMOS photometry

VNTMainGuide
Aperture/ Focal length [mm]1000 / 9000300 / 1500
CCD, binningFLI PL 1001E, 2×2WATEC 902H
Chip size [px], pixel size [μm]512 x 512, 48 x 48320 x 240, 5.6 x 5.6
Scale [arcsec/px]1.110.8
FOV [arcmin]9.47 x 9.474.1 x 3.0
Readout noise [e-] / gain [e- per ADU]8.26 / 2.39
FiltersB, V, Rc, Ic, Clear
MountFork equatorial without GoTo
Typical observing programIntermediate polars
ONTCMain
Aperture/ Focal length [mm]406 / 1800
CMOS, binningMII C4-16000, 1×1
FiltersB, V, Rc, Ic, Halpha, OIII, SII
Chip size [px], pixel size [μm]4096 x 4096, 9 x 9
Scale [arcsec/px]1.02
FOV [arcmin]70.41 x 70.41
readout noise [e-] / gain [e- per ADU]3.9 / 0.85
MountGerman equatorial, 10 Micron GM3000, no guiding needed
Typical observing programFlickering and superhumps in Cataclysmic Variables; Astrophoto campaign – nova super-remnants.

Spectroscopy

NOU-T spectrograph on C14 telescope
Spectrograph NOU-T on C14 telescopeMainGuideFinder
Aperture/ Focal length [mm]356 / 3000 with reduceroff whole80 / 325
CCD, binningATIK-460ex, 2×2Starlight Express SXVR-H9, 1×1 MI G1-2000
Chip size [px], pixel size [μm]1374 x 1099, 9.08 x 9.081392 x 1040, 6.45 x 6.451628 x 1236, 4.4 x 4.4
Scale [arcsec/px]0.92.79
FOV [arcmin] 10.3 x 7.775.7 x 57.5
Resolution power11000
MountGerman equatorial Celestron Edge HD CGE Pro 1400
Typical observing programNovaeSymbiotics stars
AZ2000 DT mount with RC16 and Pupava telescopes
Spectrograph UVEX on RC16 telescopeMainGuideSimultaneous photometry
Aperture/ Focal length [mm]408 / 3200off slit280 / 1500
CCD, binningZWO ASI 183 MM Pro, 1×1ZWO ASI 174 MM Mini, 2×2MI G2-1600, 1×1
Chip size [px], pixel size [μm]5496 x 1000, 2.4 x 2.4968×608, 11.72 x 11.721536 x 1024, 9 x 9
Scale [arcsec/px]0.761.24
FOV [arcmin] 12.2 x 7.731.6 x 21.1
FiltersB, V, Rc, Ic, Clear
Resolution power1500
MountAlt – acimuthal10 Micron AZ2000 DTdual mount
Typical observing programNovaeSymbiotics stars

Visual observations

Skywatcher 16”, Newton GoToMainFinder
Aperture/ Focal length [mm]405 / 186050 / 300
Eyepiece Explore scientific focal length/ FOV24 mm/ 68°
Eyepiece Explore scientific focal length/ FOV6.7 mm/ 82°
MountDobsonwith GoTo
Typical observing program
Dwarf novae outbursts

Binocular APM
Aperture x magnification100 x 30
MountAlt-acimuthal

M. R. Štefánik Observatory, Hlohovec, Slovakia

48°25’10.2″N 17°47’48.7″E

I had several opportunities to work with the observatory equipment in Hlohovec, western Slovakia. Regularly, I do remote observations with the main instrument – the Csere telescope.

The main dome of the Hlohovec observatory
Csere telescope
Csere telescope in Hlohovec observatory
Csere telescope
Zeiss made
MainGuide – Zeiss photolense
Aperture/ Focal length [mm]600 / 2400180 / 1000
CCD, binningAtik 383L+, 2×2Lodestar, 1×1
Chip size [px], pixel size [μm]1677 x 1264, 10.8 x 10.8762×580, 8.6 x 8.6
Scale [arcsec/px]0.931.77
FOV [arcmin] 25.95 x 19.5622.53 x 17.15
Readout noise [e-] / gain [e- per ADU]7 / 0.41
FiltersU, B, V, Rc, Ic, Clear
German equatorial mountZeiss made, semi-automatedNo meridian flip
Typical observing programCataclysmic variablesI operate the telescope of the Hlohovec observatory remotely

Former private observatory in Podbiel, Orava, Slovakia

49°18’20.6″N, 19°29’05.5″E

As an amateur visual observer, I made more than 40,000 visual estimates of variable stars from that place between 1998 and 2006.

Solar dos Esmeraldos, Ponta do Sol, Madeira

32°41’20.4″N, 17°05’31.2″W

Observing site on Madeira island. The playground behind the basic school in Lombada is relatively well protected against street lights. Visual observations with a modest Zennox 76/700 telescope and a Dobson 200/1400 are performed during winter stays on the island. Educational observations for the public (local and tourists) are performed as well.

Kamenicky 20 cm Newtonian”MainFinderTypical observing program
Aperture/ Focal length [mm]200 / 140020 / 150Semiregular and Symbiotics + brighter Cataclysmic variables
Televue eyepieces focal length26 and 8 mmThe first telescope used for regular variable star observing. First light in 1999. Transported to Madeira in 2020.
MountDobson
Zennox
Newtonian
MainFinderTypical observing program
Aperture/ Focal length [mm]76 / 70010 / 150Semiregular and Symbiotics
Televue Eyepiece focal length/FOV20 mm/ 52°The first telescope used in Madeira. First light in 2018.