DUB OPTIKA S.r.l DUB OPTIKA . . . .LIGHT YEARS AHEAD

 

 

 

Our main realizations:

New optics and electronics for Ruths telescope in Merate Observatory

 

 

 

 

 

 

 

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Atmosferic Cerenkov Light Telescopes for INFN Observatory on Gran Sasso d'Italia

 

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Carried out for our national observatory of Brera-Merate, we have changed the three old alluminium mirrors with new optics in glassceramic Astrositall:

-Primary parabolic mirror with 1340 mm of diameter

-Secondary hyperbolic mirror with 500 mm of diameter

-Tertiary flat mirror with 300 mm of diameter

The precision obtained for the optical system is about lambda/7

The telescope movements syncronized with the dome's ones, are controlled by our Oaktrack SMEC IV control system

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 Builded for the Italian National Institute of Nuclear Physics, those are 4 telescopes installed in Campo Imperatore (2300 m high) in central Italy for the experiment EAS-TOP carried out on the "Laboratori del Gran Sasso"

Each telescope carries 4 parabolas with 1 meter of diameter or 1 parabolic mirror with 2 m of diameter

The mount is a modified Alt-Alt azimouthal mount expressly designed for our customer, the 4 telescopes are linked in a local net and could be fully remotized

Mt. Generoso Observatory (Switzerland)

fai click per ingrandire fai click per ingrandire Carried out for "Società Ferrovie del Monte Generoso", the main telescope is a 610 mm F:8 Ritchey-Chretien optical configuration, on a fork equatorial mount. Lodged in an octaedric dome with 5 meters of diameter. The telescope's movements and teh dome's ones are both controlled and syncronized by the same computer through our Oaktrack SMEC IV control system, so the telescope and the dome move together syncronized whether for tracking or for pointing celestial objects

DLF Astronomical Society Observatory ( Rimini-Italy)

Builded for DLF Amateur Astronomer Society in Rimini, the telescope is a 530 mm F:8 Ritchey-Chretien on an equatorial fork mount with a 150 mm F:10 apochromatic refractor as guiding telescope. With the same mechanical and electronical cheracteristics of the Mt. Generoso's ones. The tracking is always guaranteed by a smooth grinded wheel with a diameter of 1 meter

 

National Observatory in Capodimonte (Napoli- Italy)   

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Telescope with 410 mm of diameter F:8 in Ritchey-Chretien optical configuration on an equatorial fork mount, as usual our tracking system is on a smooth grinded wheel here with a diameter of 600 mm, the movements are controlled by our Oaktrack SMEC IV

S.Benedetto Po Observatory – Ass. Astrofili Mantovani (Mantova - Italia)

 

 

 Telescope  with 410 mm of diameter with a multifocal F:10 - F:5 Cassegrain optical configuration works together with an Astrophysic apochromatic refractor with a diameter of 180 mm. The same mechanical and electronic cheracteristics

 

 

Castelgrande Obsevatory Castelgrande (Potenza - Italy)

Telescope with 410 mm of diameter F:8 Ritchey-chretien optical configuration, on an equatorial fork mount and with an apochromatic refractor with a diameter of 150 mm F:6
 

Calina Observatory in Carona (Switzerland)

Carried out for the "Società Astronomica Ticinese" (CH) the main telescope is lodged in an octagonal building that allow to install two instruments with an openable roof divided in two shells.

The telescope is a 410 mm multifocal F:10-F:5 -F:3 (at primary focus) Cassegrainian optical system on an equatorial fork mount with a tracking smooth and grinded wheel with 600 mm of diameter

Restored Newton telescope with 300 mm of diameter F:5. We have carried out the complete sobstitution of electronic components, as well as the mechanical structure that holds the optics and electronic remote focusing control

Petina Observatory (Salerno - Italy)

Telescope with a diameter of 855 mm F:8 in Ritchey-Chretien optical configuration on a fork equatorial mount with a tracking smooth and grinded wheel of 1.3 meters of diameter. Is actually the biggest amateur telescope in Italy .

As for all the other instruments described before, our Oaktrack SMEC IV system controls automatically the positioning and the tracking movements of the telescope and the dome's ones as well.

Regional Observatory in Val d’Aosta (Italy)

12 telescopes with different diameter all in a local net connection bring this structure at the top in Europe among the didactic Astronomical Observatories.