Solar refractor for white light photospheric; Herschel Prism 2’’ Baader Cool Ceramic P (hoto); CCD Atik4000 (2047x2047, 0.0074 mm, 16 bit)
Solar refractor for chromospheric observations; Solar Observer Halpha Filter S-1.5 (0.3A); CCD Atik11000 (4008x2672 px, 0.009 mm, 16 bit)
CCD Camera type SBIG STL11000M, (KAI-11000M, 36.1 x 24.7 mm, 11 million pixels, 4008 x 2745, 9 x 9 ), with UBVRI filter system (Johnson photometric system)
Photographic plates of 24 x 24 cm are used; the instrument has a field of 2 x 2 deg. The plates are measured on an Ascorecord machine (0.1). A HiSis 22 CCD camera was also attached in 1995 to this instrument.
The instrument has two declination circles each of 1 m diameter, divided at every 5'. The telescope is endowed with an impersonal micrometer. The collimation of the optical axis is measured by means of two meridian marks located at about 80-100 m from the instrument.
CPUs: SGI Altix 3700 supercomputer: 44 processors Itanium 2 1.3GHz, 92GB RAM, 5TB RAID.
GPUs: 12 cores Intel Xeon E5630, 2.3GHz, 64GB RAM, 2TB RAM , 1 GPU card NVIDIA Quadro 40000
CPUs: 12 cores Intel Xeon E5630 2.3GHz, 32GB RAM, 2TB RAM
CPUs: AMD Phenon X4 9650 Quand Core, Ram 4G, HDD 500 GB Sata
CCD camera type SBIG 8XMEI (CCD Kodak KAF1602ME, 1530x1020 pixels, 9μmx9μm), with photometric filters UBVRI Custom Scientific (Johnson-Cousins photometric system)
DSLR type camera (Canon EOS 50D, CMOS sensor, 4752 x 3168 pixels, 4.7 μmx4.7μm), or alternatively CCD camera (MEADE Pictor416, CCD Kodak KAF0401E sensor 768x512 pixels, 9μmx9μm), with BVRI Schuller filters (Johnson-Cousins photometric system)
DSLR type camera (Canon EOS 50D, CMOS sensor, 4752 x 3168 pixels, 4.7 μmx4.7μm), or alternatively CCD camera (MEADE Pictor416, CCD Kodak KAF0401E sensor 768x512 pixels, 9μmx9μm), with BVRI Schuller filters (Johnson-Cousins photometric system)
Photoelectric photometer (with photomultiplier) and UBV filter system (Johnson photometric system), with photon counting system or chart recorder system
SBIG CCD Camera with photometric filters UBVRI