Magus Epi-FL04M LED Epi-Fluorescence Attachment, fluorescence filter cubes B/G/UV (85153)

46050.97 kn

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The epi-fluorescence attachment is designed to enable fluorescence microscopy. This technique relies on the ability of certain substances to emit light when excited by illumination at a specific wavelength. Some specimens naturally exhibit autofluorescence, while others require treatment with fluorochromes to produce a fluorescent signal. The attachment is installed in the optical path between the microscope head and the stand. Inside the unit is a four-position rotating turret that holds three broadband fluorescence filter sets for blue (B), green (G), and ultraviolet (UV) excitation.

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Magus Epi-FL04 LED Epi-Fluorescence Attachment, fluorescence filter cubes FITC/TRITC/DAPI (85156)

54186.33 kn

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The epi-fluorescence attachment is designed for fluorescence microscopy. This technique is based on the ability of certain substances to emit light when excited by illumination at a specific wavelength. Some specimens show natural autofluorescence, while others require staining with fluorochromes to produce a fluorescent signal. The attachment is installed in the optical path between the microscope head and the stand. Inside the unit is a four-position rotating turret equipped with three narrow-band fluorescence filter sets for the fluorochromes DAPI, FITC, and TRITC. 

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Magus Epi-FL06 Epi-Fluorescence Attachment, mercury lamp, fluorescence filter cubes В/G/UV/V/R/FITC/TRITC/DAPI (85157)

66725.34 kn

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The epi-fluorescence attachment is designed for fluorescence microscopy. This technique is based on the ability of certain substances to emit light when excited by illumination at a specific wavelength. Some specimens naturally exhibit autofluorescence, while others require treatment with fluorochromes to produce a visible fluorescent signal. The attachment is installed in the optical path between the microscope head and the stand. Inside the unit is a six-position rotating turret fitted with fluorescence filters.

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Celestron Camera Origin 678C Color (88020)

4172.6 kn

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This camera upgrade features compact 2.0 μm pixels that increase resolution and deliver brighter images. Sony Starvis 2 technology improves quantum efficiency, enhancing light sensitivity and fine detail. The modern 16:9 widescreen aspect ratio is ideally suited to smartphone and tablet displays, ensuring images fill the entire screen without cropping. Using the latest Sony Starvis 2 CMOS technology, this high-performance camera provides higher resolution and finer detail thanks to smaller pixels and improved sensitivity to light. It captures more information from faint objects and produces clearer, more detailed astrophotography results.

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Optika CC P20CC Pro, 20MP CMOS cooled colour camera, USB3.0 (57551)

13818.03 kn

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Cameras are now an essential tool, and OPTIKA offers a range of advanced digital imaging solutions designed for demanding users and professional environments. The OPTIKA PRO Series covers a broad spectrum of applications, from routine use to high-end cooled monochrome or color cameras, available with either CMOS or CCD sensors. Renowned SONY sensors deliver true-to-life color reproduction, allowing specimens to be captured exactly as they appear, with exceptional accuracy and realism.

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Antlia Filters OIII 3 nm 36 mm (88246)

3695.21 kn

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OIII filters allow only light with a wavelength of 501 nanometres to pass through. This wavelength corresponds to the emission lines of doubly ionised oxygen, which are produced by planetary nebulae and certain emission nebulae. As a result, these objects remain visible while most other light is blocked by the filter. This selective transmission significantly increases contrast and makes faint nebulae visible for the first time.

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Artesky eADC Electronic Atmospheric Dispersion Corrector V3 (88181)

4570.83 kn

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The SunObserver eADC V3 is a third-generation electric atmospheric dispersion corrector featuring zero image shift technology, designed for demanding astrophotography and high-precision visual observation. At the core of the eADC V3 is a system of four prisms arranged in two groups, made from high-quality optical glass and treated with broadband anti-reflective coatings. An integrated sensor continuously detects the telescope’s orientation and automatically calculates the required atmospheric dispersion correction.

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Askar Filters Colour Magic OIII 3nm 2" (87816)

2954.27 kn

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The ColourMagic 3 nm Narrowband Filter features an extremely narrow bandwidth combined with excellent light transmission, allowing the capture of high-contrast, low-noise deep-sky images even under challenging conditions such as urban light pollution, atmospheric airglow, or other sources of stray light. This performance makes faint nebular structures and subtle stellar details, which are often difficult to reveal, clearly visible. The filter also incorporates an optimized optical design for improved halo control, resulting in higher image quality and greater expressive power in astrophotography.

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Askar Filters Colour Magic H-alpha 3nm 2" (87814)

2954.27 kn

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The ColourMagic 3 nm Narrowband Filter features an extremely narrow bandwidth combined with excellent light transmission, allowing you to capture high-contrast, low-noise deep-sky images even in environments affected by urban light pollution, atmospheric airglow, or other sources of stray light. This makes faint nebular structures and subtle stellar details, which are often difficult to reveal, clearly visible. In addition, the ColourMagic filter uses an optimized optical design for improved halo control, resulting in higher image quality and greater expressive impact in astrophotography.

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Askar Filters Colour Magic SII 3nm 2" (87815)

2954.27 kn

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The ColourMagic 3 nm Narrowband Filter features an extremely narrow bandwidth combined with excellent light transmission, allowing the capture of high-contrast, low-noise deep-sky images even in locations affected by urban light pollution, atmospheric airglow, or other unwanted light sources. This performance makes faint nebular structures and subtle stellar details, which are often difficult to detect, clearly visible. In addition, the ColourMagic filter incorporates an optimized optical design for effective halo control, ensuring higher image quality and enhancing the overall expressive power of astrophotography.

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Askar Filters Colour Magic H-alpha SII OIII 3nm 2" (87817)

7766.51 kn

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The ColourMagic 3 nm Narrowband Filter set features an extremely narrow bandwidth combined with excellent light transmission, allowing the capture of high-contrast, low-noise deep-sky images even in environments affected by urban light pollution, atmospheric airglow, or other stray light sources. This performance makes faint nebular structures and subtle stellar details, which are often difficult to reveal, clearly visible. In addition, the ColourMagic filters use an optimized optical design for effective halo control, resulting in higher image quality and greater expressive power in astrophotography.

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Askar Flattener 1.0x 103APO (86169)

1675.12 kn

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A field flattener is an optical lens designed to correct the slight curvature of the image field produced by a telescope’s primary optics. This natural curvature causes stars near the edges of the field of view to appear less sharp. By correcting this effect, the flattener ensures that stars remain sharp and well-defined across the entire image, from center to edge.

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Askar Flattener 1.0x 120APO (88205)

1736 kn

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A field flattener is an optical element designed to correct the slight curvature of the image field produced by a telescope’s primary optics. This natural curvature causes stars near the edges of the image to appear softer or out of focus. By compensating for this effect, the flattener ensures that stars remain sharp and well-defined across the entire field of view, from the center to the edges of the frame.

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Askar Flattener 1.0x 160 f/7 (87467)

3000 kn

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A field flattener is an optical lens designed to correct the slight curvature of the image field produced by a telescope’s primary optics. This inherent curvature causes stars near the edges of the field of view to appear less sharp. By compensating for this effect, the flattener ensures that stars remain sharp and well-defined across the entire image, from the center to the outer edges of the frame.

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Askar Reducer 0.8x 103APO (87483)

1736 kn

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A focal reducer shortens the effective focal length of a telescope, making the optical system faster for astrophotography. As a result, images appear brighter, and the field of view is expanded, allowing larger sections of the sky to be captured in a single frame.

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Askar Reducer 0.8x 120APO (88179)

1736 kn

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A focal reducer shortens the effective focal length of a telescope, making the optical system faster for astrophotography. This results in a brighter image and a wider field of view, allowing larger areas of the sky to be captured in a single exposure.

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Astronomik Filters H-alpha 12nm MaxFR XT Clip Nikon Z XL (88411)

3137.06 kn

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Astronomik XT filters for wide-angle optics are designed to deliver sharp, well-defined stars right into the corners of the image, even with extreme wide-angle lenses. With standard Astronomik filters, image quality at very short focal lengths can be limited. Although these filters use a glass substrate only one millimetre thick, certain wide-angle lenses can still introduce aberrations, causing stars near the edges of the frame to stretch into short lines.

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Baader Filters D-ERF energy protection filter 290 mm (87870)

35330.06 kn

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Plano-parallel round optical discs with both surfaces precision-polished to lambda/10 accuracy ensure excellent optical quality. An advanced infrared anti-reflection coating, based on a multi-layer dielectric interference system, prevents excessive heat from entering the telescope’s optical tube assembly. The plano-parallel D-ERF (Energy Rejection Filter) effectively blocks infrared radiation, even during extended observing sessions.

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DayStar Solar filters QUARK Gemini Combo H-Alpha (87882)

19187.83 kn

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The DayStar Quark Gemini combines both Prominence and Chromosphere bandpass filters in a single unit, allowing instant switching between the two views using a simple slide mechanism. Observers can now enjoy the strengths of both bandpasses in one easy-to-use tool, with no need to change equipment or refocus. By sliding the control arm side to side—much like during an eye exam—you can transition from the broader bandpass view, which highlights large, dramatic solar prominences, to the narrower bandpass view, delivering high-contrast detail of chromospheric features.

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Evident Olympus Software CellSens Dimension Version 4.4 CS-DI-V4.4-EL - Licence (N6457500, 88257)

55858.52 kn

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cellSens imaging software is designed for intuitive operation and a smooth, efficient workflow. It supports microscopy users with powerful tools that simplify image acquisition, processing, and analysis, helping to streamline everyday laboratory tasks as well as advanced research applications. cellSens Dimension is the most versatile and comprehensive solution within the Olympus cellSens software family. It combines automated image acquisition with advanced analysis functions, making it suitable for a wide range of microscopy applications.

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Evident Olympus Software CellSens Standard Version 4.4 CS-ST-V4.4 - Licence (N6457400, 88256)

20603.51 kn

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cellSens imaging software is designed for intuitive operation and a smooth, efficient workflow. It supports a wide range of microscopy tasks by combining user-friendly controls with advanced image acquisition, processing, and analysis capabilities. cellSens Standard is the successor to the cellSens Entry Package and expands functionality beyond single-image capture. It supports advanced image acquisition methods such as time-lapse imaging and enables control of motorized and coded microscope components.

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Evident Olympus Evident Software PRECiV Core, Pro or Desktop Extension PV-S-GS-EL Solution Licence (N6417700, 88272)

33270.88 kn

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This solution is an optional add-on for PRECiV Core, Pro, or Desktop software and is designed for grain size analysis. It enables manual measurement of ferritic or austenitic grain size in steel and supports automatic determination of grain size distribution on etched microstructures. The add-on is suitable for metallographic analysis in research, quality control, and industrial applications where standardized grain size evaluation is required.

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Evident Olympus Evident Software PRECiV Core, Pro or Desktop Extension PV-S-NMI-EL Solution Licence (N6417800, 88273)

33270.88 kn

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This solution is an optional add-on for PRECiV Core, Pro, or Desktop software and is designed for the analysis of non-metallic inclusions. It enables automatic detection of inclusions based on color, shape, and size, along with automatic classification of oxides, sulphides, silicates, and aluminates. Detected inclusions are displayed live on the screen together with the corresponding evaluation results, allowing efficient and standardized analysis.

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Evident Olympus SZX2-CPO polarisation insert (N5733500, 69490)

3037.09 kn

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This polarization plate module is designed for use with the SZX2-ILLTQ/S illumination base and supports polarization contrast techniques in stereo microscopy. It can be combined with the SZX2-AN analyzer and the KL-RA-SZX-2 ring light adapter to enable polarized light observation, making it suitable for material analysis, quality control, and educational applications.

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