These high Quantum Efficiencies make for impressive sensitivity across a vast range of wavelengths, but become particularly outstanding when imaging in narrowband, capturing stunning levels of detail in even the faintest of objects.
#Ts photoline 130 and atik 460 series#
The 460EX can also be used for OEM applications.Īll of our 4-EX series cameras use sensors embedded with Sony EXview HAD CCD II™ technology which results in outstanding Quantum Efficiency, incredibly low read noise and excellent thermal management. Cámaras : QHY-268 mono, Atik-460 mono, Canon 6D (modificada), Canon R6 Tubos : TS-Photoline 130/910, TS-Photoline 80/500, Takahashi FSQ106ED Reductor & Aplanador : Riccardi 0.75x, Takahashi 0. The desiccant port is readily accessible from outside the camera for easy maintenance, and a simple 12V power requirement is complimented by low power use to help you get the most out of your imaging sessions, whether in the observatory or out in the field. The slim, ergonomic design of these cameras naturally comes in at a low weight to help minimize stress on the corrector plate. They feature fully regulated set-point cooling which makes for easy and consistent image calibration, though they feature such low noise that dark frames are no longer even a requirement, meaning you can spend more time imaging the things that matter. The narrow body makes them ideal for use on Hyperstar and Fastar systems whilst maintaining suitability with a huge range of other telescopes. Our 4-Series is designed in such way as to combine power and control with flexibility and ease of use. TS Photoline 480/80, CGEM, ZWO ASIMMc 1600 Pro, OAG. Obtenidas en Matadepera el 31 de diciembre de 2018 y el 1 de enero de 2019. There are now cameras with both large format and small pixels using CMOS technology, however.The 460EX is ideal for those looking to invest in a camera that will provide uncompromising performance, no matter where your deep-sky imaging journey may take you. Equipo de siempre Refractor 130 x 1000 focal, cámara 9 x 9 um x 4096 pix, OAG Lodestarx2.
Deep sky object photographic data courtesy: DSS/STScI. Star charts generated using Cartes du Ciel. Here are two examples, the first with a large format, low res, large pixel Atik 11000 and the second with a small format, small pixel Atik 460. As you add equipment to the view, the details will appear below. Los telescopios TS PHOTOLINE triplete APO ofrecen imgenes de gran calidad alcanzando niveles de rendimiento que hasta ahora slo estaban al alcance de equipos mucho ms caros. This can do a good job of nebulae and galaxies if we vary the camera. Telescopio TS PHOTOLINE Triplete APO 130/910mm con enfocador RPA Objetivo Triplete APO FPL-53 de O'Hara. The nearest you can get is to use a moderate focal length (approaching a metre) and a camera which has both small pixels and a large chip. Finding a scope-camera that will do both is not easy. CGEM II 1100 EDGE HD - telescopio Schmidt-Cassegrain Edge HD da 280mm f/10 con robustissima montatura equatoriale computerizzata CGEM II. Galaxies, apart from M101, M33 and M31, are small (and packed with tiny details requiring high resolution.) Nebulae tend to be large, diffuse and lacking in fine detail.
Unfortunately this is rather like saying, I want to buy a sauce mix which works for fish and cakes. The corrector is also suitable for refractors. Optimized for the Photoline Triplet Apo 130 mm f/7 - the corrector can also be combined with similar refractor telescopes. Focal length reduction 0.8 times - the exposure time is reduced to 64. My intended targets are nebulas and galaxies - I realise galaxies are at the edge of these sorts of refractors' focal lengths, but I was hoping a smaller sensor astrocam would make this feasible. TS Photoline corrector and focal reducer 0.8x for astrophotography with the Photoline 130 mm f/7 Apo.
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