Takahashi Epsilon 180-ED F/2.8 Newtonian Astrograph OTA Package

The Takahashi Epsilon-180ED (D=180mm, F/2.8), based on catadioptric telescope design (means association of lenses and mirrors) offers a fundamental innovation compared with Newton reflector or Schmidt astrograph. Therefore, the Epsilon-180ED suits both visual observation and large field imaging needs.

The Epsilon-180ED wide field is perfectly flat and allows the use of traditional photographic formats as 24x36 (35mm) or 6x6 and even 6x9. Stellar images of less 20µ can be recorded, which highlights the extreme accuracy of this telescope. Epsilon's images provide incomparable contrast and sharpness.

The optical tube assembly (hyperbolical Newton) gives an image very contrasted even with stars located at the edge of the field. Regardless of its photographic qualities, Epsilon-180ED is a first range telescope for large field observation. Observation of stellar fields, star clusters and galaxies will bring you so much pleasure, while the sharpness of star images will reveal the extraordinary possibilities of your astrograph. It proves to be a fabulous instrument for deep sky and comet surveys. The observation of Lagoon and Trifide nebulas in the same field is extraordinarily seizing.

The rack-and-pinion focuser has a rotary system for framing. A microfocuser (MEF-1) is available on option.

The Epsilon-180ED mechanical design quality, perfectly matched with its optics, will make delicate night handling such as collimation (to be trimmed in full day) and the installation of a photographic image or CCD a lot easier, like for instance : focusing, framing of the object, pointing of the guiding star, etc. Few other telescopes on the market make these operations as easy. The comfort of use of Epsilon-180ED allows you a fast control of your telescope adjustments and therefore gives you time to concentrate on the essential : to set your imaging process.

Epsilon-180ED primary mirror cell
The primary mirror cell is equipped with 3 "double-action" collimation screws (pushing/drawing). Moreover, you have 3 screws with counter-nut to adjust the pressure under the primary mirror in order to minimize the stresses due to strong seasonal temperature changes.

The collimation of Epsilon-180ED is particularly facilitated for various reasons. It is not an high-resolution reflector thus the procedure is less rigorous than on a Cassegrain-like optical design ; collimation on a star will then not be necessary. The optical axis is represented by reference marks on the 2 mirrors. Takahashi conceived a simple system of collimation eyepiece particularly adapted to Epsilon-180ED. Consequently, you will be able to quietly collimate your Epsilon-180ED during daytime, which is a large advantage compared to a traditional reflector.

The Epsilon-180ED Newton F/2.8 hyperbolical design
Epsilon-180ED optical design

The Epsilon-180ED is a catadoptric reflector, including an hyperbolical primary mirror, an elliptical secondary mirror and a 2-lenses field corrector in the rack-and-pinion focuser. It results a perfectly flat field, ideal for wide field imaging.

Epsilon-180ED spot diagram
The perfect correction of field, covering the entire image circle, is attested by the spot-diagram. The diffraction pattern almost does not present a residue of coma in periphery. In the same way, the 2-lenses corrector practically does not generate any chromatism.

Some items that are showing as in stock are in stock at our holding warehouses, not at the shop. To double check the stock levels at the shop, please contact us on 01909774369 or sales@rothervalleyoptics.co.uk.

The delivery times for most items is 1 - 2 days but again, please double check stock levels on important orders before placing an order via the website.

The delivery costs for courier next day are for mainland UK only. If you live in the Scottish Highlands/Islands, Channel Islands or Northern Ireland, then a shipping surchage will apply. please contact us for prices. Smaller items can still go 1st class via Royal Mail.

Please note that if you are wanting to take advantage of our Saturday and Sunday timed services or next day pre 12 or pre 10:30 services, you MUST check that the stock is here at the shop before placing orders. Also, orders using the Saturday and Sunday services must be placed before 1pm the previous working day. Also, please remember to check that the stock is here at the shop before placing orders. If the stock is not at the shop, we won't be able to ship on any of the timed services. 

Please note International customers will need to contact us for a shipping price prior to ordering via the website. We don't ship all items internationally. It is at our discretion what we ship outside of the UK. This all depends on the size and weight of the items. Please get in touch with us for any postage costs. Please note we do NOT ship telescopes or heavy items outside of the UK. This is due to massive postage costs and problems regarding returns.

If you have any questions regarding stock levels or delivery, please get in touch.

Zygo Interferometer Testing For ED Refractor Telescopes!

We are extremely pleased to announce our Zygo Interferometer is now installed and ready for use! Our experienced staff can test refractor lenses up to 120mm aperture and provide a comprehensive 2 page report showing the optical quality and Strehl ratio, plus much more information. We are using the very latest Zygo MX software to provide a more detailed report compared to other standard reports.

The interferometer is essentially a measuring instrument. Within the interferometer is a calibrated laser that is pointed through the optical test surface, then onto a high quality reference sphere, then back through the test subject then to an internal camera which gives us the measurement on the screen. From this, we can adjust the position of the test optic and the reference sphere to obtain a perfectly calibrated system. The more central the laser to the test optic and then on return, the better and more accurate reading and measurement we can take. This takes a lot of adjustment to get the best results from the optical surface. Once the measurement has been taken, we are provided with a series of results that show the optical quality of the surface plus other information. Continue reading for an explanation of the individual values and you can also see a test report that was done on one of our RVO Horizon 60 OTAs. 

We are offering certain telescopes with a Zygo test at an extra cost. Mainly ED doublets and triplets. All available telescopes with a Zygo test report are listed here. Just select Zygo Test Report from the drop down box at the top of the listing and we will test the optics in house and provide a full 2 page report with your scope. This will show you the optical quality of your telescope optics. We can also offer this service on your refractor telescope. Please get in touch for more details about this. 

At Rother Valley Optics, one thing we pride ourselves on is customer service and quality of our equipment. When we test your telescope, we will ensure that it is of the highest quality otherwise, we will reject the scope under our strict quality control and test another model for your peace of mind. One of the main values to look at when testing a refractor is the Strehl ratio. The higher this number, the higher quality lens you have. At Rother Valley Optics, we will guarantee the highest possible Strehl ratio for your telescope.  We will aim to provide 0.95 Strehl or higher on Takahashi, RVO Horizon, William Optics and many more! Generally, the higher the Strehl ratio, the lower the Astigmatism and Coma meaning a better image quality from your instrument. 

Other measurements such as the PV and RMS are important too. With these measurements, the lower the number the better as it shows less curvature on the lens. The flatter an optical lens, the better it will perform. The PV rating (Peak To Valley) is a measurement from the highest point (Peak) to the lowest point (Valley). From this we get the RMS (Root, Mean, Square). This is a similar figure to the PV and measured exactly the same way. The RMS is basically an average height difference from the PV so again, the lower the better. As you can see form the example below, we measured an RMS of just 0.027 wave which is a very good value.

We also measure the Power with our systems which is essentially the error from the reference sphere to the test optic. The reference sphere we use on our system is a very high quality sphere so the closer to zero the Power, the less error between the 2 elements thus ensuring a higher quality optical surface. 

You will also see some more values such as Astigmatism and Coma. Again, these are measured by the interferometer when we take measurements of the optical surface after adjustment. These are values which ideally would be at 0 but as our test optics are all curved lenses, there will always be astigmatism and coma present. The lower the number, the less of these aberations you will effectively see but with most refractors, you can buy field flatteners which will compensate for the coma anyway. The astigmatisms value is explaining the error between the symmetrical curvature of the lens. Basically, no lens will be perfectly symmetrical, the lower the astigmatism, the more symmetrical the lens surface is. 

Once the Zygo test report has been completed, the optical alignment is thoroughly tested and tuned to ensure they are spot on before they leave us. 

All available telescopes are on the website at the link below and ones we've tested already that are available straight away are also listed.

https://www.rothervalleyoptics.co.uk/zygo-tested-refractors.html

Here is an example of the test what we provide. This was a test on one of our Horizon 60 ED OTA's.

For any questions about this amazing new service, please either call 01909774369 or email sales@rothervalleyoptics.co.uk.

Are you interested in this product but would like to speak to someone with some more information? Simply fill in the form below and we will get back to you as soon as we can!

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