• Christmas Comet Shines in Tandem with Geminid Shower

    Comet 46P/Wirtanen, commonly dubbed the ‘Christmas Comet’ thanks to its festive timing, is visible now and will reach its peak brightness on the 16th of December, 2018. Look to the Eastern horizon near the Pleiades cluster as it rises early in the evening.  The comet will be visible all night.  As we near the middle of the month, the green glow surrounding the comet should balloon to approximately twice the apparent size of the Moon making the comet appear as a diaphanous green orb. Head to dark skies to help boost natural night sky contrast and bring a telescope or binoculars for the best views.

    For astrophotographers and night sky photographers, 46P-Wirtanen’s arrival with the Geminid meteor shower offers a great opportunity to capture the green comet in tandem with a light show. The nights of the 13th and 14th of December are your best bet when the shower reaches its peak.

    Discovered in 1948 by Carl Wirtanen, an astronomer at Lick Observatory in California, 46P has been visible during every pass save one - in 1980 it was too near the Sun to see. This comet is a member of the Jupiter family whose orbits are controlled by the planet and are thought to originate from the Kuiper belt, a massive celestial lagoon of icy masses residing outside of Neptune. Their orbits are relatively short, typically less than 20 years. These are comets that we potentially see pass by Earth often. However, they are not always bright enough to see with the naked eye. Many meet an early demise by striking a planet or breaking apart in the atmosphere of one, such as Shoemaker-Levy 9 famously did in July 1992, or degrading in the intensity of the Sun.

    Jupiter family comets are not known for being very bright due to the rapid decline of their structures as they pass through our solar system. Of the over 400 Jupiter family comets known, 46P will be among the brightest to pass near Earth recently and is expected to reach a maximum magnitude of 4.2 at the nucleus as we near the middle of the month. Comet 46P holds the record for the smallest comet nucleus ever recorded.  Measured in 1996 at a likely charitable 1.1km. To give some idea of its size, that’s 1/10th the size of Halley’s comet and 1/13th the size of Hale-Bopp.  While it will not be as bright as a larger comet might have been and may not have much of a visible tail, 46P-Wirtanen is expected to reach a magnitude of 4.2 which is well into the visible-with-the-naked-eye range. This is also the closest the comet is expected to pass near Earth again.

    The comet isn’t the only one putting on a show this time of year. The Geminid meteor shower reaches its peak on the 13th and 14th. The most reliably brilliant shower every year, the Geminids put on a unique light display of noticeably slower meteor trails than other showers.  They often seem to skip and glide across the night sky sometimes lasting seconds or leaving behind green dust trails for minutes.  Because Geminid meteors are not the remnants of a typical comet tail but rather the rocky trail of a large mass called 3200 Phaethon, their composition is denser and the result is brighter longer lasting streaks of light as they enter our atmosphere.   This shower can reach peaks frequencies of up to 120 meteor per hour, promising a good showing even from suburban areas with moderate light pollution.  Peak times are about 2am your local time.


  • Eagle Manager Update

    EAGLE Manager update

    Last version 2.5 10/10/2018:

    1) Improved support to ECCO environmental computerized controller
    2) Bug fixes

    Version 2.3 18/07/2018:

    1) Added support to ECCO environmental computerized controller
    2) Improved ON-OFF management of USB ports
    3) Added "remember my choice" in power window
    4) Improved stability
    5) Bug fixes



    Click here to download.

  • Fish Head Nebula with Pixinsight by Tim Connolly

    Goodbye Photoshop! Today was the first day I used Pixinsight. After spending the last few days watching tutorials and reading guides, I gave it a shot with Fish Head Nebula (IC1795), at the bottom of the Heart Nebula, in the constellation Cassiopeia. At first, Pixinsight appeared very foreign to me and overwhelming, but I started figuring out the different features through trial and error. I still have much to learn, but I am more than satisfied with the software. I used Image Integration and Image Calibration to register and stack the images. I then used LRGB to combine the channels and produce the Hubble Palette mapping the Sulfur II channel to Red, Hydrogen Alpha channel to Green and Oxygen III channel to Blue. I then went through and tried different processing with the curves, histogram and background processes. I really found the masks to be easy to use and found different methods to make the masks. I’m going to redo my previous narrowband images of Elephant Trunk Nebula, Cygnus Wall and Wizard Nebula with Pixinsight.
    Ha - 15 - 300 second exposure images
    OIII - 15 - 300 second exposure images
    SII - 15 - 300 second exposure images
    Darks - 25
    Bias - 25
    Flats - 20 (each filter)
    Orion 8” F3.9 Newtonian
    ZWO ASI 1600 mm-pro
    ZWO 7nm narrowband filters
    Celestron CGEM DX Mount
    Captured using SGPro (Trial Version)
    Calibrated, Stacked and Processed in Pixinsight (Trial Version)
  • Warren Keller Fall 2018 Workshop

    California here we come! Warren Keller and Ron Brecher are teaming up to present a 3-day workshop, September 28-30, 2018 at Astro-Hutech in Lake Forest, California. This is a convenient commute for many imagers, whether from home or SNA and LAX airports. Register today!

    The cost for three full days of PI instruction is $595.00 USD. Registration is now open and is limited to about 20 attendees. Take your PI skills to the next level, working in an intimate setting with personal attention from two experts. Follow the link below for a detailed agenda, accommodation information, and to register. Consider that with the Advanced Imaging Conference (AIC) back in 2019, we'll not be able to repeat this class next year!

    Things our students said

    “… 5 stars. You guys are exceptional.”
    Richard Payne
    “I LOVED the hands-on approach.”
    Prof. Samantha Blair
    “I liked the fact that you covered so many topics and included many tips and shortcuts.”
    Greg Piepol
    "Instructors were very personable, entertained questions, and were available for hands-on help and pointers.”
    Bob Taylor

    This Introductory-Level course will focus on the following objectives:

    • Get you comfortable in the PixInsight working environment
    • Demonstrate a simple workflow to produce a good-looking image from raw data
    • Reveal intermediate techniques for further improving your images
    • Build your skills by processing your own data, with individual coaching from the instructors

    While the course is aimed at those nearer the beginning of their PixInsight journey, astrophotographers of all skill levels will learn new tips and tricks for successful deep-sky astro-image processing.

    Day 1 focuses on learning the user interface and processing environment, and takes a simple data set through a complete processing workflow.

    On Days 2 and 3, we'll dig deeper, mining more complex tools and techniques to enhance your workflow. The workshop includes three 'Process Your Own Data' sessions where the instructors will provide targeted coaching and advice based on individual interests and needs. These are great opportunities for the more advanced processor to get what they need from Warren and Ron.

    Follow the link below for a detailed agenda, accommodation information, and to register. Do not hesitate to contact us with any questions. Thank you!

    Register Now

  • Party Under the Stars

    Click here to check out this blog post!

  • Join LAAS at the Boeing Santa Susana Field Lab Star Party- Sept. 15th!

    Join the Los Angeles Astronomical Society on September 15th at the Boeing Santa Susana Field Lab.  This is a rare opportunity to star party at this site, and with very few lights in the surrounding 2600 acre facility, it is sure to be an enjoyable night under the stars.

    We need 72 hours advance notice for equipment set up. If you are interested in bringing your equipment, please let us know by filling in this contact form, let us know what equipment you plan to bring and we'll be in touch with more details.

    Contact Us


  • Taurus A "discovered" by SPIDER radio telescope

    This entry was posted on May 2, 2018 by Filippo Bradaschia.

    Taurus A "discovered" by SPIDER radio telescope
    Taurus A is the radio source in Taurus constellation that corresponds to the Crab Nebula (M1), the supernova remnant exploded on July 4, 1054 and noted by Chinese and Arabian astronomers of the time. Since then, the gas cloud has expanded and today is over 6 light years large. In this article we see how the SPIDER radio telescope "discovered" it by capturing the radio waves emitted by Taurus A and converting them into a radio map, a real photograph in radio waves of this nebula. In fact it is believed that Taurus A emits radio waves for synchrotron radiation caused by electrons in fast spiral motions around magnetic field lines generated by the pulsar inside it. Thanks to the large antenna and the 1420 MHz H142-One receiver, the SPIDER radio telescope was able to easily record the weak signal and, thanks to the precise mount and pointing system, it generated a radio map with the same technique used by professional radio telescopes.
    Studying the sky at the frequency of 1420 MHz has several advantages including the ability to capture radio waves even during the day and through the clouds. But at this frequency the electromagnetic emission of many radio sources is quite weak (in fact, professional radio telescopes use very large antennas and are very expensive). At the frequency of 1420 MHz the strongest radio sources are:

    Sole: flux about 40000 Jansky
    Cassiopea A: flux about 2400 Jansky
    Centaurus A: flux about 1700 Jansky
    Cygnus A: flux about 1600 Jansky
    Sagittarius A: flux about 1600 Jansky
    Vela X: flux about 1600 Jansky
    Taurus A (M1): flux about 875 Jansky
    Orion A (M42): flux about 520 Jansky
    NGC2237: flux about 260 Jansky

    With SPIDER, the Sun is so strong we can use it as reference radio source to align the mount on the fly. All the other radio sources are weaker but the high sensitivity of the SPIDER radio telescope allow you to really record them. In order to verify this, we used the SPIDER 300A radio telescope installed in Marcello Ceccarelli visitor center in Medicina (Bologna, Italy - near the professional radio telescopes of INAF) to record a radio map of Taurus A and demonstrating the features of RadioUniversePRO control software that comes with the SPIDER radio telescope.

    A radio telescope is different from an optical telescope by many aspects: one of these is that it collects radio waves from a single area in the sky. Just to give an example, it's like having a telescope with a CCD camera that comes with a single large pixel. In order to create radio maps, technique consists in moving the antenna with small movements and, for every sky position, record radio waves coming from space tracking the sky apparent movement. Then the SPIDER antenna is moved to a new position and record the next pixel value. For every pixel, RadioUniversePRO software calculates the total amount of radio waves captured and displays this value with a color based on a color scale chosen by the user.

    RadioUniversePRO software allows you to point the radio telescope to the precise sky position of the radio source, visualize in real time the bandwidth spectrum in frequency so you can see if you have artificial signal in it (allowing you to filter these from your recordings) and define radio map specifications like:

    Dimensions in degrees (AR e DEC)
    Pixel separation
    Integration time for every pixel
    Colour scale type for visualization
    Hystogram stretching
    Optional visualization with level curves

    So we started a 3 hours capture, setting the following parameters in RadioUniversePRO:

    Map dimensions: 15 x 15 degrees
    Pixel separation: 0,4 degrees
    Integration time for every pixel: 5 seconds
    The result is the map that we show in the image below. You can easily see the increase of the signal at the center of the map, corresponding to Taurus A position. The increase in the visible signal at the top right of the image is the Milky Way, in fact Taurus A does not lie perfectly on the plane of our galaxy but it is a few degrees away (as confirmed by the radio map). The image below shows the same radio map but displayed with the level curves.


    This way we demonstrated that, thanks to the high sensitivity and pointing precision of the SPIDER radio telescope, it is possible to realize radio maps also of weak radio sources using the same techniques employed by professional radio telescopes!

  • Navigating the August 2018 Sky!

    Check out the sky wheel link below!



  • Eagle Nebula

    QHY183M, Exp Sci ED127, 0.7x reducer, CGE Pro, Rayox Saddle
    Ha 6h (combined with a customers data)
    SII 1h 30m
    OIIII 1h 30m
  • Doctor D Review Sky-Watcher Evostar

    Over the course of the past 25 years, I've encountered a pretty vast number of vivid views of the solar system while comparing telescopes and I've kept a journal over that period. After you see so many images using various optical systems, you collect a visual archive or frame of reference from which to gauge other views. For this particular session the seeing started out at about a 7 and worked its way to an 8. This is where the planets remain pretty still with trifling air movement. The inversion layer was clearly visible below, over the LA basin and then the moisture kicked in. These were all tell-tale signs that the seeing would hold. Even atmospheric dispersion wasn’t an issue worth bothering with even though we had corrective measures on tap to deal with it. If these Evostar’s remain well figured like this, then I believe there’s some­­thing special on the horizon at a very reasonable price.

    Whenever I’m evaluating any telescope, I always look at the empirical evidence of the views. I sympathize with people who can’t afford to shell out several thousand dollars on a premium brand refractor and maybe our experiences can shed some light. I told my observing buddy Derek Wong I would be bringing the Evostar over so we could take a closer look at it and share opinions with two other close observing buddies Hawk and Luigi. The glass in this sample and the others at SkyWatcher are slightly improved over the original sample displayed at NEAF and as such, are expected to remain so with these production units. When we went into this, we honestly didn't expect to see what we did and we were all quite shocked to tell you the truth.

    The scope settled down about an hour and a half after setup around sunset. We primarily switched between a 7mm t6 Nagler at 171x and a 5mm t6 Nagler at 240x for the tests. I suggest having a 5mm, 6mm and 7mm for planet viewing with this scope. Derek selected one of his premium Tak diagonals which worked superbly. As the optics settled in more with Jupiter, I was starting to get the sense that this was a really impressive refractor at any cost, even compared to premium scopes costing several times more. So, we decided to star test the scope. Even before I handed Derek a green filter, he could already start to tell the optical figure was indeed excellent. With the green filter inserted, the star test looked textbook with a very slight amount of under-correction which is exactly what I was hoping to see since the optics will only improve in this circumstance. There were no visible signs of unwanted zones, astigmatism, over-correction, nothing that stood out to any of us. This really stunned us all. Even in some premium optics you can find these little optical gremlins from time to time. I usually expect to at least see something worth mentioning, but that simply wasn't the case here.

    I could even see the collimation looked excellent while I focused slightly in and out with Jupiter, another green flag. According to Skywatcher, there are several adjustable screws on the side of the cell. Checking collimation on a star with refractors is not always as easy as people may think, unlike an SCT. So, I usually use planets when the seeing is good and the telescope is reasonably acclimated to determine if collimation is an issue during observation. With regard to false color on Vega, when I ran the focus slightly back out, I could see a light greenish tint. In focus, you see some hints of violet on Vega and other bright stars more so at higher magnifications. The amount of color an observer sees may also be dependent on their age and sensitivity to color in the dark, but it's not that objectionable when the telescope was focused, especially while observing planets where it's mostly color free. The color correction on and around the globe of Jupiter looked superb and I'm pretty sensitive to false color. With Venus, you will see false color at night but remember that anyone who has experience viewing Venus knows that it’s best viewed in broad daylight, which means false color will be far less noticeable.

    All of us were very impressed. Jupiter had amazing surface detail and it was really tack sharp with surprisingly high contrast. Even our friends Hawk and Luigi were surprised and both are owners of exquisite telescopes in their own right. The rusty looking GRS was vivid right at the edge of the globe as it was starting to make its ingress. The colors on the surface had beautiful rusts and pastel hues. There was an intricate network of surface features and the globe looked completely organic as if unhampered or hindered by anything distracting. I remember saying to the guys how impressed I was. I have a world class FS152 and I have to admit that it doesn’t have much on this Evostar with planets and I’ve used it over a dozen years. With my Tak, the color on brighter stars at higher magnifications appear slightly more accurate in color correction through the FS152 but at several times the cost, it should. At lower magnification for objects such as star clusters though, the differences are even less noticeable. Most of you veteran observers who know me, know I've compared a countless number of refractors and reflectors. The images of Jupiter we saw on this night were beautiful and right up there with some of the finest optical systems I've ever seen in this aperture class. Even with Saturn on the rise, at 240x we could easily see the Crepe ring. The Encke Minima was also visible in the middle of the A ring upon careful scrutiny. At one point Derek even looked at us all and said... maybe we should set up the FC125 to see what happens. Derek’s particular FC125 is my favorite 5” ever because the optical figure is truly world class and a very special specimen. We all knew though, there would not have been enough time to properly acclimate the FC125 and as a result, the comparison would not have been fair to the 5".


    Mechanically, I'm pleased with this entire setup including the dual speed crayford focuser at this price point. It feels smooth and solid. For imaging, there's a DX model and it's the exact same telescope with a heavier duty rack&pinion focuser and Losmandy style D plate instead of a Vixen style plate on the standard model. The DX model is also heavier and as a result, should help the appearance of the balance point look more aesthetic. I did not have a finder attached on my sample, which would have added a bit of wanted back-weight. For visual work, the standard focuser is fine in my opinion. Regarding the weight of the OTA, I normally have to use three 11lb counterweights with my EM200 mount when using my FS152. With the Evostar, I only needed two counterweights. The OTA is rated at just over 20 lbs and feels considerably lighter than my FS152 and more like my loaded FS128. I think observers could do okay with mounts like the Losmandy GM8 or AVX just for visual work only. In my opinion, the hard case is a bit too large for practical transport, but makes good as a storage case. I measured the dimensions at 55.5" x 11.5" x 15.5". It does allow plenty of space for accessories though. I suggest a soft case for more practical transport which is what I use for my FS152. Orion and Pacific Design soft cases are available. Another thing some observers may want is a compression ring adapter if they're concerned about the screws used in the visual-back. These compression ring adapters are available from other suppliers such as ScopeStuff at a reasonable cost.

    The Evostar 150ED is one of the most controversial refractors right now because it was decided that the information about the glass would be undisclosed. Televue has never disclosed what type of glass they use either but maybe people figured because it's Televue, it doesn't matter. Okay, so let's talk about that. Seeing some trifling amounts of false color or false color in general by an observer is not necessarily an evaluation of a refractors performance and I can attest to that from 25 years of using, comparing, and evaluating countless refractors in the field side by side. The subject of false color is often misinterpreted because some observers don’t understand why they're seeing it out of focus in the first place and often, incorrectly assume the optics must be inferior as a result. This is a big mistake I often see, particularly among beginners in the forums who read too deeply into these topics.

    The ability to distinguish sharp contrast on the surfaces of planets in-focus and resolve fine, low contrast details is the real evaluation, but very seldom do people talk about this. Perhaps they're unable to observe for whatever their reasons are. I'm aware of the observing habits people have and I pay attention to them, even though they may not know it. If someone walks up to look through my telescope, I will sometimes ask them to take their time. If that person sits for 15 seconds, chances are they're really not really observing at all. Instead, what they're doing is just peeking. There's a huge difference between a person who peeks and a person who is observing. When you sit for good periods of time with your own telescope, scrutinizing a planet, your eyes and mind can pick up very elusive details that will often go unnoticed to a person just taking a peek, assuming the seeing allows for it. Even writing down some observational notes can help.

    After spending more evenings with this Evostar 150ED by myself, I have been more impressed with its visual performance, particularly on deep sky objects such as star clusters, which look very much like they do in my Takahashi FS152. There are some amazing refractors out there, but this Evostar can put up one heck of a fight against other premium scopes and we certainly found that out quick. The smoothness of figure is remarkable and it amazes me how high the contrast of the planets look through it after it's acclimated.


    This is what many people want to know. To put it to the test, we pulled out Hawk’s world class TEC140 under reasonably good seeing using various magnifications while viewing Jupiter and Saturn. All of us took turns going back and forth. Everybody, myself included were scratching our heads. Incredibly, there really wasn't that much difference, in fact all of us had to wait for really good moments of seeing to make any solid decisions and even then it was extremely close. Derek's daughter has young eyes and we asked her to take a look and offer her opinion. For a while she was liking the TEC140, then she went over to the Evostar and sat for a while and said.... I like this now! Then she went back to the TEC140 again and said she liked it just a bit more. In my opinion, the TEC140 had just a very slightly more refined image, but only under the steadiest moments. Even then, it wasn't by much, in fact Hawk who owns the TEC140 said multiple times that he couldn't even see much difference and certainly not three times the price difference. Saturn's globe is covered in a haze of ammonia ice crystals and as a result, has dull surface contrast on the globe compared to Jupiter. In the TEC140, the globe appeared to yield just a tad more surface contrast, but the Crepe ring unquestionably appeared to yield a bit more contrast in the Evostar, probably because of the additional 10mm of aperture. Most of the time, the seeing caused more of a difference between the two scopes than the scopes themselves.


    While you do your research, you will stumble on reviews of the APM 152ED and even a new triplet that is still questionable for a bit more money, but here's what you may not be aware of if this is all new to you. The APM 152ED was originally branded in the United States as the Lunt 152ED. This telescope is also part of my review site and was one of the earlier models which had a good, solid lens cell and as such, got a good review by BillP a very well known reviewer and friend of mine. When the Lunt 152ED was launched, I was extremely excited because it was a chance to help others get into a 6" ED at a relatively affordable price! Unfortunately, because of quality control issues, a good number of samples I evaluated were out of collimation and there were other observers who also had to work through the issues with their samples as well. There were some observers who got some decent samples, but the quality control was still in question and I ran out of steam dealing with them. Not only that, but most of them had so much under-correction, they could not even produce a diffraction pattern on the outside of focus, even in green light after they acclimated for three hours in low deltas. Here is what should happen when you star test a refractor to check the spherical correction. Usually when a refractor is still acclimating, the star test will exhibit under-correction. There’s more to it, but this basically causes the diffraction pattern to look fuzzier on the outside of focus. This is completely normal for nearly all refractors and should be expected. As the optics acclimate, the star test will normally improve and the diffraction pattern will slowly become more apparent outside of focus. Jet streams in the upper atmosphere can also wreak havoc as well as spherochromatism (use a green filter) and distort the outer rings while outside of focus. So, you have to be careful not to misjudge the optics prematurely.

    The Lunt 152ED's never reached that point and remained in a severe state of under-correction permanently for several possible reasons. The result was scattered light around the planets, almost like a faint halo of light which compromised the surface contrast of the Moon and planets. Because of these issues and the fact that there really wasn't any way to properly repair them in the US, the remaining Lunt 152ED’s were sent back overseas and rebranded under the APM 152ED name you now see today. What about these new triplets you hear about? Here's another thing you should know if you don't already. Triplets can be even more complex than doublets. Just because you have a triplet doesn't necessarily mean you will have better contrast. This is the big mistake I see beginners often make. I've evaluated plenty of highly color corrected triplets with low contrast, why? Because they can sometimes have unacceptable amounts of spherical aberration due to poor quality of optical figure. Also, what if they go out of collimation? You think collimating a doublet is hard? Wait till you try a triplet and ask yourself this question. Who will service them if they need servicing?


    I can’t believe the amount of detail beginners subject themselves to, it’s incredible to see. It reminds me of that scene in the movie Stir Crazy where Gene Wilder and Richard prior try to use Karate chops to intimidate other jail-mates when they walk into the jail cell. People that are beginners get involved in these exchanges about spot diagrams, color index, color curves, MTF’s, glass types etc. This is very technical and complex stuff that causes beginners to read too deeply on unexperienced eyes. There are really only a handful of people who truly understand the implications of these topics and how they may or may not manifest themselves in reality and even then you need to have experience using a telescope in the field to make any possible sense of it. It's just not as black & white as beginners think. The color correction for most ED refractors sold in today’s market are quite good for enjoyable visual observation with most amateurs, relax. It’s not like you’re going to look in one refractor vs another and say oh my, I made a mistake! Mistake about what? Because you saw a bit of false color? What kind of evaluation is that? The real meat & potatoes of any optical system is the spherical correction, which is the "optical figure". This is what really gives you great contrast. People are so overwhelmed because there are so many ED refractors to choose from. When I read some of the comments beginners make in the forums, it’s really easy to spot who’s drinking the Kool-aid and who is not. Since the Evostar has more spherochromatism than highly corrected triplets like the Esprit for example, that out-of-focus color can be used to determine focus. What occurs sometimes is that the seeing conditions can play games with your eyes and mind and here's where it can trick you sometimes. If the seeing is good, it's easier to find focus because when you do, the slight bit of false color you see out of focus disappears. But, if the seeing is bad, it's sometimes harder to find focus and as a result, while moving slightly in and out of focus, you'll see that bit of color, so don't freak out. Once you're in focus, it's really nice.


    I’d like to share some personal experiences about the telescope industry many people don’t acknowledge or understand. In order to bring telescopes like this into production at a very reasonable cost, a good number of them have to be made. Finding acceptable glass in certain apertures that meet the proper quality criteria have to be acquired as well as several other technical challenges like research, product development, marketing, etc. People often get ideas in their head that these companies can just do what they want and it's not that simple. You wouldn’t believe the frustrations companies and vendors go through with people regarding their gripes. People these days with internet sales are extremely demanding and vocal about issues they encounter as if they're quick and easy to fix. It's a very complicated situation.

    I've been selling telescopes for many years and I've watched this industry change over night because of an overwhelming number of mass produced products being imported from overseas. The more there is to select from, the more dubious and overwhelmed people become and the more people feel compelled to research the heck out of things and in many cases way too deeply. The beginner starts to think more and more and research these differences to a point where they often can't make a decision at all or are looking too deeply into something that's being blown completely out of proportion by others. I've seen this happen countless times because there's so much available information. On that same note, there's also a great deal of misinformation. A lot of people want to be their own opticians now and it's a huge trend that's going on. I miss the reviews of Ed Ting and Todd Gross who conducted fun comparisons and expressed their visual impressions of telescopes back in the day. They didn't go into these huge fiascos about false color and glass types we now see today.


    In my opinion, the Evostar is an exceptional value. You also have technical service and support from SkyWatcher USA should it ever be needed and I think there's value in that. This refractor also proved that it was capable of standing up to some of the finest telescopes on the market at a fraction of the cost. Also, I try to help as many people as I can. If you have any thoughts or questions, I'm happy to talk with you if I have time available.



    Steady skies,

    Daniel Mounsey aka Dr.D


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