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MarsG76

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Everything posted by MarsG76

  1. That sounds like a good plan, just be careful about how much space you create between the OAG and the camera as there is a limited amount of distance that you'll be able to pull out of the OAG before using extenders (which is not ideal).
  2. Yes I BIN2x2 my 120MM mini.... As far as imaging goes, I dont see my self going back to guide scope again... once the OAG is setup as running... and thats not that hard to do one you do it a few times... takes care of flexture and you're guiding at the same focal length as imaging. One important thing to note is make sure the OAG is parfocal with the camera, half the problems in not finding a guide star was that the OAG was not in exact focus, limiting to the brightest stars if not completely eliminating seeing any of them.
  3. I'm using a ZWO120MM mini with a OAG on my C8 at 2032mm focal length, and I don't remember having a situation where I didn't find at least one guide star within the search area. On my 500mm focal length refractor, I don't think I ever seen a starless field.
  4. Now this looks like a experiment calling out for attention... have you got a 3D printer? If so, print the mask and give it a try.
  5. Yes thats true... although if a Takahashi has this issue than it must not be a big deal... chromatic abberations are definitely of no concern when imaging with a mono camera and the telescope is refocused for each filter.
  6. I think you nailed it... thanks for that link.... Images in the link definitely resemble what I was seeing... and I think that I didn't see this phenomenon before because I was focusing at a lower resolution image BIN 2x2 or 4x4... now I did it at BIN 1x1 with the 1:1 view centered in the frame and it all became curly. I did a experiment today and again I saw the culrs but not at BIN 4x4. Nice work.
  7. Definitely not oscillations.... I think Vlaiv is on the money...
  8. I installed version 4.00 and used it as a test session tonight during the full moon and I'm happy to say, no weird adverse bugs showed up in about 5 hours of use... thank you for your hard work.
  9. Hi All, Has anyone seen this phenomenon while using a Bahtinov mask for focusing... for some reason my diffraction spikes are curly! There was no scope/mount vibration that I could detect, no other obstruction in the optical path such as dew, dirt or anything other than a UV/IR filter. No trees or other obstruction in the line of sight. There was a little bit of haze in the sky and the 88% full moon was about 25 degrees toward the east from the star I was focusing on at the time. Also these curls rotate with the rotation of the Bahtinov mask... So unless the curls are some kind of a negative moon phase reflection, I'm out of ideas at this time. The diffraction spikes on my SCT are straight, so this seems to be happening on my BOSMA Beta-RE 80mm refractor, but I haven't seen this happen before tonight. Camera is a QHY268M. This has not stopped me from focusing on the star, and doesn't look like this effect is present in my test subs exposures, but I'm very curious to what could be causing these curls. Clear Skies, Mariusz
  10. A UV/IR Cut filter will definitely improve guiding... but heres an idea I've had and tested with consistently improved guiding results... I'm now using my IRPass685 filter on my ZWO120MM mini guide cam instead of the IR cut filter and my guiding seems to have consistently improved by around 0.2" RMS.
  11. Hello All, Sharing with you the last of my 6 pictures that I imaged across the 8 clear nights that I had between 21 April and 7 May. This is NGC 3521 is a flocculent intermediate spiral galaxy located around 26 million light-years away from Earth in the constellation Leo. I think that this is a nice looking galaxy but unfortunately the end resulting image turned out quite soft, a lot softer than I was hoping for after seeing my initial subs. The stars are looking a little bit bloated and fuzzy, but I know that I didn’t have condensation problem on the corrector plate or the camera sensor, so I’m suspecting that either (and most likely) the focus was slight off or the bubble of dust that is surrounding this galaxy is obscuring the hard details… I’m leaning toward focus (or seeing) being the biggest problem because the stars are fuzzy and I had tighter stars in the past at this focal length. I’m going to have to re-image this galaxy in the future, perhaps revisit it next year. Imaged using a 8" SCT (at the native 2032mm focal length), with a QHY268M camera on a HyperTuned CGEM mount. The total exposure time of this image for all of the LRGB filters was 12 hours and 1 minutes. Exposures: L:14x600s @ FW:31 & L:6x600s, L:8x900s, R:12x120s & 7x180s, G:12x180s & 6x300s, B:12x300s & 7x600s, Hα:16x600s @ HCG:62/OFS:25 Clear Skies, Mariusz
  12. From the album: Deep Sky Imaging

    NGC 3521 is a flocculent intermediate spiral galaxy located around 26 million light-years away from Earth in the constellation Leo. Imaged using a 8" SCT (at the native 2032mm focal length), with a QHY268M camera on a HyperTuned CGEM mount. The total exposure time of this image for all of the LRGB filters was 12 hours and 1 minutes. Exposures: L:14x600s @ FW:31 & L:6x600s, L:8x900s, R:12x120s & 7x180s, G:12x180s & 6x300s, B:12x300s & 7x600s, Hα:16x600s @ HCG:62/OFS:25

    © Mariusz Goralski

  13. I think that it's a good quality image, although it does need more subs... more data (and dithering subs) will remove the noise and color mottle. That said, I love imaging with my C8, (same specs as the 8SE) and the 8SE, or any 8" SCT will have it's challenges and limitations. One is the coma at the edges which needs to be cropped off. The other problem is the fact that with 2032mm (or 1280mm with a 0.63 reducer) needs very clear skies for it to perform at it's capable resolution, otherwise the images will be oversampled and soft with bloated stars. Personally I always BIN 2x2, and if my seeing is worse than 2" I just don't bother, or image with my refractor at 500mm. But when the seeing is good, 1" or better, the details that the 8SE is capable of capturing is fantastic. So to answer your question... NO the 8SE is capable of considerable better quality images.
  14. Beautiful M51 with which to end the galaxy season.
  15. Yup, I think you got it.... that is so awesome.
  16. Hello again from down under... This is the second last object image that I have imaged during my clear and moon less nights I was lucky to have been graced with... When I was exposing The Eagle Nebula, I imaged it through all of my narrowband filters, S2, Ha, O3 and HBeta... The first image I processed was predominantly using the standard Hubble palette SHO method (with HBeta only used for star color), but a while ago I found that using a color configuration of Ha, O3 and Hb as RGB, actually delivers colors which are very close to natural looking... with the added benefit of cutting through light pollution, allowing much longer sub exposures than with broadband RGB and potentially capturing fainter matter with more contrast. This image was taken with a 8" SCT (at the native 2032mm focal length), with a QHY268M camera and tracked using a "hypertuned" CGEM mount. The total exposure time of this image was 12 hours and 45 minutes. Exposures: Hα:17x600s, OIII:17x900s, Hβ:17x1200s @ HCG:62/OFS:25 Clear Skies, Mariusz
  17. Hello Fellow lovers of Astronomy, As clouds have returned, I'm continuing in processing my captured data of the 6 DSO objects I imaged across the 8 clear and moonless nights I was lucky to have recently. The images attached are of the Sombrero Galaxy (M104) and the Antennae Galaxies (NGC4038 & 4039) through LRGB filters... The Antenna galaxies were a last minute choice when I got ready to image the Sombrero and realised that my observatory hut still obscured it, so I though that I'll spend a couple of hours on the Antennae through the same filters before moving onto the Sombrero a bit later on in the night, and perhaps score a bonus image to add to my collection. The Antennae Galaxies ( NGC 4038/NGC 4039) are a pair of interacting galaxies in the constellation Corvus. They are currently going through a starburst phase, in which the collision of clouds of gas and dust, with entangled magnetic fields, causes rapid star formation. The total exposure time of the Antennae Galaxies through all of the LRGB filters was 5 hours and 9 minutes. Exposures: L:15x600s @ FW:31, R:17x120s G:15x180s B:16x300s @ HCG:62/OFS:25 And the total exposure time the Sombrero image for all of the LRGB filters was 6 hours and 14 minutes. Exposures: L:17x600s & 15x300s @ FW:31, R:14x120s, G:12x180s, B:13x300s @ HCG:62/OFS:25 Both pictures were imaged using a 8" SCT (at the native 2032mm focal length), with a QHY268M camera. Clear Skies, Mariusz
  18. From the album: Deep Sky Imaging

    The Eagle nebula (M16/NGC6611) in the constellation Serpens exposed through narrowband filters at Hα, OIII and Hβ wavelengths to emulate natural colors as those narrowband wavelengths are closely corresponding to the RGB wide band. This image was taken with a 8" SCT (at the native 2032mm focal length), with a QHY268M camera and tracked using a "hypertuned" CGEM mount. The total exposure time of this image was 12 hours and 45 minutes. Exposures: Hα:17x600s, OIII:17x900s, Hβ:17x1200s @ HCG:62/OFS:25 The color channel assignments are HAlpha, OIII and HBeta as RGB.

    © Mariusz Goralski

  19. From the album: Deep Sky Imaging

    The Antennae Galaxies ( NGC 4038/NGC 4039) are a pair of interacting galaxies in the constellation Corvus. They are currently going through a starburst phase, in which the collision of clouds of gas and dust, with entangled magnetic fields, causes rapid star formation. Imaged using a 8" SCT (at the native 2032mm focal length), with a QHY268M camera. The total exposure time of this image for all of the LRGB filters was 5 hours and 9 minutes. Exposures: L:15x600s @ FW:31, R:17x120s G:15x180s B:16x300s @ HCG:62/OFS:25

    © Mariusz Goralski

  20. From the album: Deep Sky Imaging

    The Sombrero Galaxy, also known as M104 or NGC 4594, is a spiral galaxy in the constellation Virgo located 31 million LY from Earth. The galaxy has a diameter of approximately 50,000 light-years), a third of the size of the Milky Way. It has a bright nucleus, an unusually large central bulge, and a prominent dust lane in its inclined disk. The dark dust lane and the bulge give this galaxy the appearance of a sombrero. Imaged using a 8" SCT (at the native 2032mm focal length), with a QHY268M camera on a hypertuned CGEM mount. The total exposure time of this image for all of the LRGB filters was 6 hours and 14 minutes. Exposures: L:17x600s & 15x300s @ FW:31, R:14x120s, G:12x180s, B:13x300s @ HCG:62/OFS:25

    © Mariusz Goralski

  21. Hello Astronomers, Sharing an image of my favourite globular for observation, NGC 6752, also known as the Great Peacock Globular or the Pavo Cluster, is a globular cluster in the constellation Pavo. It is the fourth-brightest globular cluster in the sky, after Omega Centauri, 47 Tucanae and Messier 22, respectively. It is best seen from June to October in the Southern Hemisphere. I remember seeing this object in the eyepiece and the view was fantastic, and I was thinking that I have to image that globular cluster. This cluster, even though smaller, is a more interesting eyepiece sight than even the huge Omega Centauri Globular which is impressive in itself... but the Pavo Cluster has the edge due to it's mix of very bright and very dim strs, where as Omega Centauri stars are generally all of a similar brightness. This image was exposed using a 8" SCT (at the native 2032mm focal length), with a QHY268M camera. The total exposure time of this image for all of the LRGB filters was 6 hours and 2 minutes. Exposures: L:34x300s @ FW:31, R:20x120s G:19x180s B:19x300s @ HCG:62/OFS:25 Clear Skies, Mariusz
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