Jump to content



  • Content Count

  • Joined

  • Last visited

  • Days Won


alan4908 last won the day on September 3 2020

alan4908 had the most liked content!

Community Reputation

2,723 Excellent


About alan4908

  • Rank
    Sub Dwarf

Profile Information

  • Gender
  • Interests
    Astrophotography ! ....at the moment I'm concentrating on deep space imaging
  • Location
    East Sussex

Contact Methods

  • Yahoo

Recent Profile Visitors

8,886 profile views
  1. Thanks for the comment Adam. Alan
  2. Thanks for the comment Peter. I did spend quite a lot of time on the star field colours, mainly because I acquired quite a few sub frames in non ideal conditions. However, I agree, I think the end result looks OK - it is amazing what you can do in post processing ! Alan Thanks Paul - yes, not often see here - which probably due to its small apparent size. As I mentioned above, even at 0.7 arc seconds/pixel, I decided to crop the image to create more visual impact. Thanks Michael - good luck with your forthcoming capture. Alan
  3. Thanks for the comment Alan
  4. Thanks - glad that you liked the end result. (I discovered that I had a red glow around all my stars due to my FWHM of my red channel stars being much larger than the other colour channels. This was due to the fact that I acquired the majority of the subframes in non ideal conditions. However, I corrected for this effect by eroding the red channel through a star halo mask) Alan
  5. Thanks for the comment Graham - good luck with your capture. Beware that it has a small apparent size, I was imaging at 0.7 arc seconds/pixel but even at that level I decided to crop the image down to focus the viewers attention on the cluster. Alan
  6. Discovered in 1788 by William Herschel, NGC 2419 is one of the most massive and brightest globular clusters but appears as a dim 9th Magnitude object due to its large (275,000 light years) distance from Earth. The bright blue star to the left of NGC 2419 in the image below is HD60771, which is much closer, being only 350 light years distant. In 1944, the American astronomer named it the “Intergalactic Tramp”, since it was once (erroneously) thought not to be orbit around our galaxy but rather wandering the space between Earth and the even more distant galaxies. More recent observatio
  7. Thanks for the comment Thanks. Thanks Peter - I think I prefer the colour in this reprocess of the ED 80 data - this time I used Pixinsight's Photometric Colour Calibration process. Alan
  8. Whilst waiting for clear weather, I decided to reuse some data that was previously acquired by my Skywatcher ED80 and my Esprit 150. I used the Esprit data to get maximum detail on M106 and its companion NGC4248, whilst I reprocessed the ED 80 data such that the resultant background showed very faint objects. The ED 80 data is LRGB whilst the Esprit data also contains a Ha blend into the red channel. On the processing side, I used RegiStar to align the Esprit 150 and ED 80 images and then used Pixinsight's Gradient Mosaic Merge to create a seamless image. Alan M106
  9. alan4908

    Deep Sky III

    Images taken with a Trius 814 and a Esprit 150
  10. Here's five of my favorites from 2020, all taken with an Esprit 150 and a SX Trius 814. Alan NGC3718 NGC4725 NGC6995 Vdb152 M94
  11. Thanks - I don't think I could have done this without an automated set up. Thanks Martin ! I'm fortunate to live at a location which (by UK standards) has very good dark skies. I'm also at the top of a hill which helps, although it does get rather windy at times.
  12. My image generating productivity has been significantly decreased by the poor UK weather in recent months. Even with an automated observatory, my image capturing has been moving at a glacial rate. However, here’s the latest image to finally emerge from my set up – NGC 7497 NGC 7497 is a spiral galaxy in the Pegasus constellation, approximately 60 million light years distant with a disc size of approximately 91000 light years. The galaxy shows signs of warping indicating past interactions. You can (just) make out some HII regions in the image below that appear to be semi-randomly position
  13. A second attempt at the Witch’s Broom Nebula (NGC6960), this time in narrowband. It took me 3.5 months to acquire the data, which was caused by a combination of poor UK weather and the partial obstruction by trees at my location. Anyway, better late than never.... Although imaged in narrowband, I tried to go for realistic looking colours so started with Ha mapped to red and OIII mapped to blue with a synthetic green generated from a Ha/OIII mix. After a few hue adjustments, I ended up with a colour image which mainly gave blue/reddish stars and nebula. I found that detail could be boosted
  14. NGC 896 is an emission nebula located in Cassiopeia about 7500 light years away. It is also the brightest part of the Heart Nebula (IC 1805) but has a separate classification, since it was the first part of the nebula to be discovered. The dominant red colour arises from hydrogen line photon emissions created by intense ultraviolet emissions from nearby stars. It is a star forming region and also home to many dark lanes created by interstellar gas. Some very bright blue stars compete in the nebula illumination, resulting in a blue/red cast in certain parts of the image. The LRGB image ha
  • Create New...

Important Information

We have placed cookies on your device to help make this website better. You can adjust your cookie settings, otherwise we'll assume you're okay to continue. By using this site, you agree to our Terms of Use.