The image on the right is a star field showing a quasar (the nucleus of a very remote galaxy). The bottom-left inset shows my camera and telephoto lens on a star tracker (the white box). The top-left inset shows where I pointed the camera in the constellation of Draco. The top-right inset shows a blow-up of the centre region of the image. The quasar is the tiny grey dot identified by the two tick marks. |
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The light from the quasar travelled for over 12 billion years on its way to the camera. During that time the Universe has expanded and so the quasar is now about 25 billion light-years away. The image was taken with a Nikon D7500 DSLR and a 300mm f/4 lens mounted on an iOptron SkyTracker. |
The montage on the right comprises three images taken during the BASoc Star Party of 2019. All the images were taken with a Nikon D7500 DSLR and a 300mm f/4 lens mounted on an iOptron SkyTracker. |
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M45 Pleiades Cluster 14 x 60s C33 + C34 Veil Nebula 33 x 60s M31 Andromeda Galaxy 32 x 60s |
The image on the right is the centre of the Milky Way from Aquila (top left) to Scorpius (right). Jupiter is the bright 'star' above right of centre. Saturn is near the left edge. It was taken with a Nikon D7500 DSLR and a 35mm lens set at f/4 and mounted on an iOptron SkyTracker. |
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The image is a mosaic of 6 images, where each image was created by stacking (adding together) 10 individual exposures, each of which was 120s long. |
The image on the right is the centre of the Milky Way from Sagittarius (left) to Scorpius (right). Jupiter is the bright 'star' above right of centre. Saturn is near the left edge. It was taken with a Nikon D7500 DSLR and a 35mm lens set at f/4 and mounted on an iOptron SkyTracker. |
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The image is a mosaic of 4 images, where each image was created by stacking (adding together) 10 individual exposures, each of which was 120s long. |
The image on the right shows Antares (the brightest star in the constellation of Scorpius) and the Rho Ophiuchi molecular cloud complex. This star-forming region is one of the closest to us at a distance of about 400 light-years. It was taken with a Nikon D7500 DSLR and a 135mm f/2 lens mounted on an iOptron SkyTracker. |
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The image is the result of stacking (adding together) 60 individual exposures each of which was 120s long. Click here for a labelled image. |
The image on the right is the centre of the Milky Way from Scutum (top) to Sagittarius (bottom). It was taken with a Nikon D7100 DSLR and a 85mm lens set at f/2 and mounted on an iOptron SkyTracker. |
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The image is a mosaic of 4 images, where each image was created by stacking (adding together) 10 individual exposures, each of which was 120s long. Click here for a labelled image. |
The image on the right is the Milky Way from Cygnus (top left) to Scorpius (bottom right). It was taken with a Nikon D7100 DSLR and a 10-20mm lens set at 10mm and f/5.6 and mounted on an iOptron SkyTracker. |
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The image was created by stacking (adding together) 6 individual exposures, each of which was 240s long. Click here for a labelled image. |
The image on the right was taken with the K2 star tracker that I designed and built to allow long exposure images to be taken without the stars trailing due to the rotation of the Earth. |
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The image was created by stacking (adding together) 20 individual exposures, each of which was 60s long. Stacking reduces the noise levels in the images and so allows fainter detail to be captured. |
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Image processing The images were processed using the freeware Macintosh image analysis software Image SXM, a program that I wrote for use with scanning microscopy images (but which can also be used with astrophotography images). If a caption indicates '6 x 120s' this means that 6 images (each of 120 seconds exposure) were added together in software. The object(s) of interest will add up but random noise that is inherent in all images will tend to cancel out, giving a 'cleaner' resultant image compared to the original images. Mosaic images were created using Image SXM which automatically overlaps images and then removes any visible artefacts at the joins. |
Steve Barrett
October 2022 S.D.Barrett@liv.ac.uk |
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