Category Archives: mini-WASP Array

The creation and use of the New Forest Observatory mini-WASP array

Just a reminder

Here’s a reminder that I used to take deep-sky images at the New Forest Observatory. This is a single-framer of the Sadr region in Cygnus taken with the 2 x Canon 200mm prime lenses and the 2 x Trius M26C … Continue reading

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Coddington’s nebula

Last night I got 5 hours of data on Coddington’s nebula and Carbon star SAO 51274 (bottom left hand corner). I added this to around 12 hours of data taken over 2 nights some time ago.

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Greg’s “3” asterism in Leo

I recently took some data on Greg’s “3” asterism in Leo using the 200mm lenses on the MiniWASP array, around 4 hours of data in total. I have inserted some old Sky 90 data (again around 4 hours) so you … Continue reading

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M44 region with the Canon 200mm prime lenses from last night

Last night I got 18 x 15-minute subs on the M44 region with the 200mm lenses and I combined it with some earlier 200mm data.

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January 2019 – Image of the Month

I have been extremely lazy in trying to maintain an Image of the Month, so with a New Year just starting, let’s see if I can do better. Up there, right now, are the Pleaides (in Taurus) and this is … Continue reading

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Pleiades – superdeep

I took 6 hours of 40-minute subs with the Sky 90 array on 9th December 2018 and added this to 9 hours of 40-minute subs taken last year to get this result.

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Procyon and Gomeisa

Alpha and Beta Canis Minoris taken with the 200mm lenses and a 2-frame (horizontal) mosaic.

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Sky90 array image of M31 the Andromeda galaxy

9 hours of data using 20-minute subs (so 3 hours of actual imaging time) using the Sky90 array on 1st November 2018. 6:52 p.m. start and no Moonrise until midnight.

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Vega plus two Carbon stars

North is to the left in this image showing brilliant star Vega and two nearby Carbon stars.

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The Double Cluster and Stock 2 in wide-field

A wide-field image using the Canon 200mm lenses of the Double Cluster and Stock 2 open clusters. Stock 2 is the “stick man on his side” directly above the Double Cluster.

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