NGC 5907 from my own „Sterntaucher“ observatory
My next project in 2020 was the galaxy NGC 5907 in the constellation Draco.
For this I was inspired by the current discussions about the existence of the second loop of the stellar tidal stream around NGC 5907 (van Dokkum, Müller, Martinez-Delgado). Also the images of my colleagues from the group „Tief belichtete Galaxien (Long exposed galaxies)“ (TBG), cannot confirm this second loop.
My own main concern was whether I could detect anything at all of the actual stellar tidal stream from my light-polluted location on the outskirts of a major city.
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Here is an overview of the used equipment and the exposure times:
Equipment | Telescope 1 | Telescope 2 |
Location and date | Krefeld, in April 2020 | Krefeld, in April 2020 |
Telescope/Lense | 10″ Newton ohne Namen | TSQ-65ED Apo |
Focal length [mm] | 1000 | 420 |
Focal ratio | 3.9 | 6.5 |
Mount | Skywatcher EQ8 | Skywatcher EQ8 |
Camera | Moravian G2 8300 FW | Moravian G3 16200 FW |
Autoguiding | DMK21 AU04 on TSQ-65ED | DMK21 AU04 on TSQ-65ED |
Filter | L | R:G:B |
Exposure time [min] | 910 | 235:240:425 |
Resolution | 1.11″/px | 2.95″/px |
Data calibration and registration and the final processing was done with PixInsight. The RGB Data was upscaled to the luminance data. The result was as follows:
The faintest star in my image has an apparent magnitude of 22.3 magG (SDSS DR5).
The two highest redshift quasars [Flesh 2015] in the image are:
SDSS J151410.66+560555.9 z=3.10 magG=20.5 (Gaia DR2)
SDSS J151707.18+562301.7 z=3.03 magG=20.3 (Gaia DR2)
In the coloured image is only a hint of the stellar tidal stream visible. Therefore I produced a second version, with additional 654 min luminance data from 2019. In this inverted and stretched image parts of the stellar tidal stream are detectable. Please see below.
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