M 37 (Aur)

M 37 (Aur)

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Date/Site: 21. and 23. December 2024, e-EyE
Exposure/
Filter:
R: 15 x 60 seconds,
G: 16 x 60 seconds,
B: 15 x 60 seconds,
Hα: 81 x 300 seconds (-5°C)
Camera/
Optics/
Instrument:
ASI 2600MM Pro with Astronomik Type 2c-filter on 400mm f/5 Newton with 2" TS Comacorrector on AP1200 GTO
Data acquired remotely using N.I.N.A.,
Off-Axis-Guiding with ASI120,
Focusing with Microtouch,
Calibration with MaximDL 6, processing in PixInsight 1.8 using BXT and GraXpert

This winter I saw for the first time images of this well known open cluster together with a cloud of glowing Hα-gas.It is supposedly a planetary nebula apparently including much of the cluster.
This image turned out not very good. I started with a bunch of 10-second-frames for the stars, but without dark-frames. As a replacement I imaged the stars with 60-second-frames and a lot of longer Hα-frames.
Because of the extremely high humidity in this spanish winter the mirrors of the Elephant dewed over quickly. During installation of the telescope at the end of August at 40°C I dialed the heating strips in at the lowest level. This apparently was not enough now.
I had to throw away many hours of Hα-frames with a too low signal to noise ratio.
So it became clear that ventilation and heating of the mirrors had to become adjustable remotely.
So in the middle of March I sent a Pegasus Power Box to e-EyE and José Fernando installed it in place of the old manually adjustable controller.
 

© Friedhelm Hübner, last revision:  02.04.2025