A tricky target to image. The super bright star Gamma Cassiopeia, surrounded by the hydrogen-rich but faint nebulae IC59 and IC63. A combination of broadband and narrowband images allowed capturing both aspects.

NGC1499 (California Nebula), an emission nebula located in the constellation Perseus is a very large and colourful target when photographed in narrow-band. Here an SHO image of long exposure to bring out some of the very faint blue OIII signal.

On 01 February the comet reached its closest proximity to Earth. A few hours of clear skies allowed to capture this moment as a second image

A wide-field image of NGC2264, or Cone Nebula, embedded in lots of hydrogen-alpha regions. Next to the actual cone is the Christmas Tree star cluster, illuminating the surrounding gasses to emit bright blue OIII signal.

Comet C/2022 E3 (ZTF) is one of the brighter comets this year. It is still increasing in brightness, and while not likely, it could still possibly become visible with the naked eye. This post describes the image itself and also contains an animation of the comet moving across the backdrop of the stars.

The beautiful Jellyfish nebula (IC443) in the constellation Gemini. Here in a wide-field shot together with reflection nebula IC444. The narrow-band images are processed in the SHO Hubble palette.

In the constellation Cepheus this large area of nebulosity can be found with a massive star, 100,000 times bigger than our Sun, in the center that lights up the whole cloud. The nebula is registered as NGC7822.

Sh2-240, also known as the Spaghetti Nebula is a very large and faint object that requires long exposures with a wide-field telescope. A reducer on the FSQ-106 in combination with full-frame camera and > 17h of exposure resulted in the following image.

Bright comets are seldom appearances in our solar system. Comet Leonard was one of the most striking examples this year. Just days before it would become at its brightest and before it would cross the ecliptic, this image was shot in the early morning hours.

First light for a new camera, the QHY268c. Subject is M34, a very beautiful and colourful open cluster in the constellation Perseus. The cluster is pretty close-by at 1500 lightyears and rather bright at magnitude 5.5, so an ideal object to get acquainted with a new camera.

After a night of testing out guiding with the RST-135E mount, there was some time left to image a new target. M15, a globular cluster best visible in September, was just the perfect fit. One of the most dense globular clusters in our galaxy, with probably a black hole in its core.

A new reducer for the FSQ-106 turned the scope into a 380mm at f/3,6 astrograph. Together with the ASI6200MM a perfect combination to photograph the beautiful Heart and Soul Nebulae in narrowband.

Recently (2011) the Flying Squid Nebula has been discovered right within the Flying Bat Nebula (Sh2-129). The very weak OIII object is hard to image and with almost 30h of total exposure this has been one of the most challenging objects so far.

IC405 is an interesting combination of both a reflection and emission nebula that emits strongly in H-alpha. The double-star AE Aurigae shines brightly in the middle and illuminates vast clouds of hydrogen gas.

The very large emission nebula NGC2237, also known as Rosette Nebula, is part of an even much larger area of nebulosity in the constellation Monoceros.