Photon Receiver Astrophotography

Photon Receiver Astrophotography Hello and welcome to the Photon Receiver family. My goal is to share the beauty of the cosmos above us one photo at a time.

Equipment:
Quattro 200p
Poseidon C-Pro
Ceres 462M
EQ6R-PRO
Raspberry pi 5 8gb running Stellarmate

NGC 7380 (The Wizard Nebula)Located roughly 7,200 light-years away in the constellation Cepheus, the Wizard Nebula is a ...
09/09/2026

NGC 7380 (The Wizard Nebula)

Located roughly 7,200 light-years away in the constellation Cepheus, the Wizard Nebula is a massive star-forming region spanning around 100 light years. The glowing gas is part of the H II region Sh2-142, surrounding the young open cluster NGC 7380.

At the heart of the nebula are extremely young, massive stars, including the hot binary DH Cephei. Their intense ultraviolet radiation is ionizing the surrounding hydrogen and sculpting the enormous clouds of gas and dust. The dark structures throughout the nebula are dense clouds of material that resist the radiation and continue to provide the raw ingredients for new stars.

The cluster itself is only a few million years old, making this region incredibly young on astronomical timescales. What we're seeing is a snapshot of a stellar nursery still being shaped by the first generation of massive stars born within it.

1h 55m integration (23×300s)

New SHO false color edit
09/07/2026

New SHO false color edit

NGC 281(The Pacman Nebula)NGC 281 is a massive cloud of glowing gas and dust located roughly 9,000 - 9,500 light years a...
09/07/2026

NGC 281(The Pacman Nebula)

NGC 281 is a massive cloud of glowing gas and dust located roughly 9,000 - 9,500 light years away in the constellation Cassiopeia. Stretching across dozens of light years, it is an active emission nebula and stellar nursery, where enormous clouds of hydrogen are being illuminated by radiation from young, hot stars. The distinctive red glow captured in photographs comes primarily from hydrogen gas that has been energized by ultraviolet radiation from the stars forming within the region.

At the heart of NGC 281 sits the young open cluster IC 1590, containing numerous hot, massive stars that are responsible for much of the nebula's illumination. Their intense radiation is slowly carving away at the surrounding cloud, creating enormous cavities and intricate structures throughout the gas. Mixed into the glowing hydrogen are dense lanes of cold dust, which appear as dark silhouettes against the brighter nebula and give NGC 281 its unmistakable "Pacman" appearance.

One of the most fascinating features of the nebula is the collection of dark pillars and Bok globules scattered throughout it. These are incredibly dense concentrations of gas and dust that can shield their interiors from the destructive radiation of nearby stars. Some contain collapsing material that may eventually form new stars. The pillars are therefore not simply empty patches of darkness, they are some of the places where the next generation of stars is being assembled.

NGC 281 is a perfect example of the complicated relationship between massive stars and the clouds that give birth to them. The young stars inside IC 1590 illuminate and sculpt the nebula, compressing some regions of gas while simultaneously eroding others. Eventually, much of the surrounding material will be dispersed into space, leaving behind the stars that formed within it.

The Iris Nebula (NGC 7023) is a beautiful reflection nebula surrounded by the faint, dusty molecular clouds of LDN 1174–...
07/19/2026

The Iris Nebula (NGC 7023) is a beautiful reflection nebula surrounded by the faint, dusty molecular clouds of LDN 1174–1178. Unlike emission nebulae, its blue glow comes from starlight reflecting off interstellar dust, while the surrounding dark nebulae reveal intricate structures sculpted over millions of years.

This isn't my best work, as I'm still tracking down a light leak in my focuser that's affecting the data. Even so, I wanted to share this image and the incredible contrast between the bright Iris and the delicate dark dust surrounding it. Every target is another step toward improving both my equipment and my processing.

Rho Ophiuchi Processing PracticeI've been working on improving my astrophotography processing skills, so I decided to pr...
07/08/2026

Rho Ophiuchi Processing Practice

I've been working on improving my astrophotography processing skills, so I decided to practice using professional quality public data from Telescope Live. (https://app.telescope.live/en/datasets/5d0bcab7-5aad-4914-bc74-6be534de8866/ic-4605)

This is not my captured data. The source images were acquired by the CHI-5-CCD remote telescope in the Rio Hurtado Valley, Chile, using a Nikon 200mm f/2 lens and Astrodon filters.

All calibration, color work, noise reduction, sharpening, and final processing shown here were completed by me.

I'd love to hear your thoughts on the edit!

For a while now I've been wanting to upgrade the software I use to edit my images. Then I saw the awesome news that RC A...
07/05/2026

For a while now I've been wanting to upgrade the software I use to edit my images. Then I saw the awesome news that RC Astro Tools had broken away from PixInsight (a $300 piece of software) and can now be used directly with Siril, which is what I've been using all along.

Let's just say... the photo speaks for itself.

IC 1396 is a massive glowing cloud of gas and dust located about 2,400 light years away in the constellation Cepheus. St...
06/16/2026

IC 1396 is a massive glowing cloud of gas and dust located about 2,400 light years away in the constellation Cepheus. Stretching nearly 100 light years across, it is one of the largest emission nebula complexes visible from Earth. At its heart sits a young star cluster known as Trumpler 37, a collection of hot, massive stars whose intense ultraviolet radiation is carving and illuminating the surrounding hydrogen gas. What we see in photographs is not just a nebula, but an active stellar nursery where new stars are being born.

The most famous feature inside IC 1396 is the Elephant's Trunk Nebula, a dense pillar of gas and dust extending several light years into space. First cataloged by astronomers in the early twentieth century, this dark structure survives because it is dense enough to resist being completely eroded by the powerful radiation from nearby stars. Hidden within the trunk are pockets of collapsing gas where future stars are quietly taking shape. The glowing red hydrogen surrounding it tells the story of energetic young stars exciting the nebula from within.

What makes IC 1396 so fascinating is that it captures multiple stages of stellar evolution all at once. The massive stars of Trumpler 37 are shaping their environment, compressing clouds of gas and triggering the next generation of star formation. At the same time, their radiation is slowly destroying the very material that created them. The bright emission, dark dust lanes, and tiny newborn stars scattered throughout the region are all connected pieces of a cycle that has been repeating across the universe for billions of years.

Looking at IC 1396 is like witnessing creation and destruction happening side by side. Ancient clouds collapse into newborn stars while powerful radiation tears away the remnants of the nebula. Every photon captured from this region began its journey 2,400 years ago, crossing the vast darkness of space before finally reaching your camera sensor. It is a reminder that the universe is never standing still, and few places showcase that better than the Elephant's Trunk Nebula.

M106 sits about 23 million light years away in Canes Venatici, stretching roughly 135,000 light years across, and at fir...
04/25/2026

M106 sits about 23 million light years away in Canes Venatici, stretching roughly 135,000 light years across, and at first glance it looks like your standard spiral. Bright core, sweeping arms, everything where it should be. But then you look closer and realize this thing is not behaving normally.

Those faint extra arms are not just stars. They are gas being energized by activity from the supermassive black hole at the center. M106 is actively feeding, and it is pushing energy back into the galaxy, lighting up hydrogen in places that should not be glowing. So the subtle reddish and dusty structure you pulled out is not just star formation, it is the galaxy getting stirred from the inside out.

Then you start noticing everything else in the frame, and that is where it gets really cool.

NGC 4217 up top is a clean edge on spiral, around 60 million light years away. It looks like a thin blade of light cutting through space, with that bright central bulge and a perfectly flattened disk. Totally different orientation, totally different vibe, same basic physics.

NGC 4220 off to the left is another edge on system, but farther out, sitting way deeper in the background. It looks small and quiet, but that is an entire galaxy just casually sitting there minding its own business tens of millions of light years beyond M106.

NGC 4248 near M106 is part of the same general group, smaller and more subdued, almost like a satellite hanging around the bigger players. It does not scream for attention, but it helps tell the story that M106 is not alone out there.

NGC 4226 and those tiny background fuzzies scattered across the frame are even farther out. Some of those are hundreds of millions of light years away, meaning the light you captured started its journey before complex life even showed up on Earth.

What I love about this field is the color balance. You have that warm core in M106, subtle hints of hydrogen alpha regions, cooler tones in the outer arms, and then those neutral, slightly bluish edge on galaxies that are dominated more by starlight than active emission. It is not screaming neon like a nebula, it is quieter, more subtle, but it is just as real.

So this is not just a picture of one galaxy. This is depth. M106 in the foreground, its neighbors hanging nearby, and a whole background layer of galaxies stacked behind it at completely different distances.

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