
CTA 1 — Echoes of a Hidden Remnant
Project organizer: Andrew Batov (KonFuz)
Assistant: Lex Kasatkin (Darth Maul)
Image processing: Maksim Zaharov (svarschik911) https://deepskyhosting.com/svarshchik911
Processing software: PixInsight, Adobe Photoshop
Capture period: late July — mid-September 2026
Total integration: 400 hours
This project shows CTA 1 in an unusually deep and wide field, combining the faint structures of the supernova remnant in Hα and OIII with extensive regions of galactic dust and IFN. Rather than filling the frame with CTA 1 itself, the composition was built to emphasize the contrast between the relatively compact supernova remnant and the vast dust structures surrounding it across the entire image field.
The deep broadband data revealed extremely faint dust on large angular scales, while the narrowband integration brought out the subtle emission structures of CTA 1. The result is a rather rare type of image in which both the supernova remnant itself and the surrounding faint dust play comparable visual roles.
CTA 1, also known as SNR G119.5+10.2, is an ancient supernova remnant in the constellation Cepheus, located approximately 4600 light-years from Earth. Its age is estimated at approximately 10,000–14,000 years.
Its expanding shell is particularly prominent in radio, while extremely faint optical shock fronts can be observed primarily in Hα and OIII lines.
At the center of CTA 1 is PSR J0007+7303 — a neutron star completing one rotation in approximately 316 milliseconds. This object is particularly notable for being the first pulsar discovered through its gamma-ray pulsations rather than through previously detected radio pulsations.
The extensive dust structures visible throughout the image lie along the same line of sight and are not necessarily physically associated with the supernova remnant itself.
Integration
Hα — 230 h
OIII — 110 h
RGB — 51 h
L — 9 h
Total integration — 400 hours
Participants
1. Dmitry — 65 h
35 h Hα + 30 h OIII
Takahashi FSQ-106 / QHY600
2. Evgeniy Morozov — 55 h
55 h Hα
William Optics RedCat 71/350 / ZWO ASI2600MM Air
3. Poppy8micro — 39 h https://deepskyhosting.com/id1803
26 h Hα + 13 h OIII
Askar 71F + 0.75× reducer / ZWO ASI2600MM Pro
4. Lex Kasatkin — 35 h
21 h Hα + 5 h OIII + 9 h L
Askar SQA60 / ZWO ASI294MM Pro
5. Andrew Batov (KonFuz) — 29 h
23 h Hα + 6 h OIII
Askar 106SQA / SkyEye62AM
6. Alexey (lxkor) — 26 h https://deepskyhosting.com/lxkor
13 h Hα + 13 h OIII
Askar SQA55 / ToupTek ATR2600M
7. Maria-Mria — 24 h https://deepskyhosting.com/id1528
21 h OIII + 3 h Hα
Askar SQA55 / ZWO ASI2600MM Pro
8. Dmitry — 24 h
15 h Hα + 9 h OIII
Askar SQA85 / ZWO ASI2600MM Pro
9. Cho YongJun — 23 h
13 h Hα + 10 h OIII
Askar FRA400 / ZWO ASI2600MM Pro
10. Alena Kiseleva (BeautyS89)— 23 h https://deepskyhosting.com/BeautyS89
23 h RGB
Askar SQA55 / ZWO ASI2600MC Pro
11. Sergay Nazarov — 19 h
16 h Hα + 3 h OIII
Celestron C11 + HyperStar, ~580 mm / camera on IMX6200
12. Pingulator — 13 h
13 h RGB
Askar SQA55 / ZWO ASI2600MC
13. Yu Mar — 10 h
10 h Hα
Askar SQA55 / ZWO ASI2600MM Pro
14. Timofey Prozorov — 9 h
9 h RGB
Askar SQA55 / Player One Poseidon-C Pro (IMX571)
15. Anastasii — 4 h https://deepskyhosting.com/Anastasii
4 h RGB
Askar SQA55 / ZWO ASI294MC Pro
16. Serge — 2 h https://deepskyhosting.com/id2287
2 h RGB
Askar SQA85 / ZWO ASI2600MC
This image is the result of a collaboration between astrophotographers shooting with different optical systems and collecting data over nearly two months. The total integration of 400 hours made it possible to simultaneously show the extremely faint emission structures of CTA 1 and the large-scale galactic dust surrounding the object in the image field.
Many thanks to everyone who took part in this collaborative project and contributed their time and data. Each participant's contribution became an important part of the final image, and without the joint work of all participants this project would have been impossible.
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