CTA 1 - Echoes of a Hidden Remnant | 400 Hours

 Posted: Sep 20th, 2026
Technical Info
Exposure:
2760 x 300" ISO/Gain: 0 - Ha
1320 x 300" ISO/Gain: 0 - Oiii
612 x 300" ISO/Gain: 0 - rgb
108 x 300" ISO/Gain: 0 - L
Yellow, Bortle 5 zone:
 Mos Obl, Россия
400 h 0 m
94
Resolution: 6248x3923 px
Scale: 54043 KB

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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Comments

My congratulations) The project is complete. Deep respect to everyone who took part!
Today, at 16:23 Reply
It will do for beginners.
Today, at 17:01 Reply

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