Instagram: https://www.instagram.com/cybertron.astrophoto/
Facebook: https://www.facebook.com/CybertronAstroPhoto/
All images posted are taken and processed by myself.
Account managed by @mdverde.com
⚙️: ZWO AM5
🎯: ZWO ASI220MM mini + SvBony 30mm guide scope
📷: ASI2600MC-Pro - @ Gain 101, -10°C
⚡️: RGB: 144x120s = 4h48m
📷: ASI2600MM-Pro - @ Gain 100, 0°C
⚡️: Ha: 58x300s = 4h50m
📆: 21-22-23-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir+, Pixinsight
⚙️: ZWO AM5
🎯: ZWO ASI220MM mini + SvBony 30mm guide scope
📷: ASI2600MC-Pro - @ Gain 101, -10°C
⚡️: RGB: 144x120s = 4h48m
📷: ASI2600MM-Pro - @ Gain 100, 0°C
⚡️: Ha: 58x300s = 4h50m
📆: 21-22-23-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir+, Pixinsight
⚙️: ZWO AM5
🎯: ZWO ASI220MM mini + SvBony 30mm guide scope
📷: ASI2600MC-Pro - @ Gain 101, -10°C
⚡️: 144x120s = 4h48m
📆: 23-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir+, Pixinsight
⚙️: ZWO AM5
🎯: ZWO ASI220MM mini + SvBony 30mm guide scope
📷: ASI2600MC-Pro - @ Gain 101, -10°C
⚡️: 144x120s = 4h48m
📆: 23-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir+, Pixinsight
Collaborative image with @jmoneste.bsky.social .
Collaborative image with @jmoneste.bsky.social .
⚙️: ZWO AM3
🎯: ZWO ASI120MM mini + ZWO 30mm guide scope
📷: ASI294MC-Pro @ Gain 120, 0°C
⚡️: Optolong IR/UV cut - 65x180s = 3h15m
⚡️: Antlia ALP-T - 55x180s = 2h45m
📆: 25-27-28-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir Pro, Pixinsight
⚙️: ZWO AM3
🎯: ZWO ASI120MM mini + ZWO 30mm guide scope
📷: ASI294MC-Pro @ Gain 120, 0°C
⚡️: Optolong IR/UV cut - 65x180s = 3h15m
⚡️: Antlia ALP-T - 55x180s = 2h45m
📆: 25-27-28-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir Pro, Pixinsight
The LMC’s asymmetry and tidal features are a result of gravitational interactions with both the Milky Way and the Small Magellanic Cloud.
The LMC’s asymmetry and tidal features are a result of gravitational interactions with both the Milky Way and the Small Magellanic Cloud.
This image highlights key regions including the Tarantula Nebula (30 Doradus), NGC 1850, and various star-forming complexes embedded in dense hydrogen clouds.
This image highlights key regions including the Tarantula Nebula (30 Doradus), NGC 1850, and various star-forming complexes embedded in dense hydrogen clouds.
⚙️: ZWO AM5
🎯: ZWO ASI220MM mini + SvBony 30mm guide scope
📷: ASI2600MC-Pro - @ Gain 101, -10°C
⚡️: 48x120s = 1h36m
📷: ASI2600MM-Pro - @ Gain 100, 0°C
⚡️: 39x45s = 29m15s
📆: 23-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir+, Pixinsight
⚙️: ZWO AM5
🎯: ZWO ASI220MM mini + SvBony 30mm guide scope
📷: ASI2600MC-Pro - @ Gain 101, -10°C
⚡️: 48x120s = 1h36m
📷: ASI2600MM-Pro - @ Gain 100, 0°C
⚡️: 39x45s = 29m15s
📆: 23-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir+, Pixinsight
This is a collaborative image with @dompe.space who capture the luminance data with a monochrome camera, while I captured the color data.
This is a collaborative image with @dompe.space who capture the luminance data with a monochrome camera, while I captured the color data.
Unlike emission nebulae, which glow due to ionized gas, reflection nebulae shine by scattering starlight.
Unlike emission nebulae, which glow due to ionized gas, reflection nebulae shine by scattering starlight.
⚙️: ZWO AM5
🎯: ZWO ASI220MM mini + SvBony 30mm guide scope
📷: ASI2600MC-Pro - @ Gain 101, -10°C
⚡️: 45x180s = 2h15m
📆: 25-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir+, Pixinsight
⚙️: ZWO AM5
🎯: ZWO ASI220MM mini + SvBony 30mm guide scope
📷: ASI2600MC-Pro - @ Gain 101, -10°C
⚡️: 45x180s = 2h15m
📆: 25-Jul-2025
📌: Atacama, Chile, Bortle class 2.
💻: ASIAir+, Pixinsight