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Integration: Baader UvIrCut 100x180s, Total Integration: 5h 0m |
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Canon EF 200 f/2.0, Asi 2600mc, Avalon Linear, Voyager, Pixinsight Integration: Optolong L-eNhance 57x360s, Total Integration: 5h 42m |
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Canon EF 200 f/2.0, Asi 2600mm, Avalon Linear, Pixinsight Integration: Ha 20x300s, Oiii 16x300s, RGB 3x20x30s, Total Integration: 3h 30m |
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Canon EF 200 f/2.0, Asi 2600mm, Avalon Linear, Pixinsight Integration: Ha 29x300s, Oiii 32x300s, RGB 3x20x30s, Total Integration: 5h 35m |
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Takahashi FSQ106 EDX IV @ f/3.6 Integration: Ha 25x600s, Oiii 18x600s, RGB 3x20x30s, Total Integration: 7h 40m |
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Takahashi FSQ106 EDX IV @ f/3.6 Integration: Sii 45x480s, Ha 39x480s, Oiii 35x480s, Total Integration: 15h 52m |
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27/10/2022 Novezzina, 1250 mt, sqm=20.85, RGB Takahashi FSQ106 EDX IV @ f/3.6 Integration: Ha 47x600s, RGB 107x240s, Total Integration: 14h 58m |
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Samyang 135 f/2.0 @ f/3.5, Asi2600mc, Avalon Linear, Pixinsight Integration: 67x360s, Total Integration: 6h 42m AstroBin Top Pick From Wiki... Sh2-126 is a visible emission nebula in the Lacerta constellation. It is identified in the southern part of the constellation, about 1 ° westward with respect to the star 10 Lacertae, a blue star of main sequence of spectral class O9V; invisible to simple observation with amateur instruments due to its weakness... |
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Takahashi FSQ106 EDX IV @ f/3.0 Integration: Ha 37x480s, OIII 48x480s, Total Integration: 11h 20m From Wiki... NGC 7380 is a young open cluster of stars in the northern circumpolar constellation of Cepheus. The surrounding emission nebulosity is known colloquially as the Wizard Nebula, which spans an angle of 25′. It is extremely difficult to observe visually, usually requiring very dark skies and an O-III filter. The NGC 7380 complex is located at a distance of approximately 8.5 kilolight-years from the Sun, in the Perseus Arm of the Milky Way... |
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Takahashi FSQ106 EDX IV @ f/5.0 Integration: Ha 75x480s, OIII 83x480s, Total Integration: 21h 4m Juza Editor's Pick AstroBin Top Pick From Wiki... The Crescent Nebula is an emission nebula in the constellation Cygnus... From Wiki... The Soap Bubble Nebula is a planetary nebula in the constellation Cygnus... |
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Integration: 40x180s, Total Integration: 2h 0m From Wiki... Sharpless 101 (Sh2-101) is a H II region emission nebula located in the constellation Cygnus. It is sometimes also called the Tulip Nebula because it appears to resemble the outline of a tulip when imaged photographically. It was catalogued by astronomer Stewart Sharpless in his 1959 catalog of nebulae. It lies at a distance of about 6,000 light-years from Earth... |
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Integration: 24x300s, Total Integration: 2h 0m From Wiki... Gamma Cygni (γ Cygni, abbreviated Gamma Cyg, γ Cyg), officially named Sadr, is a star in the northern constellation of Cygnus, forming the intersection of an asterism of five stars called the Northern Cross. Based upon parallax measurements obtained during the Hipparcos mission, it is approximately 1,800 light-years from the Sun... |
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Integration: 219x60s, Total Integration: 3h 39m From Wiki... The North America Nebula (NGC 7000 or Caldwell 20) is an emission nebula in the constellation Cygnus, close to Deneb (the tail of the swan and its brightest star)... |
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Integration: 250x0.400ms From Wiki... The Moon is an astronomical body orbiting Earth and is the planet's only natural satellite. It is the fifth-largest satellite in the Solar System, and by far the largest among planetary satellites relative to the size of the planet that it orbits. The Moon is, after Jupiter's satellite Io, the second-densest satellite in the Solar System among those whose densities are known... |
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Integration: 57x150s, Total Integration: 2h 22m From Wiki... Brocchi's Cluster (also known as Collinder 399, Cr 399 or Al Sufi's Cluster) is a random grouping of stars located in the constellation Vulpecula near the border with Sagitta. The members of the star cluster form an asterism which has given rise to its name as the Coathanger... |
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Integration: 92x180s, Total Integration: 4h 36m From Wiki... The Heart Nebula, IC 1805, Sharpless 2-190, lies some 7500 light years away from Earth and is located in the Perseus Arm of the Galaxy in the constellation Cassiopeia. It was discovered by William Herschel on 3 November 1787. It is an emission nebula showing glowing ionized hydrogen gas and darker dust lanes... |