Explain a technique, that can be used by non-professional astronomers, and whose results could go in line with the characterization of planetary atmospheres.

Slide 1

IC 1848 – Soul Nebula

The numerous columns of gas and dust in this nebula are known areas of star formation. Taking images with different filters allows us to very well separate the elements that form it, the blue color being characteristic of Oxygen.

An amateur observatory for professional studies

Studies of Exoplanets, photometry of asteroids, supernovae, occultation of stellar objects,

astrophotography, the Anunaki Observatory at the service of professional astronomers.

Photometry

Exoplanets

Observation of Exoplanets by differential photometry. We share all the data obtained, from the .fit to the analysis of them.

Asteroids

Photometry of asteroids for morphological studies, in collaboration with the Gaia-GOSA project.

Supernovae

The most violent events in the universe within the reach of any amateur astronomer. Get to know the research group and collaborate with us.

Astrophotography

Image of galaxies, nebulae and globular clusters, from the far reaches of the universe.

The way of the photons to our detector.

Gallery

If you can do it

Why not carry it out?

Do you have an astronomical team and want to dedicate it to research?

Find the available ProAm collaboration projects.

Today more than ever you have the opportunity; observation of exoplanets, asteroids, NEO’s, light pollution studies and much more.

Projects

Latest publications

ProAm collaboration projects have their results, know the latest publications for which we have worked.

Publications

Astronomical Resources

Manuals and tutorials on observation techniques, photometry, exoplanets, astronomical software and much more.

Resources

Sh2 101 – Tulip Nebula

Sharpless 101, also called Sh2-101 is a Region HII nebula and also an emission nebula in the constellation Cygnus. It is also called the Tulip Nebula because it is shaped like a tulip in the images, cataloged by astronomer Steward Continue Reading
NGC 5907 – Splinter Galaxy

NGC 5907 is a spiral galaxy in the constellation Draco located 40 million light-years away. Of apparent magnitude 10.38, its surface brightness is 13.4 mag/arcsec. It was discovered by William Herschel in 1788. NGC 5907 appears edge-on from our perspective, Continue Reading
M94 – NGC 4736

Messier 94, also known as NGC 4736 is a spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781, and catalogued by Charles Messier 2 days later. The structure of M94 is characterized by three Continue Reading