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February 22nd, 2013
ESO's VLT reveals the Carina Nebula's hidden secrets.
This broad panorama of the Carina Nebula, a region of massive star formation in the southern skies, was taken in infrared light using the HAWK-I camera on ESO's Very Large Telescope. Many previously hidden features, scattered across a spectacular celestial landscape of gas, dust and young stars, have emerged.
Credit: ESO/T. Preibisch
August 14th, 2013
October 23rd, 2013
Although it was back in 2008 when I visited the Rockefeller Center the last time, it felt like yesterday. I noticed though that the skyline had changed quite a bit. The building in the front center (between 46th & 47th streets) must have popped up out of the ground, as it's not even in Google Maps. Nevertheless, it was a beautiful day and at last, I could experience how Rockefeller enjoyed a sunny day's ending.
Adobe Photoshop CS6, Camera RAW 8.
Photo Settings: 14mm, f/5, 1/125 second, ISO 100.
Map: 40.7587, -73.9791
February 17th, 2013
The second of three images of ESO's GigaGalaxy Zoom project is a new and wonderful 340 megapixel vista of the central parts of our galactic home, a 34 by 20-degree wide image that provides us with a view as experienced by amateur astronomers around the world. Taken by Stephane Guisard, an ESO engineer and world-renowned astrophotographer, from Cerro Paranal, home of ESO's Very Large Telescope, this image directly benefits from the quality of Paranal's sky, one of the best on the planet. The image shows the region spanning the sky from the constellation of Sagittarius (the Archer) to Scorpius (the Scorpion). The very colourful Rho Ophiuchi and Antares region features prominently to the right, as well as much darker areas, such as the Pipe and Snake Nebulae. The dusty lane of our Milky Way runs obliquely through the image, dotted with remarkable bright, reddish nebulae, such as the Lagoon and the Trifid Nebulae, as well as NGC 6357 and NGC 6334. This dark lane also hosts the very centre of our Galaxy, where a supermassive black hole is lurking.
The image was obtained by observing with a 10-cm Takahashi FSQ106Ed f/3.6 telescope and a SBIG STL CCD camera, using a NJP160 mount. Images were collected through three different filters (B, V and R) and then stitched together. This mosaic was assembled from 52 different sky fields made from about 1200 individual images totaling 200 hours exposure time, with the final image having a size of 24,403 x 13,973 pixels. Note that the final, full resolution image is only available through Stephane Guisard.
Credit: ESO/S. Guisard (www.eso.org/~sguisard)
By Robin Kamp
November 29th, 2013
By Nicolas Kamp
December 21st, 2013