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HomePhotographyAmazing view of 230 glowing galaxies from 570 megapixel dark energy camera

Amazing view of 230 glowing galaxies from 570 megapixel dark energy camera


‘The Antalia Cluster (Abell S636) is a group of at least 230 galaxies located about 130 million light years away in the direction of the constellation Antalia (Air Pump).’ , Credit: Dark Energy Survey/DOE/FNAL/DCAM/CTIO/NoIRLab/NSF/Aura, Image Processing: R. Colombari and M. Zamani (NSF NoIRLab)

unprecedented dark energy camera (DECam) entered service in 2012 and serves as the primary camera used for the Dark Energy Survey. The 570-megapixel camera, which has a total of 74 CCD image sensors, recently captured a dazzling image of the Antalia Cluster (Abell S 636), a group of at least 230 galaxies located about 130 million light years from Earth.

Located inside the Victor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory in Chile, the Dark Energy Camera is a wide-field CCD imager with 62 science CCDs and a dozen CCDs that control guidance and focus. The 62 science CCDs provide a total of 520 megapixel resolution, while the additional sensors are 50 megapixels each. The entire DECam instrument, including sensors, lenses, and filter array, weighs approximately four tons, or, to borrow from Chris Nicholls, about 1,814 knots.

A large, circular scientific instrument features a central blue mosaic pattern. The outer ring has evenly spaced bolts and a metallic finish, indicating high-tech equipment, possibly used in physics or engineering experiments.
‘The DECam focal plane consists of a science array of 62 2,048 x 4,096 CCDs. Additionally there are four 2,048 x 2,048 guider CCDs and eight 2,048 x 2,048 focus and alignment CCDs. The quantum efficiency of these LBNL-designed CCDs with their anti-reflective coating is optimized to be over 90% at 900 nm in the red and over 60% over the range of 400–1000 nm. DES CCD was manufactured by DALSA and further processing was done by LBNL. They are then packaged and tested by Fermilab.’ , Credit: DOE/FNAL/DCAM/R. Hahn/CTIO/NOIRLab/NSF/AURA

After a long calibration period, the Dark Energy Survey’s observation period ran from August 2013 to January 9, 2019. Since then, scientists have continued to work on all the data captured by the Dark Energy Camera. DECam has also been used for other surveys, including the Dark Energy Camera Legacy Survey, the DESI Legacy Imaging Survey, and the Dark Energy Camera Plane Survey.

The new image of the Antalia Cluster shows a diverse group of galaxy types, including lenticular galaxies, irregular galaxies and even ultra-compact dwarf galaxies. Per NOIRLabThe full-resolution version is available to download From NOIRLab.

A vast, starry night sky dotted with countless bright stars. Among them, a distinctive spiral galaxy glows with blue, surrounded by small clusters of stars and faint galaxies, creating a mesmerizing cosmic tapestry.
This is the millionth exposure of the Dark Energy Camera which combines with 127 other earlier exposures to form a wide field frame. The largest galaxy visible here is the spiral galaxy ESO 440-11, which is surrounded by several large galaxy clusters and thousands of other galaxies. Some stars of the Milky Way are also shown in the photo. , Credit: Dark Energy Survey/DOE/FNAL/DCAM/CTIO/NoIRLab/NSF/AURA; Acknowledgments: TA Rector (University of Alaska Anchorage/NSF’s NoIRLab), M. Zamani (NSF’s NoIRLab), and D. D. Martin (NSF’s NoIRLab)

Given that the Dark Energy Survey observation period covered 5,000 square degrees of the southern night sky, it’s no surprise that scientists are still working through the data and learning new things about the universe. Are. The Dark Energy Camera captured more than one million exposures, and one image covers an area of ​​the sky that is about 20 times the average visible size of the Moon as seen from Earth. That’s a lot of data.


Image Credit: Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA



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