Atacama Cosmology Telescope

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Atacama Cosmology Telescope

Atacama Cosmology Telescope

@ACT_Pol

...a six-meter telescope located at 5190 meters on Cerro Toco in northern Chile, dedicated to observing the structure and evolution of the universe...

Cerro Toco, Atacama Desert 가입일 Haziran 2012
72 팔로잉996 팔로워
Atacama Cosmology Telescope 리트윗함
Gerrit Farren
Gerrit Farren@farren_gerrit·
!!!New Paper out on arxiv today!!! We measure structure formation from the cross-correlation of CMB lensing and galaxy surveys, using the new @ACT_Pol DR6 lensing map and galaxies from unWISE. 1/6 arxiv.org/abs/2309.05659
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Erminia Calabrese
Erminia Calabrese@ermcalabrese·
We (@ACT_Pol) have a groundbreaking new image revealing the most detailed map of dark matter distributed across a quarter of the entire sky - drawn by CMB lensing and with implications for the growth of cosmic structures bbc.com/news/science-e…
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Atacama Cosmology Telescope
The Brick (insert brick emoji if there is one) is a massive, dense molecular cloud that has surprisingly little star formation. We find a well-ordered magnetic field in the Brick roughly aligned with its bean-like shape. (6/n) @ACT_Pol #molecularcloud
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So exciting to share our @ACT_Pol galactic science results with you! Make sure to check out the paper for more details (8/8)
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The Tornado is thought to be a supernova remnant, but the long tail is difficult to explain. We see the tail in total emission (left) but not polarized emission (right), and note that the magnetic field lines do change in the transition from head to tail. (7/n)
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We can zoom in on objects like Sgr A*, the black hole at the center of the Galaxy. The magnetic field lines in the ACT data trace even higher resolution observations from #MeerKAT at 1.28 GHz. (5/n)
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ACT also maps polarized radiation that allows us to infer the structure of magnetic fields. Most of the field lines run parallel to the Galactic plane, except in the very center where a strong vertical radio filament dominates the emission. (4/n)
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The three ACT frequencies are sensitive to different emission mechanisms at work in the Galactic center. Red highlights emission from relativistic electrons while emission from dust grains appears blue. Look at how many familiar objects we are able to see! (3/n)
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