Oooof almost 400 more in 3 months. Fuck.
3,633 Starlinks in orbit out of 3,930 launched (failure rate still ~10%, gross)
7,312 total sats in orbit. Well fuck, Starlink is finally about to pass the 50% OF ALL SATELLITES mark.
Think about that: 50% of all satellites are owned by the same ego-maniac billionaire who most of us here on Mastodon are now extremely familiar with. This is so bad.
Couldn't help it and did this last night. I'm still in awe at the level of detail in this image! Look at those spiral dust lanes.
For more details about this image and the new ERIS instrument at ESO's Very Large Telescope: https://www.eso.org/public/announcements/ann22015/
The Great Andromeda Galaxy
Nearly 2.4 million light-years away, this massive spiral galaxy is headed on an eventual collision course with the Milky Way.
The first image shows a comparison between my first attempt in 2021 and most recent study in 2022 photographing this target.
369 x150s @ ISO 800 through Redcat51 with Canon T7. Total integration time is 15 h 22 min 30 s.
See more details at https://www.astrobin.com/vrxzv7/0/
We present the second data release of the MUSE Hubble UDF surveys, which includes the deepest spectroscopic survey ever performed. The MUSE data, with their 3D content, amazing depth, wide spectral range, and excellent spatial and medium spectral resolution, are rich in information. This update of the first release incorporates a new 141-hour adaptive-optics-assisted MXDF field (1' diameter FoV) in addition to the reprocessed 10-hour mosaic (3'x3') and the single 31-hour deep field (1'x1'). We have securely identified and measured the redshift of 2221 sources, an increase of 41% compared to the first release. With the exception of 8 stars, the collected sample consists of 25 nearby galaxies (z < 0.25), 677 OII emitters (z=0.25-1.5), 201 galaxies in the MUSE redshift desert range (z=1.5-2.8), and 1308 LAEs (z=2.8-6.7). This represents an order of magnitude more redshifts than the collection of all spectroscopic redshifts obtained before MUSE in the Hubble UDF area (2221 vs 292). At z > 3, the difference is even more striking, with a factor of 65 increase (1308 vs 20). We compared the measured redshifts against three published photometric redshift catalogs and find the photo-z accuracy to be lower than the constraints provided by photo-z fitting codes. 80% of the galaxies have an HST counterpart. They are on average faint, with a median magnitude of 25.7 and 28.7 for the OII and Ly-alpha emitters, respectively. SED fits show that these galaxies tend to be low-mass star-forming galaxies, with a median stellar mass of 6.2 10**8 M and a median SFR of 0.4 M/yr. 20% of our catalog, or 424 galaxies, have no HST counterpart. The vast majority of these new sources are high EQW z>2.8 LAEs that are detected by MUSE thanks to their bright and asymmetric broad Ly-alpha line. We release advanced data products, specific software, and a web interface to select and download data sets.
So now that I have migrated to #astrodon maybe I should do a new #introduction. I'm a postdoc at Stockholm university working on #ExtraGalactic stuff and Lyman alpha in particular. My PhD focused on low redshift galaxies and with the help of #JWST I hope to extend this to higher redshifts in the future.
I am also one of the creators of the @lasd together with @antihayestamine and Max Gronke
Outside work from that I am a general nerd with special focus on outdoor life and TTRPGs :)