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@tinoeberl@mastodon.online
2026-07-21 15:17:03

#Steady #Klimacrew
#BahnMonitor-Projekt: 7. Zufall ist nicht gleich Zufall. 🤭
Nach der Verspätungsmeldung kommt ein Wissenshäppchen. Der

@kexpmusicbot@mastodonapp.uk
2026-06-22 04:42:23

🇺🇦 #NowPlaying on KEXP's #Expansions
missing project:
🎵 Poisson D’Avril (Da’ Future Given a Deep Soul mix)
#missingproject
music-from-memory.bandcamp.com
open.spotify.com/track/0GCzWPp

@doktrock@toad.social
2026-06-22 15:14:04

🚨Job Alert ! 🚨
2 year Postdoctoral Research Associate in #Biogeochemistry in Oxford using novel methods to explore organic matter stability and new proxies of rock weathering
wider team in Southampton.
#geology (h/t profbobhilton on bsky)

@mnalis@mastodon.online
2026-07-22 01:07:37

CoMaps is open-source community-oriented privacy-first navigation app for mobile devices. It is currently choosing its fiscal / umbrella host which would be most aligned with those goals, so if you have opinions, come vote at codeberg.org/comaps/Governance

@doktrock@toad.social
2026-05-22 11:57:54

Current status - 72nd Institute on Lake Superior Geology conference.
This year, in Thunder Bay, Ontario

Conference room, with a screen showing Precambrian assembling of North American continental fragments
Booklet cover:
72nd ANNUAL MEETING
Thunder Bay, Ontario - May 21-22, 2026
INSTITUTE ON LAKE SUPERIOR GEOLOGY
Part 1 - Program and Abstracts

w photos of outcrops
Drill core halves of a dark, coarse-grained rock laid out.
Rock samples laid out including ore samples of gold ore from Hemlo mining corporation, copper and PGE, bearing gabbro from the Marathon project, and veritextured leuconorite from Lac des Iles.
@BBC3MusicBot@mastodonapp.uk
2026-05-22 18:18:34

🇺🇦 #NowPlaying on BBCRadio3's #ClassicalMixtape
Philip Glass & Third Coast Percussion:
🎵 Paru River (Aguas da Amazonia)
#PhilipGlass #ThirdCoastPercussion
open.spotify.com/track/3f7nEi8

@cosmos4u@scicomm.xyz
2026-07-18 00:24:23

This month on All Space Considered, Griffith Observatory welcomed Dr. Joel Leja, Associate Professor of astronomy & astrophysics at The Pennsylvania State University, to discuss his research on the processes of galaxy formation derived from a combination of statistics, machine learning, and deep galaxy surveys with telescopes like the James Webb Space Telescope: #LittleRedDots

@raiders@darktundra.xyz
2026-05-18 02:17:16

Raiders Receive Compelling Take on Ex-Lions Taylor Decker heavy.com/sports/nfl/las-vegas

@arXiv_astrophGA_bot@mastoxiv.page
2026-07-22 07:55:10

Star formation powers optical line emission from the CGM
Huanian Zhang, Lizhi Xie, Zhijie Qu, Dennis Zaritsky, Luis C. Ho, Min Bao, Fabio Fontanot, Michaela Hirschmann, Chenxu Liu, Gabriella De Lucia, Enci Wang, Haoyan Zheng
arxiv.org/abs/2607.18385 arxiv.org/pdf/2607.18385 arxiv.org/html/2607.18385
arXiv:2607.18385v1 Announce Type: new
Abstract: Using integral field spectroscopy, we explore the disk-halo interface, or the inner circumgalactic medium (CGM), of individual galaxies by constructing and analyzing emission-line maps for a large sample (72) of normal, low-redshift galaxies spanning three orders of magnitude in stellar mass and four orders in star formation rate (SFR). We find a steep turnover occurring at $(1-2) R_e$ in the H$\alpha$, [O {\small II}], and [O {\small III}] line emission radial profiles. Beyond this radius, the slope of the line emission radial profiles becomes shallower as the SFR of the central galaxy decreases, which might reflect the strength of the feedback processes. The line emission fluxes at large radius ($(5-10) R_e$ or $\sim (0.1-0.25)r_{\rm vir}$) correlate with the galaxy's SFR, but not with its stellar mass. These findings suggest that ionizing photons escaping from star-forming regions in the central galaxy account for the observed emission line fluxes from the inner CGM, with escape fractions inferred from the [O {\small III}] and [O {\small II}] ratio. Different state-of-the-art theoretical models do not agree on the predicted dependence of cool gas on the SFR of the central galaxies, highlighting the importance of CGM emission line measurements to distinguish between different subgrid models for star formation and feedback processes.
toXiv_bot_toot

@cosmos4u@scicomm.xyz
2026-05-13 23:19:30

"We’re delighted to announce the first #GalaxyZoo workflow to include images from the NSF-DOE Vera C #Rubin Observatory, using #galaxies drawn from its first Data Preview": blog.galaxyzoo.org/2026/05/12/ - "[t]he new workflow went live on the site just now, but with only 10,359 subjects it won’t stick around for long, so do jump in and get classifying."