Tootfinder

Finishing up Blood Glacier, as I thought I'd seen it and was making sure (I haven't, I've just seen something similar). This one's weird and maybe a little cheesy.. I only noticed partway through that unfortunately, it's badly dubbed in English- like, VERY badly. I hate dubbed stuff. Wish it was subbed, but there's no choice for that on Tubi. Just this weird dubbed version. But I'm just here for the gore anyway 😂 which this one's delivering, a little.

Blood Glacier (2013)
At a climate research station in the Alps, the scientists are stunned as the nearby melting glacier is leaking a red liquid. It quickly turns to be very special juice — with unexpected genetic effects on the local wildlife.

The heart of NGC 5253 as seen with MUSE-NFM: nitrogen enrichment through stellar chemical feedback at parsec scales
Brigitte G. A. Pruijt (Leiden Observatory, Leiden University), Ana Monreal-Ibero (Leiden Observatory, Leiden University), Peter M. Weilbacher (Leibniz-Institut fur Astrophysik Potsdam), Jeremy R. Walsh (European Southern Observatory), Sebastian Kamann (Astrophysics Research Institute, Liverpool John Moores University), Azlizan A. Soemitro (Leibniz-Institut fur Astrophysik…

The heart of NGC 5253 as seen with MUSE-NFM: nitrogen enrichment through stellar chemical feedback at parsec scales
NGC 5253 is a nearby (D=3.6 Mpc) Blue Compact Dwarf galaxy, notable for its three massive young super star clusters (SSCs) and nitrogen enrichment. Its similarity to extreme star-forming galaxies at high redshift makes it a good local analogue for studying chemical enrichment at high spatial resolution. We characterise the ionised gas and dust in the giant HII region in the proximity of the three SSCs in the centre of NGC 5253 using new Multi-Unit Spectroscopic Explorer Narrow Field Mode adapti…

Moody Urbanity - Relations 👥
情绪化城市 - 关系 👥
📷 Minolta Hi-Matic AF
🎞️ Shanghai GP3 400 Pan
#filmphotography #Photography #blackandwhite

Dark Energy Survey Year 6 Results: improved mitigation of spatially varying observational systematics with masking
M. Rodr\'iguez-Monroy, N. Weaverdyck, J. Elvin-Poole, I. Sevilla-Noarbe, A. Carnero Rosell, A. Drlica-Wagner, S. Avila, M. R. Becker, K. Bechtol, M. Crocce, M. Gatti, J. Mena-Fern\'andez, A. Porredon, D. Sanchez Cid, M. Yamamoto, M. Aguena, S. S. Allam, O. Alves, F. Andrade-Oliveira, D. Bacon, J. Blazek, S. Bocquet, D. Brooks, R. Camilleri, J. Carretero, R. Cawthon…

Dark Energy Survey Year 6 Results: improved mitigation of spatially varying observational systematics with masking
As photometric surveys reach unprecedented statistical precision, systematic uncertainties increasingly dominate large-scale structure probes relying on galaxy number density. Defining the final survey footprint is critical, as it excludes regions affected by artefacts or suboptimal observing conditions. For galaxy clustering, spatially varying observational systematics, such as seeing, are a leading source of bias. Template maps of contaminants are used to derive spatially dependent correction…

The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies
Mariana P. J\'ulio, Justin I. Read, Marcel S. Pawlowski, Pengfei Li, Daniel Vaz, Jarle Brinchmann, Martin P. Rey, Oscar Agertz, Tom Holmes
https://arxiv.org/abs/2510.06905

The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies
A tight correlation between the baryonic and observed acceleration of galaxies has been reported over a wide range of mass ($10^8 < M_{\rm bar}/{\rm M}_\odot < 10^{11}$) - the Radial Acceleration Relation (RAR). This has been interpreted as evidence that dark matter is actually a manifestation of some modified weak-field gravity theory. In this paper, we study the radially resolved RAR of 12 nearby dwarf galaxies, with baryonic masses in the range $10^4 < M_{\rm bar}/{\rm M}_\odot < 10^{7.5}$, …

Ionization Sources of the Local Interstellar Clouds: Two B-stars, Three White Dwarfs, and the Local Hot Bubble
J. Michael Shull (University of Colorado, University of North Carolina), Rachel M. Curran (University of North Carolina), Michael W. Topping (University of Arizona), Jonathan D. Slavin (Harvard/SAO)
https://arxiv.org/abs/2510.0526…

Ionization Sources of the Local Interstellar Clouds: Two B-stars, Three White Dwarfs, and the Local Hot Bubble
The dominant sources of photoionizing radiation in the extreme ultraviolet (EUV) incident on the exterior of the local interstellar clouds include two nearby early B-type stars, $ε$ CMa ($124\pm2$ pc) and $β$ CMa ($151\pm5$ pc), three hot dwarfs, and the local hot bubble (LHB). Line emission (170-912A) from highly ionized metals (Fe, Ne, Mg) in million-degree LHB plasma may be responsible for the elevated ionization fractions of helium ($n_{\rm HeII}/n_{\rm He} \approx 0.4$) compared to hydro…

Series D, Episode 10 - Gold
TARRANT: Have we got a choice? [A small explosion goes off nearby.]
DAYNA: Looks as though we have.
TARRANT: Let's get up there.
[At the top of the ladder.]
DAYNA: Avon! Soolin!
TARRANT: [*inaudible*]
https://blake.torpidity.net/m/410/127

THE LESSER-KNOWN PROGRAMMING LANGUAGES #8: LAIDBACK
This language was developed at the Marin County Center for T'ai Chi,
Mellowness and Computer Programming (now defunct), as an alternative to
the more intense atmosphere in nearby Silicon Valley.
The center was ideal for programmers who liked to soak in hot tubs while
they worked. Unfortunately few programmers could survive there because the
center outlawed Pizza and Coca-Cola in favor of Tofu and Perrier…

Unveiling Obscured Accretion in the Local Universe
Indrani Pal, Stefano Marchesi, Ross Silver, Marco Ajello, Vittoria Gianolli, N\'uria Torres-Alb\`a, Isaiah Cox, Xiurui Zhao, Dhrubojyoti Sengupta, Anuvab Banerjee, Kouser Imam, Andrealuna Pizzetti
https://arxiv.org/abs/2509.21532

Unveiling Obscured Accretion in the Local Universe
Heavily obscured Active Galactic Nuclei (AGN), especially Compton-thick sources with line-of-sight column density ($N_{\rm H,los}$) $>$ 10$^{24}$ cm$^{-2}$, are critical to understanding supermassive black hole (SMBH) growth and the origin of the Cosmic X-ray Background (CXB). However, their observed fraction remains significantly below model predictions, due to strong absorption bias, even in the hard X-ray (i.e., above 10 keV) band. We analyze a sample of 26 nearby ($z < 0.1$) AGN from the Sw…

The MIRI Excesses around Degenerates (MEAD) Survey I: A candidate cold brown dwarf in orbit around the nearby white dwarf 2MASS J09424023-4637176
Lo\"ic Albert (D\'epartement de Physique and Observatoire du Mont-M\'egantic, Universit\'e de Montr\'eal, Trottier Institute for Research on Exoplanets), Sabrina R. Poulsen (Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma), \'Erika Le Bourdais (D\'epartement de physique and Institut Trot…

The MIRI Excesses around Degenerates (MEAD) Survey I: A candidate cold brown dwarf in orbit around the nearby white dwarf 2MASS J09424023-4637176
The MIRI Excesses Around Degenerates Survey is a Cycle 2 James Webb Space Telescope (JWST) Survey program designed to image nearby white dwarfs in the mid-IR with the MIRI imaging mode. Only a handful of white dwarfs have previously been observed beyond 8~\micron. This survey gathered observations for 56 white dwarfs within 25~pc at 10 and 15~\micron, probing each white dwarf for unresolved IR excesses, IR flux deficits indicative of collision induced absorption, or resolved substellar companio…