Tootfinder

I've benefited from a lot of these programs before getting into security. It turns out that trying to support a partner and a kid on $40k/yr, even in the early 2000's, is basically impossible. My parents were divorced, and my dad is a disabled vet.
Food security has always been important, long before organizing with comrades who also occasionally needed support. So if you have money, donate.
Eventually benefits will come back. Hopefully we can bridge the gap... But we won't be able to for everyone. When things come back, don't just feel relieved and move on. The system is collapsing. If it doesn't completely fall apart now, it will eventually. If you aren't affected now, you will be. Organize now around food security.
The disaster is now. The best time to prepare was years ago. The second best time is now.

"We now save over $1.2M / yr and we expect this to grow, as we grow as a business."
"AWS to Bare Metal Two Years Later: Answering Your Toughest Questions About Leaving AWS "
https://oneuptime.com/blog/post/2025-10-29-aws-to-bare-metal-tw…

Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates
D. Jadlovsk\'y, L. Moln\'ar, A. Ercolino, M. Bernini-Peron, A. M\'erand, J. Krti\v{c}ka, L. Wang, R. Z. \'Ad\'am, D. Baade, G. Gonz\'alez-Tor\`a, T. Granzer, J. Jan\'ik, J. Kol\'a\v{r}, K. Kravchenko, N. Langer, L. M. Oskinova, D. Pauli, V. Ramachandran, A. C. Rubio, A. A. C. Sander, K. G. Strassmeier, M. Weber, M. Wittkowski, R. Bra…

Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates
The majority of massive stars are part of binary systems that may interact during their evolution. This has important consequences for systems in which one star develops into a Red supergiant (RSG); however, not many RSGs are known binaries. We aim to better constrain the properties of some of the known RSGs in binaries. We first focus on the VV Cephei type RSG KQ Pup (RSG+B-type companion, orbital period of 26 yr), where we have enough data to constrain the system's properties. We use archiv…

🇺🇦 Auf radioeins läuft...
ERNIE:
🎵 Hold Yr Horses
#NowPlaying #ERNIE
https://erniethechef.bandcamp.com/track/hold-yr-horses
https://open.spotify.com/track/5gKekPljHBtFvuQcaMOnii

„Nicole“ by Prowler
Platform: Amiga
Released: 7 February 2010
Specification: 320x256px, 32 colors
Note: 1st in the Datastorm 2010 Amiga Graphics competition
#GFX_Prowler #YR_2010 #PF_Amiga

come happen with the heads at the next heads happening, 9/11 at mama tried in #brooklyn, feat. geologist from animal collective (solo hurdy gurdy!), rare NYCing by tom carter/pat murano, & yr very own sloppy heads, plus dj sets by james mcnew! amazing flyer by abraham. #nyc

High Proper Motion Discoveries from the UKIRT Hemisphere Survey
Wings Zhang, Adam C. Schneider, Thomas P. Bickle, Adam J. Burgasser, Emma Softich, Federico Marocco, Daniella Bardalez Gagliuffi, Jacqueline K. Faherty, Aaron M. Meisner, J. Davy Kirkpatrick, Marc J. Kuchner, Martin Kabatnik, Frank Kiwy, Arttu Sainio, J\"org Sch\"umann, Karl Selg-Mann, Nikolaj Stevnbak Andersen, Bruce Baller, Paul Beaulieu, John Bell, Dan Caselden, Guillaume Colin, Alexandru Dereveanco, Christoph…

High Proper Motion Discoveries from the UKIRT Hemisphere Survey
We used the third data release of the UKIRT Hemisphere Survey to locate previously unrecognized high proper motion objects. We identify a total of 127 new discoveries with total proper motions $\gtrsim$300 mas yr$^{-1}$. A significant fraction of these sources with counterparts in the Gaia DR3 catalog are found to be distant ($>$100 pc) low-mass stars, where their large tangential velocities and placement on color-magnitude diagrams suggest that they are likely low-metallicity M-type subdwarfs.…

@…
# pkg-static -o ABI=FreeBSD:15:(sysctl -n hw.machine_arch) upgrade -yr FreeBSD-base
The --yes might be very risky in some cases.
Prior use of bectl(8) was sane …
Removals of non-base packages for installations, or upgrades, that specify the FreeBSD-base repository alone · Issue #2414 · freebsd/pkg
― <

"Our intro and then a question from @plactagonic:
Q1 Where are you posting from today?
Q2 What makes bikes fun for you?
Hi! I'm posting from the north coast of Scotland, near John O'Groats (which you may have heard of). I'm a lifelong cyclist, I don't even have a driver's license 😄
I just gave away an old racer, so now I only have two bikes, a 20 yr old hybrid "city bike", and my first battery-assisted cycle, "Big Red". Here…

So apparently the lesson is that unless you are a charity that can raise a massive backlash on Hacker News then you should expect the $230bn company that is Salesforce to utterly fuck you over if you use Slack. But luckily these folks WERE one of those unicorns, so they are just going to go with it.
"Slack is extorting us with a $195k/yr bill increase "
h…

An ALMA Band 7 survey of SDSS/Herschel quasars in Stripe 82: I. The properties of the 870 micron counterparts
E. Hatziminaoglou, H. Messias, R. Souza, A. Borkar, D. Farrah, A. Feltre, G. Magdis, L. K. Pitchford, I. P\'erez-Fournon
https://arxiv.org/abs/2508.18823

An ALMA Band 7 survey of SDSS/Herschel quasars in Stripe 82: I. The properties of the 870 micron counterparts
(Abridged) Quasar studies with Herschel/SPIRE often report host luminosities ranging from 10^{12} to 10^{14} Lsun, suggestive of star formation rates (SFRs) of up to several thousand Msun/yr. Due to the limited spatial resolution of SPIRE, it is uncertain whether the far-infrared (FIR) emission originates from the quasar itself, nearby sources, or unrelated sources within the SPIRE beam. High-resolution observations at wavelengths close to the SPIRE coverage are needed to pinpoint the true sour…

„Polyman“ by Facet
Platform: Amiga
Released: 25 May 2024
Specification: 320x256px, 32 colors
Note: 3rd in the 68k Inside 2024 Graphics competition
#GFX_Facet #YR_2024 #PF_Amiga

New and updated long-periodic terms in harmonic development of the Earth tide-generating potential
Sergey M. Kudryavtsev, Rodolfo G. Cionco
https://arxiv.org/abs/2508.18111 http…

New and updated long-periodic terms in harmonic development of the Earth tide-generating potential
We present a new harmonic development of the long-periodic band of the Earth tide-generating potential (TGP). It updates the corresponding part of the previous TGP expansion, KSM03 (Kudryavtsev, J. Geodesy, 77:829, 2004), and includes 38 terms of period longer than $\simeq$18 years (yr) and amplitude not less than $10^{-8}~{\rm m}^2\,{\rm s}^{-2}$. The development is made through a modified spectral analysis of the TGP numerical values tabulated over more than 30,000 yr (13,200~BC--17,191~AD). …

#OrangeCounty prosecutors opposed judge's 5 yr plea deal for #ThirdStrike #Skinhead with #swastika & SS tattoos arrested for mur…

The NANOGrav 15 yr Data Set: Targeted Searches for Supermassive Black Hole Binaries
Nikita Agarwal, Gabriella Agazie, Akash Anumarlapudi, Anne M. Archibald, Zaven Arzoumanian, Jeremy G. Baier, Paul T. Baker, Bence Becsy, Laura Blecha, Adam Brazier, Paul R. Brook, Sarah Burke-Spolaor, Rand Burnette, Robin Case, J. Andrew Casey-Clyde, Yu-Ting Chang, Maria Charisi, Shami Chatterjee, Tyler Cohen, Paolo Coppi, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H. Thankful Cromartie, Kat…

The NANOGrav 15 yr Data Set: Targeted Searches for Supermassive Black Hole Binaries
We present the first catalog of targeted searches for continuous gravitational waves (CWs) from 114 active galactic nuclei (AGN) that may host supermassive black hole binaries (SMBHBs), using the NANOGrav 15 yr data set. By incorporating electromagnetic priors on sky location, distance, redshift, and CW frequency, our strain and chirp mass upper limits are on average 2.6$\times$ more constraining than sky-averaged limits. Bayesian model comparisons against a common uncorrelated red noise for th…

Slack is extorting us with a $195k/yr bill increase
An open letter, or something
#salesforce

John Oliver on The Ethics of Comedy, The Dalai Lama & Impacting Monica by Reclaiming with Monica Lewinsky
https://www.youtube.com/watch?v=yR-KTECQGxQ

Lensed stars in galaxy-galaxy strong lensing -- a JWST prediction for the Cosmic Horseshoe
Sung Kei Li, Luke Weisenbach, Thomas E. Collett, Jose M. Diego, Jeremy Lim, Thomas J. Broadhurst, Alex Chow, Wolfgang J. R. Enzi, Patrick L. Kelly, Carlos R. Melo-Carneiro, Jose M. Palencia, Liliya L. R. Williams, Jiashuo Zhang
https://arxiv.org/abs/…

Lensed stars in galaxy-galaxy strong lensing -- a JWST prediction for the Cosmic Horseshoe
We explore for the first time the possibility of detecting lensed star transients in galaxy-galaxy strong lensing systems upon repeated, deep imaging using the {\it James-Webb Space Telescope} ({\it JWST}). Our calculation predicts that the extremely high recent star formation rate of $\sim 100\,M_{\odot}\textrm{yr}^{-1}$ over the last 50 Myr (not accounting for image multiplicity) in the ``Cosmic Horseshoe'' lensed system ($z = 2.381$) generates many young, bright stars, of which their large a…

When I was a little kid, the only thing I ever wanted for my birthday was a tricycle. I never got one. This yr, on my 64th bday, my dream finally came true. Mr. Boots got me an electric trike.
I AM OVER THE FCKING MOON. 🥰
He’s making me get—and wear—a helmet, tho. 😒 #ZiggyTheTrike #TheCircleOfLife

12 yr Full Solar Cycle Maps from IBEX-Lo Interstellar Neutral Atom Observations (2009–2020): #IBEX

feed yr head: https://www.youtube.com/live/1Ox6gLz3qVY
https://heads.social/@bourgwick/115392604…

Lyle Menendez Also Denied #Parole This Week, Will Remain Incarcerated in #California #BOP Facility Similar To Brother Erik Who Was Also Denied Parole This Week
Last YR Ousted

pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
Sinan Deger, Hiranya V. Peiris, Stephen Thorp, Daniel J. Mortlock, Gurjeet Jagwani, Justin Alsing, Boris Leistedt, Joel Leja
https://arxiv.org/abs/2509.20430

pop-cosmos: Star formation over 12 Gyr from generative modelling of a deep infrared-selected galaxy catalogue
We study star formation over 12 Gyr using pop-cosmos, a generative model trained on 26-band photometry of 420,000 COSMOS2020 galaxies (IRAC Ch.1 $<26$). The model learns distributions over 16 SPS parameters via score-based diffusion, matching observed colours and magnitudes. We compute the star formation rate density (SFRD) to $z=3.5$ by directly integrating individual galaxy SFRs. The SFRD peaks at $z=1.3\pm0.1$, with peak value $0.08\pm0.01$ M$_{\odot}$ yr$^{-1}$ Mpc$^{-3}$. We classify star-…

Some results on the ideal-based cozero-divisor graph of a commutative ring
F. Farshadifar
https://arxiv.org/abs/2508.13222 https://arxiv.org/pdf/2508.13222…

Some results on the ideal-based cozero-divisor graph of a commutative ring
Let R be a commutative ring with identity and I be an ideal of R. The cozero-divisor graph with respect to I, denoted by $Γ''_I(R)$, is the graph of R with vertices {x \in R -I :xR +I \not=R} and two distinct vertices $x$ and $y$ are adjacent if and only if $x \not \in yR+I$ and $y \not \in xR+I$.In this paper, we obtained some results on $Γ''_I(R)$.

„Dissolving in Neon Light“ by Titus
Platform: Amiga
Released: 26 July 2025
Specification: 320x256px, 32 colors
Note: 1st in the Nordlicht 2025 Oldschool Graphics competition
#GFX_Titus #YR_2025

Driven by a boom in #ArtificialIntelligence startups #SanFrancisco’s rising rent rate now tops the nation ... again.
🟢 Apartment #Rents that now avg well over $3000 a month are up 6% this yr , more than double t…

Renting a San Francisco Apartment in the A.I. Boom? Good Luck.
The artificial intelligence gold rush has pushed San Francisco’s residential rents up by the most in the nation, as A.I. companies lease apartments and offer rent stipends to employees.

TrES-1 b: A Case Study in Detecting Secular Evolution of Exoplanet Orbits
Simone R. Hagey, Billy Edwards, Angelos Tsiaras, Aaron C. Boley, Anastasia Kokori, Norio Narita, Pedro V. Sada, Filip Walter, Robert T. Zellem, Napaporn A-thano, Kevin B. Alton, Miguel \'Angel \'Alava Amat, Paul Benni, Emmanuel Besson, Patrick Brandebourg, Marc Bretton, Mauro Cal\'o, Martin Valentine Crow, Jean-Christophe Dalouzy, Marc Deldem, T\~onis Eenm\"ae, Stephane Ferratfiat, Pere Guerra, G…

TrES-1 b: A Case Study in Detecting Secular Evolution of Exoplanet Orbits
We present a comprehensive analysis of transit, eclipse, and radial velocity data of the hot Jupiter TrES-1 b and confirm evidence of orbital variations on secular timescales. Apparent variations due to systemic motion and light travel time effects have been ruled out, indicating that the observed changes are dynamical in origin. Joint modeling of the TrES-1 b data favors an apsidal precession model, but the rapid precession rate of $4^\circ$ yr$^{-1}$ cannot be explained without invoking an un…

JADES: the chemical enrichment pattern of distant galaxies - silicon depletion and iron enhancement
Yuki Isobe, Roberto Maiolino, Xihan Ji, Francesco D'Eugenio, Charlotte Simmonds, Jan Scholtz, Ignas Juod\v{z}balis, Aayush Saxena, Joris Witstok, Chiaki Kobayashi, Irene Vanni, Stefania Salvadori, Kuria Watanabe, Stephanie Monty, Vasily Belokurov, Anna Feltre, William McClymont, Sandro Tacchella, Mirko Curti, Hannah \"Ubler, St\'ephane Charlot, Andrew J. Bunker, Jacopo Cheva…

JADES: the chemical enrichment pattern of distant galaxies - silicon depletion and iron enhancement
We present gas-phase abundances of carbon (C), $α$-elements (O, Ne, Si, and Ar) and iron (Fe) obtained from stacked spectra of high-$z$ star-forming galaxies with the deep Near Infrared Spectrograph medium-resolution data from the James Webb Space Telescope Advanced Deep Extragalactic Survey. Our 564 sources at $z=4$--7 have a median stellar mass of $\log(M_{*}/M_{\odot})=8.46$ and a median star-formation rate of $\log(\mathrm{SFR}/M_{\odot}\,\mathrm{yr^{-1}})=0.30$, placing them close to the …

„Touch The Sky“ by Luisa
Platform: 3D Render
Released: 16 August 2025
Note: 1st in the Evoke 2025 3D Scene competition
#GFX_Luisa #YR_2025 #PF_3DRender

Star-Black Hole Interactions in Young Star Clusters
Sara Rastello, Giuliano Iorio, Mark Gieles, Long Wang
https://arxiv.org/abs/2509.12318 https://arxiv.or…

Star-Black Hole Interactions in Young Star Clusters
Close encounters between stars and black holes can trigger micro-tidal disruption events (micro-TDEs) in dense young star clusters (YSCs). Using direct N-body simulations with PETAR, we found that most micro-TDEs arise from few-body multiple encounters. The inferred rate is approximately 350-450 Gpc$^{-3}$ yr$^{-1}$. Micro-TDEs could be detected both by upcoming surveys such as LSST, expected to observe roughly 10-100 events per year, and by their gravitational-wave (GW) signals peaking in the …

Constraints on WIMP-like dark matter scattering on electrons with COSINE-100
N. Carlin (COSINE-100 Collaboration), J. Y. Cho (COSINE-100 Collaboration), S. J. Cho (COSINE-100 Collaboration), S. Choi (COSINE-100 Collaboration), A. C. Ezeribe (COSINE-100 Collaboration), L. E. Franca (COSINE-100 Collaboration), O. Gileva (COSINE-100 Collaboration), C. Ha (COSINE-100 Collaboration), I. S. Hahn (COSINE-100 Collaboration), S. J. Hollick (COSINE-100 Collaboration), E. J. Jeon (COSINE-100 Coll…

Constraints on WIMP-like dark matter scattering on electrons with COSINE-100
We present results of the search for WIMP-like dark matter interaction with electrons in the NaI(Tl) crystals of the COSINE-100 experiment. The two benchmark scenarios of a heavy and a light vector boson as mediator of the interaction were studied. We found no excess events over the expected background in a data-set of 2.82 yr, with a total exposure of 172.9 kg.yr. The derived 90% confidence level upper limits exclude a WIMP-electron scattering cross section above 6.4 $\times$ 10$^{-33}$ cm$^2$…

Observation of \sigma-\pi coupling and mode selection in optically trapped artificial polariton molecules
Krzysztof Sawicki, Valt\'yr K\'ari Dan\'ielsson, Dmitriy Dovzhenko, Pavlos G. Lagoudakis, Simone De Liberato, Helgi Sigur{\dh}sson
https://arxiv.org/abs/2508.04909

Observation of σ-πcoupling and mode selection in optically trapped artificial polariton molecules
Microcavity exciton-polariton condensates under additional transverse confinement constitute a flexible optical platform to study the coupling mechanism between confined nonequilibrium and nonlinear states of matter. Driven far from equilibrium, polariton condensates can display spontaneous synchronization and instabilities depending on excitation and material parameters, showcasing emergent and intricate interference patterns based on mode competition over mutual gain landscapes. Here, we expl…

Prosecutor's release 42,000 word response to That 70's Show star #DannyMasterson's appeal to be released from 30 yr #California #prison term on forcible rape & drugging charges.
The details are not prett…

next thursday, 10/9, the sloppy heads wrap the 2025 heads happenings at mama tried in #brooklyn with a rare east coast drop-in by stephen hunking & dew claw, a solo set by greg cartwright (of reigning sound, the oblivians, etc.!), DJing by georgia the h & ira the k, plus yr sloppy heads. 7-10pm, free! #nyc

Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: I. Dependency on Mass Ratio and Orbital Period
Bhawna Mukhija, Amit Kashi
https://arxiv.org/abs/2509.12725 …

Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: I. Dependency on Mass Ratio and Orbital Period
We run numerical simulations to study high-power wind accretion in a massive binary system during a high mass loss event. The system consists of an evolved primary star with a zero age main sequence mass of $ M_{1} = \rm 100~M_{\odot}$ and a hot secondary star with a mass ranging from $ M_{2} = \rm 30-80~M_{\odot}$, orbiting in a circular orbits with periods between 455 and 1155 days. We initiate a weak eruption event with mass loss at a rate of $10^{-3}~\rm {M_{\odot}}\rm~yr^{-1}$ for 1.5 year…

35 yr old #SanFrancisco father stabbed to death in front of child while picking his son up at Commodore Sloat elementary school on Ocean Ave.
Suspect Daniel Patrick Rodriguez apparently committed violent act after a crosswalk altercation and was arrested after being located 170 miles out of town in #Tuolumne

Chandra Large Project Observations of the Supernova Remnant N132D: Measuring the Expansion of the Forward Shock
Xi Long, Paul P. Plucinsky, Terrance J. Gaetz, Vinay L. Kashyap, Aya Bamba, William P. Blair, Daniel Castro, Adam R. Foster, Charles J. Law, Dan Milisavljevic, Eric Miller, Daniel J. Patnaude, Manami Sasaki, Hidetoshi Sano, Piyush Sharda, Benjamin F. Williams, Brian J. Williams, Hiroya Yamaguchi

Chandra Large Project Observations of the Supernova Remnant N132D: Measuring the Expansion of the Forward Shock
We present results from the Chandra X-ray Observatory Large Project (878 ks in 28 observations) of the Large Magellanic Cloud supernova remnant N132D. We measure the expansion of the forward shock in the bright southern rim to be $0.\!^{\prime\prime}10 \pm 0.\!^{\prime\prime}02$ over the $\sim14.5$ yr baseline, which corresponds to a velocity of $1620\pm400~\mathrm{km\,s^{-1}}$ after accounting for several instrumental effects. We measure an expansion of $0.\!^{\prime\prime}23 \pm 0.\!^{\prime\…

Dynamical Mechanism of Episodic Gas Accretion to the Central Region of Spiral Galaxies
Naomichi Yutani, Nozomu Kawakatu, Takayuki Saitoh, Keiichi Wada
https://arxiv.org/abs/2509.14487

Dynamical Mechanism of Episodic Gas Accretion to the Central Region of Spiral Galaxies
We performed \textit{N}-body/SPH simulations of isolated spiral galaxies with various bulge-to-disk mass ratios ($M_{\rm bulge}/M_{\rm disk}$) from 0.02 to 0.2 to investigate mass transport from galactic scales (10 kpc) down to circumnuclear disk scales ($\lesssim$ 100 pc). Our analysis revealed these main findings, (1) Gravitational torque from stellar spiral arms causes gas accretion with $\sim1$ $M_\odot$ ${\rm yr}^{-1}$ along the gas spiral arms from a few kpc to a few 100 pc scale. The den…

„Fingerbanger“ by Optic
Platform: Amiga
Released: 21 January 2023
Specification: 320x256px, 32 colors
Note: 2nd in the Gerp 2023 Amiga Graphics competition
#GFX_Optic #YR_2023 #PF_Amiga

The Type II SN 2025pht in NGC 1637: A Red Supergiant with Carbon-rich Circumstellar Dust as the First JWST Detection of a Supernova Progenitor Star
Charles D. Kilpatrick, Aswin Suresh, Kyle W. Davis, Maria R. Drout, Ryan J. Foley, Alexander Gagliano, Wynn V. Jacobson-Galan, Ravjit Kaur, Kirsty Taggart, Jason Vazquez
https://arxiv.org/abs/2…

The Type II SN 2025pht in NGC 1637: A Red Supergiant with Carbon-rich Circumstellar Dust as the First JWST Detection of a Supernova Progenitor Star
We present follow-up imaging and spectroscopy and pre-explosion imaging of supernova (SN) 2025pht located in NGC 1637 at 12 Mpc. Our spectroscopy shows that SN 2025pht is a Type II SN with broad lines of hydrogen and with minimal line-of-sight extinction inferred from Na I D absorption. NGC 1637 was the target of several epochs of Hubble Space Telescope (HST) and James Webb Space Telescope (JWST) imaging covering the site of SN 2025pht from 31 to 0.7 yr prior to discovery. Using a follow-up HST…

🇺🇦 #NowPlaying on BBCRadio3's #InTune
Trad., VRï & VRï:
🎵 Yr Ehedydd
#Trad #VRï

Which Solar Latitude Follows the Sunspot Cycle Exactly?
K P Raju
https://arxiv.org/abs/2509.09974 https://arxiv.org/pdf/2509.09974

Which Solar Latitude Follows the Sunspot Cycle Exactly?
The large-scale convection in the Sun known as supergranulation is manifested as a network structure on the solar surface. The network cells have an average lifetime of 24 hr, a size of about 30 Mm, and a lane width of about 6 Mm. We have obtained the lane widths and intensities at different latitudes from the Ca {\sc ii} K spectroheliograms from the 100 yr Kodaikanal archival data. We have then calculated the cross correlation function of lane widths and intensities with sunspot number at ever…

Close Binary Open Cluster Systems: A Gaia DR3 Perspective on Alessi 36 and Collinder 135
H\"ulya Karag\"oz, Deniz Cennet \c{C}{\i}nar, Seval Ta\c{s}demir, Remziye Canbay
https://arxiv.org/abs/2509.14308

Close Binary Open Cluster Systems: A Gaia DR3 Perspective on Alessi 36 and Collinder 135
In this study, we examined the nearby open clusters (OCs) Alessi 36 and Collinder 135. Their spatial proximity was assessed using photometric and astrometric data from \textit{Gaia} DR3. Likely member stars were identified based on a membership probability threshold ($P \geq 0.5$), yielding 230 members for Alessi 36 and 342 members for Collinder 135. The mean proper-motion components ($μ_α\cosδ, μ_δ$) were determined as $(-9.681 \pm 0.072, 7.021 \pm 0.081)$ mas yr$^{-1}$ for Alessi 36 and …

Rotten decomposed body found in touring Texan's #TESLA trunk owned by 20 yr old singer of Spotify hit song #RomanticHomicide.
The fetid as yet unidentified #corpse wrapped in plastic was discovered in rising music sc…

A dead body was reportedly found in singer D4vd's impounded car: What we know
The Los Angeles Police Department has classified the case as a death investigation.

„The Lonely Remoter Watches the Stream“ by Steffest
Platform: Amiga
Released: 4 October 2025
Specification: 320x256px, 32 colors
Note: Released at Deadline 2025, Oldschool Graphics competition.
#GFX_Steffest #YR_2025

The Hot Inner AU of V883 Ori
Adolfo S. Carvalho, Lynne A. Hillenbrand, \'Agnes K\'osp\'al
https://arxiv.org/abs/2508.09939 https://arxiv.org/pd…

The Hot Inner AU of V883 Ori
The V883 Ori system is a rapidly accreting young stellar object that has been used as a laboratory for studying the molecular inventory of young circumstellar disks with high luminosity. We simultaneously fit high resolution spectroscopy and medium resolution spectrophotometry of the system to constrain the physical conditions in the inner au. Using our thin viscous accretion disk model, we find $\dot{M} = 10^{-3.9 \pm 0.2} \ M_\odot$ yr$^{-1}$, $R_\mathrm{inner} = 5.86 \pm 1 \ R_\odot$, $i = 3…

#Bandmates from defunct 80's super group still at loggerheads : Sting ( aka Gordon Sumner) sued by Andy Summers and #StewartCopeland for $2 million dollars in song arrangement royalties.
New details emerge as platinum plus Police bassist's attorneys claim the 73 yr old more likely overpaid ex ban…

Chandra/HETG and NuSTAR Observations of V750 Ara, a $\gamma\,$Cas-type Star
David P. Huenemoerder (MIT), Sean J. Gunderson (MIT), Richard Ignace (East Tennessee State University), Joy S. Nichols (Harvard,Smithsonian Center for Astrophysics), A. M. T. Pollock (University of Sheffield), Pragati Pradhan (Embry-Riddle Aeronutical University), Norbert S. Schulz (MIT), Dustin K. Swarm (University of Iowa), Jos\'e M. Torrej\'on (Universidad de Alicante)

Chandra/HETG and NuSTAR Observations of V750 Ara, a $γ\,$Cas-type Star
We present 197 ks HETG and 95 ks NuSTAR spectra of the $γ\,$Cas-type object V750 Ara. The high-resolution X-ray spectra show that the target is similar to other objects of this class. Data are interpreted under the assumption that the X-rays come from an accreting white dwarf, and our analysis implies an accretion rate of about $3\times10^{-11}M_\odot\mathrm{yr}^{-1}$. Emission lines are weak, and predominantly from hydrogen-like ions: Mg XII, Si XIV, and S XVI. H-like and He-like Fe are both …

„The Explorers“ by Critikill
Platform: Amiga
Released: 26 August 2023
Note: 2nd in the Xenium 2023 Oldschool GFX competition
#GFX_Critikill #YR_2023 #PF_Amiga

Polarization of reflected X-ray emission from Sgr A molecular complex: multiple flares, multiple sources?
Ildar Khabibullin, Eugene Churazov, Riccardo Ferrazzoli, Philip Kaaret, Jeffery J. Kolodziejczak, Fr\'ed\'eric Marin, Rashid Sunyaev, Jiri Svoboda, Alexey Vikhlinin, Thibault Barnouin, Chien-Ting Chen, Enrico Costa, Laura Di Gesu, Alessandro Di Marco, Steven R. Ehlert, William Forman, Dawoon E. Kim, Ralph Kraft, W. Peter Maksym, Giorgio Matt, Juri Poutanen, Paolo Soffitta, …

Polarization of reflected X-ray emission from Sgr A molecular complex: multiple flares, multiple sources?
Extended X-ray emission observed in the direction of several molecular clouds in the Central Molecular Zone (CMZ) of our Galaxy exhibits spectral and temporal properties consistent with the `X-ray echo' scenario. It postulates that the observed signal is a light-travel-time delayed reflection of a short ($δt<$1.5 yr) and bright ($L_{\rm X}>10^{39}~{\rm erg~s^{-1}}$) flare, most probably produced a few hundred years ago by Sgr A*. This scenario also predicts a distinct polarization signature fo…

Disclosing Submillimeter Galaxy Formation: Mergers or Secular Evolution?
Siu-Wang Chan, Yiping Ao, Qinghua Tan
https://arxiv.org/abs/2509.07913 https://arx…

Disclosing Submillimeter Galaxy Formation: Mergers or Secular Evolution?
We analyze the morphology of 125 submillimeter galaxies (SMGs) in the PRIMER-COSMOS field using double Sersic modeling on JWST NIRCam images across six bands (F150W, F200W, F277W, F356W, F410M and F444W), with SMGs being classified by bulge Sersic index (n_bulge) and bulge-to-total luminosity ratio (B/T). The Kolmogorov-Smirnov test between the bright (SFR > 175 M_sun yr^{-1}) and the faint group (SFR < 175 M_sun yr^{-1}) reveals no significant statistical differences in morphology across bands…

CHILES X: Molecular and atomic gas at intermediate redshift
Kelley M. Hess, John Hibbard, Jennifer Donovan Meyer, Hansung B. Gim, Nicholas M. Luber, Min S. Yun, Julia Blue Bird, Richard Dodson, Aeree Chung, Danielle Lucero, Emmanuel Momijian, D. J. Pisano, J. H. van Gorkom
https://arxiv.org/abs/2510.07966

CHILES X: Molecular and atomic gas at intermediate redshift
We present ALMA CO observations of 14 HI-detected galaxies from the CHILES survey found in a cosmic over-density at z~0.12. This is the largest collection of spatially resolved CO + HI observations beyond the local Universe (z>0.05) to date. While the HI-detected parent sample spans a range of stellar masses, star formation rates (SFR), and environments, we only directly detect CO in the highest stellar mass galaxies, log(M_*/M_Sun)>10.0, with SFRs greater than ~2 M_Sun/yr. The detected CO has …

New Arabic records from Cairo on supernovae 1181 and 1006
J. G. Fischer (U M\"unster, Germany), H. Halm (U T\"ubingen, Germany), R. Neuh\"auser (U Jena, Germany), D. L. Neuh\"auser (indep. scholar)
https://arxiv.org/abs/2509.04127

New Arabic records from Cairo on supernovae 1181 and 1006
The remnant of the historical supernova SN 1181 is under discussion: While the previously suggested G130.7+3.1 (3C58) appears too old (3000-5000 yr), the unusual star IRAS 00500+6713 with a surrounding nebula (Pa-30) has an expansion age not inconsistent with a SN Iax explosion in AD 1181 under the assumption that neither acceleration nor deceleration occurred. Previously, only reports from China and Japan were known, pointing to an event near the northern circumpolar region. Any further report…

Discovery of diffuse gamma-ray emission in the vicinity of G172.8 1.5: An old supernova remnant with different turbulence properties
Yuan Li, Gwenael Giacinti, Siming Liu
https://arxiv.org/abs/2510.01340

Discovery of diffuse gamma-ray emission in the vicinity of G172.8+1.5: An old supernova remnant with different turbulence properties
We report the detection of high-energy $γ$-ray emission in the vicinity of G172.8+1.5, which is debated as a Supernova remnant (SNR) or an ionized hydrogen (H$_{\rm{II}}$) region. Using 16-yr Pass 8 data from Fermi Large Area Telescope (Fermi-LAT), we found the GeV emission can be described by two extended sources with different photon spectra. Among them, the much more extended $γ$-ray source SrcA with a Power-law spectrum is spatially coincident with a giant neutral Hydrogen shell structure…

Excavating The Ruins: an Ancient $z=2.675$ Galaxy Which Formed in the First 500 Myr
Ian McConachie, Jacqueline Antwi-Danso, Wenjun Chang, M. C. Cooper, Adit Edward, Ben Forrest, Percy Gomez, Han Lei, Zach J. Lewis, Danilo Marchesini, Michael V. Maseda, Adam Muzzin, Allison Noble, Stephanie M. Urbano Stawinski, Tracy Webb, Gillian Wilson, M. E. Wisz
https://

Excavating The Ruins: an Ancient $z=2.675$ Galaxy Which Formed in the First 500 Myr
We present the analysis of an ancient galaxy at $z=2.675$ which we dub ``Eridu.'' Simultaneously modeling the JWST/NIRSpec G140M and G235M spectra from the SMILES program and $0.4-25\ μ\mathrm{m}$ HST, JWST/NIRCam, and JWST/MIRI photometry from the the JADES+SMILES photometric catalogs shows that Eridu is massive and quiescent with stellar mass $\log(M_*/\mathrm{M_\odot})=10.96^{+0.01}_{-0.01}$ and average star formation rate $<1\ \mathrm{M_\odot\ yr^{-1}}$ over the last 100 Myr. Star formatio…

MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
Sean D. Johnson, Nishant Mishra, Sowgat Muzahid, Gwen C. Rudie, Fakhri S. Zahedy, Zhijie Qu, Claude-Andr\'e Faucher-Gigu\`ere, Jonathan Stern, Jennifer I-Hsiu Li, Elise Fuller, Sebastiano Cantalupo, Hsiao-Wen Chen, Ahmad Kadri, Suyash Kumar, Zhuoqi Will Liu, Gregory Walth

MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
In dwarf galaxy models, outflows expel metal-enriched interstellar medium (ISM) into the circumgalactic medium (CGM) to reproduce their observed low metallicities, but measurements of dwarf CGM properties are scarce. We present a study of the CGM of an isolated dwarf at $z=0.5723$ with a stellar mass of $\approx5\times10^7\rm\,M_{\odot}$ and star-formation rate ($\approx0.05\,\rm M_\odot\,yr^{-1}$) and ISM metallicity ($\rm [O/H]\approx-0.9$) consistent with the star-forming main sequence and m…

51 yr old founding member of #Mastodon dead in #ATL #Motorcycle crash.
#BrentHinds, 51, who left reigning stoner metal band in a less than …

Long-period variable stars in NGC 147 and NGC 185-II. Their dust production
Hamidreza Mahani, Atefeh Javadi, Jacco van Loon, Francisca Kemper, Roya Hamedani Golshan, Iain McDonald, Habib Khosroshahi, Hedieh Abdollahi, Sajjad Mahdizadeh
https://arxiv.org/abs/2508.05596

Long-period variable stars in NGC 147 and NGC 185-II. Their dust production
This study presents a comparative analysis of mass-loss and dust-production rates in the dwarf galaxies NGC 147 and NGC 185, focusing on long-period variables (LPVs) and pulsating asymptotic giant branch (AGB) stars as primary indicators of dust feedback into the interstellar medium. For NGC 147, the total mass-loss rate is calculated as $(9.44 \pm 3.78) \times 10^{-4} M_{sun} yr^{-1}$, with LPV luminosities ranging from $(6.20 \pm 0.25) \times 10^{2} L_\odot$ to $( 7.87 \pm 0.32) \times 10^{3}…

Forecasting the Observable Rates of Gravitationally Lensed Supernovae for the PASSAGES Dusty Starbursts
Patrick S. Kamieneski, Rogier A. Windhorst, Brenda L. Frye, Min S. Yun, Kevin C. Harrington, Simon D. Mork, Nicholas Foo, Nikhil Garuda, Massimo Pascale, Belen Alcalde Pampliega, Timothy Carleton, Seth H. Cohen, Carlos Garcia Diaz, Rolf A. Jansen, Eric F. Jimenez-Andrade, Anton M. Koekemoer, James D. Lowenthal, Allison Noble, Justin D. R. Pierel, Amit Vishwas, Q. Daniel Wang, Ilsang …

Forecasting the Observable Rates of Gravitationally Lensed Supernovae for the PASSAGES Dusty Starbursts
More than 60 years have passed since the first formal suggestion to use strongly-lensed supernovae to measure the expansion rate of the Universe through time-delay cosmography. Yet, fewer than 10 such objects have ever been discovered. We consider the merits of a targeted strategy focused on lensed hyperluminous infrared galaxies-- among the most rapidly star-forming galaxies known in the Universe. With star formation rates (SFRs) $\sim {200 - 6000}~\textrm{M}_\odot~\textrm{yr}^{-1}$, the $\sim…

#ICYMI following cease & desist letter from #TrumpOrg the co-owner of #MAGA friendly #Trump themed burger restaurants in