Tootfinder

„Fire“ by Nytrik
Platform: Atari ST/E
Released: 5 July 2025
Specification: 320x200px, 16 colors
Note: 1st in the Sommarhack 2025 Lowres Graphics competition
#GFX_Nytrik #YR_2025 #PF_Atari

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

„Dark Dreams Lies Beneath“ by Duce
Platform: C64
Released: 19 July 2025
#GFX_Duce #YR_2025 #PF_C64

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 $Γ''_I(R)$.

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…

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…

„Smiling George“ by Beast
Platform: Amiga
Released: 1996
Specification: 320x256px, 256 colors
#GFX_Beast #YR_1996 #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…

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 …

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

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

„Self Portrait“ by James D. Sachs
Platform: Amiga
Released: Around 1990
Specification: 320x200px, 32 colors
#GFX_JamesDSachs #YR_1990 #PF_Amiga

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

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 …

Proof-Theoretic Functional Completeness for the Connexive Logic C
Sara Ayhan, Hrafn Valt\'yr Oddsson
https://arxiv.org/abs/2507.06854 https://

Proof-Theoretic Functional Completeness for the Connexive Logic C
We show the functional completeness for the connectives of the non-trivial negation inconsistent logic C by using a well-established method implementing purely proof-theoretic notions only. Firstly, given that C contains a strong negation, expressing a notion of direct refutation, the proof needs to be applied in a bilateralist way in that not only higher-order rule schemata for proofs but also for refutations need to be considered. Secondly, given that C is a connexive logic we need to take a …

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

„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

Tipp: trackingfreies detailreiches und zuverlässiges Wetter gibt es nicht nur für #burgos über https://www.yr.no/en/forecast/graph/2-3127461/Spain…

Graph for Burgos
Weather forecast for Burgos for the next 3 days in a graph.

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…

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

This was really interesting. It's about Topaz AI, which was a denoising/upscaling solution I looked at about nine months ago, and rejected because I wasn't really prepared to make the investment at that stage ($300/yr) https://mstdn.social/@Onmyom/114779996030982643…

wooohooo, first very early/experimental release of klutshnik running on a xiao esp32s3 over BLE: https://github.com/stef/klutshnik-zephyr

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\…

W H O A ! CONGRATS, @…

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…

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…

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.

11-yr-old: I just stole every bed in this village.
Me: What? Why would you want rhat many beds?
11-yr-old: Dad! So I can defeat the Ender Dragon, duh!

Update on the intermediate arrival-direction analyses of the Pierre Auger Observatory
Lorenzo Apollonio (for the Pierre Auger Collaboration)
https://arxiv.org/abs/2507.08544

Update on the intermediate arrival-direction analyses of the Pierre Auger Observatory
We present an update on the arrival-direction analyses conducted on intermediate angular scales using the complete Phase I data of the Pierre Auger Observatory up to the end of $2022$ with a total exposure of $135{,}000\,\text{km}^2\,\text{sr}\,\text{yr}$. We show the arrival-direction distribution of the ultra-high-energy cosmic rays along the supergalactic plane above $20\,\text{EeV}$, and an update in the search for magnetically-induced signatures in the arrival directions. Furthermore, we p…

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). …

#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…

„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

Measurement of the cosmic-ray energy spectrum above 2.5 EeV using 19 years of operation of the Pierre Auger Observatory
Diego Ravignani (for the Pierre Auger Collaboration)
https://arxiv.org/abs/2507.08573

Measurement of the cosmic-ray energy spectrum above 2.5 EeV using 19 years of operation of the Pierre Auger Observatory
We present the spectrum of cosmic rays with energies above 2.5 EeV measured at the Pierre Auger Observatory after 19 years of operation, covering the period before the AugerPrime upgrade. Two independent event sets from the surface array of 1500 m-spaced detectors are combined, yielding a total exposure of approximately 100,000 km$^2$ sr yr. The first set includes events with zenith angles less than 60$^\circ$, while the second consists of events between 60$^\circ$ and 80$^\circ$, for which azi…

GW231123 Mass Gap Event and the Primordial Black Hole Scenario
Chen Yuan, Zu-Cheng Chen, Lang Liu
https://arxiv.org/abs/2507.15701 https://

GW231123 Mass Gap Event and the Primordial Black Hole Scenario
We investigate the possibility that the recently reported GW231123 event, with component masses $M_1=137^{+22}_{-17}\,M_\odot$, $M_2=103^{+20}_{-52}\,M_\odot$ and a local merger rate $R_{\mathrm{local}}=0.08^{+0.19}_{-0.07}\,\mathrm{Gpc^{-3}\,yr^{-1}}$, originates from primordial black holes (PBHs) formed during an early matter-dominated era. We compute the PBH mass function, abundance, spin distribution and the merger rate density and find a set of choices for the parameters to reproduce the k…

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…

Spectroscopic Orbits of Subsystems in Multiple Stars. XI
Andrei Tokovinin
https://arxiv.org/abs/2507.07233 https://arxiv.org/pdf/2507…

Spectroscopic Orbits of Subsystems in Multiple Stars. XI
Adding to the large radial velocity survey of nearby solar-type stars (summary in Tokovinin, 2023a), spectroscopic orbits are determined for four hierarchical systems: HIP 49442 (inner and outer periods of 164.55 d and 34 yr, respectively), HIP 55691 (2.4 and 415 yr), HIP 61465 (86.8 d), and HIP 78662C (0.82 d). Each system is discussed individually. Seven Gaia orbits of low-mass dwarfs, each with two additional resolved (interferometric and wide) companions, i.e. potential quadruples, are test…

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

San Leandro teen charged with shooting & killing 17 yr old girlfriend in her bedroom, is freed from custody by empathetic judge who rejects #prosecution theory of intentional #murder.
#Prosecutors have refiled murder …

San Leandro teen released from jail after judge rejects girlfriend murder theory
A judge said he doubted the DA’s theory behind the recent fatal shooting of Izabella Raquedan-Retuta, allegedly shot by her boyfriend inside her bedroom.

Unambiguous GeV gamma-rays from molecular clouds illuminated by particles diffusing from the adjacent supernova remnant G335.2 0.1 that is confined in an expanding bubble
Chen Huang, Xiao Zhang, Yang Chen, Qian-Qian Zhang, Wen-Juan Zhong, Xin Zhou
https://arxiv.org/abs/2507.08709

Unambiguous GeV gamma-rays from molecular clouds illuminated by particles diffusing from the adjacent supernova remnant G335.2+0.1 that is confined in an expanding bubble
We report the detection of GeV gamma-ray emission likely associated with supernova remnant (SNR) G335.2+0.1 and the finding of a molecular cloud ($\sim20$--$30^\prime$ in angular size) that is very likely in physical contact with the SNR and responsible for the gamma-ray emission. Using the 16.8 yr Fermi-LAT data, an extended emission, with a significance of 13.5 $σ$ and a radius 0.24° in 0.2--500 GeV in the uniform-disk model, was found to the adjacent east of the SNR. With archival Mopra CO…

„Stargazer“ by Facet
Platform: C64
Released: 28 December 2018
Note: 1st in the Under Construction 2018 Oldskool GFX competition
#GFX_Facet #YR_2018 #PF_C64

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…

I think that I am replacing iTerm2 with @… Prompt on all of my machines after playing with it for a few days. They have a $20/yr or $99 price model and I don't know what makes sense. I hate renting software, though.
#Prompt #iTerm2 #Terminal #MacOS

The GAPS Programme at TNG LXVIII. Characterization of the outer substellar companion around HD 72659 with a multi-technique approach
A. Ruggieri, A. Sozzetti, S. Desidera, D. Mesa, R. Gratton, F. Marzari, M. Bonavita, K. Biazzo, V. D'Orazi, C. Ginski, M. Meyer, L. Malavolta, M. Pinamonti, D. Barbato, C. Lazzoni, A. F. Lanza, L. Mancini, L. Naponiello, D. Nardiello, T. Zingales, M. Rainer, G. Scandariato, P. Giacobbe, R. Cosentino, A. Fiorenzano, R. Claudi

The GAPS Programme at TNG LXVIII. Characterization of the outer substellar companion around HD 72659 with a multi-technique approach
Before discovering the first exoplanets, the Radial Velocity (RV) method had been used for decades to discover binary stars. Despite significant advancements in this technique, it is limited by the intrinsic mass-inclination degeneracy that can be broken when combining RVs with astrometry, which allows us to determine the orbital inclination, or direct imaging, from which we can estimate the true mass of the target. HD 72659 is a solar analog known to host a gas giant on a $\sim 10$-yr orbit an…

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}…

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…

„Glenzcore“ by Misha
Platform: Amiga
Released: 25 July 2025
Specification: 320x256px, 32 colors
Note: 4th in the BOOM! Party 2025 A500 GFX competition
#GFX_Misha #YR_2025 #PF_Amiga

Evolution of the ZTF SLRN-2020 star-planet merger
Ricardo Yarza, Morgan MacLeod, Benjamin Idini, Ruth Murray-Clay, Enrico Ramirez-Ruiz
https://arxiv.org/abs/2507.05365

Evolution of the ZTF SLRN-2020 star-planet merger
We model the optical and infrared transient ZTF SLRN-2020, previously associated with a star-planet merger. We consider the scenario in which orbital decay via tidal dissipation led to the merger, and find that tidal heating within the star was likely unobservable in the archival image of the system taken $12\mathrm{yr}$ before the merger. The observed dust formation months before the merger is consistent with a planet of mass $M_\mathrm{p} \gtrsim 5M_\mathrm{J}$ ejecting material as it skims t…

Six-yr SPIRou monitoring of the young planet-host dwarf AU Mic
J. -F. Donati, P. I. Cristofari, C. Moutou, A. L'Heureux, N. J. Cook, E. Artigau, S. H. P. Alencar, E. Gaidos, A. Vidotto, P. Petit, A. Carmona, T. Ray, the SPIRou science team
https://arxiv.org/abs/2507.01746

Six-yr SPIRou monitoring of the young planet-host dwarf AU Mic
In this paper we revisit our spectropolarimetric and velocimetric analysis of the young M dwarf AU Mic based on data collected with SPIRou at the Canada-France-Hawaii telescope, over a monitoring period of 2041 d from 2019 to 2024. The longitudinal magnetic field, the small-scale magnetic field, and the differential temperature of AU Mic, derived from the unpolarized and circularly-polarized spectra, were clearly modulated with the stellar rotation period, with a pattern that evolved over time.…

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…

„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…

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

„PAT“ by Bimber
Platform: C64
Released: 26 July 2025
Note: 2nd in the BOOM! Party 2025 C64 GFX competition
#GFX_Bimber #YR_2025 #PF_C64

<Unknown> by James D. Sachs
Platform: Amiga
Released: 1989
Specification: 320x200px, 32 colors
#GFX_JamesDSachs #YR_1989 #PF_Amiga

A Glimpse of Satellite Galaxies in the Milky Way with the 2.5-meter Wide Field Survey Telescope (WFST): Bootes III and Draco
Chao Yang, Zhizheng Pan, Min Fang, Xian Zhong Zheng, Binyang Liu, Guoliang Li, Tian-Rui Sun, Ji-An Jiang, Miaomiao Zhang, Zhen Wan, Shuang Liu, Han Qu, Ji Yang, Xu Kong, Wenhao Liu, Yiping Shu, Jiang Chang, Tinggui Wang, Lulu Fan, Yongquan Xue, Wentao Luo, Hongxin Zhang, Zheng Lou, Haibin Zhao, Bin Li, Hairen Wang, Dazhi Yao, Jian Wang, Hongfei Zhang, Feng Li, Ha…

A Glimpse of Satellite Galaxies in the Milky Way with the 2.5-meter Wide Field Survey Telescope (WFST): Bootes III and Draco
We carry out deep imaging of the Milky Way satellite galaxies, Bootes III and Draco, with WFST as one pilot observing program to demonstrate the capability of WFST. Combining catalogs with PS1 DR2 and Gaia DR3, we derive proper motions for candidate member stars in these two satellite galaxies over a 12-year time baseline, yielding uncertainties of ~1.8 mas/yr at 21 mag and ~3.0 mas/yr at 22 mag in the r band. The proper motions derived from bright and faint stars are consistent, indicating no …

The evolution of chromospheric quiet-sun bright points during their lifetime
Ll\^yr Humphries, Huw Morgan, David Kuridze
https://arxiv.org/abs/2506.19473 h…

The evolution of chromospheric quiet-sun bright points during their lifetime
Bright points (BPs) are ubiquitous, small-scale energetic events with multithermal signatures, typically observed in the chromosphere and linked to both photospheric structure and coronal composition. Their evolution is influenced by various physical processes, including plasma dynamics and magnetic interactions. This paper examines BP evolution using a large statistical sample, focusing on when they reach maximum values for key attributes, and explores differences between BPs in the "Active Qu…

„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

„Joker“ by Facet
Platform: Amiga
Released: 1992
Specification: 320x256px, 32 colors
#GFX_Facet #YR_1992 #PF_Amiga

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…

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…

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

„Predator“ by Jojo073
Platform: Amiga
Released: 25 November 2017
Specification: 320x256px, 16 colors
Note: 4th in the Syntax 2017 Graphics - Pixel competition
#GFX_Jojo073 #YR_2017

A Late-time Radio Survey of Type Ia-CSM Supernovae with the Very Large Array
Olivia Griffith, Grace Showerman, Sumit K. Sarbadhicary, Chelsea E. Harris, Laura Chomiuk, Jesper Sollerman, Peter Lundqvist, Javier Moldon, Miguel Perez-Torres, Erik C. Kool, Takashi J. Moriya
https://arxiv.org/abs/2506.19071

A Late-time Radio Survey of Type Ia-CSM Supernovae with the Very Large Array
Type Ia-CSM supernovae (SNe) are a rare and peculiar subclass of thermonuclear SNe characterized by emission lines of hydrogen or helium, indicative of a high-density circumstellar medium (CSM). Their implied mass-loss rates of $\sim 10^{-4}-10^{-1}$ M$_{\odot}$ yr$^{-1}$ (assuming $\mathrm{ \sim 100 \ km\ s^{-1}}$ winds) from optical observations are generally in excess of values observed in realistic SN Ia progenitors. In this paper, we present an independent study of CSM densities around a s…

Discovery of diffuse $\gamma$-ray emission in the vicinity of G213.0-0.6: Supernova remnant versus massive star-forming region
Yuan Li, Gwenael Giacinti, Siming Liu
https://arxiv.org/abs/2506.18146

Discovery of diffuse $γ$-ray emission in the vicinity of G213.0-0.6: Supernova remnant versus massive star-forming region
We report the discovery of high-energy $γ$-ray emission in the vicinity of G213.0-0.6, 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 three extended sources with different photon spectra in this region, which will label as SrcA, SrcB and SrcC. Among them, the $γ$-ray source SrcA with a log-parabola spectrum is spatially coincident with a star-forming region and several O…

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

42 yr old white male madman #Xtian #Terrorist who went on stabbing spree outside #Michigan #WalMart had recently authored a book about his relatio…

#SanFrancisco #nightclub owner quietly acquires 99 yr old abandoned downtown #Oakland bldg that most recently hosted homeless & illegal #raves

5 yr #House probe of into PA #GOP Congressman affirms he violated elected representative #CodeOfConduct after #insidertrading stock investmen…

#Data shows US #Liquor sales to #Canada fell by nearly 70% earlier this yr and 80% in #Ontario alone as

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