Tootfinder

W H O A ! CONGRATS, @…

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…

„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

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…

Einschlag des Asteroiden 2024 YR₄ auf Mond noch einmal etwas wahrscheinlicher
Der Asteroid 2024 YR₄ ist vorerst außer Reichweite unserer Instrumente. Laut der letzten Beobachtung ist ein Einschlag auf dem Mond nun etwas wahrscheinlicher.

„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

🇺🇦 #NowPlaying on KEXP's #SonicReducer
Shitfire:
🎵 In Yr Head
#Shitfire
https://shitfire.bandcamp.com/track/in-yr-head
https://open.spotify.com/track/2XdTm1vAx77uEq6E04O0IS

NFL news roundup: Steelers, S DeShon Elliott agree to 2-yr, $12.5 million extension https://www.nfl.com/news/nfl-news-roundup-latest-league-updates-from-monday-june-16

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

„Watchmaker of Light“ by Slayer
Platform: Amiga
Released: 20 September 2014
Specification: 320x256px, 32 colors
Note: 1st in the Riverwash 2014 Oldschool GFX competition
#GFX_Slayer #YR_2014

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.

I pay $50/yr for @… and at some point (once it's fully baked), I'm going to be paying $100/yr for @… but I don't feel like I use it enough. I need to remedy that.

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 …

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

The impact of economic policies on housing prices. Approximations and predictions in the UK, the US, France, and Switzerland from the 1980s to today
Nicolas Houli\'e
https://arxiv.org/abs/2505.09620

The impact of economic policies on housing prices. Approximations and predictions in the UK, the US, France, and Switzerland from the 1980s to today
I show that house prices can be modeled using machine learning (kNN and tree-bagging) and a small dataset composed of macro-economic factors (MEF), including an inflation metric (CPI), US treasury rates (10-yr), Gross Domestic Product (GDP), and portfolio size of central banks (ECB, FED). This set of parameters covers all the parties involved in a transaction (buyer, seller, and financing facility) while ignoring the intrinsic properties of each asset and encompassing local (inflation) and liqu…

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…

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…

Precipitation plausible: magnetized thermal instability in the intracluster medium
Benjamin D. Wibking, G. Mark Voit, Brian W. O'Shea
https://arxiv.org/abs/2506.10277

Precipitation plausible: magnetized thermal instability in the intracluster medium
Observations of galaxy-cluster cores reveal that AGN feedback is strongly associated with both a short central cooling time ($t_{\rm c} \lesssim 10^9 \, {\rm yr}$) and accumulations of cold gas ($\lesssim 10^4 \, {\rm K}$). Also, the central ratio of cooling time to freefall time is rarely observed to drop below $t_{\rm c}/t_{\rm ff} \approx 10$, and large accumulations of cold gas are rarely observed in environments with $t_{\rm c} / t_{\rm ff} \gtrsim 30$. Here we show that the critical range…

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

@… plz write a bio and update yr profile pic so I know who you are. I don't want to be followed by certain accounts like bots, right wing etc

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

The Energy Spectrum of Ultra-High Energy Cosmic Rays across Declinations $-90^\circ$ to $ 44.8^\circ$ as measured at the Pierre Auger Observatory
Collaboration, Halim, Abreu, Aglietta, Allekotte, Cheminant, Almela, Aloisio, Alvarez-Mu\~niz, Ambrosone, Yebra, Anastasi, Anchordoqui, Andrada, Dourado, Andringa, Apollonio, Aramo, Arnone, Vel\'azquez, Assis, Avila, Avocone, Bakalova, Barbato, Mocellin, Bellido, Berat, Bertaina, Bianciotto, Biermann, Binet, Bismark, Bister, Biteau, Blaze…

The Energy Spectrum of Ultra-High Energy Cosmic Rays across Declinations $-90^\circ$ to $+44.8^\circ$ as measured at the Pierre Auger Observatory
The energy spectrum of cosmic rays above 2.5 EeV has been measured across the declination range $-90^\circ \leqδ\leq +44.8^\circ$ using data from $\sim 310{,}000$ events accrued at the Pierre Auger Observatory from an exposure of $(104{,}900\pm 3{,}100)$ km$^2\,$sr$\,$yr. No significant variations of energy spectra with declination are observed, after allowing or not for non-uniformities across the sky arising from the well-established dipolar anisotropies in the arrival directions of ultra-hi…

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.

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

Vikings ink TE Oliver to 3-yr., $23.25M extension https://www.espn.com/nfl/story/_/id/45485798/vikings-sign-te-josh-oliver-3-year-2325-contract-extension

„Magician Among the Spirits“ by Slayer
Platform: Amiga
Released: 22 October 2022
Specification: 320x256px, 32 colors
Note: 1st in the Decrunch 2022 Amiga Pixel Graphics competition
#GFX_Slayer #YR_2022

Exploring the keV-scale physics potential of CUORE
CUORE Collaboration, D. Q. Adams, C. Alduino, K. Alfonso, A. Armatol, F. T. Avignone III, O. Azzolini, G. Bari, F. Bellini, G. Benato, M. Beretta, M. Biassoni, A. Branca, C. Brofferio, C. Bucci, J. Camilleri, A. Caminata, A. Campani, J. Cao, C. Capelli, S. Capelli, L. Cappelli, L. Cardani, P. Carniti, N. Casali, E. Celi, D. Chiesa, M. Clemenza, S. Copello, A. Cosoli, O. Cremonesi, R. J. Creswick, A. DAddabbo, I. Dafinei, S. DellOro, S.…

Exploring the keV-scale physics potential of CUORE
We present the analysis techniques developed to explore the keV-scale energy region of the CUORE experiment, based on more than 2 tonne yr of data collected over 5 years. By prioritizing a stricter selection over a larger exposure, we are able to optimize data selection for thresholds at 10 keV and 3 keV with 691 kg yr and 11 kg yr of data, respectively. We study how the performance varies among the 988-detector array with different detector characteristics and data taking conditions. We achiev…

If you were not already avoiding flying in new (<15 yr old) Boeing planes, this should seal the deal.
#boeing #dreamliner #union #quality #endstagecapitalism
https://prospect.org/economy/2025-06-12-dreamliner-gave-boeing-manager-nightmares-just-crashed-air-india/

The central spectra of massive star-forming galaxies
Jaimie R. Sheil, Michael J. I . Brown, Virginia A. Kilborn, Michelle E. Cluver, Thomas Jarrett
https://arxiv.org/abs/2506.08474

The central spectra of massive star-forming galaxies
We have examined the nuclear spectra of very massive star-forming galaxies at $z \sim 0$ to understand how they differ from other galaxies with comparable masses, which are typically passive. We selected a sample of 126 nearby massive star-forming galaxies ($<100~{\rm Mpc}$, $10^{11.3}~\rm{M_\odot} \leq M_{\rm stellar} \leq 10^{11.7}~\rm{M_\odot}$, $1 ~{\rm M_\odot~yr^{-1}}< {\rm SFR} <13 ~{\rm M_\odot~yr^{-1}}$) from the 2MRS-Bright WXSC catalogue. LEDA morphologies indicate at least 63\% of o…

This https://arxiv.org/abs/2412.16047 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_nuc…

Rare multi-nucleon decays with the full data sets of the Majorana Demonstrator
The Majorana Demonstrator was an ultra-low-background experiment designed for neutrinoless double-beta decay ($0νββ$) investigation in $^{76}$Ge. Located at the Sanford Underground Research Facility in Lead, South Dakota, the Demonstrator utilized modular high-purity Ge detector arrays within shielded vacuum cryostats, operating deep underground. The arrays, with a capacity of up to 40.4 kg (27.2 kg enriched to $\sim 88\%$ in $^{76}$Ge), have accumulated the full data set, totaling 64.5 kg y…

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…

A comprehensive light curve model of the very fast nova V1674 Herculis
Mariko Kato, Izumi Hachisu, Hideyuki Saio
https://arxiv.org/abs/2506.04615 https://

A comprehensive light curve model of the very fast nova V1674 Herculis
V1674 Her is one of the fastest novae, of which the very early phase is well observed including optical rise to the peak over 10 magnitudes. We present a full theoretical light curve model of V1674 Her. Our $1.35~M_\odot$ white dwarf (WD) model with the mass accretion rate of $1\times 10^{-11}~M_\odot$ yr$^{-1}$ explains overall properties including a very fast rise and decay of the optical $V$ light curve. The WD photosphere expands up to $21 ~R_\odot$, thus, a $0.26 ~M_\odot$ companion star o…

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…

„White dream“ by Prowler
Platform: Amiga
Released: 22 August 2015
Specification: 320x256px, 32 colors
Note: 1st in the Gerp 2015 Graphics competition
#GFX_Prowler #YR_2015 #PF_Amiga

If you were not already avoiding flying in new (<15 yr old) Boeing planes, this should seal the deal.
#boeing #dreamliner #union #quality #endstagecapitalism
https://prospect.org/economy/2025-06-12-dreamliner-gave-boeing-manager-nightmares-just-crashed-air-india/

Any second now... #LLM #AGI #GenAI #AI

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…

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.…

„No signal, 1081-head in the glitchy CGA swamp“ by z3k
Platform: Amiga
Released: 1 October 2022
Specification: 320x240px 66 colors
Note: 1st in the Flashparty 2022 Oldschool Pixel Art competition
#GFX_z3k #YR_2022

Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe
S. Kaviraj, B. Bichang'a, I. Lazar, A. E. Watkins, G. Martin, R. A. Jackson
https://arxiv.org/abs/2506.03265

Nearby dwarf galaxies with extreme star formation rates: a window into dwarf-galaxy evolution in the early Universe
We study a sample of nearby (z~0.2) low-luminosity dwarf (10^7 MSun < M* < 10^8 MSun) galaxies which have extreme (0.1 - 3 MSun/yr) star formation rates (SFRs) for this mass regime, making them plausible analogues of dwarfs at z~5.5. We compare the properties of these analogues to control samples of 'normal' dwarfs, which reside on the star formation main sequence (SFMS) at z~0.2 and are matched in their stellar mass and redshift distributions to the analogue population. The analogue and normal…

„Greg, The Killer Clown“ by Facet and Magic
Platform: Amiga
Released: 15 April 2017
Specification: 320x256px, 29 colors
Note: 3rd in the Revision 2017 Oldskool Graphics competition
#GFX_Facet #GFX_Magic

„Duck It“ by Pal
Platform: C64
Released: 25 October 2014
Note: 1st in the X 2014 Graphics competition
#GFX_Pal #YR_2014 #PF_C64

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…

„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

This https://arxiv.org/abs/2409.07527 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

Can slow pulsars in Milky Way globular clusters form via partial recycling?
Alongside the population of several hundred radio millisecond pulsars currently known in Milky Way globular clusters, a subset of six slowly spinning pulsars (spin periods $0.3-4\,$s) are also observed. With inferred magnetic fields $\gtrsim 10^{11}\,$G and characteristic ages $\lesssim10^8\,$yr, explaining the formation of these apparently young pulsars in old stellar populations poses a major challenge. One popular explanation is that these objects are not actually young but instead have been…

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

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 …

„Are ”Friends” Electric?“ by Mikael
Platform: C64
Released: 4 May 2022
#GFX_Mikael #YR_2022 #PF_C64

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…

This https://arxiv.org/abs/2409.18334 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

Decade-long periodicity study of 2FHL blazars with historical optical data
In our recent investigation, we utilized a century's worth of archival optical data to search for a decade-long periodicity from the blazar PG 1553+113, finding a hint of a 22-yr period. Building on this foundation, the current study extends our analysis to include 10 blazars from the Fermi-Large Area Telescope Second Catalog of Hard Sources (2FHL) catalogue to uncover similar long-term periodic behaviour. To ensure the reliability of our findings, we consider the impact of observational limita…

„Broken Mirror“ by Fairfax
Platform: Amiga
Released: 3 April 1994
Specification: 320x256px, 64 colors
Note: Picture used in Andromeda's Sequential demo that got a 1st in the The Gathering 1994 Amiga Demo competition.
#GFX_Fairfax #YR_1994

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…

„Eden 377“ by Made
Platform: Amiga
Released: 30 December 1996
Specification: 320x256px 128 colors
Note: 2nd in the The Party 1996 Graphics competition
#GFX_Made #YR_1996 #PF_Amiga

„Head With Bubbles“ by Mon
Platform: Amiga
Released: 14 August 1995
Specification: 320x256px, 128 Colors
Note: 7th in the 'Gainful Awesome Summer Party' (GASP) 1995 Graphics competition.
#GFX_MoN #YR_1995

„Galactic Gaze“ by Mikael
Platform: C64
Released: 11 August 2020
#GFX_Mikael #YR_2020 #PF_C64 #C64

„Area 64“ by Pal
Platform: C64
Released: Released 29 October 2016
#GFX_Pal #YR_2016 #PF_C64 #C64