Tootfinder

#Mac #MacPaint #MacWrite

Dock für Mac mini M4 im klassischen Macintosh-Design und Screen
Die Wokyis Retro Docking Station packt Apples kleinen Desktop in ein Achtzigerjahre-Gehäuse. Besonderheit ist das Display.
https://www.…

Characterization of the Host Binary of the Directly Imaged Exoplanet HD 143811 AB b
Anne E. Peck, William Roberson, Eric L. Nielsen, Robert J. De Rosa, Nathalie Jones, Jason Wang, Bruce Macintosh, Bailey L. Lewis, Gaspard Duch\^ene, Stanimir Metchev, Asif Abbas, Jerry W. Xuan, Aniket Sanghi, Jennifer Panience, Travis S. Barman, Joanna Bulger, Jeffrey K. Chilcote, Thomas M. Esposito, Michael P. Fitzgerald, Katherine B. Follette, Hannah Gallamore, Stephen Goodsell, James R. Graham, Alexa…

Characterization of the Host Binary of the Directly Imaged Exoplanet HD 143811 AB b
HD~143811~AB is the host star to the directly imaged planet HD~143811~AB~b, which was recently discovered using data from the Gemini Planet Imager and Keck NIRC2. A member of the Sco-Cen star-forming region with an age of $13 \pm 4$ Myr, HD~143811~AB is somewhat rare among hosts of directly imaged planets as it is a close stellar binary, with an $\sim$18 day period. Accurate values for the orbital and stellar parameters of this binary are needed to understand the formation and evolutionary hist…

We have lost our way. https://mastodon.social/@jwz/114983588990828450

Oooh! MAE on a PrecisionBook!
http://oldvcr.blogspot.com/2025/08/a-real-powerbook-macintosh-application.html
#HPUX

Oooh! MAE on a PrecisionBook!
http://oldvcr.blogspot.com/2025/08/a-real-powerbook-macintosh-application.html
#HPUX

Wow what a nice Macintosh Color Classic

HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen
Nathalie K. Jones, Jason J. Wang, Eric L. Nielsen, Robert J. De Rosa, Anne E. Peck, William Roberson, Jean-Baptiste Ruffio, Jerry W. Xuan, Bruce A. Macintosh, S. Mark Ammons, Vanessa P. Bailey, Travis S. Barman, Joanna Bulger, Eugene Chiang, Jeffrey K. Chilcote, Gaspard Duch\^ene, Thomas M. Esposito, Michael P. Fitzgerald, Katherine B. Follette, Stephen Goodsell, James R. Graham, Alexandra Z. Greenbaum,…

HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen
We present confirmation of HD 143811 AB b, a substellar companion to spectroscopic binary HD 143811 AB through direct imaging with the Gemini Planet Imager (GPI) and Keck NIRC2. HD 143811 AB was observed as a part of the Gemini Planet Imager Exoplanet Survey (GPIES) in 2016 and 2019 and is a member of the Sco-Cen star formation region. The companion object is detected $\sim 430$ mas from the host star by GPI. With two GPI epochs and one from Keck/NIRC2 in 2022, we confirm through common proper …

discovered a new Mac emulator https://github.com/twvd/snow

Mmmh-Macs: Als Apple Silicon den Macintosh rettete | Mac & i-Podcast
Nervende Lüfter, unzuverlässige Tastaturen und Adapter-Bonanza: MacBooks steckten in der Krise – bis Apple Silicon kam und alles änderte.

Save me your fake nostalgia, people. There is only one true #BSOD, and it never was blue. 💣

Attn Lawyers & Legal Assistants. Continuously updated guides for Legal Professionals are also available by subscription for Word, Excel, PowerPoint, Outlook & a special ed. for Word for Macintosh.

Original post: https://bsky.app/profile/did:plc:gwp6j

Apache Point Observatory follow-up of ACcelerating Candidate ExopLanet host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
Anne E. Peck (Department of Astronomy, New Mexico State University), Eric L. Nielsen (Department of Astronomy, New Mexico State University), Robert J. De Rosa (European Southern Observatory), William Thompson (National Research Council, Herzberg Astronomy and Astrophysics), Bruce Macintosh (Department of Astronomy and Astrophysics, U…

Apache Point Observatory follow-up of ACcelerating Candidate ExopLanet host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
Directly imaged substellar companions with well-constrained ages and masses serve as vital empirical benchmarks for planet formation and evolution models. Potential benchmark companions can be identified from astrometric accelerations of their host stars. We use Gaia DR3 and Hipparcos astrometry to identify 166 northern hemisphere stars with astrometric accelerations consistent with a substellar companion between 0.5'' and 1''. For this accelerating sample we identify young stars using APO/ARCE…

from my link log —
Apple's sillyballs (1988).
https://devnonsense.com/posts/apple-sillyballs/
saved 2025-04-30 https://

Experimental validation of photonic lantern imaging and wavefront sensing performance
Aditya R. Sengupta, Vincent Chambouleyron, Jordan Diaz, Matthew DeMartino, Rebecca Jensen-Clem, Benjamin L. Gerard, Michael J. Messerly, Paul Pax, Daren Dillon, Kevin Bundy, Maria Cuevas, Sylvain Cetre, Bruce Macintosh, Caleb Dobias, Tara Crowe, Stephen S. Eikenberry, Rodrigo Amezcua-Correa, Stephanos Yerolatsitis

Experimental validation of photonic lantern imaging and wavefront sensing performance
Photonic lanterns (PLs) are fiber-based waveguides that are capable of focal-plane wavefront sensing while simultaneously directing light to downstream science instruments. The optimal choice of wavefront reconstruction algorithm has yet to be determined, and likely depends on the particular observing scenario under consideration. Previous work in simulation suggests that PLs can be used for nonlinear wavefront sensing for several applications, including sensing the low-wind effect and correcti…

Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
Kielan K. W. Hoch, Melanie Rowland, Simon Petrus, Evert Nasedkin, Carl Ingebretsen, Jens Kammerer, Marshall Perrin, Valentina D'Orazi, William O. Balmer, Travis Barman, Mickael Bonnefoy, Gael Chauvin, Christine Chen, Rob J. De Rosa, Julien Girard, Eileen Gonzales, Matt Kenworthy, Quinn M. Konopacky, Bruce Macintosh, Sarah E. Moran, Caroline V. Morley, Paulina Palma-Bifani, Laurent Pueyo, Bin Ren, Emily Rickma…

Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
Young exoplanets provide a critical link between understanding planet formation and atmospheric evolution. Direct imaging spectroscopy allows us to infer the properties of young, wide orbit, giant planets with high signal-to-noise. This allows us to compare this young population to exoplanets characterized with transmission spectroscopy, which has indirectly revealed the presence of clouds, photochemistry, and a diversity of atmospheric compositions. Direct detections have also been made for br…