Tootfinder

Oha. Diese heftige, ab Juli gültige Rentenkürzung ist ja komplett an mir vorbei gegangen: https://verbraucherschutzforum.berlin/2025-04-26/mehr-geld-fuer-hinterbliebene-das-aendert-sich-bei-der-witwenrente-ab-…

Große Reform der Witwenrente ab Juli 2025: Was sich ändert – Zahlen, Fakten und Beispielrechnung - Das Verbraucherschutzforum
Ab Juli 2025 wird die Witwen- und Witwerrente in Deutschland umfassend reformiert. Ziel der Neuerungen ist es, das…

Flare frequency in M dwarfs belonging to Young Moving Groups
E. Mamonova, Y. Shan, A. F. Kowalski, S. Wedemeyer S. C. Werner
https://arxiv.org/abs/2506.04465

Flare frequency in M dwarfs belonging to Young Moving Groups
Context. M stars are preferred targets for studying terrestrial exoplanets, for which we hope to obtain their atmosphere spectra in the next decade. However, M dwarfs have long been known for strong magnetic activity and the ability to frequently produce optical, broadband emission flares. Aims. We aim to characterise the flaring behaviour of young M dwarfs in the temporal, spectral, and energetic dimensions, as well as examine the stellar parameters governing this behaviour, in order to improv…

Prachtig afscheidsinterview met Peter de Bie, de weduwnaar van Dieuwertje Blok
https://archive.ph/XkH1C

Voor wie niet slapen kan..
Enjoy!
Pickup On South Street (1953) Richard Widmark, Jean Peters - #FilmNoir : #InternetArchive
…

A high mutual inclination system around KOI-134 revealed by transit timing variations
Emma Nabbie, Chelsea X. Huang, Judith Korth, Hannu Parviainen, Su Wang, Alexander Venner, Robert Wittenmyer, Allyson Bieryla, David W. Latham, Gongjie Li, Douglas N. C. Lin, George Zhou
https://arxiv.org/abs/2507.02238

A high mutual inclination system around KOI-134 revealed by transit timing variations
Few planetary systems have measured mutual inclinations, and even less are found to be non-coplanar. Observing the gravitational interactions between exoplanets is an effective tool to detect non-transiting companions to transiting planets. Evidence of these interactions can manifest in the light curve through transit timing variations (TTVs) and transit duration variations (TDVs). Through analysis of Kepler photometry and joint TTV-TDV modeling, we confirm the detection of KOI-134 b, a transit…

https://gallery.davidwhittemore.com/1987/10/23/tina_turner_1.html
https://

Conformational properties of strictly two-dimensional equilibrium polymers
J. P. Wittmer, A. Cavallo, A. Johner
https://arxiv.org/abs/2507.00649 https://…

Conformational properties of strictly two-dimensional equilibrium polymers
Two-dimensional monodisperse linear polymer chains are known to adopt for sufficiently large chain lengths $N$ and surface fractions $ϕ$ compact configurations with fractal perimeters. We show here by means of Monte Carlo simulations of reversibly connected hard disks (without branching, ring formation and chain intersection) that polydisperse self-assembled equilibrium polymers with a finite scission energy $E$ are characterized by the same universal exponents as their monodisperse peers. Con…

Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
Hans Kjeldsen, Timothy R. Bedding, Yaguang Li, Frank Grundahl, Mads Fredslund Andersen, Duncan J. Wright, Jack Soutter, Robert Wittenmyer, Claudia Reyes, Dennis Stello, Courtney Crawford, Yixiao Zhou, Mathieu Clerte, Pere L. Palle, Sergio Simon-Diaz, Joergen Christensen-Dalsgaard, Rasmus Handberg, Hasse Hansen, Paul Heeren, Jens Jessen-Hansen, Mikkel Lund, Mia S. Lundkvist, Karsten Brogaard, Re…

Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
We present radial velocities of the G8 subgiant star beta Aql obtained in 2022 and 2023 using SONG-Tenerife and SONG-Australia. We also analysed a sector of TESS photometry that overlapped with the 2022 SONG data. We processed the time series to assign weights and to remove bad data points. The power spectrum clearly shows solar-like oscillations centred at 430 muHz. The TESS data show the oscillations at lower signal-to-noise because photometric measurements are much more affected by the granu…

WDMIR: Wavelet-Driven Multimodal Intent Recognition
Weiyin Gong, Kai Zhang, Yanghai Zhang, Qi Liu, Xinjie Sun, Junyu Lu, Linbo Zhu
https://arxiv.org/abs/2506.10011

WDMIR: Wavelet-Driven Multimodal Intent Recognition
Multimodal intent recognition (MIR) seeks to accurately interpret user intentions by integrating verbal and non-verbal information across video, audio and text modalities. While existing approaches prioritize text analysis, they often overlook the rich semantic content embedded in non-verbal cues. This paper presents a novel Wavelet-Driven Multimodal Intent Recognition(WDMIR) framework that enhances intent understanding through frequency-domain analysis of non-verbal information. To be more spe…

Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M-dwarf
Atul Mohan, Peter H. Hauschildt, Birgit Fuhrmeister, Surajit Mondal, Vladimir Airapetian, Sven Wedemeyer
https://arxiv.org/abs/2506.19779

Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M-dwarf
Millimeter (mm) emission from F - M dwarfs (cool stars) primarily traces chromospheric activity, with thermal emission thought to dominate in quiescence. Despite the high chromospheric activity, the quiescent mm spectral fluence (mm-S($ν$)) of young (< 1 Gyr) M dwarfs (dMs) remain largely unexplored. We present the quiescent mm-S($ν$) of a young dM, ADLeo, observed around 94 GHz using the Northern Extended Millimetre Array (NOEMA). The observed quiescent mm-S($ν$) exceeds the thermal flux de…