reapxdev/zenodo-scraper huggingface dataset:
Figure 6 from: Huang J-F, Liao Y-C, Chan T-Y, Chen H-M, Smith DG (2026) The congrid eel genus Gnathophis in Taiwan (Anguilliformes, Congridae), with descriptions of three new species. ZooKeys 1287: 11-46. https://doi.org/10.3897/zookeys.1287.183842
Authors: Huang, Jian-Fu, Liao, Yun-Chih, Chan, Tin-Yam, Chen, Hong-Ming, Smith, David G.
Type: Figure
Published: 2026-07-31
Keywords: Biodiversity, Congrinae, DNA barcoding, new species, taxonomy

Figure 6 Lateral view of head showing the head pores and anterior lateral-line pores, arrow indicates the ST pore. A. Gnathophis asanoi Karmovskaya, 2004, NMMB-P30378, 350 mm TL; B. Gnathophis heterognathos (Bleeker, 1858), TOU-AE 9900, 329 mm TL; C. Gnathophis kbalanensis sp. nov. Holotype, TOU-AE 9480, 472 mm TL; D. Gnathophis melanurum sp. nov. Holotype, TOU-AE 8777, 300 mm TL; E. Gnathophis nanhaiensis sp. nov. Holotype, ASIZP66800, 245 mm TL.
Figure 5 from: Huang J-F, Liao Y-C, Chan T-Y, Chen H-M, Smith DG (2026) The congrid eel genus Gnathophis in Taiwan (Anguilliformes, Congridae), with descriptions of three new species. ZooKeys 1287: 11-46. https://doi.org/10.3897/zookeys.1287.183842
Authors: Huang, Jian-Fu, Liao, Yun-Chih, Chan, Tin-Yam, Chen, Hong-Ming, Smith, David G.
Type: Figure
Published: 2026-07-31
Keywords: Biodiversity, Congrinae, DNA barcoding, new species, taxonomy

Figure 5 Gnathophis nanhaiensis sp. nov. Holotype, ASIZP66800, 245 mm TL. A. Lateral view; B. Lateral view of anterior portion of head.
Figure 4 from: Huang J-F, Liao Y-C, Chan T-Y, Chen H-M, Smith DG (2026) The congrid eel genus Gnathophis in Taiwan (Anguilliformes, Congridae), with descriptions of three new species. ZooKeys 1287: 11-46. https://doi.org/10.3897/zookeys.1287.183842
Authors: Huang, Jian-Fu, Liao, Yun-Chih, Chan, Tin-Yam, Chen, Hong-Ming, Smith, David G.
Type: Figure
Published: 2026-07-31
Keywords: Biodiversity, Congrinae, DNA barcoding, new species, taxonomy

Figure 4 Gnathophis melanurum sp. nov. Holotype, TOU-AE 8777, 300 mm TL. A. Lateral view; B. Lateral view of anterior portion of head; C. Preserved.
Figure 3 from: Huang J-F, Liao Y-C, Chan T-Y, Chen H-M, Smith DG (2026) The congrid eel genus Gnathophis in Taiwan (Anguilliformes, Congridae), with descriptions of three new species. ZooKeys 1287: 11-46. https://doi.org/10.3897/zookeys.1287.183842
Authors: Huang, Jian-Fu, Liao, Yun-Chih, Chan, Tin-Yam, Chen, Hong-Ming, Smith, David G.
Type: Figure
Published: 2026-07-31
Keywords: Biodiversity, Congrinae, DNA barcoding, new species, taxonomy

Figure 3 Gnathophis kbalanensis sp. nov. Holotype, TOU-AE 9480, 472 mm TL. A. Lateral view; B. Lateral view of anterior portion of head; C. Preserved.
Figure 2 from: Huang J-F, Liao Y-C, Chan T-Y, Chen H-M, Smith DG (2026) The congrid eel genus Gnathophis in Taiwan (Anguilliformes, Congridae), with descriptions of three new species. ZooKeys 1287: 11-46. https://doi.org/10.3897/zookeys.1287.183842
Authors: Huang, Jian-Fu, Liao, Yun-Chih, Chan, Tin-Yam, Chen, Hong-Ming, Smith, David G.
Type: Figure
Published: 2026-07-31
Keywords: Biodiversity, Congrinae, DNA barcoding, new species, taxonomy

Figure 2 Gnathophis heterognathos (Bleeker, 1858), TOU-AE 9900, 329 mm TL. A. Lateral view; B. Lateral view of anterior portion of head; C. Holotype of Myrophis heterognathos Bleeker, 1858, BMNH 1867.11.28.305, 137 mm TL.
Figure 1 from: Huang J-F, Liao Y-C, Chan T-Y, Chen H-M, Smith DG (2026) The congrid eel genus Gnathophis in Taiwan (Anguilliformes, Congridae), with descriptions of three new species. ZooKeys 1287: 11-46. https://doi.org/10.3897/zookeys.1287.183842
Authors: Huang, Jian-Fu, Liao, Yun-Chih, Chan, Tin-Yam, Chen, Hong-Ming, Smith, David G.
Type: Figure
Published: 2026-07-31
Keywords: Biodiversity, Congrinae, DNA barcoding, new species, taxonomy

Figure 1 Gnathophis asanoi Karmovskaya, 2004, NMMB-P30378, 350 mm TL. A. Lateral view; B. Lateral view of anterior portion of head.
Figure 9 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 9 Ptychoptera annandalei Brunetti, 1918. Female terminalia. A. Unmacerated, lateral; B. Macerated, lateral; C. Epigynium and cerci, ventral; D. Hypogynium, hypogynial valves and genital plate, dorsal; E. Genital plate. Scale bars: 0.5 mm (A, B); 0.25 mm (C–E).
Figure 8 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 8 Ptychoptera annandalei Brunetti, 1918. Male terminalia. A. Hypandrium, posterior; B. Hypandrium, ventral; C. Aedeagus, anterior; D. Aedeagus, lateral. Scale bar: 0.5 mm.
Figure 7 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 7 Ptychoptera annandalei Brunetti, 1918. Male terminalia. A. Overall, lateral; B. Epandrium, dorsal; C. Gonopods and parameres, dorsal; D. Gonopods and parameres, posterior; E. Gonopod, outer lateral; F. Gonostylus, outer later, slightly bent ventrally. Scale bar: 0.5 mm.
Figure 6 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 6 Ptychoptera annandalei Brunetti, 1918. Unmacerated male terminalia. A. Lateral; B. Posterior; C. Ventral. Scale bar: 0.5 mm.
Figure 5 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 5 Ptychoptera annandalei Brunetti, 1918. Wing. Scale bar: 0.5 mm.
Figure 42 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 42 Ptychoptera srilankaensis Paramonov, sp. nov. A. Hypandrium and aedeagus, lateral; B. Hypandrium, lateral; C. Overall, posterior; D. Hypandrium and aedeagus, posterior; E. Hypandrium, posterior; F. Aedeagus, lateral; G. Aedeagus, anterior (slightly rotated). Scale bar: 0.5 mm.
Figure 41 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 41 Ptychoptera srilankaensis Paramonov, sp. nov. A. Epandrium, dorsal; B. Epandrium, ventral; C. Gonopod and paramere, dorsal; D. Gonopod and paramere, ventral; E. Gonopod, outer lateral; F. Paramere. Scale bar: 0.5 mm.
Figure 40 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 40 Ptychoptera srilankaensis Paramonov, sp. nov. Wing. Scale bar: 0.5 mm.
Figure 4 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 4 Ptychoptera annandalei Brunetti, 1918. Male habitus. A. Dorsal; B. Lateral. Scale bar: 1 mm.
Figure 39 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 39 Ptychoptera srilankaensis Paramonov, sp. nov. Habitus. Scale bar: 2 mm.
Figure 38 from: Kolcsár L-P, Fasbender A, Paramonov N, Srisuka W, Ang Y (2026) Descriptions of five new Oriental Ptychoptera Meigen, 1803 (Diptera, Ptychopteridae). ZooKeys 1287: 91-152. https://doi.org/10.3897/zookeys.1287.183917
Authors: Kolcsár, Levente-Péter, Fasbender, Andrew, Paramonov, Nikolai, Srisuka, Wichai, Ang, Yuchen
Type: Figure
Published: 2026-07-31
Keywords: Fold-winged crane flies, identification key, Indo-Malayan realm, male genitalia, new species, phantom craneflies

Figure 38 Ptychoptera phutphi Kolcsár & Fasbender, sp. nov. Male terminalia. A. Hypandrium, posterior; B. Hypandrium, ventral; C. Aedeagus, anterior; D. Aedeagus, lateral. Scale bar: 0.5 mm.
GEOMETRIC ORIGINS OF THE COUPLING CONSTANTS AND DETERMINISTIC OPTICAL METRIC ENGINEERING
Authors: Aksman, Michael
Type: Presentation
Published: 2026-08-03

<p>In standard quantum field theory, the fundamental coupling constants (α, αs, αw) and<br>particle masses are empirical free parameters. We present a rigorous, self-contained derivation proving that elementary particles are dynamically selected stable extrema of a topological energy landscape, and interaction strengths are strictly deterministic geometric aspect ratios of these manifolds. From the 1985 vorton interaction kernel, we derive the exact mechanical balance equation stabilizing the electron at N = 861 discrete nodes and the Borromean proton at a confinement multiplier of M = 43. From these strict mathematical roots, the electromagnetic, strong, and weak coupling constants are calculated directly via acoustic impedance matching. Finally, we propose a falsifiable experimental regime: by utilizing optical vortices carrying orbital angular momentum (OAM) of ℓ = 72 to perfectly phase-match the 72-fold rotational symmetry of the vacuum, deterministic light-by-light scattering and optical metric engineering can be achieved well below the Schwinger limit.</p>
Priority Tier - An Alternate Charge-back Model
Authors: Nelson, Kaylea, Langford, Thomas
Type: Presentation
Published: 2026-08-03

<p>Slides from the short paper presentation of "Priority Tier: An Opt-In Priority-Based Chargeback Model for<br>Yale Research Computing", Kaylea Nelson & Thomas Langford<br>https://doi.org/10.1145/3785462.3815884</p>
Chunk Manifests: How We Got Here
Authors: Gallagher, James
Type: Presentation
Published: 2026-07-28

<p class="isSelectedEnd"><strong>Abstract: </strong><br>As scientific data increasingly move from traditional file systems to cloud object storage, new approaches are needed to preserve efficient, scalable access to chunked datasets. This presentation explores the evolution of chunk manifests, which are machine-readable descriptions that expose the information required to locate, decode, and retrieve chunked data independently of the original file access API. Drawing on the history of HDF5 and its design goals of machine independence, self-description, and efficient I/O, the presentation explains how chunk manifests extend these principles to modern cloud-native data access.</p>
<p>The talk examines the common elements shared across manifest implementations, including chunk locations, compression and filter information, variable definitions, dimensions, and semantic metadata, while discussing emerging interoperability efforts across formats such as DMR++, Kerchunk, Zarr, and IceChunk. It also highlights practical implementation challenges, including support for inline data, externally computed data, and complex data types that increase client complexity. Finally, the presentation considers the evolving boundary between data and metadata and poses open questions about what capabilities should be standardized to maximize interoperability while minimizing implementation burden. Together, these topics provide a framework for understanding how chunk manifests can enable more portable, efficient, and interoperable access to large scientific datasets in cloud environments.</p>
Constraining surface differential rotation in solar-like stars
Authors: Amaral, Juliana H., Santos, Ângela R. G., Cunha, Margarida S., García, Rafael A.
Type: Presentation
Published: 2026-07-10

<p>Surface differential rotation is a key driver of magnetic activity in solar-like stars, yet its measurement from photometric data remains challenging. In this work, we apply the peak-height ratios (PHR) technique to constrain surface differential rotation. The method uses the ratio between the amplitudes of the second and first rotational harmonics in the periodogram of quasi-periodic flux modulations induced by active regions rotating across the stellar disc. This ratio depends on the latitude of the active regions and the stellar inclination, allowing each detected rotation period to be associated with a likely active-region latitude.</p>
<p>We analyse a sample of 56 solar-like stars observed with long-cadence Kepler data, all with well-constrained inclinations from asteroseismology and detected rotational modulation. The sample includes 11 benchmark stars with independent asteroseismic measurements of differential rotation, enabling a direct validation of the method. For each target, we first construct star-specific relations between PHR and active-region latitude. We then identify robust harmonic pairs across independent light-curve segments and compute the respective observed PHR. These measurements together with the derived PHR relations are used to infer the surface differential rotation profile, including the equatorial rotation period and latitudinal shear, using weighted fitting and bootstrap uncertainty estimation.</p>
<p>For the benchmark sample, the PHR-based shear values are consistent with asteroseismic results, supporting the reliability of the method despite the different depths probed by the two techniques. Across the full sample, we recover the expected trend of decreasing equatorial rotation period with increasing effective temperature. We also find that hotter, F-type stars tend to exhibit larger relative shear, with indications of a systematic increase above ~6000 K.</p>
<p>Overall, our results demonstrate that the PHR technique provides a viable photometric diagnostic of surface differential rotation, enabling new constraints on stellar dynamos and magnetic activity across large stellar samples.</p>
Pulsating stars in binaries
Authors: Hey, Daniel
Type: Presentation
Published: 2026-07-10

<p>Binary stars are of fundamental importance to asteroseismology. Eclipses and orbital dynamics yield model-independent masses and radii that calibrate asteroseismology, while pulsations reveal the ages, internal rotation, and mixing that orbital geometry alone cannot constrain. In this talk I review how this relationship has matured into a precision science. Eclipsing binaries hosting $\delta$ Scuti, $\gamma$ Doradus, slowly pulsating B, and red-giant components now serve as benchmark systems for testing the physics of stellar interiors. Pulsation timing, through phase and frequency modulation and the classical O−C diagram, has turned coherent oscillators into instruments sensitive to stellar, substellar, and even compact companions. In parallel, tidal interactions in close and eccentric systems produce a rich array of phenomena, from heartbeat stars and tidally excited oscillations to tidally tilted pulsators whose pulsation axes track the orbital geometry. The all-sky TESS photometric coverage has expanded these samples by orders of magnitude and uncovered an outstanding sample of interesting systems. I will highlight recent results, some modeling challenges they expose, and the prospects for binary asteroseismology as we move toward the next era of high precision photometry.</p>
Detecting Solar-Like Oscillations in the Highest Mass TESS Giants
Authors: Downing, Noah, Howell, Madeline, Pinsonneault, Marc, García, Rafael A., PALAKKATHARAPPIL, DINIL BOSE, Borg, Lina, Mathur, Savita
Type: Presentation
Published: 2026-07-10

<p>Red-giant asteroseismology yields precise stellar parameters, making it a powerful tool for studying stellar structure and evolution, as demonstrated by the Kepler mission. However, due to Kepler’s limited field of view, it primarily sampled the more populous low-mass red giants found outside of the Galactic plane, leading to limited detections of intermediate-mass red giants (3 M⊙ ≲ M∗ ≲ 8 M⊙). Here we use the all-sky TESS data to isolate intermediate-mass stars from large catalogs with a pre-selection based on photometric and spectroscopic data. We optimize TESS light curves using a boutique light curve detrending method with custom apertures. Compared to the MIT Quick Look Pipeline, this yields a 12% average increase in the signal-to-noise ratio within the oscillation envelope, even in the heavily crowded Galactic plane. We find a total of 98 solar-like oscillators in a pre-selected sample of 227 APOGEE DR19 red giants. We find 43 stars in this sample to be intermediate-mass, with 10 stars having masses greater than 5 M⊙, among the highest-mass solar-like oscillators detected to date. From our detections, we measure that the APOGEE DR19 spectroscopic log g is systematically larger by, on average, 0.23 dex compared to the seismic log g. This offset is possibly due to the lack of intermediate-mass giants observed by Kepler, which was used to calibrate the spectroscopic log g in the APOGEE pipeline. Extending the same pre-selection criteria to TESS targets with Gaia XP spectroscopic parameters identifies up to 37,000 candidate intermediate-mass solar-like oscillators for follow-up and population studies. Because quiescent helium ignition, angular momentum transport, and internal mixing processes (e.g., convective boundary mixing and rotational mixing) differ substantially at intermediate mass, this sample enables new asteroseismic constraints on intermediate-mass stellar structure and evolution. These targets help bridge the gap between well-studied low-mass giants and the progenitors of massive stars that ultimately end as supernovae.</p>
Modeling strange mode Cepheids with MESA and RSP
Authors: Tarczay-Nehéz, Dóra
Type: Presentation
Published: 2026-07-09

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<p>Strange-mode pulsations in classical Cepheids are characterized as shallow, low-amplitude, short-period surface oscillations that develop when higher-overtone modes become trapped in the outer layers and are effectively decoupled from the stellar interior. Their excitation is found to be highly sensitive to the underlying stellar structure and confined to a narrow region of the mass–metallicity parameter space.</p>
<p>We computed a grid of stellar evolution models with MESA, and carried out linear stability calcu- lations using the MESA RSP module to map the conditions under which these modes may arise. This combined approach allowed the influence of convective overshoot, metallicity, and stellar mass on strange- mode excitation to be systematically explored. The resulting instability domains were placed on both the Hertzsprung–Russell diagram and the Gaia colour–magnitude diagram, where strange-mode pulsators occupy a distinct and isolated locus, clearly separated from classical Cepheids and other nearby variable classes.</p>
<p>Although the strange-mode phase is intrinsically brief, it can represent a non-negligible fraction of post-main-sequence evolution in regions where the ratio of strange-mode duration to instability-strip crossing time is enhanced. The predicted periods and amplitudes fall within the sensitivity range of current space-based photometry, indicating that strange-mode pulsators may already be detectable with TESS and, in the near future, with Gaia epoch photometry, despite challenges posed by blending and extinction.</p>
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An observed decoupling of stellar granulation timescales for dwarf stars
Authors: Lundkvist, Mia Sloth, Nielsen, Martin Bo, Davies, Guy, Zhou, Yixiao, Lund, Mikkel Nørup
Type: Presentation
Published: 2026-07-13

<p>Granulation is the surface manifestation of near-surface convection and forms the background signal upon which solar-like oscillations are observed. Yet, its observational properties on the main sequence remain comparatively underexplored relative to giants. This is a limitation, as accurate modelling of the granulation background is crucial for both asteroseismic inference and the mitigation of stellar variability in exoplanet detection. To bridge this gap, we present a characterisation of granulation in main-sequence and subgiant stars, establishing a continuous picture across evolutionary stages. We analysed 753 <em>Kepler</em> short-cadence targets using a Bayesian framework, testing multiple background prescriptions and quantifying model preference on a star-by-star basis, enabling robust assessment of systematic effects associated with background modelling. Notably, when turning to the parameters of the granulation signal itself, we found that while granulation amplitudes broadly follow established giant-based scalings, a deviation occurs for the timescale. For main-sequence stars cooler than the Sun, the granulation timescale becomes decoupled from the oscillation timescale. The observed decoupling is supported by 3D hydrodynamical simulations, where reduced convective velocities – arising from more efficient energy transport in denser envelopes and a lower luminosity – lead to longer granulation timescales. The immediate consequence in stellar power spectra is an increased separation between the granulation background and the oscillation envelope, affecting mode detectability on the lower main sequence. More broadly, we have shown that the typical scaling relations assumed for the granulation signal do not hold for dwarfs – an important detail when modelling detection probabilities in preparation for PLATO.</p>