Tootfinder

Study of $\tau\rightarrow e M^ M^-$ decays in the N-B-LSSM
Rong-Zhi Sun, Shu-Min Zhao, Shuang Di, Xing-Xing Dong
https://arxiv.org/abs/2507.01276 https://…

Study of $τ\rightarrow e M^+ M^-$ decays in the N-B-LSSM
Within the framework of the next to the minimal supersymmetric (SUSY) extension of the Standard Model (SM) with a local B-L gauge symmetry (N-B-LSSM), we study lepton flavor violating (LFV) $τ\rightarrow e M^+ M^-$ decays: $τ\rightarrow e π^+π^-$,~$τ\rightarrow e π^+K^-$,~$τ\rightarrow e K^+K^-$. According to the latest experimental data, the influence of different sensitive parameters on the branching ratios is considered. It can be seen from the numerical analysis that the main sensiti…

Picturesque convolution-like recurrences and partial sums' generation
Ignas Gasparavi\v{c}ius, Andrius Grigutis, Juozas Petkelis
https://arxiv.org/abs/2507.23619 https://

Picturesque convolution-like recurrences and partial sums' generation
Let ${\pmb b}=\{b_0,\,b_1,\,\ldots\}$ be the known sequence of numbers such that $b_0\neq0$. In this work, we develop methods to find another sequence ${\pmb a}=\{a_0,\,a_1,\,\ldots\}$ that is related to ${\pmb b}$ as follows: $a_n=a_0\,b_{n+m}+a_1\,b_{n+m-1}+\ldots+a_{n+m}\,b_0$, $n\in\mathbb{N}\cup\{0\}$, $m\in\mathbb{N}$. We show the connection of $\lim_{n\to\infty}a_n$ with $a_0,\,a_1,\,\ldots,\,a_{m-1}$ and provide varied examples of finding the sequence ${\pmb a}$ when ${\pmb b}$ is given…

Search for Magnetic Monopoles with the Complete ANTARES Dataset
A. Albert, S. Alves, M. Andr\'e, M. Ardid, S. Ardid, J. -J. Aubert, J. Aublin, B. Baret, S. Basa, Y. Becherini, B. Belhorma, F. Benfenati, V. Bertin, S. Biagi, J. Boumaaza, M. Bouta, M. C. Bouwhuis, H. Branzas, R. Bruijn, J. Brunner, J. Busto, B. Caiffi, D. Calvo, S. Campion, A. Capone, F. Carenini, J. Carr, V. Carretero, T. Cartraud, S. Celli, L. Cerisy, M. Chabab, R. Cherkaoui El Moursli, T. Chiarusi, M. Circella, J.…

Search for Magnetic Monopoles with the Complete ANTARES Dataset
This study presents a novel search for magnetic monopoles using data collected over a 14 year period (2008-2022) by the ANTARES neutrino telescope. The interaction of magnetic monopoles with matter was modeled according to Kazama, Yang, and Goldhaber cross-section. Upper limits on the flux of magnetic monopoles are obtained for velocities both above and below the Cherenkov threshold. No events consistent with the passage of magnetic monopoles were detected, enabling the setting of an upper flux…

Orbit and atmosphere of HIP 99770 b through the eyes of VLTI/GRAVITY
T. O. Winterhalder, J. Kammerer, S. Lacour, A. M\'erand, M. Nowak, T. Stolker, W. O. Balmer, G. -D. Marleau, R. Abuter, A. Amorim, R. Asensio-Torres, J. -P. Berger, H. Beust, S. Blunt, M. Bonnefoy, H. Bonnet, M. S. Bordoni, G. Bourdarot, W. Brandner, F. Cantalloube, P. Caselli, B. Charnay, G. Chauvin, A. Chavez, E. Choquet, V. Christiaens, Y. Cl\'enet, V. Coud\'e du Foresto, A. Cridland, R. Davies, R. Demb…

Orbit and atmosphere of HIP 99770 b through the eyes of VLTI/GRAVITY
Context: Inferring the likely formation channel of giant exoplanets and brown dwarf companions from orbital and atmospheric observables remains a formidable challenge. Further and more precise directly measured dynamical masses of these companions are required to inform and gauge formation, evolutionary, and atmospheric models. We present an updated study of HIP 99770 b based on observations conducted with VLTI/GRAVITY. Aims: Combining the new data with previous observations from the literature…

#FuckEricAdams so so much. And fuck Hochul for not removing him. #BikeNYC
https://hellgateny…

Series B, Episode 05 - Pressure Point
BLAKE: I'd rather not try. But if I have to, I will not be alone. I've already contacted a Resistance leader.
[Wooded area near the Forbidden Zone]
VERON: No sign of them?
https://blake.torpidity.net/m/205/62 B7B6

Blakes7Bot | Search
Companion site to the Blakes7Bot Twitter, Mastodon, and Bluesky accounts. Automated lines of Blakes 7 dialog. Includes a script search facility.

Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
M. Archipley, A. Hryciuk, L. E. Bleem, K. Kornoelje, M. Klein, A. J. Anderson, B. Ansarinejad, M. Aravena, L. Balkenhol, P. S. Barry, K. Benabed, A. N. Bender, B. A. Benson, F. Bianchini, S. Bocquet, F. R. Bouchet, E. Camphuis, M. G. Campitiello, J. E. Carlstrom, J. Cathey, C. L. Chang, S. C. Chapman, P. Chaubal, P. M. Chichura, A. Chokshi, T. -L. Chou…

Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
Context. The South Pole Telescope third-generation camera (SPT-3G) has observed over 10,000 square degrees of sky at 95, 150, and 220 GHz (3.3, 2.0, 1.4 mm, respectively) overlapping the ongoing 14,000 square-degree Euclid Wide Survey. The Euclid collaboration recently released Euclid Deep Field observations in the first quick data release (Q1). Aims. With the goal of releasing complementary millimeter-wave data and encouraging legacy science, we performed dedicated observations of a 57-square-…

Full Stokes magnetometry of the active M dwarfs AU Mic and EV Lac with SPIRou
J. -F. Donati, P. I. Cristofari, B. Klein, B. Finociety, C. Moutou
https://arxiv.org/abs/2507.01754

Full Stokes magnetometry of the active M dwarfs AU Mic and EV Lac with SPIRou
We report in this paper circularly and linearly polarized observations of the young active M dwarfs AU Mic and EV Lac with the near-infrared SPIRou spectropolarimeter at the Canada-France-Hawaii Telescope, collected from August to October 2023 over a few rotation cycles of both stars. Applying Least-Squares Deconvolution (LSD) to our spectra, we detected Zeeman signatures in circular (Stokes V) and linear (Stokes QU) polarization, and Zeeman broadening in unpolarized (Stokes I) LSD profiles, al…

SPT-3G D1: Axion Early Dark Energy with CMB experiments and DESI
A. R. Khalife, L. Balkenhol, E. Camphuis, A. J. Anderson, B. Ansarinejad, M. Archipley, P. S. Barry, K. Benabed, A. N. Bender, B. A. Benson, F. Bianchini, L. E. Bleem, F. R. Bouchet, L. Bryant, M. G. Campitiello, J. E. Carlstrom, C. L. Chang, P. Chaubal, P. M. Chichura, A. Chokshi, T. L. Chou, A. Coerver, T. M. Crawford, C. Daley, T. de Haan, K. R. Dibert, M. A. Dobbs, M. Doohan, A. Doussot, D. Dutcher, W. Everett, C. Fen…

SPT-3G D1: Axion Early Dark Energy with CMB experiments and DESI
We present the most up-to-date constraints on axion early dark energy (AEDE) from cosmic microwave background (CMB) and baryon acoustic oscillation (BAO) measurements. In particular, we assess the impact of data from ground-based CMB experiments, the South Pole Telescope (SPT) and the Atacama Cosmology Telescope (ACT) -- both with and without $Planck$ -- on constraints on AEDE. We also highlight the impact that BAO information from the Dark Energy Spectroscopic Instrument (DESI) has on these co…

Series B, Episode 05 - Pressure Point
JENNA: It's over an hour since our last contact.
CALLY: It can't be a communicator fault.
JENNA: Not on all four bracelets, no.
CALLY: What do you think has happened?
JENNA: They've run into trouble.
https://blake.torpidity.net/m/205/407

Blakes7Bot | Search
Companion site to the Blakes7Bot Twitter, Mastodon, and Bluesky accounts. Automated lines of Blakes 7 dialog. Includes a script search facility.

Rapid yet accurate Tile-circuit and device modeling for Analog In-Memory Computing
J. Luquin, C. Mackin, S. Ambrogio, A. Chen, F. Baldi, G. Miralles, M. J. Rasch, J. B\"uchel, M. Lalwani, W. Ponghiran, P. Solomon, H. Tsai, G. W. Burr, P. Narayanan
https://arxiv.org/abs/2506.00004

Rapid yet accurate Tile-circuit and device modeling for Analog In-Memory Computing
Analog In-Memory Compute (AIMC) can improve the energy efficiency of Deep Learning by orders of magnitude. Yet analog-domain device and circuit non-idealities -- within the analog ``Tiles'' performing Matrix-Vector Multiply (MVM) operations -- can degrade neural-network task accuracy. We quantify the impact of low-level distortions and noise, and develop a mathematical model for Multiply-ACcumulate (MAC) operations mapped to analog tiles. Instantaneous-current IR-drop (the most significant circ…

This https://arxiv.org/abs/2503.10025 has been replaced.
initial toot: https://mastoxiv.page/@ar…

A Demonstration of Slowed Electron ${\bf E} \times {\bf B}$ Drift for PTOLEMY
To resolve the effective neutrino mass $m_β$ with an energy resolution of 50 meV, the PTOLEMY experiment has proposed a novel transverse electromagnetic filtering process. Perniciously reducing the kinetic energy of tritium $β$-decay electrons by counteracting motion from ${\bf E}$ $\times$ ${\bf B}$ and $\nabla{\rm B}$ drift, the PTOLEMY filter requires an input of emitted electron kinematic information to generate a tailored, suitable electric field for each endpoint candidate. The collabor…

Resonant interlayer coupling in NbSe$_2$-graphite epitaxial moir{\'e} superlattices
S. Mo, K. Kovalenka, S. Buchberger, B. K. Saika, A. Azhar, A. Rajan, A. Zivanovic, Y. -C. Yao, R. V. Belosludov, M. D. Watson, M. S. Bahramy, P. D. C. King
https://arxiv.org/abs/2506.00449

Resonant interlayer coupling in NbSe$_2$-graphite epitaxial moir{é} superlattices
Moir{é} heterostructures, created by stacking two-dimensional (2D) materials together with a finite lattice mismatch or rotational twist, represent a new frontier of designer quantum materials. Typically, however, this requires the painstaking manual assembly of heterostructures formed from exfoliated materials. Here, we observe clear spectroscopic signatures of moir{é} lattice formation in epitaxial heterostructures of monolayer (ML) NbSe$_2$ grown on graphite substrates. Our angle-resolved …

The Soviet way with words 😂
(from https://en.m.wikipedia.org/wiki/Trofim_Lysenko)

Trofim Lysenko - Wikipedia

Distribution of Farey fractions with $k$-free denominators
Bittu Chahal, Tapas Chatterjee, Sneha Chaubey
https://arxiv.org/abs/2507.00228 https://

Distribution of Farey fractions with $k$-free denominators
We study the global and local distribution of Farey fractions with $k$-free denominators in residue classes defined as \[\mathscr{F}_{Q,k}^{(m)}:=\left\{\frac{a}{q}\ |\ 1\leq a\leq q\leq Q,\ \gcd(a,q)=1,\ q\ \text{is}\ k\text{-free}\ \&\ q\equiv b\pmod{m} \right\}.\] We show that $\left(\mathscr{F}_{Q,k}^{(m)}\right)_{Q\ge 1}$ is equidistributed modulo one, and prove analogues of the classical results of Franel, Landau, and Niederreiter for $\left(\mathscr{F}_{Q,k}^{(m)}\right)_{Q\ge 1}$, …

Structure studies of 257Db through combined {\alpha}, {\gamma} and internal-conversion-electron spectroscopy
P. Brionnet, A. Lopez-Martens, O. Dorvaux, Z. Asfari, M. L. Chelnokov, V. I. Chepigin, H. Faure, B. Gall, K. Hauschild, A. V. Isaev, I. N. Izosimov, A. A. Kuznetsova, O. N. Malyshev, R. S Mukhin, J. Piot, A. G. Popeko, Y. A. Popov, K. Rezynkina, B. Sailaubekov, E. A. Sokol, A. I. Svirikhin, M. S. Tezekbayeva, A. V. Yeremin, N. I. Zamyatin

Structure studies of 257Db through combined α, γ and internal-conversion-electron spectroscopy
This work reports on the study of the decay properties along the $^{257}$Db decay chain using the GABRIELA setup. The first observation of a high-K isomer in $^{257}$Db is presented. In addition, an unreported $α$-decay branch in $^{249}$Md has been evidenced, allowing to constrain the differences in energy of the $α$-decaying levels in $^{249}$Md, $^{253}$Lr and $^{257}$Db. Finally, the combination of the observed fine structure $α$-decay from the high-spin state in $^{257}$Db with the firs…

Improved belief propagation is sufficient for real-time decoding of quantum memory
Tristan M\"uller, Thomas Alexander, Michael E. Beverland, Markus B\"uhler, Blake R. Johnson, Thilo Maurer, Drew Vandeth
https://arxiv.org/abs/2506.01779

Improved belief propagation is sufficient for real-time decoding of quantum memory
We introduce a new heuristic decoder, Relay-BP, targeting real-time quantum circuit decoding for large-scale quantum computers. Relay-BP achieves high accuracy across circuit-noise decoding problems: significantly outperforming BP+OSD+CS-10 for bivariate-bicycle codes and comparable to min-weight-matching for surface codes. As a lightweight message-passing decoder, Relay-BP is inherently parallel, enabling rapid low-footprint decoding with FPGA or ASIC real-time implementations, similar to stan…

On the Visibility Polynomial of Graphs
Tonny K B, Shikhi M
https://arxiv.org/abs/2507.01851 https://arxiv.org/pdf/2507.01851

On the Visibility Polynomial of Graphs
Let G(V,E) be a simple graph and let X subset of V. Two vertices u and v are said to be X-visible if there exists a shortest u,v-path P such that V(P) intersection X is a subset of {u, v}. A set X is called a mutual-visibility set of G if every pair of vertices in X are X-visible. The visibility polynomial of a graph G is defined as nu (G)=sum_{i >= 0} r_i x^i, where r_i denotes the number of mutual-visibility sets in G of cardinality i. In the present paper, the visibility polynomial is studie…

Measurement of charged-current muon neutrino-argon interactions without pions in the final state using the MicroBooNE detector
MicroBooNE collaboration, P. Abratenko, D. Andrade Aldana, L. Arellano, J. Asaadi, A. Ashkenazi, S. Balasubramanian, B. Baller, A. Barnard, G. Barr, D. Barrow, J. Barrow, V. Basque, J. Bateman, O. Benevides Rodrigues, S. Berkman, A. Bhat, M. Bhattacharya, M. Bishai, A. Blake, B. Bogart, T. Bolton, M. B. Brunetti, L. Camilleri, D. Caratelli, F. Cavanna, G. Cerat…

Measurement of charged-current muon neutrino-argon interactions without pions in the final state using the MicroBooNE detector
We report a new measurement of flux-integrated differential cross sections for charged-current (CC) muon neutrino interactions with argon nuclei that produce no final state pions $(ν_μ\mathrm{CC}0π)$. These interactions are of particular importance as a topologically defined signal dominated by quasielastic-like interactions. This measurement was performed with the MicroBooNE liquid argon time projection chamber detector located at the Fermilab Booster Neutrino Beam (BNB), and uses an exposu…

High-Precision Quantum Dynamics of He$_2$ b $^3\Pi_\mathrm{g}$-c $^3\Sigma_\mathrm{g}^ $ including Non-adiabatic, Relativistic and QED Corrections and Couplings
Bal\'azs R\'acsai, P\'eter Jeszenszki, \'Ad\'am Marg\'ocsy, Edit M\'atyus
https://arxiv.org/abs/2506.23879

High-Precision Quantum Dynamics of He$_2$ b $^3Π_\mathrm{g}$-c $^3Σ_\mathrm{g}^+$ including Non-adiabatic, Relativistic and QED Corrections and Couplings
Relativistic, quantum electrodynamics, as well as non-adiabatic corrections and couplings, are computed for the b $^3Π_\mathrm{g}$ and c $^3Σ_\mathrm{g}^+$ electronic states of the helium dimer. The underlying Born-Oppenheimer potential energy curves are converged to 1 ppm ($1:10^6$) relative precision using a variational explicitly correlated Gaussian approach. % The quantum nuclear motion is computed over the b $^3Π_\mathrm{g}$-c $^3Σ_\mathrm{g}^+$ (and B $^1Π_\mathrm{g}$-C $^1Σ_\mathrm…

Every week sr. management reviews a slide I update. For months I have been warning (on that slide) that proj-A and proj-B, both due roughly the same time will conflict, I can only do 1 at a time, and no one has told me whether A or B is more important so I'm starting with A, B will start after A.
mgmnt just now: zOMG why are you working on A, B is super critical!?
<sigh> I've already started A. I'm deep into A, up to my eyeballs.
Fine, but context switch…

Simulation-based inference for Precision Neutrino Physics through Neural Monte Carlo tuning
A. Gavrikov, A. Serafini, D. Dolzhikov, A. Garfagnini, M. Gonchar, M. Grassi, R. Brugnera, V. Cerrone, L. V. D'Auria, R. M. Guizzetti, L. Lastrucci, G. Andronico, V. Antonelli, A. Barresi, D. Basilico, M. Beretta, A. Bergnoli, M. Borghesi, A. Brigatti, R. Bruno, A. Budano, B. Caccianiga, A. Cammi, R. Caruso, D. Chiesa, C. Clementi, C. Coletta, S. Dusini, A. Fabbri, G. Felici, G. Ferrante, M.…

Simulation-based inference for Precision Neutrino Physics through Neural Monte Carlo tuning
Precise modeling of detector energy response is crucial for next-generation neutrino experiments which present computational challenges due to lack of analytical likelihoods. We propose a solution using neural likelihood estimation within the simulation-based inference framework. We develop two complementary neural density estimators that model likelihoods of calibration data: conditional normalizing flows and a transformer-based regressor. We adopt JUNO - a large neutrino experiment - as a cas…

Isospin-violating vacuum polarization in the muon $(g-2)$ with SU(3) flavour symmetry from lattice QCD
Dominik Erb, Antoine G\'erardin, Harvey B. Meyer, Julian Parrino, Volodymyr Biloshytskyi, Vladimir Pascalutsa
https://arxiv.org/abs/2505.24344

Isospin-violating vacuum polarization in the muon $(g-2)$ with SU(3) flavour symmetry from lattice QCD
We compute the isospin-violating part $a_μ^{\text{HVP}, 38}$ of the hadronic-vacuum-polarization (HVP) contribution to the muon $(g-2)$ in lattice QCD at the SU$(3)_{\rm f}$-symmetric point where $M_π=M_K\simeq 416$ MeV. All diagrams involving internal photons are evaluated in coordinate space, employing a Pauli-Villars-regulated photon propagator with a cutoff scale $Λ$ well below the lattice cutoff. The counterterm $(m_u-m_d)$, whose $Λ$ dependence follows the expected logarithmic behavio…

$g$ Factor of Boron-like Tin
J. Morgner (Max-Planck-Institut f\"ur Kernphysik, Heidelberg, Germany), B. Tu (Max-Planck-Institut f\"ur Kernphysik, Heidelberg, Germany, Shanghai EBIT laboratory, Institute of Modern Physics, Fudan University, Shanghai, China), M. Moretti (Max-Planck-Institut f\"ur Kernphysik, Heidelberg, Germany), C. M. K\"onig (Max-Planck-Institut f\"ur Kernphysik, Heidelberg, Germany), F. Hei{\ss}e (Max-Planck-Institut f\"ur Kernphysik, Hei…

Series B, Episode 12 - The Keeper
FOOL: Let us out. [Blake unlocks his door, then the old man's. He is lying on his bed.]
BLAKE: Who is the keeper?
FOOL: Leave him - let my master die in peace.
BLAKE: Who is the keeper?
https://blake.torpidity.net/m/212/511 B7B5

Lie algebras generated by reflections in types BCD
Christopher M. Drupieski, Jonathan R. Kujawa
https://arxiv.org/abs/2506.01198 https://

Lie algebras generated by reflections in types BCD
We consider the group algebra over the field of complex numbers of the Weyl group of type B (the hyperoctahedral group, or the group of signed permutations) and of the Weyl group of type D (the demihyperoctahedral group, or the group of even-signed permutations), viewed as Lie algebras via the commutator bracket, and determine the structure of the Lie subalgebras generated by the sets of reflections.

Error Estimates for the Arnoldi Approximation of a Matrix Square Root
James H. Adler, Xiaozhe Hu, Wenxiao Pan, Zhongqin Xue
https://arxiv.org/abs/2506.22615

Error Estimates for the Arnoldi Approximation of a Matrix Square Root
The Arnoldi process provides an efficient framework for approximating functions of a matrix applied to a vector, i.e., of the form $f(M)\mathbf{b}$, by repeated matrix-vector multiplications. In this paper, we derive an \textit{a priori} error estimate for approximating the action of a matrix square root using the Arnoldi process, where the integral representation of the error is reformulated in terms of the error for solving the linear system $M\mathbf{x}=\mathbf{b}$. The results extend the er…

A Precise Metallicity and Carbon-to-Oxygen Ratio for a Warm Giant Exoplanet from its Panchromatic JWST Emission Spectrum
Lindsey S. Wiser, Taylor J. Bell, Michael R. Line, Everett Schlawin, Thomas G. Beatty, Luis Welbanks, Thomas P. Greene, Vivien Parmentier, Matthew M. Murphy, Jonathan J. Fortney, Kenny Arnold, Nishil Mehta, Kazumasa Ohno, Sagnick Mukherjee

A Precise Metallicity and Carbon-to-Oxygen Ratio for a Warm Giant Exoplanet from its Panchromatic JWST Emission Spectrum
WASP-80 b, a warm sub-Jovian (equilibrium temperature ~820 K, 0.5 Jupiter masses), presents an opportunity to characterize a rare gas giant exoplanet around a low-mass star. In addition, its moderate temperature enables its atmosphere to host a range of carbon and oxygen species (H$_2$O, CH$_4$, CO, CO$_2$, NH$_3$). In this paper, we present a panchromatic emission spectrum of WASP-80 b, the first gas giant around a late K/early M-dwarf star and the coolest planet for which the James Webb Space…

DESI DR2 reference mocks: clustering results from Uchuu-BGS and LRG
E. Fern\'andez-Garc\'ia, F. Prada, A. Smith, J. DeRose, A. J. Ross, S. Bailey, M. S. Wang, Z. Ding, C. Guandalin, C. Lamman, R. Vaisakh, R. Kehoe, J. Lasker, T. Ishiyama, S. M. Moore, S. Cole, M. Siudek, A. Amalbert, A. Salcedo, A. Hearin, B. Joachimi, A. Rocher, S. Saito, A. Krolewski, Z. Slepian, Q. Li, K. S. Dawson, E. Jullo, J. Aguilar, S. Ahlen, D. Bianchi, D. Brooks, T. Claybaugh, A. de la Macorra, P. Doe…

DESI DR2 reference mocks: clustering results from Uchuu-BGS and LRG
The aim of this work is to construct mock galaxy catalogues that accurately reproduce the redshift evolution of galaxy number density, clustering statistics, and baryonic properties, such as stellar mass for luminous red galaxies (LRGs) and absolute magnitude in the $r$-band for the bright galaxy sample (BGS), based on the first three years of observations from the Dark Energy Spectroscopic Instrument (DESI). To achieve this, we applied the subhalo abundance matching (SHAM) technique to the Uch…

Optimising Photothermal Silver Nanoparticles for Efficient Light-Activated Shape Memory Response in AgNP-Polymer Composites
K. Krizmane, M. Dile, E. Einbergs, V. Vitola, A. Knoks, B. Hamawandi, A. Zolotarjovs
https://arxiv.org/abs/2507.00620

Optimising Photothermal Silver Nanoparticles for Efficient Light-Activated Shape Memory Response in AgNP-Polymer Composites
The study presents the synthesis and integration of silver nanoparticles (AgNPs) into a polyurethane (PU) matrix to create a light-activated shape memory polymer (SMP). AgNPs were synthesized using a microwave-assisted solvothermal method with polyvinylpyrrolidone (PVP) as a stabilizer, where varying the molecular weight of PVP and the AgNO3/PVP ratio influenced nanoparticle size and distribution. Characterisation via scanning electron microscopy (SEM) and dynamic light scattering (DLS) confirm…

JWST Observations of SN 2023ixf I: Completing the Early Multi-Wavelength Picture with Plateau-phase Spectroscopy
J. M. DerKacy, C. Ashall, E. Baron, K. Medler, T. Mera, P. Hoeflich, M. Shahbandeh, C. R. Burns, M. D. Stritzinger, M. A. Tucker, B. J. Shappee, K. Auchettl, C. R. Angus, D. D. Desai, A. Do, J. T. Hinkle, W. B. Hoogendam, M. E. Huber, A. V. Payne, D. O. Jones, J. Shi, M. Y. Kong, S. Romagnoli, A. Syncatto, S. Moran, E. Fereidouni, P. J. Brown, M. Engesser, O. D. Fox, L. Galb…

JWST Observations of SN 2023ixf I: Completing the Early Multi-Wavelength Picture with Plateau-phase Spectroscopy
We present and analyze panchromatic (0.35-14 $μ$m) spectroscopy of the Type II supernova 2023ixf, including near- and mid-infrared spectra obtained 33.6 days after explosion during the plateau-phase, with the James Webb Space Telescope (JWST). This is the first in a series of papers examining the evolution of SN 2023ixf with JWST spanning the initial 1000 days after explosion, monitoring the formation and growth of molecules and dust in ejecta and surrounding environment. The JWST infrared spe…

Benchmark brown dwarfs -- I. A blue M2 T5 wide binary and a probable young M4 [T7 T8] hierarchical triple
Z. H. Zhang, F. Navarete, M. C. G\'alvez-Ortiz, H. R. A. Jones, A. J. Burgasser, P. Cruz, F. Marocco, N. Lodieu, Y. Shan, B. Gauza, R. Raddi, M. R. Huang, R. L. Smart, S. Baig, G. Cheng, D. J. Pinfield
https://arxi…

Benchmark brown dwarfs -- I. A blue M2 + T5 wide binary and a probable young M4 + [T7 + T8] hierarchical triple
Benchmark brown dwarfs in wide binary systems are crucial for characterizing substellar objects and calibrating atmospheric and evolutionary models. However, brown dwarf benchmarks with subsolar metallicity, very cool temperatures, or suitability for dynamical mass measurements are rare, limiting our understanding across the full range of mass, age, and metallicity. We present the discovery of two new multiple systems containing T dwarf companions, identified through a targeted search using Cat…

Surface waves and axoplasmic pressure waves in action potential propagation: fundamentally different physics or two sides of the same coin?
Marat M. Rvachev, Benjamin Drukarch
https://arxiv.org/abs/2505.24580

Surface waves and axoplasmic pressure waves in action potential propagation: fundamentally different physics or two sides of the same coin?
We argue that El Hady and Machta's "surface wave" model describes the same underlying process as the "axoplasmic pressure wave" model introduced earlier by Rvachev. Note. We, the authors, contacted A. El Hady and B. Machta for comment on the ideas presented herein. They suggested that we "submit a Matters Arising Letter to Nature Communications and we will be asked to respond in due time." Nature Communications ultimately rejected the manuscript, citing: "... Our main criterion for consider…

Versatile multi-q antiferromagnetic charge order in correlated vdW metals
Y. Fujisawa, P. Wu, R. Okuma, B. R. M. Smith, D. Ueta, R. Kobayashi, N. Maekawa, T. Nakamura, C-H. Hsu, Chandan De, N. Tomoda, T. Higashihara, K. Morishita, T. Kato, Z. Y. Wang, Y. Okada
https://arxiv.org/abs/2507.00750

Versatile multi-q antiferromagnetic charge order in correlated vdW metals
Following the discovery of graphene, interest in van der Waals (vdW) materials has surged; yet, advancing "beyond graphene" physics requires the development of quantum material platforms that host versatile many-body states. Using scanning tunneling microscopy and spectroscopy at 300 mK, we uncover two competing states in vdW metal CeTe3: charge-ordered in-plane antiferromagnetic phases forming stripe and checkerboard patterns. Remarkably, the competition between them is tuned through a modest …

Search for decays of the Higgs boson into scalar particles decaying into four or six $b$-quarks using $pp$ collisions at $\sqrt{s}= 13\,\mathrm{TeV}$ with the ATLAS detector
ATLAS Collaboration
https://arxiv.org/abs/2507.01165

Search for decays of the Higgs boson into scalar particles decaying into four or six $b$-quarks using $pp$ collisions at $\sqrt{s}= 13\,\mathrm{TeV}$ with the ATLAS detector
A search for exotic decays of the Higgs boson $H$ into new scalar or pseudoscalar particles that subsequently decay into $b$-quarks is presented. The search considers $ZH$ production with several decay scenarios for the Higgs boson: first to a pair of identical scalars, $H\rightarrow 2a \rightarrow 4b$, second to a pair of scalars with different masses ($m_{a1}

Structural, dielectric, and ferroelectric characteristics of the low-temperature sintered 65PMN-35PT sample for electroceramic applications
B. Ramachandran, N. Sudarshan, G. Mangamma, M. S. Ramachandra Rao
https://arxiv.org/abs/2507.00614

Structural, dielectric, and ferroelectric characteristics of the low-temperature sintered 65PMN-35PT sample for electroceramic applications
A single-phase 65PMN-35PT ceramic was synthesized at a relatively low temperature (875 oC) using a modified columbite method. X-ray diffraction analysis confirmed the single-phase formation of perovskite 65PMN-35PT with a tetragonal structure. Morphological studies indicated that the sample consisted of small grains with a size of about 2 micro-m. The dielectric properties of the material demonstrate its relaxor behavior near the ferroelectric transition temperature, TC = 457 K. The saturation …

Series B, Episode 13 - Star One
ORAC: Each of which performs a dual function; namely, to indicate the approach of an intruder and then to destroy that intruder by a powerful anti-matter implosion.
JENNA: So it's a combined alarm system and minefield.
https://blake.torpidity.net/m/213/338

Axial-vector molecular structures $B_{c}^{\ast \pm} B_{c}^{\mp}$
S. S. Agaev, K. Azizi, H. Sundu
https://arxiv.org/abs/2507.18735 https://arxiv.org/pdf/250…

Axial-vector molecular structures $B_{c}^{\ast \pm} B_{c}^{\mp}$
The axial-vector molecular structure $\mathcal{M}_{\mathrm{AV}}=(B_{c}^{\ast +}B_{c}^{-} + B_{c}^{\ast - } B_{c}^{+})/2$ is explored in QCD sum rule framework. The mass and current coupling of this compound are found by means of the two-point sum rule method. It turns out that the mass of $\mathcal{M} _{\mathrm{AV}}$ is equal to $m=(12770 \pm 60)~\mathrm{MeV}$ making possible its dissociations to pairs of $J/ψη_b$, $Υη_c$, $ B_{c}^{\ast +} B_{c}^{-}$, and $B_{c}^{\ast - } B_{c}^{+}$ mesons.…

Universal Effective Charges in the $sd$ and $fp$ Shells
T. H. Ogunbeku, J. M. Allmond, T. J. Gray, W. -J. Ong, B. A. Brown, A. Gargano, R. Grzywacz, J. D. Holt, A. O. Macchiavelli, T. Miyagi, S. Neupane, B. C. Rasco, H. Schatz, B. M. Sherrill, O. B. Tarasov, H. Arora, A. D. Ayangeakaa, H. C. Berg, J. M. Berkman, D. L. Bleuel, K. Bosmpotinis, M. P. Carpenter, G. Cerizza, A. Chester, J. M. Christie, I. Cox, H. L. Crawford, B. P. Crider, J. Davis, A. A. Doetsch, J. G. Duarte, A. Estrade, …

Universal Effective Charges in the $sd$ and $fp$ Shells
The 247-keV state in $^{54}$Sc, populated in the $β$ decay of $^{54}$Ca, is reported here as a nanosecond isomer with a half-life of 26.0(22) ns. The state is interpreted as the $1^+$ member of the $πf_{7/2}\otimesνf_{5/2}$ spin-coupled multiplet, which decays to the $3^+,πf_{7/2} \otimes νp_{1/2}$ ground state. The new half-life corresponds to a pure $E2$ transition with a strength of 1.93(16) W.u., providing the most precise, unambiguous $B(E2)$ value in the neutron-rich $fp$ region to d…

The real-time data processing and acquisition system for Project 8 Phase II
A. Ashtari Esfahani, A. Banducci, S. B\"oser, N. Buzinsky, R. Cervantes, C. Claessens, L. de Viveiros, M. Fertl, J. A. Formaggio, L. Gladstone, M. Grando, M. Guigue, J. Hartse, K. M. Heeger, A. M. Jones, K. Kazkaz, B. H. LaRoque, A. Lindman, B. Monreal, J. A. Nikkel, E. Novitski, N. S. Oblath, W. Pettus, R. G. H. Robertson, G. Rybka, L. Salda\~na, P. L. Slocum, Y. -H. Sun, P. T. Surukuchi, A. B. Telles, F.…

The real-time data processing and acquisition system for Project 8 Phase II
In Phase II of the Project 8 neutrino mass experiment, electrons from the decays of tritium or ${}^{83\mathrm{m}}$Kr are detected via their $\approx$26 GHz cyclotron radiation while contained within a circular waveguide. The signal from a given electron is characterized as a brief chirp, lasting $\lesssim$10 ms and changing in frequency by $\lesssim$1 MHz/ms. To detect these signals, the Project 8 collaboration developed a data acquisition (DAQ) system tailored to the signal properties. The DAQ…

Recent advances in arrow relations and traces of sets
Mingze Li, Jie Ma, Mingyuan Rong
https://arxiv.org/abs/2507.23375 https://arxiv.org/pdf/2507.23375

Recent advances in arrow relations and traces of sets
The arrow relation, a central concept in extremal set theory, captures quantitative relationships between families of sets and their traces. Formally, the arrow relation $(n, m) \rightarrow (a, b)$ signifies that for any family $\mathcal{F} \subseteq 2^{[n]}$ with $|\mathcal{F}| \geqslant m$, there exists an $a$-element subset $T \subseteq [n]$ such that the trace $\mathcal{F}_{|T} = \{ F \cap T : F \in \mathcal{F} \}$ contains at least $b$ distinct sets. This survey highlights r…

The Hot Neptune Initiative (HONEI) II. TOI-5795 b: A hot super-Neptune orbiting a metal-poor star
F. Manni, L. Naponiello, L. Mancini, S. Vissapragada, K. Biazzo, A. S. Bonomo, D. Polychroni, D. Turrini, D. Locci, A. Maggio, V. D Orazi, M. Damasso, C. Briceno, D. R. Ciardi, C. A. Clark, K. A. Collins, D. W. Latham, N. Law, M. Lopez-Morales, M. B. Lund, L. Malavolta, A. W. Mann, G. Mantovan, D. Nardiello, M. Pinamonti, D. J. Radford, R. P. Schwarz, A. Shporer, A. Sozzetti, C. N., Watki…

The Hot Neptune Initiative (HONEI) II. TOI-5795 b: A hot super-Neptune orbiting a metal-poor star
The formation of Neptune planets with orbital periods less than 10\,days remains uncertain. They might have developed similarly to longer-period counterparts, emerged from rare collisions between smaller planets, or could be the remnant cores of stripped giant planets. Characterizing a large number of them is important to advance our understanding of how they form and evolve. We aimed at confirming the planetary nature and characterizing the properties of a close-in Neptune-type transiting exop…

Series B, Episode 03 - Weapon
ORAC: No. It was a priority one - for automatic relay to the senior officer present.
BLAKE: Orac, I want more information. I want to know everything there is to know about this man Coser; I want to know how he got out of the base; and I want to know what IMIPAK is.
https://blake.torpidi…

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LiteBIRD Science Goals and Forecasts: Improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
M. Ruiz-Granda, P. Diego-Palazuelos, C. Gimeno-Amo, P. Vielva, A. I. Lonappan, T. Namikawa, R. T. G\'enova-Santos, M. Lembo, R. Nagata, M. Remazeilles, D. Adak, E. Allys, A. Anand, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, R. B. Barreiro, N. Bartolo, S. Basak, M. Bersanelli, A. Besnard, D. Blinov, M. Bortolam…

LiteBIRD Science Goals and Forecasts: Improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
Cosmic microwave background (CMB) photons are deflected by large-scale structure through gravitational lensing. This secondary effect introduces higher-order correlations in CMB anisotropies, which are used to reconstruct lensing deflections. This allows mapping of the integrated matter distribution along the line of sight, probing the growth of structure, and recovering an undistorted view of the last-scattering surface. Gravitational lensing has been measured by previous CMB experiments, with…

lol I'm gonna need an emoji of this or something
https://bsky.app/profile/truebluemajority.bsky.social/post/3lvc7muokqk2w

TrueBlueMajority (@truebluemajority.bsky.social)
ask and ye shall receive

Analysis of Forbidden Neon Emission lines in HAeBe Stars using Spitzer IRS spectra
D. Akhila, Blesson Mathew, S. Nidhi, B. Shridharan, R. Arun, Hema Anilkumar, G. Maheswar, Sreeja S. Kartha, P. Manoj, Suman Bhattacharyya
https://arxiv.org/abs/2506.01036

Analysis of Forbidden Neon Emission lines in HAeBe Stars using Spitzer IRS spectra
We analyzed high-resolution mid-infrared spectra of 78 well-known Herbig Ae/Be (HAeBe) stars using Spitzer InfraRed Spectrograph data, focusing on the detection of [Ne {\sc II}] and [Ne {\sc III}] emission lines as indicators of ionized outflows or disk winds. Emission from [Ne {\sc II}] at 12.81 $μ$m or [Ne {\sc III}] at 15.55 $μ$m was identified in 25 sources, constituting the largest sample of HAeBe stars with these detected lines. Our analysis revealed a higher detection frequency of [Ne …

Characterization of spurious-electron signals in the double-phase argon TPC of the DarkSide-50 experiment
50 Collaboration, P. Agnes, I. F. Albuquerque, T. Alexander, A. K. Alton, M. Ave, H. O. Back, G. Batignani, E. Berzin, K. Biery, V. Bocci, W. M. Bonivento, B. Bottino, S. Bussino, M. Cadeddu, M. Cadoni, F. Calaprice, A. Caminata, M. D. Campos, N. Canci, M. Caravati, N. Cargioli, M. Cariello, M. Carlini, V. Cataudella, P. Cavalcante, S. Cavuoti, S. Chashin, A. Chepurnov, C. Cical\`o…

Characterization of spurious-electron signals in the double-phase argon TPC of the DarkSide-50 experiment
Spurious-electron signals in dual-phase noble-liquid time projection chambers have been observed in both xenon and argon Time Projection Chambers (TPCs). This paper presents the first comprehensive study of spurious electrons in argon, using data collected by the DarkSide-50 experiment at the INFN Laboratori Nazionali del Gran Sasso (LNGS). Understanding these events is a key factor in improving the sensitivity of low-mass dark matter searches exploiting ionization signals in dual-phase noble l…

H${\beta}$ line shape and radius-luminosity relation in 2.5D FRADO
M. H. Naddaf, M. L. Martinez-Aldama, D. Hutsemekers, D. Savic, B. Czerny
https://arxiv.org/abs/2506.01159

H$β$ line shape and radius-luminosity relation in 2.5D FRADO
Galaxies with active galactic nuclei (AGN) exhibit broad emission lines as a key spectral feature. The shape of emission-line profiles depends on the complex dynamics of discrete clouds within a spatially extended region known as the Broad Line Region (BLR). The distribution of cloud positions within BLR, or the geometry of BLR indeed, is directly linked to measurements of time lags of BLR. In this paper, we convolve a large grid of physically-based simulations of cloud distributions in BLR wit…

Series B, Episode 05 - Pressure Point
AVON: If I can fire at ground level, the beam radiation should be great enough to cut a narrow channel through the sensor mesh. That would give you eight seconds to get from here to the blockhouse. The mesh would start its repair cycle instantly. Take one step off the channel and you're dead. I know it's a slim chance, but it's the best I can come up with.
BLAKE: Let's try it.

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Identical Vanishing of Coefficients in the Series Expansion of Eta Quotients, modulo 4, 9 and 25
Tim Huber, James McLaughlin, Dongxi Ye
https://arxiv.org/abs/2507.20298 https://…

Identical Vanishing of Coefficients in the Series Expansion of Eta Quotients, modulo 4, 9 and 25
Let $A(q)=\sum_{n=0}^{\infty}a_n q^n$ and $B(q)=\sum_{n=0}^{\infty}b_n q^n$ be two eta quotients. Previously, we considered the problem of when \[ a_n=0 <=> b_n=0. \] Here we consider the ``mod $m$'' version of this problem, i.e. eta quotients $A(q)$ and $B(q)$ and integers $m>1$ such that \[ a_n \equiv 0 \pmod m <=> b_n \equiv 0 \pmod m? \] We found results for $m=p^2$, $p=2, 3$ and $5$. For $m=4,9$, we found results which apply to infinite families of eta quotients. For example: Let $A(q)$ ha…

Structure-Property Correlations in Sb, Ge, and Ga Doped AlFe$_2$B$_2$ for Magnetocaloric Applications
R. Preyadarshini, S. Kavita, Ashutosh Kumar, D. Sivaprahasam
https://arxiv.org/abs/2506.22422

Structure-Property Correlations in Sb, Ge, and Ga Doped AlFe$_2$B$_2$ for Magnetocaloric Applications
This study investigates the effects of Sb, Ge, and Ga doping in AlFe$_2$B$_2$ on magnetic and magneto-caloric properties. Samples of AlFe$_2$B$_2$ and AlFe$_{1.9}$M$_{0.1}$B$_2$ (M= Ge, Ga and Sb) with 20\% excess Al were synthesized by arc melting, and the powder processed were investigated for their phase constituents, microstructure, magnetic and magneto-caloric effect. The parent compounds prepared showed the AlFe$_2$B$_2$ phase with a FeB secondary phase. However, in Sb and Ga-doped sample…

New Physics in inclusive semileptonic $B$ decays
Alexandre Carvunis, Gael Finauri, Paolo Gambino, Martin Jung, Sandro M\"achler
https://arxiv.org/abs/2507.22123 https://

New Physics in inclusive semileptonic $B$ decays
We study inclusive semileptonic $\bar{B}\to X_c \ell \barν$ decays ($\ell = e,μ$) in the presence of generic physics Beyond the Standard Model (BSM) that is heavy compared to the $b$-quark mass. Its effect is encoded in the Wilson coefficients of dimension-six operators of the Weak Effective Theory (WET). We compute the resulting BSM contributions to the experimentally measured kinematic moments and the total decay rate through order $\mathcal{O}(Λ_{\rm QCD}^3/m_b^3)$ in the Heavy Quark Expa…

Multipacking in Hypercubes
Deepak Rajendraprasad, Varun Sani, Birenjith Sasidharan, Jishnu Sen
https://arxiv.org/abs/2507.01565 https://

Multipacking in Hypercubes
For an undirected graph $G$, a dominating broadcast on $G$ is a function $f : V(G) \rightarrow \mathbb{N}$ such that for any vertex $u \in V(G)$, there exists a vertex $v \in V(G)$ with $f(v) \geqslant 1$ and $d(u,v) \leqslant f(v)$. The cost of $f$ is $\sum_{v \in V} f(v)$. The minimum cost over all the dominating broadcasts on $G$ is defined as the broadcast domination number $γ_b(G)$ of $G$. A multipacking in $G$ is a subset $M \subseteq V(G)$ such that, for every vertex $v \in V(G)$ and ev…

Modeling blazar broadband emission with convolutional neural networks -- III. proton synchrotron and hybrid models
N. Sahakyan, D. B\'egu\'e, A. Casotto, H. Dereli-B\'egu\'e, V. Vardanyan, M. Khachatryan, P. Giommi, A. Pe'er
https://arxiv.org/abs/2506.23885

Modeling blazar broadband emission with convolutional neural networks -- III. proton synchrotron and hybrid models
Modeling the broadband emission of blazars has become increasingly challenging with the advent of multimessenger observations. Building upon previous successes in applying convolutional neural networks (CNNs) to leptonic emission scenarios, we present an efficient CNN-based approach for modeling blazar emission under proton synchrotron and hybrid lepto-hadronic frameworks. Our CNN is trained on extensive numerical simulations generated by SOPRANO, which span a comprehensive parameter space acco…

#Blakes7 Series B, Episode 13 - Star One
DURKIM: She can't be, it's unmanned. The systems are automatic.
SERVALAN: A group of scientists and technicians elected to spend the rest of their lives refining, checking and guarding the systems.

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So if Mamdani's already Mayor, we can assume the Bedford Ave bike lanes will not be ripped out and we're about to get a whole shitload of new bike & bus lanes, right? Like, starting immediately?
Oh hang on, I'm being told that formerly indicted corrupt-af Eric Adams is still Mayor.

First observation of quantum oscillations by transport measurements in semi-destructive pulsed magnetic fields up to 125 T
M. Massoudzadegan, S. Badoux, N. Bruyant, I. Gilmutdinov, I. Haik-Dunn, G. de Oliveira Rodrigues, N. Lourenco Prata, A. Zitouni, M. Nardone, O. Drashenko, O. Portugall, S. Wiedmann, B. Fauqu\'e, D. Vignolles, B. Reulet, C. Proust

First observation of quantum oscillations by transport measurements in semi-destructive pulsed magnetic fields up to 125 T
High magnetic fields have proven instrumental in exploring the physical properties of condensed matter, leading to groundbreaking discoveries such as the quantum Hall effect in 2D heterostructures and quantum oscillations in cuprate superconductors. The ability to conduct precise measurements at progressively higher magnetic fields continues to push the frontiers of knowledge and enable new discoveries. In this work, we present the development of a microwave technique for performing two-point t…

The star HIP 41378 potentially misaligned with its cohort of long-period planets
S. Grouffal, A. Santerne, V. Bourrier, V. Kunovac, C. Dressing, B. Akinsanmi, C. Armstrong, S. Baliwal, O. Balsalobre-Ruza, S. C. C. Barros, D. Bayliss, I. J. M. Crossfield, O. Demangeon, X. Dumusque, S. Giacalone, C. K. Harada, H. Isaacson, H. Kellermann, J. Lillo-Box, J. Llama, A. Mortier, E. Palle, A. S. Rajpurohit, M. Rice, N. C. Santos, J. V. Seidel, R. Sharma, S. G. Sousa, L. Thomas, E. V. Turtelboom…

The star HIP 41378 potentially misaligned with its cohort of long-period planets
The obliquity between the stellar spin axis and the planetary orbit, detected via the Rossiter-McLaughlin (RM) effect, is a tracer of the formation history of planetary systems. While obliquity measurements have been extensively applied to hot Jupiters and short-period planets, they remain rare for cold and long-period planets due to observational challenges, particularly their long transit durations. We report the detection of the RM effect for the 19-hour-long transit of HIP 41378 f, a temper…

Requirements on bandpass resolution and measurement precision for LiteBIRD
S. Giardiello, A. Carones, T. Ghigna, L. Pagano, F. Piacentini, L. Montier, R. Takaku, E. Calabrese, D. Adak, E. Allys, A. Anand, J. Aumont, M. Ballardini, A. J. Banday, R. B. Barreiro, N. Bartolo, S. Basak, M. Bersanelli, A. Besnard, M. Bortolami, T. Brinckmann, F. J. Casas, K. Cheung, M. Citran, L. Clermont, F. Columbro, A. Coppolecchia, F. Cuttaia, P. de Bernardis, E. de la Hoz, M. De Lucia, S. Della Torre, E…

Requirements on bandpass resolution and measurement precision for LiteBIRD
In this work, we study the impact of an imperfect knowledge of the instrument bandpasses on the estimate of the tensor-to-scalar ratio $r$ in the context of the next-generation LiteBIRD satellite. We develop a pipeline to include bandpass integration in both the time-ordered data (TOD) and the map-making processing steps. We introduce the systematic effect by having a mismatch between the ``real'', high resolution bandpass $τ$, entering the TOD, and the estimated one $τ_s$, used in the map-ma…

Fundamental Nuclear and Particle Physics At Neutron Sources
H. Abele, J. Amaral, W. R. Anthony, L. AAstrand, M. Atzori Corona, S. Baessler, M. Bartis, E. Baussan, D. H. Beck, J. Bijnens, K. Bodek, J. Bosina, E. Bossio, G. Brooijmans, L. J. Broussard, G. Brunetti, A. Burgman, M. Cadeddu, N. Cargioli, J. Cederkall, A. Chambon, T. W. Choi, P. Christiansen, V. Cianciolo, C. B. Crawford, S. Degenkolb, N. Delarosa, M. Demarteau, K. Dickerson, D. D. DiJulio, F. Dordei, Y. Efremenko, T. Ekelof…

Fundamental Nuclear and Particle Physics At Neutron Sources
Fundamental neutron and neutrino physics at neutron sources, combining precision measurements and theory, can probe new physics at energy scales well beyond the highest energies probed by the LHC and possible future high energy collider facilities. The European Spallation Source (ESS) will in the not too far future be a most powerful pulsed neutron source and simultaneously the world's brightest pulsed neutrino source. The ESS, and neutron sources in general, can provide unprecedented and uniqu…

JWST Observations of SN 2023ixf II: The Panchromatic Evolution Between 250 and 720 Days After the Explosion
K. Medler, C. Ashall, P. Hoeflich, E. Baron, J. M. DerKacy, M. Shahbandeh, T. Mera, C. M. Pfeffer, W. B. Hoogendam, D. O. Jones, S. Shiber, E. Fereidouni, O. D. Fox, J. Jencson, L. Galbany, J. T. Hinkle, M. A. Tucker, B. J. Shappee, M. E. Huber, K. Auchettl, C. R. Angus, D. D. Desai, A. Do, A. V. Payne, J. Shi, M. Y. Kong, S. Romagnoli, A. Syncatto, G. Clayton, M. Dulude, M. Enge…

JWST Observations of SN 2023ixf II: The Panchromatic Evolution Between 250 and 720 Days After the Explosion
We present the nebular phase spectroscopic and photometric observations of the nearby hydrogen-rich core-collapse supernova (CC-SN) 2023ixf, obtained through our JWST programs. These observations, combined with ground-based optical and near-infrared spectra, cover +252.67 - 719.96 d, creating a comprehensive, panchromatic time-series dataset spanning 0.32 - 30$μ$m. In this second paper of the series, we focus on identifying key spectral emission features and tracking their evolution through th…

Heavy scalar molecule $B_{c}^{ } B_{c}^{-}$
S. S. Agaev, K. Azizi, H. Sundu
https://arxiv.org/abs/2506.19927 https://arxiv.org/pdf/25…

Heavy scalar molecule $B_{c}^{+} B_{c}^{-}$
Mass and full width of the heavy scalar molecule $\mathcal{M}$ composed of the mesons $B_{c}^{+}$ and $B_{c}^{-}$ are calculated in QCD sum rule framework. To find its mass and current coupling we apply the two-point sum rule method. The width of the hadronic molecule $\mathcal{M} =B_{c}^{+}B_{c}^{-}$ is evaluated by taking into account its dissociation to $η_cη_{b}, J/ψΥ$, and $ B_{c}^{+}B_{c}^{-} $ mesons. Decays into $D$ and $B$ meson pairs with appropriate charges and quantum numbers tr…

Series B, Episode 13 - Star One
AVON: There is only Lurgan's word. Everybody else who knew is either dead or amnesiac. One clue. Just one, and we have got it. Why are you listening to this drivel, Blake? We can take Star One, let's get on with it.
JENNA: Very stirring. When did you become a believer?
https://blake.torpi…

Precise Asteroseismic Ages for the Helmi Streams
Christopher J. Lindsay, Marc Hon, J. M. Joel Ong, Rafael A. Garc\'ia, Dinil B. Palakkatharappil, Jie Yu, Tanda Li, Tom\'as Ruiz-Lara, Amina Helmi
https://arxiv.org/abs/2507.01091

Precise Asteroseismic Ages for the Helmi Streams
The Helmi streams are remnants of a dwarf galaxy that was accreted by the Milky Way and whose stars now form a distinct kinematic and chemical substructure in the Galactic halo. Precisely age-dating these typically faint stars of extragalactic origin has been notoriously difficult due to the limitations of using only spectroscopic data, interferometry, or coarse asteroseismic measurements. Using observations from NASA's Transiting Exoplanet Survey Satellite, we report the detailed asteroseismic…

Mocking IFU observations and metallicity diagnostics from cosmological simulations
A. Cornejo-C\'ardenas, E. Sillero, P. B. Tissera, M. Boquien, J. Vilchez, G. Bruzual, P. Jofr\'e
https://arxiv.org/abs/2506.00460

Mocking IFU observations and metallicity diagnostics from cosmological simulations
Hydrodynamic simulations are powerful tools for studying galaxy formation. However, it is crucial to test and improve the sub-grid physics underlying these simulations by comparing their predictions with observations. To this aim, observable quantities can be derived for simulated galaxies, enabling the analysis of simulated properties through an observational approach. Our goal is to develop a new numerical tool capable of generating synthetic emission line spectra from spatially resolved regi…

This https://arxiv.org/abs/2212.00636 has been replaced.
link: https://scholar.google.com/scholar?q=a

Newman's conjecture for the partition function modulo integers with at least two distinct prime divisors
Let $M$ be a positive integer and $p(n)$ be the number of partitions of a positive integer $n$. Newman's Conjecture asserts that for each integer $r$, there are infinitely many positive integers $n$ such that \[ p(n)\equiv r \pmod{M}. \] For a positive integer $d$, let $B_{d}$ be the set of positive integers $M$ such that the number of prime divisors of $M$ is $d$. In this paper, we prove that for each positive integer $d$, the density of the set of positive integers $M$ for which Newman's Conj…

Intruder structures in $^{32}$Si and $^{29}$Al
J. Williams, G. Hackman, K. Starosta, R. S. Lubna, Priyanka Choudhary, Subhrajit Sahoo, P. C. Srivastava, C. Andreoiu, D. Annen, H. Asch, M. D. H. K. G. Badanage, G. C. Ball, M. Beuschlein, H. Bidaman, V. Bildstein, R. J. Coleman, A. B. Garnsworthy, B. Greaves, G. Leckenby, V. Karayonchev, M. S. Martin, C. Natzke, C. M. Petrache, A. Radich, E. Raleigh-Smith, D. Rhodes, R. Russell, M. Satrazani, P. Spagnoletti, C. E. Svensson, D. Tam, F. Wu…

Intruder structures in $^{32}$Si and $^{29}$Al
We have studied $^{32}$Si and $^{29}$Al using $^{12}$C($^{22}$Ne,2p) and $^{12}$C($^{22}$Ne,$α$p) fusion-evaporation reactions. In both cases, we observed significant population of high-spin structures distinct from the ground-state yrast bands. In $^{32}$Si, most of the high-energy states feed into a $J^π = 5^-$ nanosecond isomer. In $^{29}$Al, we identified a rotor-like negative-parity band with a $J^π = 7/2^-$ band-head. Doppler shift lifetime measurements were performed for all observed …

Series B, Episode 07 - Killer
VILA: Avon, come here!
AVON: What's the matter?
https://blake.torpidity.net/m/207/454 B7B3

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SMA and NOEMA reveal asymmetric sub-structure in the protoplanetary disk of IRAS23077 6707
Joshua B. Lovell, Leon Trapman, Kristina Monsch, Sean M. Andrews, Alice S. Booth, Garrett K. Keating, Takahiro Ueda, David J. Wilner
https://arxiv.org/abs/2507.00122

SMA and NOEMA reveal asymmetric sub-structure in the protoplanetary disk of IRAS23077+6707
We present high-resolution data of IRAS 23077+6707 (`Dracula's Chivito') with the Submillimeter Array (SMA at 1.33 mm/225.5 GHz) and the Northern Extended Millimeter Array (NOEMA at 2.7 mm/111.7 GHz and 3.1 mm/96.2 GHz). IRAS 23077+6707 is a highly-inclined and newly discovered protoplanetary disk, first reported in 2024. We combine SMA baselines from the Compact, Extended and Very Extended arrays, and NOEMA baselines from its A and C configurations, and present continuum images with resolution…

Extending the sensitivity of heavy sterile neutrino searches with solar neutrino experiments
Yutao Zhu, Haoyang Fu, Wentai Luo, Shaomin Chen, Litao Yang, Zhicai Zhang
https://arxiv.org/abs/2507.01675

Extending the sensitivity of heavy sterile neutrino searches with solar neutrino experiments
A sensitivity study of the search for heavy sterile neutrinos ($ν_H$) in the MeV mass range using solar neutrino experiments is presented. $ν_H$, with masses ranging from a few MeV up to 15 MeV, can be produced in the Sun through $^8$B decay and subsequently decay into $ν_e e^+ e^-$. Its flux and lifetime strongly depend on the mixing parameter $|U_{eH}|^2$ and mass $m_{ν_H}$. The $ν_H$ signal can be detected via its decay products, either the $e^+e^-$ pair or $ν_e$, depending o…

Y'know, I have an incredibly stinky dead possum in my garbage can (Queens shit, don't ask), and somehow NYC Sanitation didn't pick up garbage last night.. And we're about to get potentially historic flooding starting in another hour?
I'm not chasing down that bloated carcass if it fucking floats away, NYC.

Series B, Episode 03 - Weapon
GAN: That doesn't sound very promising. Someone must have made an attack on the base.
VILA: Who'd be stupid enough to do that?
AVON: [Snaps his fingers] Justify "stupid."
https://blake.torpidity.net/m/203/112 B7B2

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Evolutionary Map of the Universe: Detection and Analysis of the Shell Surrounding the Runaway Wolf-Rayet Star WR16
A. C. Bradley, M. D. Filipovi\'c, Z. J. Smeaton, H. Sano, Y. Fukui, C. Bordiu, S. Cichowolski, N. F. H. Tothill, R. Z. E. Alsaberi, F. Bufano, S. Dai, Y. A. Gordon, A. M. Hopkins, T. H. Jarrett, B. S. Koribalski, S. Lazarevi\'c, C. J. Riseley, G. Rowell, M. Sasaki, D. Uro\v{s}evi\'c, T. Vernstrom

Evolutionary Map of the Universe: Detection and Analysis of the Shell Surrounding the Runaway Wolf-Rayet Star WR16
We present the first radio--continuum detection of the circumstellar shell around the well-known WN8 type Wolf-Rayet star WR16 at 943.5\,MHz using the \ac{ASKAP} \ac{EMU} survey. At this frequency, the shell has a measured flux density of 72.2$\pm$7.2\,mJy. Using previous \ac{ATCA} measurements at 2.4, 4.8, and 8.64~GHz, as well as the \ac{EMU} observations of the star itself, we determine a spectral index of $α\,=\,+0.74\pm0.02$, indicating thermal emission. We propose that the shell and star…

The Atacama Cosmology Telescope: DR6 Sunyaev-Zel'dovich Selected Galaxy Clusters Catalog
HSC Collaboration, M. Aguena, S. Aiola, S. Allam, F. Andrade-Oliveira, D. Bacon, N. Bahcall, N. Battaglia, E. S. Battistelli, S. Bocquet, B. Bolliet, J. R. Bond, D. Brooks, E. Calabrese, J. Carretero, S. K. Choi, L. N. da Costa, M. Costanzi, W. Coulton, T. M. Davis, S. Desai, M. J. Devlin, S. Dicker, P. Doel, A. J. Duivenvoorden, J. Dunkley, S. Ferraro, B. Flaugher, J. Frieman, P. A. Gallardo, …

The Atacama Cosmology Telescope: DR6 Sunyaev-Zel'dovich Selected Galaxy Clusters Catalog
We present the results of a search for galaxy clusters in the Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) microwave sky maps covering 16293 square degrees in three frequency bands, using data obtained over the lifetime of the project (2008-2022). We report redshifts and mass estimates for 9977 clusters detected via their Sunyaev-Zel'dovich (SZ) effect with signal-to-noise greater than 4 at a 2.4 arcminute filter scale. The catalog includes 1166 clusters at redshifts greater than 1, a…

The Lockman-SpReSO project. Spectroscopic analysis of Type 1 AGN
Castalia Alenka Negrete, Hector J. Ibarra-Medel, Erika Benitez, Irene Cruz-Gonzalez, Yair Krongold, J. Jesus Gonzalez, Jordi Cepa, Carmen Padilla-Torres, Miguel Cervino, Mirjana Povic, Martin Herrera-Endoqui, Nancy Jenaro-Ballesteros, Takamitsu Miyaji, Mauricio Elias-Chavez, Miguel Sanchez-Portal, Bernabe Cedres, Jacub Nadolny, Mauro Gonzalez-Otero, Bereket Assefa, Hector Hernandez-Toledo, J. Antonio de Diego, J. Ignacio …

The Lockman-SpReSO project. Spectroscopic analysis of Type 1 AGN
We present the first optical-UV spectral systematic analysis of 30 Type 1 AGN selected in the FIR and X-ray in the Lockman-SpReSO Survey. The sample of faint objects (m_B = 19.6-21.8) covers a large redshift range of 0.33 > z > 4.97 with high S/N (~21 on average). A detailed spectral analysis based on the Quasar Main Sequence phenomenology prescription was applied to deblend the principal optical-UV emitting regions. Our sample spans a bolometric luminosity range of 44.85 < log Lbol < 47.87, ab…

Bridging Unstratified and Stratified Simulations of the Streaming Instability for $\tau_s=0.1$ Grains
Jeonghoon Lim, Stanley A. Baronett, Jacob B. Simon, Chao-Chin Yang, Debanjan Sengupta, Orkan M. Umurhan, Wladimir Lyra
https://arxiv.org/abs/2505.23902

Bridging Unstratified and Stratified Simulations of the Streaming Instability for $τ_s=0.1$ Grains
The streaming instability (SI), driven by aerodynamic coupling between solids and the gas under a global radial pressure gradient, concentrates solids and facilitates planetesimal formation. Unstratified simulations are commonly used to study the SI, based on the assumption that they approximate conditions near the disk midplane. However, it remains unclear how accurately these unstratified simulations capture the midplane dust-gas dynamics in stratified disks. To address this, we examine the s…

I deleted my linkedin account ~15 years ago (maybe longer? it was around the time that they started sucking in peoples' gmail inbox, which was creepy)
I re-joined 6 months ago to look for a job, but so far it has just wasted my time. The jobs I see on linkedin have 3000 people applying for them, and the applications that I've actually gotten callbacks from have been ones where I randomly checked a webpage of a company I respect to see if they're hiring.
I'm extrem…

Detection of Molecular Hydrogen in a Proton Trap
J. Caylor (Thomas Jefferson National Accelerator Facility, Newport News USA), R. Biswas (Tulane University, New Orleans USA), B. Crawford (Gettysburg College, Gettysburg USA), M. S. Dewey (National Institute of Standards and Technology, Gaithersburg USA), N. Fomin (University of Tennessee, Knoxville USA), G. L. Greene (University of Tennessee, Knoxville USA, Tulane University, New Orleans USA), S. F. Hoogerheide (National Institute of St…

Detection of Molecular Hydrogen in a Proton Trap
One method of determining the free neutron lifetime involves the absolute counting of neutrons and trapped decay protons. In such experiments, a cold neutron beam traverses a segmented proton trap inside a superconducting solenoid while the neutron flux is continuously monitored. Protons that are born within the fiducial volume of the trap are confined radially by the magnetic field and axially by the electrostatic potential supplied by trap electrodes. They are periodically released and counte…

Three fast-spinning medium-sized Hilda asteroids uncovered by TESS
N\'ora Tak\'acs, Csaba Kiss, R\'obert Szak\'ats, Emese Plachy, Csilla E. Kalup, Gyula M. Szab\'o, L\'aszl\'o Moln\'ar, Kriszti\'an S\'arneczky, R\'obert Szab\'o, Attila B\'odi, Andr\'as P\'al
https://arx…

Three fast-spinning medium-sized Hilda asteroids uncovered by TESS
Hilda asteroids, which orbit in a 3:2 resonance with Jupiter, serve as key indicators of dynamical processes in the early solar system. Their spin rates, an important probe of these mechanisms, can constrain their density and collisional evolution, offering valuable insights into their origin. In this paper, we report on the identification of three fast-rotating Hilda asteroids with spin periods in the 3.2--3.7 h range using data from the Transiting Exoplanet Survey Satellite. These rotation pe…

A Catalog of Galactic Supernova Remnants and Supernova Remnant Candidates from the EMU/POSSUM Radio Sky Surveys. I
B. D. Ball, R. Kothes, E. Rosolowsky, C. Burger-Scheidlin, M. D. Filipovi\'c, S. Lazarevi\'c, Z. J. Smeaton, W. Becker, E. Carretti, B. M. Gaensler, A. M. Hopkins, D. Leahy, M. Tahani, J. L. West, C. S. Anderson, S. Loru, Y. K. Ma, N. M. McClure-Griffiths, M. J. Micha{\l}owski

A Catalog of Galactic Supernova Remnants and Supernova Remnant Candidates from the EMU/POSSUM Radio Sky Surveys. I
We use data from the EMU (Evolutionary Map of the Universe) and POSSUM (Polarization Sky Survey of the Universe's Magnetism) radio southern sky surveys, conducted with the Australian Square Kilometre Array Pathfinder (ASKAP), to compile a catalogue of Galactic supernova remnants (SNRs) and candidate SNRs within the region of $277.5^\circ \leq \ell \leq 311.7^\circ$ Galactic longitude, $|b| \leq 5.4^\circ$ Galactic latitude, as well as an additional field along the Galactic plane, appr…

Series B, Episode 03 - Weapon
TRAVIS: What?
SERVALAN: If he's cornered, he might destroy the weapon.
TRAVIS: I should have realized.
SERVALAN: I don't find stupidity amusing, Travis.
TRAVIS: No.
https://blake.torpidity.net/m/203/266 B7B2

Potential absence of observed $\pi^2$ linear-chain structures in $^{14}$O via $^{10}$C($\alpha,\alpha$) resonant scattering
J. Bishop, A. Hollands, Tz. Kokolova, G. V. Rogachev, C. Wheldon, E. Aboud, S. Ahn, M. Barbui, N. Curtis, J. Hooker, C. Hunt, H. Jayatissa, E. Koshchiy, S. Pirrie, B. T. Roeder, A. Saastamoinen, S. Upadhyayula
https://

Potential absence of observed $π^2$ linear-chain structures in $^{14}$O via $^{10}$C($α,α$) resonant scattering
Background: The preference for light nuclear systems to coagulate into $α$-particle clusters has been well-studied. The possibility of a linear chain configuration of $α$-particles would allow for a new way to study this phenomenon. Purpose: A rotational band of states in $^{14}$C has been claimed showing a $π^2$ linear chain structure. The mirror system, $^{14}$O, has been studied here to examine how this linear chain structure is affected by replacing the valence neutrons with protons. Met…

Series B, Episode 04 - Horizon
ORAC: Of course, should it be necessary.
AVON: Failing that, we are powerful enough to resist all but an attack by three Federation pursuit ships at once.
ORAC: Is that a question?
https://blake.torpidity.net/m/204/496 B7B3

A systematic bias in template-based RV extraction algorithms
Andr\'e M. Silva, N. C. Santos, J. P. Faria, J. H. C. Martins, E. A. S. Cristo, S. G. Sousa, P. T. P. Viana, \'E. Artigau, K. Al Moulla, A. Castro-Gonz\'alez, D. F. M. Folha, P. Figueira, T. Schmidt, F. Pepe, X. Dumusque, O. D. S. Demangeon, T. L. Campante, X. Delfosse, B. Wehbe, J. Lillo-Box, A. R. Costa Silva, J. Rodrigues, J. I. Gonz\'alez Hern\'andez, T. Azevedo Silva, S. Cristiani, H. M. Tabernero, E.…

A systematic bias in template-based RV extraction algorithms
In this paper we identify and explore a previously unidentified, multi meter-per-second, systematic correlation between time and RVs inferred through TM and LBL methods. We evaluate the influence of the data-driven stellar template in the RV bias and hypothesize on the possible sources of this effect. We first use the s-BART pipeline to extract RVs from three different datasets gathered over four nights of ESPRESSO and HARPS observations. Then, we demonstrate that the effect can be recovered on…

Man, some of our Republican MAGA electeds are just completely off the r.. *touches earpiece*
Hang on, I'm being told that it's a Democrat. Oh, a NY Democrat, at that?
https://flipboard.com/@rollingstone/politic…

N.Y. Senator 'Misspoke' When She Flasely Claimed Zohran Mamdani Condoned 'Global Jihad'
During a radio interview Thursday, New York Democratic Senator Kirsten Gillibrand appeared to suggest that Zohran Mamdani had condoned “global …

The z = 9.625 Cosmic Gems Galaxy was a "Compact Blue Monster" Propelled by Massive Star Clusters
E. Vanzella, M. Messa, A. Adamo, F. Loiacono, M. Oguri, K. Sharon, L. D. Bradley, P. Bergamini, M. Meneghetti, A. Claeyssens, B. Welch, M. Bradac, A. Zanella, A. Bolamperti, F. Calura, T. Y-Y. Hsiao, E. Zackrisson, M. Ricotti, L. Christensen, J. M. Diego, F. E. Bauer, X. Xu, S. Fujimoto, C. Grillo, M. Lombardi, P. Rosati, T. Resseguier, A. Zitrin, A. Bik, J. Richard, Abdurro'…

The z = 9.625 Cosmic Gems Galaxy was a "Compact Blue Monster" Propelled by Massive Star Clusters
The recent discovery of five massive stellar clusters at z=9.625 in the Cosmic Gems has raised the question about the formation mechanism of star clusters in the first half Gyr after the Big-Bang. We infer the total stellar mass in clusters by normalizing and integrating the stellar cluster mass function (SCMF, dn(M)/dM ~ (n$_0$) $M^β$), assuming three different slopes $β$ = -1.5, -2.0 and -2.5 and different lower-mass limits between $10^2$ and $10^5$ Msun. The total integrated cluster stella…

The nebular phase of SN 2024ggi: a low-mass progenitor with no signs of interaction
L. Ferrari, G. Folatelli, K. Ertini, H. Kuncarayakti, T. Regna, M. C. Bersten, C. Ashall, E. Baron, C. R. Burns, L. Galbany, W. B. Hoogendam, K. Maeda, K. Medler, N. I. Morrel, B. Shapee, M. D. Stritzinger, H. Xiao
https://arxiv.org/abs/2507.22794

The nebular phase of SN 2024ggi: a low-mass progenitor with no signs of interaction
Context: SN 2024ggi is a Type II supernova (SN) discovered in the nearby galaxy NGC 3621 (D $\approx6.7\pm0.d$ Mpc) on 2024 April 03.21 UT. Its proximity enabled a detailed investigation of the SN's properties and its progenitor star. This work focuses on the optical evolution of SN 2024ggi at the nebular phase. Aims: We investigate the progenitor properties and possible asymmetries in the ejecta by studying the nebular phase evolution between days 287 and 400 after the explosion. Methods: We p…

I keep seeing posts about Sydney Sweeney (who I'm aware is a terrible person), and almost every single response is "wait, who is she and why should we care?"
And while I agree that we shouldn't care (I certainly don't!), I can't help but be shocked that no one's seen Euphoria?
[edit: forgot about White Lotus, but it's not as good as Euphoria imo]

Series B, Episode 03 - Weapon
[Messroom. Travis enters]
SERVALAN: Are the guards in clear view?
TRAVIS: Three of them, as you ordered, Supreme Commander.
SERVALAN: And the fourth is concealed?
https://blake.torpidity.net/m/203/429 B7B3

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Series B, Episode 11 - Gambit
JENNA: She's right, Blake. He's led a privileged life. He's got money.
BLAKE: He's also been on the move for a long time.
JENNA: But even so, a man with his skills can always earn it.
https://blake.torpidity.net/m/211/170 B…

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Series B, Episode 11 - Gambit
JENNA: She's right, Blake. He's led a privileged life. He's got money.
BLAKE: He's also been on the move for a long time.
JENNA: But even so, a man with his skills can always earn it.
https://blake.torpidity.net/m/211/170 B…

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Series B, Episode 08 - Hostage
JENNA: [To Cally] You know what all this is about, don't you?
CALLY: [Nodding] I think I can guess.
JENNA: It is a trap, isn't it?
CALLY: Avon thinks so.
JENNA: Well Avon always thinks so.
https://blake.torpidity.net/m/208/321

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Series B, Episode 11 - Gambit
SERVALAN: Yes, well, let's forget the pleasantries. Tell me where to find Docholli, I'll let you have Blake.
TRAVIS: You haven't got Blake.
https://blake.torpidity.net/m/211/235 B7B2

Series B, Episode 10 - Voice from the Past
JENNA: Complaining of some sort of noise.
AVON: A sort of tone, he said.
CALLY: Oscillating. It was there again just now.
AVON: As a part of his nightmare?
CALLY: Yes, I think so.
https://blake.torpidity.net/m/210/85

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Series B, Episode 10 - Voice from the Past
JENNA: Complaining of some sort of noise.
AVON: A sort of tone, he said.
CALLY: Oscillating. It was there again just now.
AVON: As a part of his nightmare?
CALLY: Yes, I think so.
https://blake.torpidity.net/m/210/85

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Series B, Episode 01 - Redemption
AVON: Don't worry. At the right time, I will remind you of it.
[Flight deck]
VILA: [Accepts cup from Jenna and swallows pill] Thanks.
JENNA: [To Blake who has just entered flight deck with Avon] You all right?
https://blake.torpidity.net/m/201/242

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#Blakes7 Series B, Episode 02 - Shadow
CALLY: I think Blake can look after himself.
VILA: He's led a very sheltered life.
CALLY: What, Blake has led a sheltered life?
https://blake.torpidity.net/m/202/119

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#Blakes7 Series B, Episode 02 - Shadow
CALLY: I think Blake can look after himself.
VILA: He's led a very sheltered life.
CALLY: What, Blake has led a sheltered life?
https://blake.torpidity.net/m/202/119

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Series B, Episode 06 - Trial
COMPUTER: Holding.
THANIA: Defence requests the names of the alleged victims and the cause of death in each case be specified.
SAMOR: All of them?
THANIA: If it pleases the arbiter.
https://blake.torpidity.net/m/206/58 B7B5

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Series B, Episode 02 - Shadow
ORAC: The bridge is complete.
VILA: What? What did he say?
GAN: Something's wrong.
VILA: No, that wasn't it.
ZEN: Information. Liberator is losing power from all systems. Orbital maintenance is threatened.
https://blake.torpidity.net/m/202/555

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