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@arXiv_astrophSR_bot@mastoxiv.page
2024-03-29 08:42:07

This arxiv.org/abs/2403.09568 has been replaced.
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@kunstbanause@nrw.social
2024-03-29 10:58:08

Well, that was close...
Was printing two items in #byobject mode. First one was doing well so I decided to go grocery shopping and check remotely from time to time. Obviously I forgot about that and when I remembered, the print was about 50% into the second item but nothing on the build plate. 🙈 I cancelled it remotely, but of course was worried about the desaster on the

Hotend blob in white material. The blob shows the shape of the hotend as a negative.
@arXiv_nuclex_bot@mastoxiv.page
2024-04-30 08:48:30

This arxiv.org/abs/2310.04736 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_physicsplasmph_bot@mastoxiv.page
2024-01-30 07:33:53

This arxiv.org/abs/2308.03938 has been replaced.
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@arXiv_mathAP_bot@mastoxiv.page
2024-02-29 07:19:31

Linear inviscid damping in the presence of an embedding eigenvalue
Siqi Ren, Zhifei Zhang
arxiv.org/abs/2402.18229 ar…

@arXiv_csSI_bot@mastoxiv.page
2024-02-29 06:57:12

Towards spatiotemporal integration of bus transit with data-driven approaches
J\'ulio Borges, Altieris M. Peixoto, Thiago H. Silva, Anelise Munaretto, Ricardo Luders
arxiv.org/abs/2402.17866

@arXiv_heplat_bot@mastoxiv.page
2024-04-30 07:02:14

Flow-based Nonperturbative Simulation of First-order Phase Transitions
Yang Bai, Ting-Kuo Chen
arxiv.org/abs/2404.18323

@arXiv_condmatquantgas_bot@mastoxiv.page
2024-03-29 08:43:03

This arxiv.org/abs/2312.09848 has been replaced.
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@arXiv_mathDS_bot@mastoxiv.page
2024-03-28 06:55:58

$L^\infty$-error bounds for approximations of the Koopman operator by kernel extended dynamic mode decomposition
Frederik K\"ohne, Friedrich M. Philipp, Manuel Schaller, Anton Schiela, Karl Worthmann
arxiv.org/abs/2403.18809

@arXiv_qfinCP_bot@mastoxiv.page
2024-02-27 07:15:40

Optimizing Portfolio Management and Risk Assessment in Digital Assets Using Deep Learning for Predictive Analysis
Qishuo Cheng, Le Yang, Jiajian Zheng, Miao Tian, Duan Xin
arxiv.org/abs/2402.15994 arxiv.org/pdf/2402.15994
arXiv:2402.15994v1 Announce Type: new
Abstract: Portfolio management issues have been extensively studied in the field of artificial intelligence in recent years, but existing deep learning-based quantitative trading methods have some areas where they could be improved. First of all, the prediction mode of stocks is singular; often, only one trading expert is trained by a model, and the trading decision is solely based on the prediction results of the model. Secondly, the data source used by the model is relatively simple, and only considers the data of the stock itself, ignoring the impact of the whole market risk on the stock. In this paper, the DQN algorithm is introduced into asset management portfolios in a novel and straightforward way, and the performance greatly exceeds the benchmark, which fully proves the effectiveness of the DRL algorithm in portfolio management. This also inspires us to consider the complexity of financial problems, and the use of algorithms should be fully combined with the problems to adapt. Finally, in this paper, the strategy is implemented by selecting the assets and actions with the largest Q value. Since different assets are trained separately as environments, there may be a phenomenon of Q value drift among different assets (different assets have different Q value distribution areas), which may easily lead to incorrect asset selection. Consider adding constraints so that the Q values of different assets share a Q value distribution to improve results.

@arXiv_mathAP_bot@mastoxiv.page
2024-02-29 07:19:31

Linear inviscid damping in the presence of an embedding eigenvalue
Siqi Ren, Zhifei Zhang
arxiv.org/abs/2402.18229 ar…

@arXiv_mathOC_bot@mastoxiv.page
2024-04-26 08:39:36

This arxiv.org/abs/2402.06139 has been replaced.
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@arXiv_statME_bot@mastoxiv.page
2024-03-27 07:10:59

Statistical analysis and method to propagate the impact of measurement uncertainty on dynamic mode decomposition
P. Algikar, P. Sharma, M. Netto, L. Mili
arxiv.org/abs/2403.17318

@losttourist@social.chatty.monster
2024-03-22 20:02:05

This must have been one of the very first appearances of Depeche Mode on #TOTP. Previously there was some other band called Depeshay Mode.

@guerda@ruhr.social
2024-02-23 12:18:43

Help needed with #LibreraReader: I cannot find out how to open the menu to change between dark and light mode while having a document open. It appeared the first time I opened the book, but not anymore.
Any idea? Tested it with the F-Droid and the Play store version.
Android 14
#Librera

@arXiv_csCR_bot@mastoxiv.page
2024-02-22 08:29:18

This arxiv.org/abs/2304.01580 has been replaced.
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@arXiv_eessSY_bot@mastoxiv.page
2024-03-21 09:07:52

This arxiv.org/abs/2304.02433 has been replaced.
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@arXiv_grqc_bot@mastoxiv.page
2024-04-23 08:56:22

This arxiv.org/abs/2310.06018 has been replaced.
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@thomasfuchs@hachyderm.io
2024-03-10 02:22:49

One for the “she’s so stupid how can you put your car into reverse accidentally!!!1” replyguys:
Some Teslas don’t have a gear-selector stalk and literally guess what gear you want.
Yes, you read that right.
theverge.com/22348668/tesla-pr

@arXiv_csIT_bot@mastoxiv.page
2024-02-20 08:28:04

This arxiv.org/abs/2306.08353 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_astrophHE_bot@mastoxiv.page
2024-04-24 06:59:58

Magnetic amplification in pre-merger neutron stars through resonance-induced magnetorotational instabilities
Arthur G. Suvorov, Hao-Jui Kuan, Alexis Reboul-Salze, Kostas D. Kokkotas
arxiv.org/abs/2404.14529

@arXiv_quantph_bot@mastoxiv.page
2024-03-20 07:22:05

Multiplexed quantum state transfer in waveguides
Guillermo F. Pe\~nas, Ricardo Puebla, Juan Jos\'e Garc\'ia-Ripoll
arxiv.org/abs/2403.12222

@arXiv_csAR_bot@mastoxiv.page
2024-02-20 06:47:01

Stochastic Nonlinear Dynamical Modelling of SRAM Bitcells in Retention Mode
L\'eopold Van Brandt, Denis Flandre, Jean-Charles Delvenne
arxiv.org/abs/2402.11691

@arXiv_physicsplasmph_bot@mastoxiv.page
2024-03-26 07:21:33

Core performance predictions in projected SPARC first-campaign plasmas with nonlinear CGYRO
P. Rodriguez-Fernandez, N. T. Howard, A. Saltzman, L. Shoji, T. Body, D. J. Battaglia, J. W. Hughes, J. Candy, G. M. Staebler, A. J. Creely
arxiv.org/abs/2403.15633

@andycarolan@social.lol
2024-04-03 07:24:55

Oh wow... I never knew! 🤯
aus.social/@kauer/112205938142

@arXiv_csCR_bot@mastoxiv.page
2024-02-22 08:29:18

This arxiv.org/abs/2304.01580 has been replaced.
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@arXiv_condmatmeshall_bot@mastoxiv.page
2024-03-21 09:13:41

This arxiv.org/abs/2009.10985 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_physicsfludyn_bot@mastoxiv.page
2024-03-18 08:47:06

This arxiv.org/abs/1911.04730 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_csLG_bot@mastoxiv.page
2024-04-10 06:51:40

Exploring Neural Network Landscapes: Star-Shaped and Geodesic Connectivity
Zhanran Lin, Puheng Li, Lei Wu
arxiv.org/abs/2404.06391 <…

@jamesthebard@social.linux.pizza
2024-04-04 14:13:11

Finally started work on the new #Pathfinder Second Edition character sheet. I'm trying to keep the same feel as the one I made for first edition, but since they are significantly different so will be the layout. The goal is to keep the first page very dense info-wise while still keeping it readable. #ttrpgs

A screenshot of Adobe InDesign in preview mode showing a partially laid-out Pathfinder 2E character sheet.  The top section has all of the character info such as name, player name, hero points, ancestry, heritage, class, deity, XP, background, etc.  The sections below that are labelled "Statistics and Saves" which contain ability scores, saves, and speed; "Health and Armor" which has max HP, how much HP gained on resting, AC, AC Bonus, and Shield information; "Status" which contains damage take…
@arXiv_condmatsoft_bot@mastoxiv.page
2024-04-24 07:01:21

Irreversible Boltzmann samplers in dense liquids: weak-coupling approximation and mode-coupling theory
Federico Ghimenti, Ludovic Berthier, Grzegorz Szamel, Fr\'ed\'eric van Wijland
arxiv.org/abs/2404.14863

@arXiv_astrophSR_bot@mastoxiv.page
2024-04-23 07:00:43

On the incidence rate of RR Lyrae stars with non-radial modes
H. Netzel, V. Varga, R. Szabo, R. Smolec, E. Plachy
arxiv.org/abs/2404.14373

@kennysmith@mstdn.social
2024-03-07 15:49:39

If you can play it, you can be it.
#Esports #RepresentationMatters
From: @…

@arXiv_condmatmtrlsci_bot@mastoxiv.page
2024-03-19 09:05:05

This arxiv.org/abs/2306.08347 has been replaced.
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@nemobis@mamot.fr
2024-03-05 10:44:43

#CJEU:
«a harmonised standard, adopted on the basis of a directive [...] forms part of EU law»
«the rule of law, which requires free access to EU law for all natural or legal persons of the European Union»
«there is an overriding public interest [...] justifying the disclosure of the requested harmonised standards»
«As is apparent [...] the Commission should have acknowledged [...]…

@redstarfish@social.linux.pizza
2024-02-02 19:03:25

When did Enriched mode come to #Emacs?? This is the first time I'm reading about it.

@arXiv_nuclth_bot@mastoxiv.page
2024-03-19 09:05:55

This arxiv.org/abs/2305.08401 has been replaced.
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@arXiv_astrophGA_bot@mastoxiv.page
2024-03-06 07:16:18

GA-NIFS: NIRSpec reveals evidence for non-circular motions and AGN feedback in GN20
Hannah \"Ubler, Francesco D'Eugenio, Michele Perna, Santiago Arribas, Gareth C. Jones, Andrew J. Bunker, Stefano Carniani, St\'ephane Charlot, Roberto Maiolino, Bruno Rodr\'iguez del Pino, Chris J. Willott, Torsten B\"oker, Giovanni Cresci, Nimisha Kumari, Isabella Lamperti, Eleonora Parlanti, Jan Scholtz, Giacomo Venturi
arxiv.org/abs/2403.03192 arxiv.org/pdf/2403.03192
arXiv:2403.03192v1 Announce Type: new
Abstract: We present rest-frame optical data of the z~4 sub-millimeter galaxy GN20 obtained with JWST/NIRSpec in integral field spectroscopy (IFS) mode. The H$\alpha$ emission is asymmetric and clumpy and extends over a projected distance of more than 15 kpc. To first order, the large-scale ionised gas kinematics are consistent with a turbulent ($\sigma\sim90$ km/s), rotating disc ($v_{\rm rot}\sim500$ km/s), congruent with previous studies of its molecular and ionised gas kinematics. However, we also find clear evidence for non-circular motions in the H$\alpha$ kinematics. We discuss their possible connection with various scenarios, such as external perturbations, accretion or radial flows. In the centre of GN20, we find broad line emission (FWHM $\sim1000-2000$ km/s) in the H$\alpha$ [N II] complex, suggestive of fast, AGN-driven winds or, alternatively, of the broad-line region of an active black hole. Elevated values of [N II]$\lambda6583$/H$\alpha>0.4$ and EW(H$\alpha)>6$ \r{A}, throughout large parts of GN20 suggest that feedback from the active black hole is able to photo-ionise the interstellar medium. Our data corroborates that GN20 offers a unique opportunity to observe key processes in the evolution of the most massive present-day galaxies acting in concert, over 12 billion years ago.

@arXiv_physicsinsdet_bot@mastoxiv.page
2024-02-15 08:45:49

This arxiv.org/abs/2402.01060 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_condmatsuprcon_bot@mastoxiv.page
2024-04-22 07:26:11

Magnetic-field driven evolution of zero-energy mode on Bi islands deposited on Fe(Te,Se)
Kailun Chen, Chuanhao Wen, Zhiyong Hou, Huan Yang, Hai-Hu Wen
arxiv.org/abs/2404.12708

@fell@ma.fellr.net
2024-01-31 11:10:25

Day 3 of attempting to daily drive postmarketOS Linux on a OnePlus 6T:
I had my first crash! I wanted to unlock the phone while waiting for some coffee to finish brewing, and after a few seconds of black screen I got this.
After a hard reset it booted up fine again.
#postmarketOS #Linux

Photo of a smartphone on a wooden table surface. The screen is showing: "QUALCOMM CrashDump Mode" in blue, red and yellow letters.
@arXiv_physicsspaceph_bot@mastoxiv.page
2024-03-19 07:07:38

A new launch pad failure mode: Analysis of fine particles from the launch of the first Starship orbital test flight
B. Dotson, P. Metzger, J. Hafner, A. Shackelford, K. Birkenfeld, D. Britt, A. Ford, R. Truscott, S. Truscott, J. Zavaleta, J. Zemke, K. Purvis, M. Scudder, C. Johnson, J. Galloway, J. DeShetler
arxiv.org/ab…

@arXiv_physicsoptics_bot@mastoxiv.page
2024-02-20 07:07:15

Light storage in wavy dielectric grating with Kerr nonlinearity
Ma Luo
arxiv.org/abs/2402.12020 arxiv.org/pdf/2402.12…

@copsewood@social.linux.pizza
2024-03-15 18:06:52

@…
I first used Linux when a student loaned me a Red Hat 3.0.3 CD - version released 1 May 1996 according to Wikipedia - and I booted it and was soon able to get it doing useful stuff in text mode, including running some of my shell scripts developed on Solaris.
Have made much use of it since on all classes of device from embedded routers t…

@arXiv_astrophSR_bot@mastoxiv.page
2024-03-21 07:10:58

The VELOCE Modulation Zoo I. Spectroscopic detection of non-radial modes in the first-overtone Cepheids BG Crucis, QZ Normae, V0391 Normae, and V0411 Lacertae
H. Netzel, R. I. Anderson, G. Viviani
arxiv.org/abs/2403.13796

@arXiv_hepex_bot@mastoxiv.page
2024-04-03 07:01:52

Search of CP violation in baryons with the LHCb detector
Chiara Mancuso
arxiv.org/abs/2404.01793 arxiv.org/pdf/2404.0…

@arXiv_eessSP_bot@mastoxiv.page
2024-03-13 07:33:44

Experimental analysis of the TRC benchmark system
Arati Bhattu, Svenja Hermann, Nidhal Jamia, Florian M\"uller, Maren Scheel, Christoph Schwingshackl, H. Nevzat \"Ozg\"uven, Malte Krack
arxiv.org/abs/2403.07438

@arXiv_hepph_bot@mastoxiv.page
2024-04-09 07:16:46

Boosted four-top production at the LHC : a window to Randall-Sundrum or extended color symmetry
Debajyoti Choudhury, Kuldeep Deka, Lalit Kumar Saini
arxiv.org/abs/2404.04409

@arXiv_astrophCO_bot@mastoxiv.page
2024-03-07 06:59:35

The first high-redshift cavity power measurements of cool-core galaxy clusters with the International LOFAR Telescope
R. Timmerman, R. J. van Weeren, A. Botteon, H. J. A. R\"ottgering, L. K. Morabito, F. Sweijen
arxiv.org/abs/2403.03242

@arXiv_condmatstrel_bot@mastoxiv.page
2024-02-21 07:01:36

Ultrafast dynamics of a fermion chain in a terahertz field-driven optical cavity
Mohsen Yarmohammadi, John Sous, Marin Bukov, Michael H. Kolodrubetz
arxiv.org/abs/2402.12591

@arXiv_mathOC_bot@mastoxiv.page
2024-02-12 06:57:59

Sliding Mode Observers for Set-valued Lur'e Systems with Uncertainties Beyond Observational Range
Samir Adly, Jun Huang, Ba Khiet Le
arxiv.org/abs/2402.06139

@arXiv_condmatmtrlsci_bot@mastoxiv.page
2024-03-19 09:05:05

This arxiv.org/abs/2306.08347 has been replaced.
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@arXiv_eessSY_bot@mastoxiv.page
2024-04-11 07:14:48

Dynamic Mode Decomposition with Non-uniform Sampling
Ramachandran Anantharaman, Alexandre Mauroy
arxiv.org/abs/2404.07133

@arXiv_physicsfludyn_bot@mastoxiv.page
2024-04-16 09:11:53

This arxiv.org/abs/2310.19044 has been replaced.
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@arXiv_physicsappph_bot@mastoxiv.page
2024-02-20 07:31:48

23.8 GHz Acoustic Filter in Periodically Poled Piezoelectric Film Lithium Niobate with 1.52 dB IL and 19.4% FBW
Sinwoo Cho, Omar Barrera, Jack Kramer, Vakhtang Chulukhadze, Tzu-Hsuan Hsu, Joshua Campbell, Ian Anderson, Ruochen Lu
arxiv.org/abs/2402.12194

@arXiv_grqc_bot@mastoxiv.page
2024-04-09 09:00:35

This arxiv.org/abs/2308.15886 has been replaced.
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@arXiv_physicsplasmph_bot@mastoxiv.page
2024-03-18 07:19:37

Tokamak H-mode edge-SOL global turbulence simulations with an electromagnetic, transcollisional drift-fluid model
W. Zholobenko, K. Zhang, A. Stegmeir, J. Pfennig, K. Eder, C. Pitzal, P. Ulbl, M. Griener, L. Radovanovic, U. Plank, ASDEX Upgrade Team
arxiv.org/abs/2403.10113

@arXiv_condmatsuprcon_bot@mastoxiv.page
2024-04-22 07:26:11

Magnetic-field driven evolution of zero-energy mode on Bi islands deposited on Fe(Te,Se)
Kailun Chen, Chuanhao Wen, Zhiyong Hou, Huan Yang, Hai-Hu Wen
arxiv.org/abs/2404.12708

@arXiv_astrophSR_bot@mastoxiv.page
2024-02-20 07:00:13

Using Bright-Point Shapes to Constrain Wave-Heating of the Solar Corona: Predictions for DKIST
Samuel J. Van Kooten, Steven R. Cranmer
arxiv.org/abs/2402.10915

@arXiv_eessSY_bot@mastoxiv.page
2024-03-04 07:27:25

Mode Consensus Algorithms With Finite Convergence Time
Chao Huang, Hyungbo Shim, Siliang Yu, Brian D. O. Anderson
arxiv.org/abs/2403.00221

@arXiv_astrophCO_bot@mastoxiv.page
2024-04-03 08:47:46

This arxiv.org/abs/2310.06729 has been replaced.
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@arXiv_grqc_bot@mastoxiv.page
2024-04-09 09:00:35

This arxiv.org/abs/2308.15886 has been replaced.
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@arXiv_physicsclassph_bot@mastoxiv.page
2024-04-04 07:05:13

Correlation and Spectral Density Functions in Mode-Stirred Reverberation -- I. Theory
Luk R. Arnaut
arxiv.org/abs/2404.02347

@arXiv_astrophSR_bot@mastoxiv.page
2024-03-19 07:12:33

Radiative loss and ion-neutral collisional effects in astrophysical plasmas
Beatrice Popescu Braileanu, Rony Keppens
arxiv.org/abs/2403.11900

@arXiv_hepph_bot@mastoxiv.page
2024-03-04 07:27:26

J/psi-pair production at NLL in TMD factorisation at the LHC
Alice Colpani Serri, Jelle Bor, Daniel Boer, Jean-Philippe Lansberg
arxiv.org/abs/2403.00640

@arXiv_eessSP_bot@mastoxiv.page
2024-03-04 07:28:44

User Localization with HRIS and Backscatter Modulation for Next-Generation Networks
Mattia Piana, Stefano Tomasin
arxiv.org/abs/2403.00568

@arXiv_physicschemph_bot@mastoxiv.page
2024-04-03 08:52:59

This arxiv.org/abs/2309.17331 has been replaced.
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@arXiv_physicsplasmph_bot@mastoxiv.page
2024-02-23 07:32:36

Global gyrokinetic analysis of Wendelstein 7-X discharge: unveiling the importance of trapped-electron-mode and electron-temperature-gradient turbulence
Felix Wilms, Alejandro Ba\~n\'on Navarro, Thomas Windisch, Sergey Bozhenkov, Felix Warmer, Golo Fuchert, Oliver Ford, Daihong Zhang, Torsten Stange, Frank Jenko, the W7-X Team

@arXiv_physicsoptics_bot@mastoxiv.page
2024-04-17 07:31:21

Realization of Planar Optical Tweezer (2D-LOT) Powered by Light Sheet
Neptune Baro, Partha Pratim Mondal
arxiv.org/abs/2404.10265

@arXiv_astrophSR_bot@mastoxiv.page
2024-02-15 07:06:12

Variable stars in galactic globular Clusters I. The population of RR Lyrae stars
Mauricio Cruz Reyes, Richard I. Anderson, Lucas Johansson, Henryka Netzel, Zo\'e Medaric
arxiv.org/abs/2402.08843

@arXiv_grqc_bot@mastoxiv.page
2024-04-05 08:42:09

This arxiv.org/abs/2403.18673 has been replaced.
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@arXiv_mathAP_bot@mastoxiv.page
2024-03-11 06:54:48

Incompleteness of Sinclair-type continuum flexible boundary conditions for atomistic fracture simulations
Julian Braun, Maciej Buze
arxiv.org/abs/2403.05462

@arXiv_condmatmeshall_bot@mastoxiv.page
2024-04-03 07:20:05

Reaching Curzon-Ahlborn limit in linear response and Whitney limit in nonlinear response in edge mode quantum thermoelectrics and refrigeration
Sachiraj Mishra, Colin Benjamin
arxiv.org/abs/2404.02118

@arXiv_condmatmtrlsci_bot@mastoxiv.page
2024-02-14 07:00:42

Effect of electron-phonon coupling on thermal transport in metals: a Monte Carlo approach for solving the coupled electron-phonon Boltzmann transport equations
Jie Peng, W. Ryan Deskins, Maria Helena Braga, Anter El-Azab
arxiv.org/abs/2402.08150

@arXiv_astrophGA_bot@mastoxiv.page
2024-04-03 07:11:35

Stellar Variability and Distance Indicators in the Near-infrared in Nearby Galaxies. I. RR Lyrae and Anomalous Cepheids in Draco dwarf spheroidal
Anupam Bhardwaj, Marina Rejkuba, Chow-Choong Ngeow, Marcella Marconi, Vincenzo Ripepi, Abhinna Sundar Samantaray, Harinder P. Singh
arxiv.org/abs/2404.01394

@arXiv_physicsoptics_bot@mastoxiv.page
2024-02-12 08:46:37

This arxiv.org/abs/2312.11048 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_condmatsuprcon_bot@mastoxiv.page
2024-03-14 07:01:42

Light-driven interlayer propagation of collective-mode excitations in layered superconductors
Niklas Ziereis, Kazuaki Takasan, Naoto Tsuji
arxiv.org/abs/2403.08734

@arXiv_grqc_bot@mastoxiv.page
2024-04-05 08:42:09

This arxiv.org/abs/2403.18673 has been replaced.
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@arXiv_astrophSR_bot@mastoxiv.page
2024-04-01 08:40:37

This arxiv.org/abs/2403.02250 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_physicschemph_bot@mastoxiv.page
2024-04-03 08:52:59

This arxiv.org/abs/2309.17331 has been replaced.
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@arXiv_physicsplasmph_bot@mastoxiv.page
2024-04-09 09:03:43

This arxiv.org/abs/2312.05216 has been replaced.
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@arXiv_astrophSR_bot@mastoxiv.page
2024-03-20 07:26:57

Kaleidoscope of irradiated disks: MUSE observations of proplyds in the Orion Nebula Cluster. I. Sample presentation and ionization front sizes
Mari-Liis Aru, K. Mauco, C. F. Manara, T. J. Haworth, S. Facchini, A. F. McLeod, A. Miotello, M. G. Petr-Gotzens, M. Robberto, G. P. Rosotti, S. Vicente, A. Winter, M. Ansdell
arx…

@arXiv_physicsoptics_bot@mastoxiv.page
2024-02-12 08:46:37

This arxiv.org/abs/2312.11048 has been replaced.
link: scholar.google.com/scholar?q=a

@arXiv_astrophSR_bot@mastoxiv.page
2024-03-15 07:00:19

Determining stellar accretion rates from $Pa_{\alpha}$ and $Br_{\beta}$ emission lines with JWST NIRSpec
Ciar\`an Rogers, Guido de Marchi, Bernhard Brandl
arxiv.org/abs/2403.09568

@arXiv_physicsoptics_bot@mastoxiv.page
2024-03-06 07:06:57

Observation of Replica Symmetry Breaking in Standard Mode-Locked Fiber Laser
Nicolas P. Alves, Wesley F. Alves, Andr\'e C. A. Siqueira, Naudson L. L. Matias, Anderson S. L. Gomes, Ernesto P. Raposo, Marcio H. G. de Miranda
arxiv.org/abs/2403.02477

@arXiv_physicsplasmph_bot@mastoxiv.page
2024-03-01 07:06:55

Analytic solutions for the linearized first-order magnetohydrodynamics and implications for causality and stability
Zhe Fang, Koichi Hattori, Jin Hu
arxiv.org/abs/2402.18601

@arXiv_astrophSR_bot@mastoxiv.page
2024-03-12 07:24:39

The influence of different coronal hole geometries on simulations of coronal wave - coronal hole interaction
I. Piantschitsch, J. Terradas, E. Soubrie, S. G. Heinemann, S. J. Hofmeister, R. Soler, M. Temmer
arxiv.org/abs/2403.06614

@arXiv_astrophSR_bot@mastoxiv.page
2024-03-12 07:24:39

The influence of different coronal hole geometries on simulations of coronal wave - coronal hole interaction
I. Piantschitsch, J. Terradas, E. Soubrie, S. G. Heinemann, S. J. Hofmeister, R. Soler, M. Temmer
arxiv.org/abs/2403.06614