Zobrazeno 1 - 10
of 15 678
pro vyhledávání: '"P, Mandel"'
Autor:
Boyd, Benjamin M., Narayan, Gautham, Mandel, Kaisey S., Grayling, Matthew, Berres, Aidan, Li, Mai, Do, Aaron, Saha, Abhijit, Axelrod, Tim, Matheson, Thomas, Olszewski, Edward W., Bohlin, Ralph C., Calamida, Annalisa, Holberg, Jay B., Hubeny, Ivan, Mackenty, John W., Rest, Armin, Sabbi, Elena, Stubbs, Christopher W.
We use hierarchical Bayesian modelling to calibrate a network of 32 all-sky faint DA white dwarf (DA WD) spectrophotometric standards ($16.5 < V < 19.5$) alongside the three CALSPEC standards, from 912 \r{A} to 32 $\mu$m. The framework is the first o
Externí odkaz:
http://arxiv.org/abs/2412.08809
The pseudo-observations approach has been gaining popularity as a method to estimate covariate effects on censored survival data. It is used regularly to estimate covariate effects on quantities such as survival probabilities, restricted mean life, c
Externí odkaz:
http://arxiv.org/abs/2412.04109
Autor:
The Multimodal Universe Collaboration, Audenaert, Jeroen, Bowles, Micah, Boyd, Benjamin M., Chemaly, David, Cherinka, Brian, Ciucă, Ioana, Cranmer, Miles, Do, Aaron, Grayling, Matthew, Hayes, Erin E., Hehir, Tom, Ho, Shirley, Huertas-Company, Marc, Iyer, Kartheik G., Jablonska, Maja, Lanusse, Francois, Leung, Henry W., Mandel, Kaisey, Martínez-Galarza, Juan Rafael, Melchior, Peter, Meyer, Lucas, Parker, Liam H., Qu, Helen, Shen, Jeff, Smith, Michael J., Stone, Connor, Walmsley, Mike, Wu, John F.
We present the MULTIMODAL UNIVERSE, a large-scale multimodal dataset of scientific astronomical data, compiled specifically to facilitate machine learning research. Overall, the MULTIMODAL UNIVERSE contains hundreds of millions of astronomical observ
Externí odkaz:
http://arxiv.org/abs/2412.02527
Autor:
van Son, L. A. C., Roy, S. K., Mandel, I., Farr, W. M., Lam, A., Merritt, J., Broekgaarden, F. S., Sander, A., Andrews, J. J.
Both detailed and rapid population studies alike predict that binary black hole (BHBH) formation is orders of magnitude more efficient at low metallicity than high metallicity, while binary neutron star (NSNS) formation remains mostly flat with metal
Externí odkaz:
http://arxiv.org/abs/2411.02484
Autor:
Kwatra, Amritansh, Wienberg, Tobias, Mandel, Ilan, Batra, Ritik, He, Peter, Guimbretiere, Francois, Roumen, Thijs
As tools for designing and manufacturing hardware become more accessible, smaller producers can develop and distribute novel hardware. However, there aren't established tools to support end-user hardware troubleshooting or routine maintenance. As a r
Externí odkaz:
http://arxiv.org/abs/2411.02332
Autor:
Sivakumar, Viswanath, Seely, Jeffrey, Du, Alan, Bittner, Sean R, Berenzweig, Adam, Bolarinwa, Anuoluwapo, Gramfort, Alexandre, Mandel, Michael I
Surface electromyography (sEMG) non-invasively measures signals generated by muscle activity with sufficient sensitivity to detect individual spinal neurons and richness to identify dozens of gestures and their nuances. Wearable wrist-based sEMG sens
Externí odkaz:
http://arxiv.org/abs/2410.20081
Stellar-mass black holes (BHs) embedded in active galactic nuclei (AGN) may be major sources of astrophysical gravitational waves (GWs), contributing both to the observed LIGO-Virgo-KAGRA population of binary BH mergers and to future populations of L
Externí odkaz:
http://arxiv.org/abs/2410.19904
Large language models (LLMs) have taken the world by storm by making many previously difficult uses of AI feasible. LLMs are controlled via highly expressive textual prompts and return textual answers. Unfortunately, this unstructured text as input a
Externí odkaz:
http://arxiv.org/abs/2410.19135
Autor:
Mandel, Ilya
In this invited talk at the 41st Li\`ege International Astrophysical Colloquium on "The eventful life of massive star multiples", I reviewed some aspects of our current understanding of neutron stars and black holes as end products of stellar evoluti
Externí odkaz:
http://arxiv.org/abs/2410.07747
We construct a semi-analytical model that describes the convective core mass evolution of massive stars experiencing mass loss during the main-sequence stage. We first conduct a suite of 1D stellar evolution calculations to build insight into how con
Externí odkaz:
http://arxiv.org/abs/2409.00460