no code implementations • 20 Jan 2022 • J. Yang, Lei He
To further improve the speaker similarity, joint training with a speaker classifier is proposed.
no code implementations • 4 Mar 2021 • A. F. Fang, R. Zhou, H. Tukada, J. Yang, Z. Deng, X. C. Wang, C. Q. Jin, Guo-qing Zheng
Identifying the uniqueness of FeP-based superconductors may shed new lights on the mechanism of superconductivity in iron-pnictides.
Superconductivity Strongly Correlated Electrons
no code implementations • 12 Jan 2021 • J. Yang, I. van Bemmel, Z. Paragi, S. Komossa, F. Yuan, X. Yang, T. An, J. Y. Koay, C. Reynolds, J. B. R. Oonk, X. Liu, Q. Wu
Broad Balmer emission lines in active galactic nuclei (AGN) may display dramatic changes in amplitude, even disappearance and re-appearance in some sources.
High Energy Astrophysical Phenomena Astrophysics of Galaxies
1 code implementation • 9 Jul 2020 • F. Kirsten, M. Snelders, M. Jenkins, K. Nimmo, J. van den Eijnden, J. Hessels, M. Gawronski, J. Yang
The recent CHIME/FRB and STARE2 detection of an extremely bright (fluence ~MJy ms) radio burst from the Galactic magnetar SGR 1935+2154 supports the hypothesis that (some) fast radio bursts (FRBs) are emitted by magnetars at cosmological distances.
High Energy Astrophysical Phenomena
no code implementations • 17 Mar 2020 • R. Dong, J. Yang, Y. Chen
The community detection in real-life networks, the majority of which are weighted temporal text networks, is confronted with two main problems - how to model the weight of edges and how to exploit the temporal information.
no code implementations • 18 Oct 2019 • T. Braine, R. Cervantes, N. Crisosto, N. Du, S. Kimes, L. J Rosenberg, G. Rybka, J. Yang, D. Bowring, A. S. Chou, R. Khatiwada, A. Sonnenschein, W. Wester, G. Carosi, N. Woollett, L. D. Duffy, R. Bradley, C. Boutan, M. Jones, B. H. LaRoque, N. S. Oblath, M. S. Taubman, J. Clarke, A. Dove, A. Eddins, S. R. O'Kelley, S. Nawaz, I. Siddiqi, N. Stevenson, A. Agrawal, A. V. Dixit, J. R. Gleason, S. Jois, P. Sikivie, N. S. Sullivan, D. B. Tanner, E. Lentz, E. J. Daw, J. H. Buckley, P. M. Harrington, E. A. Henriksen, K. W. Murch
This paper reports on a cavity haloscope search for dark matter axions in the galactic halo in the mass range $2. 81$-$3. 31$ ${\mu}eV$.
High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics Instrumentation and Detectors
no code implementations • 3 Jun 2019 • X. Huang, M. Domingo, A. Pilon, V. Ravi, C. Storfer, D. J. Schlegel, S. Bailey, A. Dey, D. Herrera, S. Juneau, M. Landriau, D. Lang, A. Meisner, J. Moustakas, A. D. Myers, E. F. Schlafly, F. Valdes, B. A. Weaver, J. Yang, C. Yeche
We compile a training set that consists of known lensing systems in the Legacy Surveys and DES as well as non-lenses in the footprint of DECaLS.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
no code implementations • 12 Feb 2019 • S. Deshpande, J. Shuttleworth, J. Yang, S. Taramonli, M. England
In this study, we present a novel tool, PLIT, for the identification of lncRNAs in plants RNA-seq datasets.
no code implementations • 3 Jan 2019 • C. Boutan, M. Jones, B. H. LaRoque, N. S. Oblath, R. Cervantes, N. Du, N. Force, S. Kimes, R. Ottens, L. J. Rosenberg, G. Rybka, J. Yang, G. Carosi, N. Woollett, D. Bowring, A. S. Chou, R. Khatiwada, A. Sonnenschein, W. Wester, R. Bradley, E. J. Daw, A. Agrawal, A. V. Dixit, J. Clarke, S. R. O'Kelley, N. Crisosto, J. R. Gleason, S. Jois, P. Sikivie, I. Stern, N. S. Sullivan, D. B. Tanner, P. M. Harrington, E. Lentz
The $\mu$eV axion is a well-motivated extension to the standard model.
High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics Instrumentation and Detectors
1 code implementation • 1 Aug 2018 • G. Ghirlanda, O. S. Salafia, Z. Paragi, M. Giroletti, J. Yang, B. Marcote, J. Blanchard, I. Agudo, T. An, M. G. Bernardini, R. Beswick, M. Branchesi, S. Campana, C. Casadio, E. Chassande-Mottin, M. Colpi, S. Covino, P. D'Avanzo, V. D'Elia, S. Frey, M. Gawronski, G. Ghisellini, L. I. Gurvits, P. G. Jonker, H. J. van Langevelde, A. Melandri, J. Moldon, L. Nava, A. Perego, M. A. Perez-Torres, C. Reynolds, R. Salvaterra, G. Tagliaferri, T. Venturi, S. D. Vergani, M. Zhang
The first binary neutron star merger, detected through both electromagnetic radiation and gravitational waves on the 17th of August 2017, raised the question whether a narrow relativistic jet or a more isotropic outflow was launched as a consequence of the merger.
High Energy Astrophysical Phenomena