Zobrazeno 1 - 10
of 340
pro vyhledávání: '"gonzalez, A. Perez"'
Publikováno v:
IEEE Ubiquitous Robots 2024, New York City
This paper underscores the importance of environmental monitoring, and specifically of freshwater ecosystems, which play a critical role in sustaining life and global economy. Despite their importance, insufficient data availability prevents a compre
Externí odkaz:
http://arxiv.org/abs/2410.23722
Autor:
Saidel, Morgan, Vissapragada, Shreyas, Spake, Jessica, Knutson, Heather A., Linssen, Dion, Zhang, Michael, Greklek-McKeon, Michael, González, Jorge Pérez, Oklopčić, Antonija
The lack of close-in Neptune-mass exoplanets evident in transit surveys has largely been attributed either to photoevaporative mass loss or high-eccentricity migration. To distinguish between these two possibilities, we investigate the origins of TOI
Externí odkaz:
http://arxiv.org/abs/2404.08736
Autor:
Vissapragada, Shreyas, Greklek-McKeon, Michael, Linssen, Dion, MacLeod, Morgan, Thorngren, Daniel P., Gao, Peter, Knutson, Heather A., Latham, David W., López-Morales, Mercedes, Oklopčić, Antonija, González, Jorge Pérez, Saidel, Morgan, Tumborang, Abigail, Yoshida, Stephanie
Super-puffs are planets with exceptionally low densities ($\rho \lesssim 0.1$~g~cm$^{-3}$) and core masses ($M_c \lesssim 5 M_\oplus$). Many lower-mass ($M_p\lesssim10M_\oplus$) super-puffs are expected to be unstable to catastrophic mass loss via ph
Externí odkaz:
http://arxiv.org/abs/2403.05614
Autor:
González, Jorge Pérez, Greklek-McKeon, Michael, Vissapragada, Shreyas, Saidel, Morgan, Knutson, Heather A., Linssen, Dion, Oklopčić, Antonija
Photoevaporative mass-loss rates are expected to be highest when planets are young and the host star is more active, but to date there have been relatively few measurements of mass-loss rates for young gas giant exoplanets. In this study we measure t
Externí odkaz:
http://arxiv.org/abs/2307.09515
Autor:
Vissapragada, Shreyas, Chontos, Ashley, Greklek-McKeon, Michael, Knutson, Heather A., Dai, Fei, González, Jorge Pérez, Grunblatt, Sam, Huber, Daniel, Saunders, Nicholas
We present evidence of tidally-driven inspiral in the Kepler-1658 (KOI-4) system, which consists of a giant planet (1.1$R_\mathrm{J}$, 5.9$M_\mathrm{J}$) orbiting an evolved host star (2.9$R_\odot$, 1.5$M_\odot$). Using transit timing measurements fr
Externí odkaz:
http://arxiv.org/abs/2212.09752
VarStar Detect is a Python package available on PyPI optimized for the detection of variability inside photometric measurements. Based off of the Least Squares method of regression, VarStar Detect calculates the amplitude of a Fourier Polynomial fit
Externí odkaz:
http://arxiv.org/abs/2109.06347
Autor:
Nooralahzadeh, Farhad, Gonzalez, Nicolas Perez, Frauenfelder, Thomas, Fujimoto, Koji, Krauthammer, Michael
Inspired by Curriculum Learning, we propose a consecutive (i.e., image-to-text-to-text) generation framework where we divide the problem of radiology report generation into two steps. Contrary to generating the full radiology report from the image at
Externí odkaz:
http://arxiv.org/abs/2102.09777
Autor:
Martin, Montse Villar, Perna, Michele, Humphrey, Andrew, Rodriguez, Nieves Castro, Binette, Luc, Gonzalez, Pablo Perez, Mateos, Silvia, Lavers, Antonio Cabrera
Publikováno v:
A&A 634, A116 (2020)
Core-extremely red quasars (core-ERQ) have been proposed to represent an intermediate evolutionary phase in which a heavily obscured quasar is blowing out the circumnuclear interstellar medium with very energetic outflows prior to becoming an optical
Externí odkaz:
http://arxiv.org/abs/2001.03379
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