Results 261 to 270 of about 5,043,235 (296)

Predicting the diversity of photosynthetic light-harvesting using thermodynamics and machine learning. [PDF]

PLoS Comput Biol
Gray C, Chitnavis S, Buja T, Duffy CDP.
europepmc   +1 more source

dynoGP: Deep Gaussian Processes for Dynamic System Identification

International Journal of Adaptive Control and Signal Processing, EarlyView.
This work introduces a novel class of deep models for system identification, dynamical deep Gaussian processes, which combine the strengths of data‐driven methods, such as those based on neural network architectures, with the ability to output a probability distribution for uncertainty representation.
Alessio Benavoli, Marco Forgione, Dario Piga, Marco Zaffalon   +3 more
wiley   +1 more source

The connection between the fastest astrophysical jets and the spin axis of their black hole. [PDF]

Nat Astron
Fender RP, Motta SE.
europepmc   +1 more source

Research on Star Sensor Imaging Simulation Under Near-Space Hypersonic Non-Equilibrium Flow Conditions. [PDF]

Sensors (Basel)
Liao Z, Wang H, Cheng X, Liu B, Zang Y, Lu Y, Yao S, Yan Z.   +7 more
europepmc   +1 more source

Spectral synthesis techniques for supernovae and kilonovae. [PDF]

Living Rev Comput Astrophys
Jerkstrand A.
europepmc   +1 more source

Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]

Living Rev Sol Phys
Veronig AM, Dissauer K, Kliem B, Downs C, Hudson HS, Jin M, Osten R, Podladchikova T, Prasad A, Qiu J, Thompson B, Tian H, Vourlidas A.   +12 more
europepmc   +1 more source

Spotlight on challenges and novel methods in highly multiplexed tissue imaging-based spatial proteomics. [PDF]

J Transl Med
Yang L, Yang Z.
europepmc   +1 more source

Classification of LAMOST spectra of B-type and hot subdwarf stars using kernel support vector machine. [PDF]

Sci Rep
Tahir M, Yude B, Mehmood T, Bashir S, Zhenping Y, Awais M.   +5 more
europepmc   +1 more source

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Stellar Spectral Types and the H-R Diagram

2021
We know stars are large balls of hot, glowing plasma fueled by the nuclear fusion occurring in their cores. This hot plasma emits blackbody radiation. At the surface of the star, the peak intensity in the spectrum corresponds to the surface temperature of the star. This peak in the spectrum correlates to a wavelength on the electromagnetic spectrum. As
openaire   +1 more source

SPIDER VIII – constraints on the stellar initial mass function of early-type galaxies from a variety of spectral features [PDF]

Monthly Notices of the Royal Astronomical Society, 2013
34 pages, 27 figures; V2.
Marina Trevisan, Jesús Falcón-Barroso, Reinaldo Ramos de Carvalho   +2 more
exaly   +3 more sources