no code implementations • 5 Apr 2024 • Tianze Wang, Maryam Honari-Jahromi, Styliani Katsarou, Olga Mikheeva, Theodoros Panagiotakopoulos, Sahar Asadi, Oleg Smirnov
Methods for learning latent user representations from historical behavior logs have gained traction for recommendation tasks in e-commerce, content streaming, and other settings.
no code implementations • 21 Nov 2022 • Oleg Smirnov, Aditya Tewari
In this paper, we introduce a new dataset of room interior pictures with overlaying and scene text, totalling to 4836 annotated images in 25 product categories.
2 code implementations • 27 May 2021 • Oleg Smirnov
The adoption of neural networks and deep learning in non-Euclidean domains has been hindered until recently by the lack of scalable and efficient learning frameworks.
no code implementations • 1 Jan 2021 • Simphiwe Zitha, Arun Aniyan, Oleg Smirnov, Risuna Nkolele
The average prediction error obtained during the testing of our models on testing data is $ \approx 0. 01 < rmse < 0. 09$ for gain amplitude per antenna, and $0. 2 rad < rmse <0. 5 rad$ for gain phase.
no code implementations • 29 Nov 2020 • Tim Johnson, Oleg Smirnov
We study a spatial, one-shot prisoner's dilemma (PD) model in which selection operates on both an organism's behavioral strategy (cooperate or defect) and its choice of when to implement that strategy across a set of discrete time slots.
no code implementations • 26 Aug 2020 • Philipp Arras, Richard A. Perley, Hertzog L. Bester, Reimar Leike, Oleg Smirnov, Rüdiger Westermann, Torsten A. Enßlin
CLEAN, the commonly employed imaging algorithm in radio interferometry, suffers from a number of shortcomings: in its basic version it does not have the concept of diffuse flux, and the common practice of convolving the CLEAN components with the CLEAN beam erases the potential for super-resolution; it does not output uncertainty information; it produces images with unphysical negative flux regions; and its results are highly dependent on the so-called weighting scheme as well as on any human choice of CLEAN masks to guiding the imaging.
Instrumentation and Methods for Astrophysics Applications
1 code implementation • 24 Feb 2015 • Oleg Smirnov, Cyril Tasse
We apply these developments to the problem of radio interferometric gain calibration, and show how the general complex Jacobian formalism, when combined with conventional optimization approaches, yields a whole new family of calibration algorithms, including those for the polarized and direction-dependent gain regime.
Instrumentation and Methods for Astrophysics
no code implementations • 30 Jan 2015 • Simon Perkins, Patrick Marais, Jonathan Zwart, Iniyan Natarajan, Cyril Tasse, Oleg Smirnov
Chi-squared values computed from the model and observed visibilities are used as likelihood values to drive the Bayesian sampling process and select the best sky model.