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Risa H. Wechsler

Researcher at Stanford University

Publications -  572
Citations -  63450

Risa H. Wechsler is an academic researcher from Stanford University. The author has contributed to research in topics: Galaxy & Dark matter. The author has an hindex of 116, co-authored 528 publications receiving 54728 citations. Previous affiliations of Risa H. Wechsler include University of Illinois at Urbana–Champaign & Massachusetts Institute of Technology.

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Localization and broadband follow-up of the gravitational-wave transient GW150914

B. P. Abbott, +1540 more
TL;DR: In this paper, the sky localization of the first observed compact binary merger is presented, where the authors describe the low-latency analysis of the LIGO data and present a sky localization map.
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Analyzing interferometric observations of strong gravitational lenses with recurrent and convolutional neural networks

TL;DR: In this paper, the authors used convolutional neural networks and recurrent neural networks (RNNs) to estimate the parameters of strong gravitational lenses from interferometric observations, and found that the best results are obtained when the effects of the dirty beam are first removed from the images with deconvolution performed with an RNN-based structure before estimating the parameters.
Journal ArticleDOI

Data-driven Reconstruction of Gravitationally Lensed Galaxies Using Recurrent Inference Machines

TL;DR: In this paper, a machine learning method for the reconstruction of the undistorted images of background sources in strongly lensed systems is presented, which treats the source as a pixelated image and utilizes the Recurrent Inference Machine (RIM) to iteratively reconstruct the background source given a lens model.
Journal ArticleDOI

Unbound Particles in Dark Matter Halos

TL;DR: In this paper, the authors investigate unbound dark matter particles in halos by tracing particle trajectories in a simulation run to the far future (a = 100) and find that the traditional sum of kinetic and potential energies is a very poor predictor of which dark matter particle will eventually become unbound from halos.