Search Results for author: Barak Zackay

Found 5 papers, 5 papers with code

New approach to template banks of gravitational waves with higher harmonics: Reducing matched-filtering cost by over an order of magnitude

2 code implementations23 Oct 2023 Digvijay Wadekar, Tejaswi Venumadhav, Ajit Kumar Mehta, Javier Roulet, Seth Olsen, Jonathan Mushkin, Barak Zackay, Matias Zaldarriaga

To model aligned-spin $(3, 3)$, $(4, 4)$ waveforms corresponding to a given $(2, 2)$ waveform, we use a combination of post-Newtonian formulae and machine learning tools.

New Binary Black Hole Mergers in the Second Observing Run of Advanced LIGO and Advanced Virgo

1 code implementation15 Apr 2019 Tejaswi Venumadhav, Barak Zackay, Javier Roulet, Liang Dai, Matias Zaldarriaga

The most secure new event, GW170121 ($p_{\rm astro} > 0. 99$), is also notable due to its inferred negative value of $\chi_{\rm eff}$, which is inconsistent with being positive at the $\approx 95. 8\%$ confidence level.

High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology

A Highly Spinning and Aligned Binary Black Hole Merger in the Advanced LIGO First Observing Run

1 code implementation27 Feb 2019 Barak Zackay, Tejaswi Venumadhav, Liang Dai, Javier Roulet, Matias Zaldarriaga

We report a new binary black hole merger in the publicly available LIGO First Observing Run (O1) data release.

High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology

How to coadd images? II. A coaddition image that is optimal for any purpose in the background dominated noise limit

2 code implementations21 Dec 2015 Barak Zackay, Eran O. Ofek

Here, we build on these results and derive from first principles a coaddition technique which is optimal for any hypothesis testing and measurement (e. g., source detection, flux or shape measurements and star/galaxy separation), in the background-noise-dominated case.

Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics

How to coadd images? I. Optimal source detection and photometry using ensembles of images

2 code implementations21 Dec 2015 Barak Zackay, Eran O. Ofek

We show that for these purposes the best way to combine images is to apply a matched filter to each image using its own point spread function (PSF) and only then to sum the images with the appropriate weights.

Instrumentation and Methods for Astrophysics

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