1 code implementation • 13 Mar 2024 • Siddharth Mishra-Sharma, Yiding Song, Jesse Thaler
We present PAPERCLIP (Proposal Abstracts Provide an Effective Representation for Contrastive Language-Image Pre-training), a method which associates astronomical observations imaged by telescopes with natural language using a neural network model.
1 code implementation • 28 Nov 2023 • Carolina Cuesta-Lazaro, Siddharth Mishra-Sharma
We introduce a diffusion-based generative model to describe the distribution of galaxies in our Universe directly as a collection of points in 3-D space (coordinates) optionally with associated attributes (e. g., velocities and masses), without resorting to binning or voxelization.
1 code implementation • 18 Aug 2023 • Aizhan Akhmetzhanova, Siddharth Mishra-Sharma, Cora Dvorkin
The influx of massive amounts of data from current and upcoming cosmological surveys necessitates compression schemes that can efficiently summarize the data with minimal loss of information.
1 code implementation • 21 Jun 2023 • Lukas Heinrich, Siddharth Mishra-Sharma, Chris Pollard, Philipp Windischhofer
When analyzing real-world data it is common to work with event ensembles, which comprise sets of observations that collectively constrain the parameters of an underlying model of interest.
1 code implementation • 29 Aug 2022 • Gemma Zhang, Siddharth Mishra-Sharma, Cora Dvorkin
Strong gravitational lensing has emerged as a promising approach for probing dark matter models on sub-galactic scales.
1 code implementation • 26 Aug 2022 • Tri Nguyen, Siddharth Mishra-Sharma, Reuel Williams, Lina Necib
Dwarf galaxies are small, dark matter-dominated galaxies, some of which are embedded within the Milky Way.
1 code implementation • 29 Jun 2022 • Siddharth Mishra-Sharma, Ge Yang
From the nature of dark matter to the rate of expansion of our Universe, observations of distant galaxies distorted through strong gravitational lensing have the potential to answer some of the major open questions in astrophysics.
no code implementations • 15 Mar 2022 • Cora Dvorkin, Siddharth Mishra-Sharma, Brian Nord, V. Ashley Villar, Camille Avestruz, Keith Bechtol, Aleksandra Ćiprijanović, Andrew J. Connolly, Lehman H. Garrison, Gautham Narayan, Francisco Villaescusa-Navarro
Methods based on machine learning have recently made substantial inroads in many corners of cosmology.
1 code implementation • 13 Oct 2021 • Siddharth Mishra-Sharma, Kyle Cranmer
The nature of the Fermi gamma-ray Galactic Center Excess (GCE) has remained a persistent mystery for over a decade.
1 code implementation • 4 Oct 2021 • Siddharth Mishra-Sharma
Astrometry -- the precise measurement of positions and motions of celestial objects -- has emerged as a promising avenue for characterizing the dark matter population in our Galaxy.
1 code implementation • 20 Oct 2020 • Siddharth Mishra-Sharma, Kyle Cranmer
Mismodeling the uncertain, diffuse emission of Galactic origin can seriously bias the characterization of astrophysical gamma-ray data, particularly in the region of the Inner Milky Way where such emission can make up over 80% of the photon counts observed at ~GeV energies.
2 code implementations • 8 Sep 2020 • Andrea Caputo, Hongwan Liu, Siddharth Mishra-Sharma, Maxim Pospelov, Joshua T. Ruderman, Alfredo Urbano
Within the context of a kinetically mixed dark photon, we demonstrate how resonant dark photon-to-photon conversions can imprint distinctive spectral features in the observed 21-cm brightness temperature, with implications for current, upcoming, and proposed experiments targeting the cosmic dawn and the dark ages.
Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology
2 code implementations • 14 Apr 2020 • Andrea Caputo, Hongwan Liu, Siddharth Mishra-Sharma, Joshua T. Ruderman
A dark photon may kinetically mix with the Standard Model photon, leading to observable cosmological signatures.
Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology
2 code implementations • 4 Mar 2020 • Siddharth Mishra-Sharma, Ken Van Tilburg, Neal Weiner
Astrometric weak gravitational lensing is a powerful probe of the distribution of matter on sub-Galactic scales, which harbor important information about the fundamental nature of dark matter.
Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena Instrumentation and Methods for Astrophysics High Energy Physics - Phenomenology
2 code implementations • 12 Feb 2020 • Andrea Caputo, Hongwan Liu, Siddharth Mishra-Sharma, Joshua T. Ruderman
A dark photon may kinetically mix with the ordinary photon, inducing oscillations with observable imprints on cosmology.
Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology
3 code implementations • 4 Sep 2019 • Johann Brehmer, Siddharth Mishra-Sharma, Joeri Hermans, Gilles Louppe, Kyle Cranmer
The subtle and unique imprint of dark matter substructure on extended arcs in strong lensing systems contains a wealth of information about the properties and distribution of dark matter on small scales and, consequently, about the underlying particle physics.
1 code implementation • 12 Sep 2018 • Siddharth Mishra-Sharma
This framework is then applied to Fermi data and existing group catalogs to search for annihilating dark matter in extragalactic galaxies and clusters.
Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology
no code implementations • 1 Sep 2017 • Mariangela Lisanti, Siddharth Mishra-Sharma, Nicholas L. Rodd, Benjamin R. Safdi, Risa H. Wechsler
Applying this procedure to a catalog of sources, one can create a full-sky map of the brightest extragalactic dark matter targets in the nearby Universe ($z\lesssim 0. 03$), supplementing sources of dark matter annihilation from within the Local Group.
Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
1 code implementation • 30 Aug 2017 • Mariangela Lisanti, Siddharth Mishra-Sharma, Nicholas L. Rodd, Benjamin R. Safdi
We use 413 weeks of publicly-available $\textit{Fermi}$ Pass 8 gamma-ray data, combined with recently-developed galaxy group catalogs, to search for evidence of dark matter annihilation in extragalactic halos.
Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
1 code implementation • 9 Dec 2016 • Siddharth Mishra-Sharma, Nicholas L. Rodd, Benjamin R. Safdi
The NPTF was first applied to Fermi gamma-ray data to give evidence that the excess of ~GeV gamma-rays observed in the inner regions of the Milky Way likely arises from a population of sub-threshold point sources, and the NPTF has since found additional applications studying sub-threshold extragalactic sources at high Galactic latitudes.
High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics Instrumentation and Methods for Astrophysics High Energy Physics - Phenomenology