402 citations · 1.2k across the 25 of their papers we have counts for
25 papers
Method to search for inspiraling planetary-mass ultra-compact binaries using the generalized frequency-Hough transform in LIGO O3a data
Andrew L. Miller, Nancy Aggarwal, Sebastien Clesse +6
Gravitational waves from sub-solar mass primordial black holes could be detected in LIGO, Virgo and KAGRA data. Here, we apply a method originally designed to look for rapidly spin…
Enabling multi-messenger astronomy with continuous gravitational waves: early warning and sky localization of binary neutron stars in Einstein Telescope
Andrew L. Miller, Neha Singh, Cristiano Palomba
Next-generation gravitational-wave detectors will provide unprecedented sensitivity to inspiraling binary neutron stars and black holes, enabling detections at the peak of star for…
Characterizing Gravitational Wave Detector Networks: From A to Cosmic Explorer
Ish Gupta, Chaitanya Afle, K. G. Arun +44
Gravitational-wave observations by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo have provided us a new tool to explore the Universe on all scales from n…
Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee
Matthew Evans, Alessandra Corsi, Chaitanya Afle +73
Gravitational-wave astronomy has revolutionized humanity's view of the universe, a revolution driven by observations that no other field can make. This white paper describes an obs…
Recent results from continuous gravitational wave searches using data from LIGO/Virgo/KAGRA's third observing run
Andrew L. Miller
The third observing run of advanced LIGO, Virgo and KAGRA brought unprecedented sensitivity towards a variety of quasi-monochromatic, persistent gravitational-wave signals. Continu…
Science with the Einstein Telescope: a comparison of different designs
Marica Branchesi, Michele Maggiore, David Alonso +73
The Einstein Telescope (ET), the European project for a third-generation gravitational-wave detector, has a reference configuration based on a triangular shape consisting of three…
First search for ultralight dark matter with a space-based gravitational-wave antenna: LISA Pathfinder
Andrew L. Miller, Luis Mendes
We present here results from the first-ever search for dark photon dark matter that could have coupled to baryons in LISA Pathfinder, the technology demonstrator for a space-based…
Probing the pulsar explanation of the Galactic-Center GeV excess using continuous gravitational-wave searches
Andrew L. Miller, Yue Zhao
Over ten years ago, Fermi observed an excess of GeV gamma rays from the Galactic Center whose origin is still under debate. One explanation for this excess involves annihilating da…
Measuring neutron-star distances and properties with gravitational-wave parallax
Magdalena Sieniawska, David Ian Jones, Andrew Lawrence Miller
Gravitational-wave astronomy allows us to study objects and events invisible to electromagnetic waves. So far, only signals triggered by coalescing binaries have been detected. How…
Assessing the impact of non-Gaussian noise on convolutional neural networks that search for continuous gravitational waves
Takahiro S. Yamamoto, Andrew L. Miller, Magdalena Sieniawska +1
We present a convolutional neural network that is capable of searching for continuous gravitational waves, quasi-monochromatic, persistent signals arising from asymmetrically rotat…
Distinguishing between dark-matter interactions with gravitational-wave detectors
Andrew L. Miller, Francesca Badaracco, Cristiano Palomba
Ground-based gravitational-wave interferometers could directly probe the existence of ultralight dark matter ( eV/) that couples to standard-mo…
Searching for Mini Extreme Mass Ratio Inspirals with Gravitational-Wave Detectors
Huai-Ke Guo, Andrew Miller
A compact object with a mass , such as a black hole of stellar or primordial origin or a neutron star, and a much lighter exotic compact object…
Stochastic gravitational-wave background searches and constraints on neutron-star ellipticity
Federico De Lillo, Jishnu Suresh, Andrew L. Miller
Rotating neutron stars (NSs) are promising sources of gravitational waves (GWs) in the frequency band of ground-based detectors. They are expected to emit quasi-monochromatic, long…
Detection of Early-Universe Gravitational Wave Signatures and Fundamental Physics
Robert Caldwell, Yanou Cui, Huai-Ke Guo +34
Detection of a gravitational-wave signal of non-astrophysical origin would be a landmark discovery, potentially providing a significant clue to some of our most basic, big-picture…
Constraints on planetary and asteroid-mass primordial black holes from continuous gravitational-wave searches
Andrew L. Miller, Nancy Aggarwal, Sébastien Clesse +1
We present new constraints on the merging rates of planetary-mass and asteroid-mass primordial black hole binaries using limits on continuous waves(quasi-monochromatic, quasi-infin…
Probing planetary-mass primordial black holes with continuous gravitational waves
Andrew L. Miller, Sébastien Clesse, Federico De Lillo +3
Gravitational waves can probe the existence of planetary-mass primordial black holes. Considering a mass range of , inspiraling primordial black holes cou…
Probing new light gauge bosons with gravitational-wave interferometers using an adapted semi-coherent method
Andrew L. Miller, Pia Astone, Giacomo Bruno +12
We adapt a method, originally developed for searches for quasi-monochromatic, quasi-infinite gravitational-wave signals, to directly detect new light gauge bosons with laser interf…
A Machine Learning Based Source Property Inference for Compact Binary Mergers
Deep Chatterjee, Shaon Ghosh, Patrick R. Brady +4
The detection of the binary neutron star (BNS) merger, GW170817, was the first success story of multi-messenger observations of compact binary mergers. The inferred merger rate alo…
Direct constraints on ultra-light boson mass from searches for continuous gravitational waves
Cristiano Palomba, Sabrina D'Antonio, Pia Astone +10
\textit{Superradiance} can trigger the formation of an ultra-light boson cloud around a spinning black hole. Once formed, the boson cloud is expected to emit a nearly periodic, lon…
How effective is machine learning to detect long transient gravitational waves from neutron stars in a real search?
Andrew L. Miller, Pia Astone, Sabrina D'Antonio +12
We present a comprehensive study of the effectiveness of Convolution Neural Networks (CNNs) to detect long duration transient gravitational-wave signals lasting fro…
Matched-filter study and energy budget suggest no detectable gravitational-wave 'extended emission' from GW170817
Miquel Oliver, David Keitel, Andrew L. Miller +2
Van Putten & Della Valle (2018) have reported a possible detection of gravitational-wave 'extended emission' from a neutron star remnant of GW170817. Starting from the time-frequen…
A method to search for long duration gravitational wave transients from isolated neutron stars using the generalized FrequencyHough
Andrew Miller, Pia Astone, Sabrina D'Antonio +10
We describe a method to detect gravitational waves lasting emitted by young, isolated neutron stars, such as those that could form after a supernova or a binary neu…
How beaming of gravitational waves compares to the beaming of electromagnetic waves: impacts to gravitational wave detection
Andrew L. Miller, Thulsi Wickramasinghe
We focus on understanding the beaming of gravitational radiation from gamma ray bursts (GRBs) by approximating GRBs as linearly accelerated point masses. For accelerated point mass…
A comparison of methods for the detection of gravitational waves from unknown neutron stars
Sinead Walsh, Matthew Pitkin, Miquel Oliver +17
Rapidly rotating neutron stars are promising sources of continuous gravitational wave radiation for the LIGO and Virgo interferometers. The majority of neutron stars in our galaxy…