359 citations · 637 across the 13 of their papers we have counts for
13 papers
A compact time-frequency representation for gravitational-wave data analysis
Noah Pearson, Mesut Çalışkan, Sophie Bini +1
Time-frequency (wavelet) domain analyses are seeing greater use for gravitational-wave data analysis due to the advantages they have in handling non-stationary noise. A popular cho…
The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries
David Izquierdo-Villalba, Melanie Habouzit, Matteo Bonetti +67
In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the…
A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
Neha Anil Kumar, Mesut Çalışkan, Selim C. Hotinli +2
Recent advancements in small-scale observations of the cosmic microwave background (CMB) have provided a unique opportunity to characterize the distribution of baryons in the outsk…
Multi-messenger Gravitational Lensing
Graham P. Smith, Tessa Baker, Simon Birrer +38
We introduce the rapidly emerging field of multi-messenger gravitational lensing - the discovery and science of gravitationally lensed phenomena in the distant universe through the…
Dissecting the Stochastic Gravitational Wave Background with Astrometry
Mesut Çalışkan, Yifan Chen, Liang Dai +3
Astrometry, the precise measurement of star motions, offers an alternative avenue to investigate low-frequency gravitational waves through the spatial deflection of photons, comple…
Linear polarization of the stochastic gravitational-wave background with pulsar timing arrays
Neha Anil Kumar, Mesut Çalışkan, Gabriela Sato-Polito +2
Pulsar-timing collaborations have recently reported evidence for the detection of an isotropic stochastic gravitational-wave background consistent with one sourced by a population…
Reconstructing patchy helium reionization using the cosmic microwave background and large-scale structure
Mesut Çalışkan, Neha Anil Kumar, Selim C. Hotinli +1
The intergalactic helium became fully ionized by the end of cosmic noon (). Similarly to the reionization of hydrogen, helium reionization is expected to be patchy, driven…
Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
Mesut Çalışkan, Neha Anil Kumar, Lingyuan Ji +4
The Laser Interferometer Space Antenna (LISA) will detect gravitational waves (GWs) emitted by massive black hole binaries (MBHBs) in the low-frequency (mHz) band. Low-mass l…
Subtracting Compact Binary Foregrounds to Search for Subdominant Gravitational-Wave Backgrounds in Next-Generation Ground-Based Observatories
Bei Zhou, Luca Reali, Emanuele Berti +4
Stochastic gravitational-wave backgrounds (SGWBs) derive from the superposition of numerous individually unresolved gravitational-wave (GW) signals. Detecting SGWBs provides us wit…
Cosmology with the Laser Interferometer Space Antenna
Pierre Auclair, David Bacon, Tessa Baker +177
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravita…
Lensing or luck? False alarm probabilities for gravitational lensing of gravitational waves
Mesut Çalışkan, Jose María Ezquiaga, Otto A. Hannuksela +1
Strong gravitational lensing of gravitational waves (GWs) has been forecasted to become detectable in the upcoming observing runs. However, definitively distinguishing pairs of len…
Tungsten Thermionic Emission as a Gauge for Low Pressures of Cesium Vapor
João F. Shida, Fangjian Wu, Eric Spieglan +1
Heated metal filaments under electric fields and low pressures of alkali metal gaseject electrons by thermionic emission as a function of the pressure of the gas and thetemperature…
Localizing merging black holes with sub-arcsecond precision using gravitational-wave lensing
Otto A. Hannuksela, Thomas E. Collett, Mesut Çalışkan +1
The current gravitational-wave localization methods rely mainly on sources with electromagnetic counterparts. Unfortunately, a binary black hole does not emit light. Due to this, i…