activity
20162026
most citedAstrometric Limits on the Stochastic Gravitational Wave Background

42 citations · 96 across the 6 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2026

The Nancy Grace Roman Space Telescope Wide Field Instrument: Characterization of the Brighter-Fatter Effect in a Roman H4RG-10 Detector using the Talbot Effect

Jennie Paine, Ami Choi, Christopher Merchant +14

The Nancy Grace Roman Space Telescope will conduct several community-driven surveys using its Wide Field Instrument (WFI), which contains 18 Teledyne H4RG-10 near-infrared detector…

astro-ph.IM2026

Nancy Grace Roman Space Telescope Wide Field Instrument: Bright Point Source Saturation Response and Persistence Properties from Thermal-Vacuum Testing

Dana R. Louie, Robert F. Wilson, Thomas Barclay +19

The Nancy Grace Roman Space Telescope's Wide Field Instrument (WFI) will observe hundreds of thousands of bright stars across its Core Community Surveys, particularly in the dense…

astro-ph.CO2026

Impact and interplay of CDM analysis choices for LSST cosmic shear

N. C. Robertson, C. Heymans, J. Zuntz +9

We forecast cosmological parameter constraints for a cosmic shear analysis of the Rubin Observatory Legacy Survey of Space and Time (LSST), defining an analysis framework that can…

astro-ph.GA2023

An Updated Reference Frame for the Galactic Inner Parsec

Jeremy Darling, Jennie Paine, Mark J. Reid +3

Infrared observations of stellar orbits about Sgr A* probe the mass distribution in the inner parsec of the Galaxy and provide definitive evidence for the existence of a massive bl…

astro-ph.GA2021★ 3 cited

3D Kinematics of Stellar SiO Masers in the Galactic Center

Jennie Paine, Jeremy Darling

We present 3D velocity measurements and acceleration limits for stars within a few parsec of the Galactic Center (GC) black hole, Sgr A*, based on observations of 43 and 86 GHz cir…

astro-ph.CO2019★ 12 cited

Secular Extragalactic Parallax: Measurement Methods and Predictions for Gaia

Jennie Paine, Jeremy Darling, Romain Graziani +1

Secular extragalactic parallax caused by the solar system's velocity relative to the cosmic microwave background rest frame may be observable as a dipole proper motion field with a…

astro-ph.CO2019

Extragalactic Proper Motions: Gravitational Waves and Cosmology

Jeremy Darling, Alexandra Truebenbach, Jennie Paine

Extragalactic proper motions can reveal a variety of cosmological and local phenomena over a range of angular scales. These include observer-induced proper motions, such as the sec…

astro-ph.CO2018

Extragalactic Proper Motions: Gravitational Waves and Cosmology

Jeremy Darling, Alexandra Truebenbach, Jennie Paine

Extragalactic proper motions can reveal a variety of cosmological and local phenomena over a range of angular scales. These include observer-induced proper motions, such as the sec…

astro-ph.GA2018★ 12 cited

The Gaia-WISE Extragalactic Astrometric Catalog

Jennie Paine, Jeremy Darling, Alexandra Truebenbach

The Gaia mission has detected a large number of active galactic nuclei (AGN) and galaxies, but these objects must be identified among the 1000-fold more numerous stars. Extant astr…

astro-ph.IM2018★ 42 cited

Astrometric Limits on the Stochastic Gravitational Wave Background

Jeremy Darling, Alexandra E. Truebenbach, Jennie Paine

The canonical methods for gravitational wave detection are ground- and space-based laser interferometry, pulsar timing, and polarization of the cosmic microwave background. But as…

astro-ph.GA2016★ 27 cited

The Geometry of the Infrared and X-ray Obscurer in a Dusty Hyperluminous Quasar

Duncan Farrah, Mislav Balokovic, Daniel Stern +24

We study the geometry of the AGN obscurer in IRAS 09104+4109, an IR-luminous, radio-intermediate FR-I source at , using infrared data from Spitzer and Herschel, X-ray data…