Eric C. Bellm

Bulge RR Lyrae stars in the VVV tile b201

A large systematic search for close supermassive binary and rapidly recoiling black holes – III. Radial velocity variations

The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

The X‐Ray‐Emitting Components toward ℓ = 111o: The Local Hot Bubble and Beyond

Type Ia Supernovae Are Excellent Standard Candles in the Near-infrared

Near-infrared variability study of the central 2.3 × 2.3 arcmin2 of the Galactic Centre – II. Identification of RR Lyrae stars in the Milky Way nuclear star cluster

AN X-RAY-SELECTED GALAXY CLUSTER IN THE LOCKMAN HOLE AT REDSHIFT 1.753

A Hidden Friend for the Galactic Center Black Hole, Sgr A*

A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s⁻¹ Mpc⁻¹ Uncertainty from the Hubble Space Telescope and the SH0ES Team

Corral framework: Trustworthy and fully functional data intensive parallel astronomical pipelines

On the use of deep learning for computational imaging

Coded-aperture imaging systems: Past, present and future development – A review

The Zwicky transient facility observing system

TRACING THE ORPHAN STREAM TO 55 kpc WITH RR LYRAE STARS

A population of short-period variable quasars from PTF as supermassive black hole binary candidates

Laboratory coded-aperture imaging experiments: radial hole coded masks and depth-sensitive CZT detectors

Origins of the 1/4 keV Soft X-Ray Background

Origins of the \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\frac{1}{4}$ \end{document} keV Soft X‐Ray Background

The IPAC Image Subtraction and Discovery Pipeline for the Intermediate Palomar Transient Factory