papers

Publications (14)

astro-ph.GA2014

A substantial population of massive quiescent galaxies at z~4 from ZFOURGE

Caroline M. S. Straatman, Ivo Labbé, Lee R. Spitler +21

We report the likely identification of a substantial population of massive M~10^11M_Sun galaxies at z~4 with suppressed star formation rates (SFRs), selected on rest-frame optical…

astro-ph.CO2012

First Results from Z-FOURGE: Discovery of a Candidate Cluster at z = 2.2 in COSMOS

Lee R. Spitler, Ivo Labbé, Karl Glazebrook +13

We report the first results from the Z-FOURGE survey: the discovery of a candidate galaxy cluster at z = 2.2 consisting of two compact overdensities with red galaxies detected at >…

astro-ph.HE2017

SPIRITS: Uncovering Unusual Infrared Transients With Spitzer

Mansi M. Kasliwal, John Bally, Frank Masci +44

We present an ongoing, systematic search for extragalactic infrared transients, dubbed SPIRITS --- SPitzer InfraRed Intensive Transients Survey. In the first year, using Spitzer/IR…

astro-ph.CO2013

Calibration of the Mid-Infrared Tully-Fisher Relation

Jenny G. Sorce, Helene M. Courtois, R. Brent Tully +7

Distance measures on a coherent scale around the sky are required to address the outstanding cosmological problems of the Hubble Constant and of departures from the mean cosmic flo…

astro-ph.CO2012

Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant

Wendy L. Freedman, Barry F. Madore, Victoria Scowcroft +5

Using a mid-infrared calibration of the Cepheid distance scale based on recent observations at 3.6 um with the Spitzer Space Telescope, we have obtained a new, high-accuracy calibr…

astro-ph.CO2011

The Carnegie Hubble Program

Wendy L. Freedman, Barry F. Madore, Vicky Scowcroft +6

We present an overview of and preliminary results from an ongoing comprehensive program that has a goal of determining the Hubble constant to a systematic accuracy of 2%. As part o…

astro-ph.IM2025

POKEMON: print optimization for kilo-fiber experiments using micro-optics and nanostructures

Megan Delamer, Suvrath Mahadevan, Chad Bender +7

The most pressing problems in modern astrophysics have often required the largest telescopes. With the cost scaling of mirror diameters, the field as a whole is faced with a challe…

astro-ph.GA2013

A Preliminary Calibration of the RR Lyrae Period-Luminosity Relation at Mid-Infrared Wavelengths: WISE Data

Barry F. Madore, Douglas Hoffman, Wendy L. Freedman +6

Using time-resolved, mid-infrared data from WISE and geometric parallaxes from HST for four Galactic RR Lyrae variables, we derive the following Population II Period-Luminosity (PL…

astro-ph.EP2025

The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems

Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson +26

We present a set of companion dynamical masses and orbital parameters of seven star systems from the NEID Earth Twin Survey with significant absolute astrometric accelerations betw…

astro-ph.GA2015

The Differential Size Growth of Field and Cluster Galaxies at z=2.1 Using the ZFOURGE Survey

Rebecca J. Allen, Glenn G. Kacprzak, Lee R. Spitler +13

There is ongoing debate regarding the extent that environment affects galaxy size growth beyond z>1. To investigate the differences in star-forming and quiescent galaxy properties…

astro-ph.EP2025

The First Spin-Orbit Obliquity of an M dwarf/brown dwarf System: An eccentric and aligned TOI-2119 b

Lauren Doyle, Caleb I. Cañas, Jessica E. Libby-Roberts +15

We report the first instance of an M dwarf/brown dwarf obliquity measurement for the TOI-2119 system using the Rossiter-McLaughlin effect. TOI-2119 b is a transiting brown dwarf or…

astro-ph.IM2019

Improving the Thermal Stability of a CCD Through Clocking

Cullen H. Blake, Dan Li, Joseph R. Tufts +6

Modern precise radial velocity spectrometers are designed to infer the existence of planets orbiting other stars by measuring few-nm shifts in the positions of stellar spectral lin…

astro-ph.GA2015

The Carnegie Hubble Program: The Distance and Structure of the SMC as Revealed by Mid-infrared Observations of Cepheids

Victoria Scowcroft, Wendy L. Freedman, Barry F. Madore +5

Using Spitzer observations of classical Cepheids we have measured the true average distance modulus of the SMC to be mag (corresponding to $6…

astro-ph.EP2025

The Super-Puff WASP-193b is On A Well-Aligned Orbit

Samuel W. Yee, Gudmundur Stefansson, Daniel Thorngren +8

The "super-puffs" are a population of planets that have masses comparable to that of Neptune but radii similar to Jupiter, leading to extremely low bulk densities ($ρ_p \lesssim 0…