collaborators

5 papers

astro-ph.GA2026

A 1% distance to the Large Magellanic Cloud measured by population-II pulsating stars using Gaia Data Release 3

Bastian Lengen, Richard I. Anderson, Mauricio Cruz Reyes

Population-II pulsating stars provide a route to extragalactic distances that is independent of the classical Cepheid distance scale and complementary to geometric and tip-of-the-r…

astro-ph.SR2026

Calibrating the Tip of the Red Giant Branch and measuring Magellanic Cloud distances to 2% exclusively with Gaia

Mauricio Cruz Reyes, Richard I. Anderson, Bastian Lengen

We have calibrated the Tip of the Red Giant Branch (TRGB) using our recent catalog of homogeneous, high-accuracy Globular Cluster (GC) distances. The GC distances were determined b…

astro-ph.CO2025

The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision

H0DN Collaboration, Stefano Casertano, Gagandeep Anand +35

The direct, empirical determination of the local value of the Hubble constant (H0) has markedly advanced thanks to improved instrumentation, measurement techniques, and distance es…

astro-ph.SR2025

A joint 1% calibration of the RR Lyrae & type-II Cepheid Leavitt laws yields homogeneous distances to 93 Galactic globular clusters

Bastian Lengen, Richard I. Anderson, Mauricio Cruz Reyes +1

Recent work has established large samples of astrometrically confirmed RR Lyrae and type-II Cepheid members of Galactic globular clusters (GCs). Any given GC can contain multiple s…

astro-ph.SR2025

Variable stars in Galactic globular clusters II. Population II Cepheids

Mauricio Cruz Reyes, Richard I. Anderson, Susmita Das

We identified a sample of 88 bona fide Population II Cepheids (henceforth referred to as Cepheids) and 44 candidates in Galactic globular clusters (GCs). Seventy-eight of the Cephe…