activity
20102023
most citedMilky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant

616 citations · 2.2k across the 52 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2023★ 11 cited

Standardized Luminosity of the Tip of the Red Giant Branch utilizing Multiple Fields in NGC 4258 and the CATs Algorithm

Siyang Li, Adam G. Riess, Dan Scolnic +6

The Tip of the Red Giant Branch provides a luminous standard candle for calibrating distance ladders that reach Type Ia supernova (SN Ia) hosts. However, recent work reveals that t…

astro-ph.GA2023★ 14 cited

Reeling in the Whirlpool: the distance to M 51 clarified by Cepheids and the Type IIP SN 2005cs

G. Csörnyei, R. I. Anderson, C. Vogl +4

Despite being one of the best-known galaxies, the distance to the Whirlpool Galaxy, M 51, is still debated. Current estimates range from 6.02 to 9.09 Mpc, and different methods yie…

astro-ph.GA2023★ 1 cited

Young stellar distance indicators and the extragalactic distance scale

Richard I. Anderson

The extragalactic distance scale is perhaps the most important application of stellar distance indicators. Among these, classical Cepheids are high-accuracy standard candles that s…

astro-ph.GA2022★ 36 cited

Do the majority of stars form as gravitationally unbound?

František Dinnbier, Pavel Kroupa, Richard I. Anderson

Some of the youngest stars (age Myr) are clustered, while many others are observed scattered throughout star forming regions or in complete isolation. It has been int…

astro-ph.GA2021★ 12 cited

On the dynamical evolution of Cepheids in star clusters

František Dinnbier, Richard I. Anderson, Pavel Kroupa

We investigate the occurrence of classical (type-I) Cepheid variable stars (henceforth: Cepheids) in dynamically evolving star clusters from birth to an age of approximately 300 My…

astro-ph.GA2012★ 83 cited

Cepheids in Open Clusters: An 8-D All-sky Census

Richard I. Anderson, Laurent Eyer, Nami Mowlavi

Cepheids in open clusters (cluster Cepheids: CCs) are of great importance as zero-point calibrators of the Galactic Cepheid period-luminosity relationship (PLR). We perform an 8-di…