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Distances of galaxies in the Hubble Space Telescope Key Project are based on the Cepheid period-luminosity relation. An alternative basis is the tip of the red giant branch. Using archival HST data, we calibrate the infrared Tully-Fisher…

Astrophysics · Physics 2011-02-11 Jeremy Mould , Shoko Sakai

The extragalactic distance scale is perhaps the most important application of stellar distance indicators. Among these, classical Cepheids are high-accuracy standard candles that support a $1.4\%$ measurement of Hubble's constant, $H_0$.…

Astrophysics of Galaxies · Physics 2023-03-01 Richard I. Anderson

A Cepheid-based calibration is derived for four distance indicators that utilize stars in the old stellar populations: the tip of the red giant branch (TRGB), the planetary nebula luminosity function (PNLF), the globular cluster luminosity…

New theoretical evaluations of the Red Giant Branch Tip (TRGB) luminosity, by adopting the most updated physical inputs in computing canonical stellar models, are presented. Theoretical relations for the run of the TRGB bolometric and I…

Astrophysics · Physics 2015-06-24 M. Salaris , S. Cassisi

We review the use of Cepheids as distance indicators with particular emphasis on the methods which have been applied to HST observations of Cepheids. The calibration of the period-luminosity relations is examined in detail and we identify…

Astrophysics · Physics 2007-05-23 N. R. Tanvir

We have used the Wide Field and Planetary Camera 2 on board the Hubble Space Telescope to obtain V and I images of seven nearby galaxies. For each, we have measured a distance using the tip of the red giant branch (TRGB) method. By…

Astrophysics · Physics 2009-11-10 Shoko Sakai , Laura Ferrarese , Rob Kennicutt , Abi Saha

The final efforts of the HST Key Project on the Extragalactic Distance Scale are presented. Four distance indicators, the Surface Brightness Fluctuation method, the Fundamental Plane for early-type galaxies, the Tully-Fisher relation and…

We present an overview of the Carnegie-Chicago Hubble Program, an ongoing program to obtain a 3 per cent measurement of the Hubble constant using alternative methods to the traditional Cepheid distance scale. We aim to establish a…

Since the launch of the Hubble Space Telescope nine years ago, Cepheid distances to 25 galaxies have been determined for the purpose of calibrating secondary distance indicators. A variety of these can now be calibrated, and the…

The cosmological distance ladder crucially depends on classical Cepheids (with P=3-80 days), which are primary distance indicators up to 33 Mpc. Within this volume, very few SNe Ia have been calibrated through classical Cepheids, with…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-16 G. Fiorentino , G. Clementini , M. Marconi , I. Musella , A. Saha , M. Tosi , R. Contreras Ramos , F. Annibali , A. Aloisi , R. van der Marel

The extragalactic distance scale relies heavily on Cepheids. However, it has become clear from observations and pulsation models that the slope and zero point of their P-L relations differ from galaxy to galaxy. This makes the determination…

Astrophysics · Physics 2009-11-13 G. A. Tammann , A. Sandage , B. Reindl

While the tip of the red giant branch (TRGB) has been used as a distance indicator since the early 1990's, its application to measure the Hubble Constant as a primary distance indicator occurred only recently. The TRGB is also currently at…

Cosmology and Nongalactic Astrophysics · Physics 2024-04-02 Siyang Li , Rachael L. Beaton

The tip of the red giant branch has been used to measure distances to 500 nearby galaxies with the Hubble Space Telescope (HST) which are available in the Color-Magnitude Diagrams and Tip of the Red Giant Branch (CMDs/TRGB) catalog on the…

Cosmology and Nongalactic Astrophysics · Physics 2022-06-15 Gagandeep S. Anand , R. Brent Tully , Luca Rizzi , Adam G. Riess , Wenlong Yuan

Six of the principal galaxy distance indicators are discussed: Cepheid variables, the Tully-Fisher relation, the Dn-sigma relation, Surface Brightness Fluctuations, Brightest Cluster Galaxies, and Type Ia Supernovae. The role they play in…

Astrophysics · Physics 2007-05-23 Jeffrey A. Willick

The luminosity of the Tip of the Red Giant Branch (TRGB) provides an excellent measure of galaxy distances and is easily determined in the resolved images of nearby galaxies observed with Hubble Space Telescope. There is now a large amount…

The Hubble Tension, a >5 sigma discrepancy between direct and indirect measurements of the Hubble constant (H0), has persisted for a decade and motivated intense scrutiny of the paths used to infer H0. Comparing independently-derived…

The theoretical evaluations of the Red Giant Branch Tip (TRGB) luminosity presented in Salaris & Cassisi (1997) are extended to higher metallicities, and compared with analogous independent results recently published. The comparison between…

Astrophysics · Physics 2009-10-30 M. Salaris , S. Cassisi

The relationship between the integrated H$\beta$ line luminosity and the velocity dispersion of the ionized gas of HII galaxies and giant HII regions represents an exciting standard candle that presently can be used up to redshifts…

Cosmology and Nongalactic Astrophysics · Physics 2023-09-28 David Fernández-Arenas , Ricardo Chávez

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 of this program, we are currently obtaining 3.6 micron data…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Wendy L. Freedman , Barry F. Madore , Vicky Scowcroft , Andy Monson , S. E. Persson , Mark Seibert , Jane Rigby , Laura Sturch , Peter Stetson

Blue supergiant distances of nearby galaxies obtained with the flux-weighted gravity-luminosity relationship are used for a measurement of the zero points of Tully-Fisher relationships at different photometric passbands. The Cousins I-band…

Cosmology and Nongalactic Astrophysics · Physics 2025-10-24 Rolf-Peter Kudritzki , Fabio Bresolin , Miguel A. Urbaneka , Eva Sextl
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