activity
20032009
most citedH-delta in the Integrated Light of Galaxies: What Are We Actually Measuring?

18 citations · 26 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

17 papers · 1 filter

astro-ph2008139 cited

Dissecting the Red Sequence--I. Star Formation Histories of Quiescent Galaxies: The Color-Magnitude vs. the Color-Sigma Relation

Genevieve J. Graves, S. M. Faber, Ricardo P. Schiavon

We use a sample of ~16,000 non-emission line galaxies from the SDSS to investigate the physical parameters underlying the well-known color-magnitude and color-sigma relations. Gala…

astro-ph2008140 cited

Star Clusters in M31: I. A Catalog and a Study of the Young Clusters

Nelson Caldwell, Paul Harding, Heather Morrison +3

We present an updated catalog of 1300 objects in the field of M31, including 670 likely star clusters of various types. Archival images were inspected to confirm cluster classifica…

astro-ph2008162 cited

APOGEE: The Apache Point Observatory Galactic Evolution Experiment

C. Allende Prieto, S. R. Majewski, R. Schiavon +8

APOGEE is a large-scale, NIR, high-resolution (R~20,000) spectroscopic survey of Galactic stars. It is one of the four experiments in SDSS-III. Because APOGEE will observe in the H…

astro-ph20088 cited

Abundance variations in the globular cluster M71 (NGC 6838)

A. Alves-Brito, R. P. Schiavon, B. Castilho +1

Abundance variations in moderately metal-rich globular clusters can give clues about the formation and chemical enrichment of globular clusters. CN, CH, Na, Mg and Al indices in sp…

astro-ph2008142 cited

Measuring Ages and Elemental Abundances from Unresolved Stellar Populations: Fe, Mg, C, N, and Ca

Genevieve J. Graves, Ricardo P. Schiavon

We present a method for determining mean light-weighted ages and abundances of Fe, Mg, C, N, and Ca, from medium resolution spectroscopy of unresolved stellar populations. The meth…

astro-ph2007123 cited

Ages and Abundances of Red Sequence Galaxies as a Function of LINER Emission Line Strength

Genevieve J. Graves, Sandra M. Faber, Ricardo P. Schiavon +1

Although the spectrum of a prototypical early-type galaxy is assumed to lack emission lines, a substantial fraction (likely as high as 30%) of nearby red sequence galaxy spectra co…