activity
20022023
most citedClues to Nuclear Star Cluster Formation from Edge-on Spirals

169 citations · 794 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2023

Empirical 2MASS-WFC3/IR filter transformations from synthetic photometry

M. J. Durbin, R. L. Beaton, A. J. Monson +2

Near-infrared bandpasses on spaceborne observatories diverge from their ground-based counterparts as they are free of atmospheric telluric absorption. Available transformations bet…

astro-ph.CO2009★ 46 cited

Photometric redshifts and cluster tomography in the ESO Distant Cluster Survey

R. Pello, G. Rudnick, G. De Lucia +17

This paper reports the results obtained on the photometric redshifts measurement and accuracy, and cluster tomography in the ESO Distant Cluster Survey (EDisCS) fields. Photometric…

astro-ph.CO2009★ 114 cited

Feedback and the Formation of Dwarf Galaxy Stellar Halos

Greg Stinson, Julianne Dalcanton, Tom Quinn +3

Stellar population studies show that low mass galaxies in all environments exhibit stellar halos that are older and more spherically distributed than the main body of the galaxy. I…

astro-ph2007★ 168 cited

Breathing in Low Mass Galaxies: A Study of Episodic Star Formation

G. S. Stinson, J. J. Dalcanton, T. Quinn +2

We simulate the collapse of isolated dwarf galaxies using SPH + N-Body simulations including a physically motivated description of the effects of supernova feedback. As the gas col…

astro-ph2007★ 152 cited

The Morphological Content of Ten EDisCS Clusters at 0.5 < z < 0.8

V. Desai, J. J. Dalcanton, A. Aragon-Salamanca +12

We describe Hubble Space Telescope (HST) imaging of 10 of the 20 ESO Distant Cluster Survey (EDisCS) fields. Each ~40 square arcminute field was imaged in the F814W filter with the…

astro-ph2006★ 169 cited

Clues to Nuclear Star Cluster Formation from Edge-on Spirals

Anil C. Seth, Julianne J. Dalcanton, Paul W. Hodge +1

We find 9 nuclear cluster candidates in a sample of 14 edge-on, late-type galaxies observed with HST/ACS. These clusters have magnitudes (M_I ~ -11) and sizes (r_eff ~ 3pc) similar…