activity
20032009
most citedNew Constraints on the Lyman Continuum Escape Fraction at z~1.3

167 citations · 271 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.CO200929 cited

Structures of Local Galaxies Compared to High Redshift Star-forming Galaxies

Sara M. Petty, Duilia F. de Mello, John S. Gallagher +4

The rest-frame far-ultraviolet (FUV) morphologies of 8 nearby interacting and starburst galaxies (Arp 269, M 82, Mrk 8, NGC 520, NGC 1068, NGC 3079, NGC 3310, NGC 7673) are compare…

astro-ph200769 cited

Star-formation in the HI bridge between M81 and M82

Duilia F. de Mello, L. J. Smith, E. Sabbi +3

We present multi-wavelength observations of stellar features in the HI tidal bridge connecting M81 and M82 in the region called Arp's Loop. We identify eight young star-forming reg…

astro-ph2007167 cited

New Constraints on the Lyman Continuum Escape Fraction at z~1.3

Brian Siana, Harry I. Teplitz, James Colbert +8

We examine deep far-ultraviolet (1600 Angstrom) imaging of the Hubble Deep Field-North (HDFN) and the Hubble Ultra Deep Field (HUDF) to search for leaking Lyman continuum radiation…

astro-ph20066 cited

Near Ultraviolet sources in the Great Observatories Origins Deep Survey Fields

Duilia de Mello, T. Dahlen, J. P. Gardner +1

We present an Ultraviolet (UV) selected sample of 268 objects in the two fields of the Great Observatories Origins Deep Survey (GOODS). We used the parallel observations taken with…

astro-ph2004

The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models

L. -G. Strolger, A. G. Riess, T. Dahlen +33

We present results from the Hubble Higher-z Supernova Search, the first space-based open field survey for supernovae (SNe). In cooperation with the Great Observatories Origins Deep…

astro-ph2003

Evolution in the Colors of Lyman-Break Galaxies from Z~4 to Z~3

Casey Papovich, Mark Dickinson, Henry C. Ferguson +11

The integrated colors of distant galaxies provide a means for interpreting the properties of their stellar content. Here, we use rest-frame UV-to-optical colors to constrain the sp…