activity
20002020
most citedThe Hubble Deep Fields

135 citations · 636 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.SR2020★ 3 cited

Line Identification and Excitation of Autoionizing States in a Late-Type, Low Mass Wolf-Rayet Star

Robert Williams, Catherine Manea, Bruce Margon +1

Identifications of a large fraction of previously unidentified lines in the complex spectrum of the low mass, late-type LMC [WC11] star J060819.93-715737.4 have been made utilizing…

astro-ph.IM2020★ 6 cited

Hubble Telescope 30 Years in Orbit: Personal Reflections

Robert Williams

With an initial requirement to make observations a minimum of 5-10 years, Hubble Space Telescope (HST) has continued to operate well for 30 years. It has relied upon five servicing…

astro-ph.SR2018★ 12 cited

The Long-Term Secular Mass Accretion Rate of the Recurrent Nova T Pyxidis

Patrick Godon, Edward Sion, Robert Williams +1

We present Hubble Space Telescope ultraviolet spectroscopy of the recurrent nova T Pyxidis obtained more than 5 years after its 2011 outburst indicating that the system might not h…

astro-ph.SR2016

Third Parameter Classification of Transients and Novae Ejecta as Ballistically Ejected Globules

Robert Williams

A third parameter, in addition to luminosity and rate of brightness decline, derived from the spectra of transients is suggested as a means of more accurately classifying objects i…

astro-ph.SR2016★ 62 cited

A Systematic Study of Mid-Infrared Emission from Core-Collapse Supernovae with SPIRITS

Samaporn Tinyanont, Mansi M. Kasliwal, Ori D. Fox +12

We present a systematic study of mid-infrared (mid-IR) emission from 141 nearby supernovae (SNe) observed with the InfraRed Array Camera (IRAC) on Spitzer.These SNe reside in one o…

astro-ph.SR2015★ 89 cited

Early optical spectra of nova V1369 Cen show presence of Lithium

L. Izzo, M. Della Valle, E. Mason +10

We present early high resolution spectroscopic observations of the nova V1369 Cen. We have detected an absorption feature at 6695.6 Å\, that we have identified as blue--shifted $^7…