activity
19962023
most citedMulti-Wavelength Observations of Supernova 2011ei: Time-Dependent Classification of Type IIb and Ib Supernovae and Implications for their Progenitors

93 citations · 643 across the 24 of their papers we have counts for

collaborators

25 papers

astro-ph.HE2023★ 11 cited

A Numerical Study of the Impact of Jet Magnetic Topology on Radio Galaxy Evolution

Yi-Hao Chen, Sebastian Heinz, Eric Hooper

The propagation of active galactic nucleus jets depends both on the environment into which they propagate and on their internal structure. To test the impact that different magneti…

astro-ph.GA2023★ 24 cited

A Quick Look at the 3GHz Radio Sky. II. Hunting for DRAGNs in the VLA Sky Survey

Yjan A. Gordon, Lawrence Rudnick, Heinz Andernach +9

Active Galactic Nuclei (AGN) can often be identified in radio images as two lobes, sometimes connected to a core by a radio jet. This multi-component morphology unfortunately creat…

astro-ph.GA2022

How does environment affect the morphology of radio AGN?

Melissa Elizabeth Morris, Eric Wilcots, Eric Hooper +1

Galaxies hosting Active Galactic Nuclei (AGN) with bent radio jets are used as tracers of dense environments, such as galaxy groups and clusters. The assumption behind using these…

astro-ph.IM2018

The WIYN One Degree Imager in 2018: An Extended 30-Detector Focal Plane

Daniel R. Harbeck, Mike Lesser, Wilson Liu +14

We report on the upgraded One Degree Imager (ODI) at the WIYN 3.5 meter telescope at the Kitt Peak Observatory after the focal plane was expanded by an additional seventeen detecto…

astro-ph.GA2014★ 4 cited

Simple Stellar Population Modeling of Low S/N Galaxy Spectra and Quasar Host Galaxy Applications

Gregory Mosby, Christy Tremonti, Eric Hooper +3

To study the effect of supermassive black holes (SMBHs) on their host galaxies it is important to study the hosts when the SMBH is near its peak activity. A method to investigate t…

astro-ph.SR2013★ 33 cited

Abell 48 - a rare WN-type central star of a planetary nebula

H. Todt, A. Y. Kniazev, V. V. Gvaramadze +18

A considerable fraction of the central stars of planetary nebulae (CSPNe) are hydrogen-deficient. Almost all of these H-deficient central stars (CSs) display spectra with strong ca…