activity
20032020
most citedIdentification of 1.4 Million AGNs in the Mid-Infrared using WISE Data

165 citations · 1.3k across the 24 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2020★ 17 cited

Detection of a Radio Bubble around the Ultraluminous X-ray Source Holmberg IX X-1

Ciprian T. Berghea, Megan C. Johnson, Nathan J. Secrest +3

We present C and X-band radio observations of the famous utraluminous X-ray source (ULX) Holmberg IX X-1, previously discovered to be associated with an optical emission line nebul…

astro-ph.HE2016★ 10 cited

Spitzer IRAC observations of IR excess in Holmberg IX X-1: A circumbinary disk or a variable jet?

R. P. Dudik, C. T. Berghea, T. P. Roberts +4

We present Spitzer Infrared Array Camera (IRAC) photometric observations of the Ultra-luminous X-ray Source (ULX, X-1) in Holmberg IX. We construct a spectral energy distribution (…

astro-ph.HE2014★ 17 cited

The Local Environment of Ultraluminous X-ray Sources Viewed by XMM Newton's Optical Monitor

Ciprian T. Berghea, Rachel P. Dudik, Jonathan Tincher +1

We have used XMM-Newton's Optical Monitor (OM) images to study the local environment of a sample of 27 Ultraluminous X-ray Sources (ULXs) in nearby galaxies. UVW1 fluxes were extra…

astro-ph.HE2012★ 21 cited

Spitzer Observations of MF 16 Nebula and the associated Ultraluminous X-ray Source

Ciprian T. Berghea, Rachel P. Dudik

We present Spitzer Infrared Spectrograph (IRS) observations of the ultra-luminous X-ray source (ULX) NGC 6946 X-1 and its associated nebula MF 16. This ULX has very similar propert…

astro-ph.HE2009★ 36 cited

The First Detection of [O IV] from an Ultraluminous X-ray Source with Spitzer. II. Evidence for High Luminosity in Holmberg II ULX

C. T. Berghea, R. P. Dudik, K. A. Weaver +1

This is the second of two papers examining Spitzer Infrared Spectrograph (IRS) observations of the ultraluminous X-ray source (ULX) in Holmberg II. Here we perform detailed photoio…

astro-ph.HE2009★ 25 cited

The First Detection of [O IV] from an Ultraluminous X-ray Source with Spitzer I. Observational Results for Holmberg II ULX

C. T. Berghea, R. P. Dudik, K. A. Weaver +1

We present the first Spitzer Infrared Spectrograph (IRS) observations of the [O IV] 25.89 m emission line detected from the ultraluminous X-ray source (ULX) in Holmberg II. This…