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19972026
most citedThe First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey

195 citations · 1.3k across the 49 of their papers we have counts for

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9 papers · 1 filter

astro-ph2008★ 31 cited

Uncertainties in Theoretical HeI Emissivities: HII Regions, Primordial Abundance, and Cosmological Recombination

R. L. Porter, G. J. Ferland, K. B. MacAdam +1

A number of recent works in astronomy and cosmology have relied upon theoretical He I emissivities, but we know of no effort to quantify the uncertainties in the atomic data. We an…

astro-ph2007★ 35 cited

Determination of the Physical Conditions of the Knots in the Helix Nebula from Optical and Infrared Observations

C. R. O'Dell, W. J. Henney, G. J. Ferland

[Abridged] We use new HST and archived images to clarify the nature of the knots in the Helix Nebula. We employ published far infrared spectrophotometry and existing 2.12 micron im…

astro-ph2006★ 73 cited

He~I Emission in the Orion Nebula and Implications for Primordial Helium Abundance

R. L. Porter, G. J. Ferland, K. B. MacAdam

We apply a recently developed theoretical model of helium emission to observations of both the Orion Nebula and a sample of extragalactic H II regions. In the Orion analysis, we el…

astro-ph2006★ 6 cited

Determining the H+ Region/PDR Equation of State in Star Forming Regions

N. P. Abel, G. J. Ferland

The emission line regions of starburst galaxies and active nuclei reveal a wealth of spectroscopic information. A unified picture of the relationship between ionized, atomic, and m…

astro-ph2005★ 135 cited

The H II Region/PDR Connection: Self-Consistent Calculations of Physical Conditions in Star-Forming Regions

N. P. Abel, G. J. Ferland, G. Shaw +1

We have performed a series of calculations designed to reproduce infrared diagnostics used to determine physical conditions in star forming regions. We self-consistently calculate…

astro-ph2005★ 43 cited

J-resolved He I emission predictions in the low-density limit

R. P. Bauman, R. L. Porter, G. J. Ferland +1

Determinations of the primordial helium abundance are used in precision cosmological tests. These require highly accurate He I recombination rate coefficients. Here we reconsider t…