output
19972026
most citedSINGS: The SIRTF Nearby Galaxies Survey

1.3k citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2015★ 13 cited

Determination of resonance locations in barred spiral galaxies using multiband photometry

Amber D. Sierra, Marc S. Seigar, Patrick Treuthardt +1

In this paper, we apply a method identified by Puerari & Dottori (1997) to find the corotation radii (CR) in spiral galaxies. We apply our method to 57 galaxies, 17 of which have a…

astro-ph.GA2014★ 22 cited

Constraining dark matter halo profiles and galaxy formation models using spiral arm morphology. II. Dark and stellar mass concentrations for 13 nearby face-on galaxies

Marc S. Seigar, Benjamin L. Davis, Joel Berrier +1

We investigate the use of spiral arm pitch angles as a probe of disk galaxy mass profiles. We confirm our previous result that spiral arm pitch angles (P) are well correlated with…

astro-ph.GA2014★ 59 cited

The Black Hole Mass Function Derived from Local Spiral Galaxies

Benjamin L. Davis, Joel C. Berrier, Lucas Johns +6

We present our determination of the nuclear supermassive black hole (SMBH) mass function for spiral galaxies in the Local Universe, established from a volume-limited sample consist…

astro-ph.GA2013★ 60 cited

Further Evidence for a Supermassive Black Hole Mass - Pitch Angle Relation

Joel C. Berrier, Benjamin L. Davis, Daniel Kennefick +7

We present new and stronger evidence for a previously reported relationship between galactic spiral arm pitch angle P (a measure of the tightness of spiral structure) and the mass…

astro-ph.GA2012★ 104 cited

Measurement of Galactic Logarithmic Spiral Arm Pitch Angle Using Two-Dimensional Fast Fourier Transform Decomposition

Benjamin L. Davis, Joel C. Berrier, Douglas W. Shields +5

A logarithmic spiral is a prominent feature appearing in a majority of observed galaxies. This feature has long been associated with the traditional Hubble classification scheme, b…