49 citations · 193 across the 8 of their papers we have counts for
16 papers · 1 filter
Decoding the star forming properties of gas-rich galaxy pairs
Jamie Bok, Michelle E. Cluver, Thomas H. Jarrett +3
We extend the analysis of Bok et al. (2020) in which the HI content of isolated galaxies from the AMIGA sample and selected paired galaxies from ALFALFA were examined as a potentia…
Star Formation and Quenching of Central Galaxies from Stacked HI Measurements
Hong Guo, Michael G. Jones, Jing Wang +1
We quantitatively investigate the dependence of central galaxy HI mass () on the stellar mass (), halo mass (), star formation rate (SFR), and centra…
A diffuse tidal dwarf galaxy destined to fade out as a "dark galaxy"
Javier Román, Michael G. Jones, Mireia Montes +3
We have explored the properties of a peculiar object detected in deep optical imaging and located at the tip of an HI tail emerging from Hickson Compact Group 16. Using multiband p…
Satellites Around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations Versus Simulations
Ananthan Karunakaran, Kristine Spekkens, Kyle A. Oman +13
We compare the star-forming properties of satellites around Milky Way (MW) analogs from the Stage~II release of the Satellites Around Galactic Analogs Survey (SAGA-II) to those fro…
Evidence for Ultra-Diffuse Galaxy Formation Through Tidal Heating of Normal Dwarfs
Michael G. Jones, Paul Bennet, Burcin Mutlu-Pakdil +5
We have followed up two ultra-diffuse galaxies (UDGs), detected adjacent to stellar streams, with Hubble Space Telescope (HST) imaging and HI mapping with the Jansky Very Large Arr…
The dependence of subhalo abundance matching on galaxy photometry and selection criteria
Richard Stiskalek, Harry Desmond, Thomas Holvey +1
Subhalo abundance matching (SHAM) is a popular technique for assigning galaxy mass or luminosity to haloes produced in N-body simulations. The method works by matching the cumulati…