Emily C. Cunningham
Affiliations: | 2019 | Astronomy & Astrophysics | University of California, Santa Cruz, Santa Cruz, CA, United States |
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| Cunningham EC, Garavito-Camargo N, Deason AJ, et al. (2020) Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics The Astrophysical Journal. 898: 4 |
| Escala I, Gilbert KM, Kirby EN, et al. (2020) Elemental Abundances in M31: A Comparative Analysis of Alpha and Iron Element Abundances in the the Outer Disk, Giant Stellar Stream, and Inner Halo of M31 The Astrophysical Journal. 889: 177 |
| Hunt JAS, Johnston KV, Pettitt AR, et al. (2020) The power of coordinate transformations in dynamical interpretations of Galactic structure Monthly Notices of the Royal Astronomical Society. 497: 818-828 |
| Cunningham EC, Deason AJ, Sanderson RE, et al. (2019) HALO7D II : the halo velocity ellipsoid and velocity anisotropy with distant main-sequence stars. The Astrophysical Journal. 879: 120-120 |
| Escala I, Kirby EN, Gilbert KM, et al. (2019) Elemental Abundances in M31: Alpha and Iron Element Abundances from Low-resolution Resolved Stellar Spectroscopy in the Stellar Halo The Astrophysical Journal. 878: 42 |
| Cunningham EC, Deason AJ, Rockosi CM, et al. (2019) HALO7D I. The Line-of-sight Velocities of Distant Main-sequence Stars in the Milky Way Halo The Astrophysical Journal. 876: 124 |
| Yesuf HM, Koo DC, Faber SM, et al. (2017) No Evidence for Feedback: Unexceptional Low-ionization Winds in Host Galaxies of Low Luminosity Active Galactic Nuclei at Redshiftz∼ 1 The Astrophysical Journal. 841: 83 |
| Plant KA, Margon B, Guhathakurta P, et al. (2016) Runaway Dwarf Carbon Stars As Candidate Supernova Ejecta The Astrophysical Journal. 833: 232 |
| Cunningham EC, Deason AJ, Guhathakurta P, et al. (2016) ISOTROPIC at the BREAK? 3D KINEMATICS of MILKY WAY HALO STARS in the FOREGROUND of M31 Astrophysical Journal. 820 |
| Liu C, Peng EW, Toloba E, et al. (2015) THE MOST MASSIVE ULTRA-COMPACT DWARF GALAXY in the VIRGO CLUSTER Astrophysical Journal Letters. 812 |