Evan Skillman - Academia.edu (original) (raw)
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Papers by Evan Skillman
arXiv (Cornell University), Jun 17, 2005
American Astronomical Society Meeting Abstracts #235, 2020
American Astronomical Society Meeting Abstracts #227, 2016
American Astronomical Society Meeting Abstracts #225, 2015
University of Minnesota M.S. thesis. May 2016. Major: Astrophysics. Advisors: Evan Skillman, Dan ... more University of Minnesota M.S. thesis. May 2016. Major: Astrophysics. Advisors: Evan Skillman, Dan Weisz. 1 computer file (PDF); vii, 41 pages.
The astrophysical journal, Oct 25, 2019
The Astrophysical Journal, Nov 21, 2019
The Astrophysical Journal, Jun 24, 2014
Monthly Notices of the Royal Astronomical Society, Jul 22, 2019
The Astronomical Journal, Jul 16, 2014
The Astrophysical Journal, Nov 10, 2015
Carolina Digital Repository (University of North Carolina at Chapel Hill), 2017
The Astrophysical Journal, Oct 21, 2019
arXiv (Cornell University), Nov 25, 2022
American Astronomical Society Meeting Abstracts, 2020
The Astrophysical Journal, Aug 24, 2015
The Astrophysical Journal, Dec 22, 2017
The Astrophysical Journal, Dec 29, 2009
The Astrophysical Journal, Jun 24, 2014
The Astrophysical Journal, Jul 1, 2023
We present a new selection of 358 blue compact dwarf galaxies (BCDs) from 5000 square degrees in ... more We present a new selection of 358 blue compact dwarf galaxies (BCDs) from 5000 square degrees in the Dark Energy Survey, and the spectroscopic follow-up of a subsample of 68 objects. For the subsample of 34 objects with deep spectra, we measure the metallicity via the direct T e method using the auroral [O iii]λ 4363 emission line. These BCDs have an average oxygen abundance of 12+log(O/H) = 7.8, with stellar masses between 107 and 108 M ⊙ and specific star-formation rates between ∼10−9 and 10−7 yr−1. We compare the position of our BCDs with the mass–metallicity (M–Z) and luminosity–metallicity (L–Z) relation derived from the Local Volume Legacy sample. We find the scatter about the M–Z relation is smaller than the scatter about the L–Z relation. We identify a correlation between the offsets from the M–Z and L–Z relation that we suggest is due to the contribution of metal-poor inflows. Finally, we explore the validity of the mass–metallicity–SFR fundamental plane in the mass range probed by our galaxies. We find that BCDs with stellar masses smaller than 108 M ⊙ do not follow the extrapolation of the fundamental plane. This result suggests that mechanisms other than the balance between inflows and outflows may be at play in regulating the position of low-mass galaxies in the M–Z–SFR space.
arXiv (Cornell University), Jun 17, 2005
American Astronomical Society Meeting Abstracts #235, 2020
American Astronomical Society Meeting Abstracts #227, 2016
American Astronomical Society Meeting Abstracts #225, 2015
University of Minnesota M.S. thesis. May 2016. Major: Astrophysics. Advisors: Evan Skillman, Dan ... more University of Minnesota M.S. thesis. May 2016. Major: Astrophysics. Advisors: Evan Skillman, Dan Weisz. 1 computer file (PDF); vii, 41 pages.
The astrophysical journal, Oct 25, 2019
The Astrophysical Journal, Nov 21, 2019
The Astrophysical Journal, Jun 24, 2014
Monthly Notices of the Royal Astronomical Society, Jul 22, 2019
The Astronomical Journal, Jul 16, 2014
The Astrophysical Journal, Nov 10, 2015
Carolina Digital Repository (University of North Carolina at Chapel Hill), 2017
The Astrophysical Journal, Oct 21, 2019
arXiv (Cornell University), Nov 25, 2022
American Astronomical Society Meeting Abstracts, 2020
The Astrophysical Journal, Aug 24, 2015
The Astrophysical Journal, Dec 22, 2017
The Astrophysical Journal, Dec 29, 2009
The Astrophysical Journal, Jun 24, 2014
The Astrophysical Journal, Jul 1, 2023
We present a new selection of 358 blue compact dwarf galaxies (BCDs) from 5000 square degrees in ... more We present a new selection of 358 blue compact dwarf galaxies (BCDs) from 5000 square degrees in the Dark Energy Survey, and the spectroscopic follow-up of a subsample of 68 objects. For the subsample of 34 objects with deep spectra, we measure the metallicity via the direct T e method using the auroral [O iii]λ 4363 emission line. These BCDs have an average oxygen abundance of 12+log(O/H) = 7.8, with stellar masses between 107 and 108 M ⊙ and specific star-formation rates between ∼10−9 and 10−7 yr−1. We compare the position of our BCDs with the mass–metallicity (M–Z) and luminosity–metallicity (L–Z) relation derived from the Local Volume Legacy sample. We find the scatter about the M–Z relation is smaller than the scatter about the L–Z relation. We identify a correlation between the offsets from the M–Z and L–Z relation that we suggest is due to the contribution of metal-poor inflows. Finally, we explore the validity of the mass–metallicity–SFR fundamental plane in the mass range probed by our galaxies. We find that BCDs with stellar masses smaller than 108 M ⊙ do not follow the extrapolation of the fundamental plane. This result suggests that mechanisms other than the balance between inflows and outflows may be at play in regulating the position of low-mass galaxies in the M–Z–SFR space.