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Merge pull request #48 from DukeCosmology/erik-new_photo
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erikpeterson23 authored Jul 2, 2024
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# Display name
title: Erik Peterson

# Full Name (for SEO)
first_name: Erik
last_name: Peterson

# Role/position
role: PhD Candidate

# Organizations/Affiliations
organizations:
- name: Duke University

# Short bio (displayed in user profile at end of posts)
bio:

interests:
- Type Ia Supernovae
- Sports

education:
courses:
- course: PhD in Physics
institution: Duke University
year: 2025
- course: BS in Physics
institution: University of Notre Dame
year: 2019

# Social/Academic Networking
# For available icons, see: https://wowchemy.com/docs/getting-started/page-builder/#icons
# For an email link, use "fas" icon pack, "envelope" icon, and a link in the
# form "mailto:your-email@example.com" or "#contact" for contact widget.
social:
- icon: envelope
icon_pack: fas
link: 'mailto:erp28@duke.edu'
- icon: github
icon_pack: fab
link: https://github.com/erikpeterson23
- icon: linkedin
icon_pack: fab
link: https://www.linkedin.com/in/erik-peterson-010b10199
- icon: orcid
icon_pack: ai
link: https://orcid.org/0000-0002-8150-9591
# Link to a PDF of your resume/CV from the About widget.
# To enable, copy your resume/CV to `static/files/cv.pdf` and uncomment the lines below.
# - icon: cv
# icon_pack: ai
# link: files/cv.pdf

# Enter email to display Gravatar (if Gravatar enabled in Config)
email: ''

# Highlight the author in author lists? (true/false)
highlight_name: false

# Organizational groups that you belong to (for People widget)
# Set this to `[]` or comment out if you are not using People widget.
user_groups:
- Graduate Students
---
---

I am a graduate student in the Duke Cosmology group expecting to graduate in early 2025.

My research focuses on supernova cosmology. I have spent the majority of my time in grad school working on NIR SN analysis as well as peculiar velocities. In the NIR, I have been the lead of the DEHVILS survey, and I have recently begun leading the SAINTS team which will compile and analyze all existing NIR LCs in the literature. With peculiar velocities, I was the first to correct for PVs in a SN analysis as a part of Pantheon+, and I am leading a pilot program to define galaxy groups for SN hosts. Finally, I am also working on constraining dust by analyzing SN color evolution. My work will be both applicable and useful for both LSST and Roman, and I hope to spend my career working on these projects.
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