CP
Caeley V. Pittman
Boston University, William Jewell College, European Organization for Nuclear Research, University of Oxford
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies · Astrophysical Phenomena and Observations
0000-0001-9301-6252
About
NSF Graduate Research Fellow studying star and planet formation with Dr. Catherine Espaillat at Boston University
Employment
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Boston University Graduate Student2020 - Present
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William Jewell College Fluid Dynamics Research Assistant (funded by the NSF)2019 - 2020
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European Organization for Nuclear Research University of Michigan - CERN REU Student2019 - 2019
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Maria Mitchell Association Astronomy REU Intern2018 - 2018
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William Jewell College Pillsbury Research Scholar2017 - 2017
Education
- 2020 - 2026
- 2016 - 2020
Projects & Funding
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National Science Foundation Graduate Research Fellow National Science Foundation2021 - 2026
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Barry M. Goldwater Scholarship Barry M. Goldwater Scholarship & Excellence in Education Foundation2019 - 2020
Publications (28)
- IPA: Accretion Rate of a Low-mass Class 0 Protostar, Measured via Mid-IR Fluorescent OH Emission Save
- Indications of Rapid Dust Formation in the Inner Region of a Protoplanetary Disk Save
- JWST Reveals Carbon-rich Chemistry in a Transitional Disk Save
- The ODYSSEUS Survey. Spatial Correlation of Magnetospheric Inclinations Points to Parsec-scale Star–Cloud Connection Save
- IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission Save
- PENELLOPE Save
- The ODYSSEUS Survey. Using Accretion and Stellar Rotation to Reveal the Star–Disk Connection in T Tauri Stars Save
- JWST Reveals Carbon-rich Chemistry in a Transitional Disk Save
- The ODYSSEUS Survey. Characterizing Magnetospheric Geometries and Hotspot Structures in T Tauri Stars Save
- The ODYSSEUS Survey. Spatial correlation of magnetospheric inclinations points to parsec-scale star-cloud connection Save
- PENELLOPE VII: Revisiting empirical relations to measure accretion luminosity Save
- The ODYSSEUS Survey. Using accretion and stellar rotation to reveal the star-disk connection in T Tauri stars Save
- Probing Accretion and Inner Disk Gas in the Youngest Planet System with HST Save
- The ODYSSEUS Survey. Characterizing magnetospheric geometries and hotspot structures in T Tauri stars Save
- A Model of the C iv λ λ1548, 1550 Doublet Line in T Tauri Stars Save
- A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. III. Optical Spectra* Save
- Evidence for Dust Depletion in a Misaligned Protoplanetary Disk with JWST Save
- A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. I. HST Far-UV and Near-UV Spectra Save
- A Multiwavelength, Multiepoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. II. Photometric Light Curves Save
- Modeling accretion in the HST ULLYSES sample: the most comprehensive NUV study of T Tauri star accretion Save