Locate family members with the last name DOMAGAL-GOLDMAN.

JENNIFER DOMAGAL-GOLDMAN is an academic who published a paper in 2018 entitled Hig,,er Education's Role in Enacting a Thriving Democracy. JENNIFER DOMAGAL-GOLDMAN published this work as part of a team: Hoffman, David. Here is a description of this work: The,,essays in this collection reflect the collaborative work and thoughts of participants in three national higher education networks focused on civic learning and democratic engagement. The three networks, the American Association of State College and Universities' American Democracy Project, the NASPA LEAD Initiative, and The Democracy Commitment, first convened together in New Orleans for the inaugural Civic Learning and Democratic Engagement (CLDE) Meeting in 2015. Since then, the three organizations have convened the annual CLDE conference and worked with colleagues to envision the thriving democracy toward which our work is directed, aligning learning outcomes, pedagogies, and strategies with this vision. The five essays in this collection were originally published on the Forbes platform from November 2017 to April 2018. The emergent CLDE Theory of Change described in these essay.

SHAWN DOMAGAL-GOLDMAN is an academic who published a paper in 2020 entitled L 98-59: A Benchmark System of Terrestrial Planets for Future Atmospheric Characterization. SHAWN DOMAGAL-GOLDMAN published this work as part of a team: Pidhorodetska, Daria.

SHAWN-D. DOMAGAL-GOLDMAN is an academic who published a paper in 2020 entitled Detectability of Molecular Signatures on TRAPPIST-1e through Transmission Spectroscopy Simulated for. SHAWN-D. DOMAGAL-GOLDMAN published this work as part of a team: Pidhorodetska, Daria. Here is a description of this work: Dis,,overies of terrestrial, Earth-sized exoplanets that lie within the habitable zone (HZ) of their host stars continue to occur at increasing rates. Transit spectroscopy can potentially enable the detection of molecular signatures from such worlds, providing an indication of the presence of an atmosphere and its chemical composition, including gases potentially indicative of a biosphere. Such planets around nearby M-dwarf starsâ€"such as TRAPPIST-1â€"provide a relatively good signal, high signal-to-noise ratio, and frequent transits for follow-up spectroscopy. However, even with these advantages, transit spectroscopy of terrestrial planets in the HZ of nearby M-stars will still be a challenge. Herein, we examine the potential for future space observatories to conduct such observations, using a global climate model, a photochemical model.