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From the 1 of 7 linked papers with an AI index.

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20242026
most citedThe climates and thermal emission spectra of prime nearby temperate rocky exoplanet targets

1 citations · 1 across the 1 of their papers we have counts for

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7 papers

astro-ph.EP20261 cited

The climates and thermal emission spectra of prime nearby temperate rocky exoplanet targets

Tobi Hammond, Thaddeus D. Komacek, Ravi K. Kopparapu +9

The paper uses climate simulations and spectral modeling to assess how future infrared observations, especially with the proposed MIRECLE mission, could detect atmospheric CO₂ and…

astro-ph.EP2026

Accretion Rate Changes Detected in a Polluted White Dwarf

Jay Farihi, Hiba Tu Noor, Carl Melis +6

This letter reports statistically significant changes in the equivalent widths of MgII and CaII lines in the dusty and polluted white dwarf WD 0106-328, based on six epochs of spec…

astro-ph.EP2026

A New Strategy for Using Spectroscopic Phase Curves to Characterize Non-Transiting Planets

Ted M. Johnson, Avi M. Mandell

We introduce a new time-series analysis strategy for combined-light exoplanet spectroscopic phase curves called the Variable Planetary Infrared Excess (VPIE) method. VPIE can be us…

astro-ph.EP2025

The fraction of polar aligned circumbinary disks

Ted M. Johnson, Rebecca G. Martin, Stephen Lepp +1

Circumbinary gas disks that are misaligned to the binary orbital plane evolve toward either a coplanar or a polar-aligned configuration with respect to the binary host. The preferr…

astro-ph.EP2025

Asymmetric Temperature Variations In Protoplanetary disks: I. Linear Theory, Corotating Spirals, and Ring Formation

Zhaohuan Zhu, Shangjia Zhang, Ted Johnson

Protoplanetary disks can exhibit asymmetric temperature variations due to phenomena such as shadows cast by the inner disk or localized heating by young planets. We investigate the…

astro-ph.EP2024

The pale blue dot: using the Planetary Spectrum Generator to simulate signals from hyper realistic exo-Earths

Vincent Kofman, Geronimo Villanueva, Thomas Fauchez +5

The atmospheres and surfaces of planets show tremendous amount of spatial variation, which has a direct effect on the spectrum of the object, even if this may not be spatially reso…