Stellar Cartography Archives - Astrobiology

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REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A Population of 74 Resolved Planetesimal Belts at Millimetre Wavelengths

Stellar Cartography

REsolved ALMA and SMA Observations of Nearby Stars (REASONS): A Population of 74 Resolved Planetesimal Belts at Millimetre Wavelengths

Radial Velocity Homogeneous Analysis of M Dwarfs Observed With HARPS. I. Exoplanet Detection and Candidates

Exoplanetology: Exoplanets & Exomoons

Radial Velocity Homogeneous Analysis of M Dwarfs Observed With HARPS. I. Exoplanet Detection and Candidates

A Primordial Radius Valley As A Consequence Of Planet Formation

Exoplanetology: Exoplanets & Exomoons

A Primordial Radius Valley As A Consequence Of Planet Formation

Searching for Low-Mass Exoplanets Amid Stellar Variability with a Fixed Effects Linear Model of Line-by-Line Shape Changes

Exoplanetology: Exoplanets & Exomoons

Searching for Low-Mass Exoplanets Amid Stellar Variability with a Fixed Effects Linear Model of Line-by-Line Shape Changes

Performance of the Stellar Abundances and Atmospheric Parameters Pipeline Adapted for M Dwarfs I. Atmospheric Parameters from the Spectroscopic Module

Habitable Zones & Global Climate

Performance of the Stellar Abundances and Atmospheric Parameters Pipeline Adapted for M Dwarfs I. Atmospheric Parameters from the Spectroscopic Module

The Magnetically Induced Radial Velocity Variation of Gliese 341 and an Upper Limit to the Mass of Its Transiting Earth-sized Planet

Exoplanetology: Exoplanets & Exomoons

The Magnetically Induced Radial Velocity Variation of Gliese 341 and an Upper Limit to the Mass of Its Transiting Earth-sized Planet

The Fastest Exoplanet System Yet Discovered

Exoplanetology: Exoplanets & Exomoons

The Fastest Exoplanet System Yet Discovered

Short-Period Small Planets with High Mutual Inclinations are more Common around Metal-Rich Stars

Exoplanetology: Exoplanets & Exomoons

Short-Period Small Planets with High Mutual Inclinations are more Common around Metal-Rich Stars

A Data-Driven M Dwarf Model and Detailed Abundances for ∼17,000 M Dwarfs in SDSS-V

News Summary Archives

A Data-Driven M Dwarf Model and Detailed Abundances for ∼17,000 M Dwarfs in SDSS-V

Exoplanet Occurrence Rate with Age for FGK Stars in Kepler

Exoplanetology: Exoplanets & Exomoons

Exoplanet Occurrence Rate with Age for FGK Stars in Kepler

Have We Discovered The Smallest Extra-solar Planet?

Exoplanetology: Exoplanets & Exomoons

Have We Discovered The Smallest Extra-solar Planet?

Near-circular Orbits for Planets Around M/K-type Stars With Earth-like Sizes and Instellations

Exoplanetology: Exoplanets & Exomoons

Near-circular Orbits for Planets Around M/K-type Stars With Earth-like Sizes and Instellations

Where in the Milky Way Do Exoplanets Preferentially Form?

Exoplanetology: Exoplanets & Exomoons

Where in the Milky Way Do Exoplanets Preferentially Form?

Stellar Cartography: Intricate Layers of Supernova Remnant Cassiopeia A

Astrochemistry

Stellar Cartography: Intricate Layers of Supernova Remnant Cassiopeia A

Planetary Rhythms: Synchronous Circulation On Variably Irradiated Asynchronous Planets

Exoplanetology: Exoplanets & Exomoons

Planetary Rhythms: Synchronous Circulation On Variably Irradiated Asynchronous Planets

Studying Wolf 359: Habitable Exoplanets Need To Be Prepared For Extreme Space Weather

Space Weather & Heliophysics

Studying Wolf 359: Habitable Exoplanets Need To Be Prepared For Extreme Space Weather

Architecture Classification For Extrasolar Planetary Systems

Exoplanetology: Exoplanets & Exomoons

Architecture Classification For Extrasolar Planetary Systems

From Stability to Instability: Characterizing the Eccentricities of Multi-planet Systems in the California Kepler Survey as a Means of Studying Stability

Exoplanetology: Exoplanets & Exomoons

From Stability to Instability: Characterizing the Eccentricities of Multi-planet Systems in the California Kepler Survey as a Means of Studying Stability

Planetary Edge Trends (PET). I. The Inner Edge-Stellar Mass Correlation

Exoplanetology: Exoplanets & Exomoons

Planetary Edge Trends (PET). I. The Inner Edge-Stellar Mass Correlation

Identifying Flare Locations Through Exoplanet Transit Occultations

Space Weather & Heliophysics

Identifying Flare Locations Through Exoplanet Transit Occultations