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UR: Rethinking our transiting exoplanet detection approaches: A method for optimizing small transiting planet detection.

UR: Rethinking our transiting exoplanet detection approaches: A method for optimizing small transiting planet detection.

by Guest | Nov 7, 2023 | Undergraduate Research

In the latest of our #UndergradResearch series, discover how Yash Gondhalekar optimized periodogram searches to more effectively find small transiting planets!

Tilted Tatooines can serve as a source of strange, solo planets

Tilted Tatooines can serve as a source of strange, solo planets

by Mark Dodici | Nov 1, 2023 | Daily Paper Summaries

Free-floating planets are hard to explain. Can the messy evolution of tilted planetary systems around binary stars help?

Siblings or Only Child: M Dwarf Planets

Siblings or Only Child: M Dwarf Planets

by Jack Lubin | Oct 23, 2023 | Daily Paper Summaries

M dwarf stars host single planet systems (only child) and multi-planet systems (siblings). Let’s explore the differences!

To the [Exo]Moon and Back: Understanding Limitations of Exomoon Detections

To the [Exo]Moon and Back: Understanding Limitations of Exomoon Detections

by Junellie Perez | Oct 18, 2023 | Daily Paper Summaries

Could we detect exomoons through transmission spectroscopy of exoplanets? Today’s authors seek to understand if HIP 41378 f could potentially host an exomoon!

Astronomers Join Forces Against The Sun

Astronomers Join Forces Against The Sun

by Jack Lubin | Oct 16, 2023 | Daily Paper Summaries

Our own Sun holds the keys to our understanding of how stellar activity signals present in radial velocity data sets. Now four international spectrograph teams have joined forces to combine data.

Where do Hot-Jupiters come from? RV population statistics suggests planet-planet interactions

Where do Hot-Jupiters come from? RV population statistics suggests planet-planet interactions

by William Balmer | Oct 11, 2023 | Daily Paper Summaries

Astronomers still aren’t completely certain how Hot Jupiters form. Today’s paper presents a population level study that suggests HJs form far away from their host star, and are herded inwards by dynamical interactions with coplanar outer giant companions.

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