Strain variation identifies a neural substrate for behavioral evolution in Drosophila

Kavli Affiliate: Vanessa Ruta | Anna Ryba, Philipp Brand, Rory T. Coleman, Yarden Greenfeld, Yael N. Tsitohay, Florian Hollunder, Katharine Keller, Murtaza Hathiyari, Tianyi Wei, Paolo Emilio Barbano and Vanessa Ruta | Summary: Sexual selection acts on heritable differences within species, driving the parallel diversification of signal production in one sex and behavioral responses in […]


Continue.. Strain variation identifies a neural substrate for behavioral evolution in Drosophila

Towards individualized deep brain stimulation: A stereoencephalography-based workflow for unbiased neurostimulation target identification

Kavli Affiliate: Edward Chang | Authors: Jeremy Saal, Kelly Kadlec, Anusha B. Allawala, Lucille Johnston, Ryan Leriche, Ritwik Vatsyayan, Yiyuan Han, Audrey Kist, Tommaso Di Ianni, Heather E. Dawes, Edward F. Chang, A Moses Lee, Andrew D. Krystal, Khaled Moussawi, Prasad Shirvalkar and Kristin K. Sellers | Summary: Background: Deep-brain stimulation (DBS) is increasingly being […]


Continue.. Towards individualized deep brain stimulation: A stereoencephalography-based workflow for unbiased neurostimulation target identification

The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30-day Orbit and a More Massive Outer World

Kavli Affiliate: Saul Rappaport | Summary:We present the discovery of the planetary system orbiting the bright (V = 7.2), nearby (35 pc), Sun-like star HD 60779, which has a mass of 1.050 +/- 0.044 solar masses and a radius of 1.129 +/- 0.013 solar radii. We report two TESS transits and a subsequent CHEOPS transit […]


Continue.. The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30-day Orbit and a More Massive Outer World

The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30-day Orbit and a More Massive Outer World

Kavli Affiliate: Saul A. Rappaport | First 5 Authors: Victoria DiTomasso, Victoria DiTomasso, , , | Summary: We present the discovery of the planetary system orbiting the bright (V = 7.2), nearby (35 pc), Sun-like star HD 60779, which has a mass of 1.050 +/- 0.044 solar masses and a radius of 1.129 +/- 0.013 […]


Continue.. The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30-day Orbit and a More Massive Outer World

On the Variability Features of Active Galactic Nuclei in Little Red Dots

Kavli Affiliate: Luis C. Ho | First 5 Authors: Shuying Zhou, Shuying Zhou, , , | Summary: The high-redshift ($z>4$) compact sources with “V-shaped" spectral energy distributions (SEDs), known as Little Red Dots (LRDs), are discovered by the James Webb Space Telescope and provide valuable clues to the physics of active galactic nuclei (AGNs) in […]


Continue.. On the Variability Features of Active Galactic Nuclei in Little Red Dots

The Atacama Cosmology Telescope: Release of A databaSe of millimeTeR ObservatioNs of Asteroids Using acT ($mathttASTRONAUT$)

Kavli Affiliate: Jeffrey McMahon | Summary:We present A databaSe of millimeTeR ObservatioNs of Asteroids Using acT ($mathttASTRONAUT$) hosted on Amazon Web Services, Inc. (AWS) in the form of a public Amazon Simple Storage Service (S3) bucket. This bucket is an Amazon cloud storage database containing flux measurements for a group of asteroids at millimeter (mm) […]


Continue.. The Atacama Cosmology Telescope: Release of A databaSe of millimeTeR ObservatioNs of Asteroids Using acT ($mathttASTRONAUT$)

A Comparison of Full Spectral Fitting Codes for Measuring the Stellar Initial Mass Function and Other Stellar Population Properties in Elliptical Galaxies

Kavli Affiliate: Wendy Freedman | Summary:We present a comparative test of four widely used full spectral fitting codes, with the aim of answering the question: how robust is the retrieval of the stellar initial mass function (IMF) and other stellar properties of galaxies? We used ALF, PyStaff, Starlight, and pPXF to fit a set of […]


Continue.. A Comparison of Full Spectral Fitting Codes for Measuring the Stellar Initial Mass Function and Other Stellar Population Properties in Elliptical Galaxies