TOI 4201 b and TOI 5344 b: Discovery of Two Transiting Giant Planets Around M Dwarf Stars and Revised Parameters for Three Others

Kavli Affiliate: Alan M. Levine | First 5 Authors: J. D. Hartman, G. Á. Bakos, Z. Csubry, A. W. Howard, H. Isaacson | Summary: We present the discovery from the TESS mission of two giant planets transiting M dwarf stars: TOI 4201 b and TOI 5344 b. We also provide precise radial velocity measurements and […]


Continue.. TOI 4201 b and TOI 5344 b: Discovery of Two Transiting Giant Planets Around M Dwarf Stars and Revised Parameters for Three Others

Current status and desired accuracy of the isotopic production cross-sections relevant to astrophysics of cosmic rays II. Fluorine to Silicon (and updated LiBeB)

Kavli Affiliate: Igor V. Moskalenko | First 5 Authors: Yoann Génolini, David Maurin, Igor V. Moskalenko, Michael Unger, | Summary: High-precision cosmic-ray data from ongoing and recent past experiments (Voyager, ACE-CRIS, PAMELA, ATIC, CREAM, NUCLEON, AMS-02, CALET, DAMPE) are being released in the tens of MeV/n to multi-TeV/n energy range. Astrophysical and dark matter interpretations […]


Continue.. Current status and desired accuracy of the isotopic production cross-sections relevant to astrophysics of cosmic rays II. Fluorine to Silicon (and updated LiBeB)

Current status and desired accuracy of the isotopic production cross-sections relevant to astrophysics of cosmic rays II. Fluorine to Silicon (and updated LiBeB)

Kavli Affiliate: Igor V. Moskalenko | First 5 Authors: Yoann Génolini, David Maurin, Igor V. Moskalenko, Michael Unger, | Summary: High-precision cosmic-ray data from ongoing and recent past experiments (Voyager, ACE-CRIS, PAMELA, ATIC, CREAM, NUCLEON, AMS-02, CALET, DAMPE) are being released in the tens of MeV/n to multi-TeV/n energy range. Astrophysical and dark matter interpretations […]


Continue.. Current status and desired accuracy of the isotopic production cross-sections relevant to astrophysics of cosmic rays II. Fluorine to Silicon (and updated LiBeB)

A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images

Kavli Affiliate: George R. Ricker | First 5 Authors: Tianjun Gan, Charles Cadieux, Farbod Jahandar, Allona Vazan, Sharon X. Wang | Summary: Observations and statistical studies have shown that giant planets are rare around M dwarfs compared with Sun-like stars. The formation mechanism of these extreme systems remains under debate for decades. With the help […]


Continue.. A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images

A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images

Kavli Affiliate: Avi Shporer | First 5 Authors: Tianjun Gan, Charles Cadieux, Farbod Jahandar, Allona Vazan, Sharon X. Wang | Summary: Observations and statistical studies have shown that giant planets are rare around M dwarfs compared with Sun-like stars. The formation mechanism of these extreme systems remains under debate for decades. With the help of […]


Continue.. A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images

A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images

Kavli Affiliate: Avi Shporer | First 5 Authors: Tianjun Gan, Charles Cadieux, Farbod Jahandar, Allona Vazan, Sharon X. Wang | Summary: Observations and statistical studies have shown that giant planets are rare around M dwarfs compared with Sun-like stars. The formation mechanism of these extreme systems remains under debate for decades. With the help of […]


Continue.. A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images

A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images

Kavli Affiliate: Roland Vanderspek | First 5 Authors: Tianjun Gan, Charles Cadieux, Farbod Jahandar, Allona Vazan, Sharon X. Wang | Summary: Observations and statistical studies have shown that giant planets are rare around M dwarfs compared with Sun-like stars. The formation mechanism of these extreme systems remains under debate for decades. With the help of […]


Continue.. A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images

An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low Redshift Lyman-$α$ Forest

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan | Summary: We explore the role of galactic feedback on the low redshift Lyman-$alpha$ (Ly$alpha$)~forest ($z lesssim 2$) statistics and its potential to alter the thermal state of the intergalactic medium. Using the Cosmology and […]


Continue.. An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low Redshift Lyman-$α$ Forest

An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low Redshift Lyman-$α$ Forest

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Megan Taylor Tillman, Blakesley Burkhart, Stephanie Tonnesen, Simeon Bird, Greg L. Bryan | Summary: We explore the role of galactic feedback on the low redshift Lyman-$alpha$ (Ly$alpha$)~forest ($z lesssim 2$) statistics and its potential to alter the thermal state of the intergalactic medium. Using the Cosmology and […]


Continue.. An Exploration of AGN and Stellar Feedback Effects in the Intergalactic Medium via the Low Redshift Lyman-$α$ Forest

The Atacama Cosmology Telescope: Galactic Dust Structure and the Cosmic PAH Background in Cross-correlation with WISE

Kavli Affiliate: Susan E. Clark | First 5 Authors: Rodrigo Córdova Rosado, Brandon S. Hensley, Susan E. Clark, Adriaan J. Duivenvoorden, Zachary Atkins | Summary: We present a cross-correlation analysis between $1’$ resolution total intensity and polarization observations from the Atacama Cosmology Telescope (ACT) at 150 and 220 GHz and 15$”$ mid-infrared photometry from the […]


Continue.. The Atacama Cosmology Telescope: Galactic Dust Structure and the Cosmic PAH Background in Cross-correlation with WISE