Full forward model of galaxy clustering statistics with AbacusSummit lightcones

Kavli Affiliate: Tom Abel | First 5 Authors: Sihan Yuan, Boryana Hadzhiyska, Tom Abel, , | Summary: Novel summary statistics beyond the standard 2-point correlation function (2PCF) are necessary to capture the full astrophysical and cosmological information from the small-scale (r < 30Mpc/h) galaxy clustering. However, the analysis of beyond-2PCF statistics on small scales is […]


Continue.. Full forward model of galaxy clustering statistics with AbacusSummit lightcones

TESS Giants Transiting Giants III: An eccentric warm Jupiter supports a period-eccentricity relation for giant planets transiting evolved stars

Kavli Affiliate: Edward H. Morgan | First 5 Authors: Samuel K. Grunblatt, Nicholas Saunders, Ashley Chontos, Soichiro Hattori, Dimitri Veras | Summary: The fate of planets around rapidly evolving stars is not well understood. Previous studies have suggested that relative to the main sequence population, planets transiting evolved stars ($P$ $<$ 100 d) tend to […]


Continue.. TESS Giants Transiting Giants III: An eccentric warm Jupiter supports a period-eccentricity relation for giant planets transiting evolved stars

TESS Giants Transiting Giants III: An eccentric warm Jupiter supports a period-eccentricity relation for giant planets transiting evolved stars

Kavli Affiliate: Edward H. Morgan | First 5 Authors: Samuel K. Grunblatt, Nicholas Saunders, Ashley Chontos, Soichiro Hattori, Dimitri Veras | Summary: The fate of planets around rapidly evolving stars is not well understood. Previous studies have suggested that relative to the main sequence population, planets transiting evolved stars ($P$ $<$ 100 d) tend to […]


Continue.. TESS Giants Transiting Giants III: An eccentric warm Jupiter supports a period-eccentricity relation for giant planets transiting evolved stars

CodeEditor: Learning to Edit Source Code with Pre-trained Models

Kavli Affiliate: Zhuo Li | First 5 Authors: Jia Allen Li, Ge Li, Zhuo Li, Zhi Jin, Xing Hu | Summary: Developers often perform repetitive code editing activities for various reasons (e.g., code refactoring) during software development. Pre-trained code editing models have achieved the state-of-the-art (SOTA) results. Pre-trained models are first pre-trained with pre-training tasks […]


Continue.. CodeEditor: Learning to Edit Source Code with Pre-trained Models

CodeEditor: Learning to Edit Source Code with Pre-trained Models

Kavli Affiliate: Zhuo Li | First 5 Authors: Jia Li, Ge Li, Zhuo Li, Zhi Jin, Xing Hu | Summary: Developers often perform repetitive code editing activities for various reasons (e.g., code refactoring) during software development. Pre-trained code editing models have achieved the state-of-the-art (SOTA) results. Pre-trained models are first pre-trained with pre-training tasks and […]


Continue.. CodeEditor: Learning to Edit Source Code with Pre-trained Models

Mass-Metallicity Relation during the Epoch of Reionization in the CROC Simulations

Kavli Affiliate: Nickolay Gnedin | First 5 Authors: Isaac Noel, Hanjue Zhu, Nickolay Gnedin, , | Summary: The low-redshift mass-metallicity relation (MZR) is well studied, but the high-redshift MZR remains difficult to observe. To study the early MZR further, we analyze the Cosmic Reionization on Computers (CROC) simulations with a focus on the MZR from […]


Continue.. Mass-Metallicity Relation during the Epoch of Reionization in the CROC Simulations

Precise Estimate of Charged Wino Decay Rate

Kavli Affiliate: Satoshi Shirai | First 5 Authors: Masahiro Ibe, Masataka Mishima, Yuhei Nakayama, Satoshi Shirai, | Summary: The Wino is an $mathrm{SU}(2)_{L}$ triplet Majorana fermion and a well-motivated dark matter candidate. The mass difference between the charged and the neutral Winos is small thanks to the $mathrm{SU}(2)_{L}$ symmetry. The small mass difference makes the […]


Continue.. Precise Estimate of Charged Wino Decay Rate

Precise Estimate of Charged Wino Decay Rate

Kavli Affiliate: Satoshi Shirai | First 5 Authors: Masahiro Ibe, Masataka Mishima, Yuhei Nakayama, Satoshi Shirai, | Summary: The Wino is an $mathrm{SU}(2)_{L}$ triplet Majorana fermion and a well-motivated dark matter candidate. The mass difference between the charged and the neutral Winos is small thanks to the $mathrm{SU}(2)_{L}$ symmetry. The small mass difference makes the […]


Continue.. Precise Estimate of Charged Wino Decay Rate