Cosmic Reionization On Computers: Statistics, Physical Properties and Environment of Lyman Limit Systems at $zsim6$

Kavli Affiliate: Nickolay Y. Gnedin | First 5 Authors: Jiawen Fan, Hanjue Zhu, Camille Avestruz, Nickolay Y. Gnedin, | Summary: Lyman Limit Systems (LLSs) are dense hydrogen clouds with high enough HI column densities ($N_{rm HI}$) to absorb Lyman continuum photons emitted from distant quasars. Their high column densities imply an origin in dense environments; […]


Continue.. Cosmic Reionization On Computers: Statistics, Physical Properties and Environment of Lyman Limit Systems at $zsim6$

Cosmic Reionization On Computers: Statistics, Physical Properties and Environment of Lyman Limit Systems at $zsim6$

Kavli Affiliate: Nickolay Y. Gnedin | First 5 Authors: Jiawen Fan, Hanjue Zhu, Camille Avestruz, Nickolay Y. Gnedin, | Summary: Lyman Limit Systems (LLSs) are dense hydrogen clouds with high enough HI column densities ($N_{rm HI}$) to absorb Lyman continuum photons emitted from distant quasars. Their high column densities imply an origin in dense environments; […]


Continue.. Cosmic Reionization On Computers: Statistics, Physical Properties and Environment of Lyman Limit Systems at $zsim6$

Cosmic Reionization On Computers: Statistics, Physical Properties and Environment of Lyman Limit Systems at $zsim6$

Kavli Affiliate: Nickolay Y. Gnedin | First 5 Authors: Jiawen Fan, Hanjue Zhu, Camille Avestruz, Nickolay Y. Gnedin, | Summary: Lyman limit systems (LLSs) are dense hydrogen clouds with high enough HI column densities to absorb Lyman continuum photons emitted from distant quasars. Their high column densities imply an origin in dense environments; however, the […]


Continue.. Cosmic Reionization On Computers: Statistics, Physical Properties and Environment of Lyman Limit Systems at $zsim6$

COOL-LAMPS IV: A Sample of Bright Strongly-Lensed Galaxies at $3 < z < 4$

Kavli Affiliate: Michael D. Gladders | First 5 Authors: Yunchong Zhang, Viraj Manwadkar, Michael D. Gladders, Gourav Khullar, Håkon Dahle | Summary: We report the discovery of five bright strong gravitationally lensed galaxies at $3 < z < 4$: COOLJ0101$+$2055 ($z = 3.459$), COOLJ0104$-$0757 ($z = 3.480$), COOLJ0145$+$1018 ($z = 3.310$), COOLJ0516$-$2208 ($z = 3.549$), […]


Continue.. COOL-LAMPS IV: A Sample of Bright Strongly-Lensed Galaxies at $3 < z < 4$

Strong Lensing Parameter Estimation on Ground-Based Imaging Data Using Simulation-Based Inference

Kavli Affiliate: Joshua A. Frieman | First 5 Authors: Jason Poh, Ashwin Samudre, Aleksandra Ćiprijanović, Brian Nord, Gourav Khullar | Summary: Current ground-based cosmological surveys, such as the Dark Energy Survey (DES), are predicted to discover thousands of galaxy-scale strong lenses, while future surveys, such as the Vera Rubin Observatory Legacy Survey of Space and […]


Continue.. Strong Lensing Parameter Estimation on Ground-Based Imaging Data Using Simulation-Based Inference

Strong Lensing Parameter Estimation on Ground-Based Imaging Data Using Simulation-Based Inference

Kavli Affiliate: Joshua A. Frieman | First 5 Authors: Jason Poh, Ashwin Samudre, Aleksandra Ćiprijanović, Brian Nord, Gourav Khullar | Summary: Current ground-based cosmological surveys, such as the Dark Energy Survey (DES), are predicted to discover thousands of galaxy-scale strong lenses, while future surveys, such as the Vera Rubin Observatory Legacy Survey of Space and […]


Continue.. Strong Lensing Parameter Estimation on Ground-Based Imaging Data Using Simulation-Based Inference

Strong Lensing Parameter Estimation on Ground-Based Imaging Data Using Simulation-Based Inference

Kavli Affiliate: Joshua A. Frieman | First 5 Authors: Jason Poh, Ashwin Samudre, Aleksandra Ćiprijanović, Brian Nord, Gourav Khullar | Summary: Current ground-based cosmological surveys, such as the Dark Energy Survey (DES), are predicted to discover thousands of galaxy-scale strong lenses, while future surveys, such as the Vera Rubin Observatory Legacy Survey of Space and […]


Continue.. Strong Lensing Parameter Estimation on Ground-Based Imaging Data Using Simulation-Based Inference

Mirror Dark Sector Solution of the Hubble Tension with Time-varying Fine-structure Constant

Kavli Affiliate: Joshua Frieman | First 5 Authors: John Zhang, Joshua Frieman, , , | Summary: We explore a model introduced by Cyr-Racine, Ge, and Knox (arXiv:2107.13000(2)) that resolves the Hubble tension by invoking a “mirror world" dark sector with energy density a fixed fraction of the “ordinary" sector of Lambda-CDM. Although it reconciles cosmic […]


Continue.. Mirror Dark Sector Solution of the Hubble Tension with Time-varying Fine-structure Constant

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