Robust cosmological inference from non-linear scales with k-th nearest neighbor statistics

Kavli Affiliate: Tom Abel | First 5 Authors: Sihan Yuan, Tom Abel, Risa H. Wechsler, , | Summary: We present the methodology for deriving accurate and reliable cosmological constraints from non-linear scales (<50Mpc/h) with k-th nearest neighbor (kNN) statistics. We detail our methods for choosing robust minimum scale cuts and validating galaxy-halo connection models. Using […]


Continue.. Robust cosmological inference from non-linear scales with k-th nearest neighbor statistics

Exploring chemical enrichment of the intracluster medium with the Line Emission Mapper

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: François Mernier, Yuanyuan Su, Maxim Markevitch, Congyao Zhang, Aurora Simionescu | Summary: Synthesized in the cores of stars and supernovae, most metals disperse over cosmic scales and are ultimately deposited well outside the gravitational potential of their host galaxies. Since their presence is well visible through their […]


Continue.. Exploring chemical enrichment of the intracluster medium with the Line Emission Mapper

The Supersonic Project: Lighting up the faint end of the JWST UV luminosity function

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Claire E. Williams, William Lake, Smadar Naoz, Blakesley Burkhart, Tommaso Treu | Summary: The James Webb Space Telescope (JWST) is capable of probing extremely early eras of our Universe when the supersonic relative motions between dark matter and baryonic overdensities modulate structure formation ($z>sim 10$). We study […]


Continue.. The Supersonic Project: Lighting up the faint end of the JWST UV luminosity function

The Supersonic Project: Lighting up the faint end of the JWST UV luminosity function

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Claire E. Williams, William Lake, Smadar Naoz, Blakesley Burkhart, Tommaso Treu | Summary: The James Webb Space Telescope (JWST) is capable of probing extremely early eras of our Universe when the supersonic relative motions between dark matter and baryonic overdensities modulate structure formation ($z>sim 10$). We study […]


Continue.. The Supersonic Project: Lighting up the faint end of the JWST UV luminosity function

The Supersonic Project: Lighting up the faint end of the JWST UV luminosity function

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Claire E. Williams, William Lake, Smadar Naoz, Blakesley Burkhart, Tommaso Treu | Summary: The James Webb Space Telescope (JWST) is capable of probing extremely early eras of our Universe when the supersonic relative motions between dark matter and baryonic overdensities modulate structure formation ($z>sim 10$). We study […]


Continue.. The Supersonic Project: Lighting up the faint end of the JWST UV luminosity function

Searching for [CII] Emission from the First Sample of $zsim 6$ OI Absorption-Associated Galaxies with ALMA

Kavli Affiliate: Ran Wang | First 5 Authors: Yunjing Wu, Zheng Cai, Jianan Li, Kristian Finlator, Marcel Neeleman | Summary: We report the first statistical analyses of [CII] and dust continuum observations in six strong OI absorber fields at the end of the reionization epoch obtained by the Atacama Large Millimeter/Submillimeter Array (ALMA). Combined with […]


Continue.. Searching for [CII] Emission from the First Sample of $zsim 6$ OI Absorption-Associated Galaxies with ALMA

Searching for [CII] Emission from the First Sample of $zsim 6$ OI Absorption-Associated Galaxies with ALMA

Kavli Affiliate: Ran Wang | First 5 Authors: Yunjing Wu, Zheng Cai, Jianan Li, Kristian Finlator, Marcel Neeleman | Summary: We report the first statistical analyses of [CII] and dust continuum observations in six strong OI absorber fields at the end of the reionization epoch obtained by the Atacama Large Millimeter/Submillimeter Array (ALMA). Combined with […]


Continue.. Searching for [CII] Emission from the First Sample of $zsim 6$ OI Absorption-Associated Galaxies with ALMA

Looking in the axion mirror: An all-sky analysis of stimulated decay

Kavli Affiliate: Kiyoshi Wesley Masui | First 5 Authors: Yitian Sun, Katelin Schutz, Harper Sewalls, Calvin Leung, Kiyoshi Wesley Masui | Summary: Axion dark matter (DM) produces echo images of bright radio sources via stimulated decay. These images appear as a faint radio line centered at half the axion mass, with the line width set […]


Continue.. Looking in the axion mirror: An all-sky analysis of stimulated decay

The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Meredith Neyer, Aaron Smith, Rahul Kannan, Mark Vogelsberger, Enrico Garaldi | Summary: An important characteristic of cosmic reionization is the growth of ionized gas bubbles surrounding early luminous objects. Understanding the connections between the formation and coalescence of these bubbles and their originating astrophysical sources is equally […]


Continue.. The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization

The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization

Kavli Affiliate: Mark Vogelsberger | First 5 Authors: Meredith Neyer, Aaron Smith, Rahul Kannan, Mark Vogelsberger, Enrico Garaldi | Summary: An important characteristic of cosmic hydrogen reionization is the growth of ionized gas bubbles surrounding early luminous objects. Ionized bubble sizes are beginning to be probed using Lyman-$alpha$ emission from high-redshift galaxies, and will also […]


Continue.. The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization