The Nineteenth Data Release of the Sloan Digital Sky Survey

Kavli Affiliate: Michael Zucker| First 5 Authors: SDSS Collaboration, SDSS Collaboration, , , | Summary:Mapping the local and distant Universe is key to our understanding of it. For decades, the Sloan Digital Sky Survey (SDSS) has made a concerted effort to map millions of celestial objects to constrain the physical processes that govern our Universe. […]


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The Nineteenth Data Release of the Sloan Digital Sky Survey

Kavli Affiliate: Alexander P. Ji | First 5 Authors: SDSS Collaboration, SDSS Collaboration, , , | Summary: Mapping the local and distant Universe is key to our understanding of it. For decades, the Sloan Digital Sky Survey (SDSS) has made a concerted effort to map millions of celestial objects to constrain the physical processes that […]


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Sloan Digital Sky Survey-V: Pioneering Panoptic Spectroscopy

Kavli Affiliate: Michael Zucker| First 5 Authors: Juna A. Kollmeier, Juna A. Kollmeier, , , | Summary:The Sloan Digital Sky Survey-V (SDSS-V) is pioneering panoptic spectroscopy: it is the first all-sky, multi-epoch, optical-to-infrared spectroscopic survey. SDSS-V is mapping the sky with multi-object spectroscopy (MOS) at telescopes in both hemispheres (the 2.5-m Sloan Foundation Telescope at […]


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Longitudinal Study of Facial Biometrics at the BEZ: Temporal Variance Analysis

Kavli Affiliate: Norbert Schulz| First 5 Authors: Mathias Schulz, Mathias Schulz, , , | Summary:This study presents findings from long-term biometric evaluations conducted at the Biometric Evaluation Center (bez). Over the course of two and a half years, our ongoing research with over 400 participants representing diverse ethnicities, genders, and age groups were regularly assessed […]


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The Distribution of Atomic Hydrogen in the Host Galaxies of FRBs

Kavli Affiliate: Jing Wang | First 5 Authors: Hugh Roxburgh, Hugh Roxburgh, , , | Summary: We probe the atomic hydrogen (HI) emission from the host galaxies of fast radio bursts (FRBs) to investigate the emerging trend of disturbance and asymmetry in the population. Quadrupling the sample size, we detect 13 of 14 new hosts […]


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Gap reopening as signature of coupling between Majorana zero modes in Sn-(Bi,Sb)2(Te,S)3-based Josephson trijunctions

Kavli Affiliate: Xiang Zhang | First 5 Authors: Duolin Wang, Duolin Wang, , , | Summary: In the past two decades, enormous efforts have been made to search for possible platforms and schemes to implement topological quantum computation (TQC). In exploring the Fu-Kane scheme of TQC based on Josephson trijunctions constructed on topological insulators, the […]


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Intergalactic Medium Tomography with the Sunburst Arc

Kavli Affiliate: Michael D. Gladders | First 5 Authors: Michelle A. Berg, Michelle A. Berg, , , | Summary: Gravitational lensing has transformed the field of gas tomography in the intergalactic medium (IGM) and circumgalactic medium (CGM). Here we use the brightest lensed galaxy identified to date, the Sunburst Arc ($z$$approx$2.37), to constrain the physical […]


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Wakes from Companion Interactions in Type Ia Supernovae Nebular Emission Line Profiles

Kavli Affiliate: Lars Bildsten | Summary:Thermonuclear supernovae (SNe) are the result of the nuclear transformation of carbon/oxygen (C/O) white dwarfs (WDs) to the radioactive element $^56mathrmNi$ and intermediate mass elements (IMEs) like Ca, Ar, etc. Most progenitor scenarios involve a companion star which donates matter to the exploding white dwarf, implying a fundamental prediction: the […]


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Before its time: a remarkably evolved protocluster core at z=7.88

Kavli Affiliate: Debora Sijacki | Summary:Protoclusters represent the most extreme environments in the very early Universe. They form from large-scale dark matter overdensities, harbouring an overabundance of galaxies fed by large gas reservoirs. Their early and accelerated evolution results in a distinct difference in the properties of galaxies resident in protoclusters versus the field, which […]


Continue.. Before its time: a remarkably evolved protocluster core at z=7.88