THRILS -- The High-(Redshift+Ionization) Line Search: Program Description & Redshift Catalog
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arXiv
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OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots
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Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS
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The GlimmIr: Spectroscopic Variability in a z~7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions
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Preliminary Evidence for Lensing-Induced Alignments of High-Redshift Galaxies in JWST-CEERS
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Can UVB Variations Reconcile Simulated Quasar Absorption Lines at High Redshift?
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Magnetically Driven Relativistic Jet in the High-Redshift Blazar OH~471
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Photometric Redshift Estimation for Rubin Observatory Data Preview 1 with Redshift Assessment Infrastructure Layers (RAIL)
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Galaxies Going Bananas: Inferring the 3D Geometry of High-Redshift Galaxies with JWST-CEERS
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Double Dots: Compact Pairs Mark Little Red Dots and High-Redshift Broad-line AGNs
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Emission-Line Diagnostics at z>4: [OIII]λ4363/Hγ
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A Redshift-based Red Selection of Dusty Star-forming Galaxies
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Deep Extragalactic VIsible Legacy Survey (DEVILS): Satellite Quenching at Intermediate Redshift
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Em tempo: uso indevido e excessivo de fórmulas de aminoácidos na alergia ao leite de vaca
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HETDEX-LOFAR Spectroscopic Redshift Catalog
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The Energy Exclusion Principle: A Dynamical Mechanism for Cosmological Redshift and Vacuum Evolution
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Hidden Vela Supercluster Revealed by First Hybrid Redshift & Peculiar Velocity Reconstruction
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Deep Spectroscopy with DESI for Photometric Redshift Training and Calibration
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A Deep ALMA Survey of the Redshift Distribution of Dusty Star-forming Galaxies
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Chromatic Cardinalities via Redshift
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The Early Maturity of High-Redshift Galaxies: Insights from sSFR, M/L and SFHs at z~7-14
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The Prevalence of Bursty Star Formation in Low-Mass Galaxies at z=1-7 from Hα-to-UV Diagnostics
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Dead or Alive? How Bursty Star Formation and Patchy Dust Can Cause Temporary Quiescence in High Redshift Galaxies
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Optical Strong Line Ratios Cannot Distinguish Between Stellar Populations and Accreting Black Holes at High Ionization Parameters and Low Metallicities
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STag II: Classification of Serendipitous Supernovae Observed by Galaxy Redshift Surveys
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Optimizing Photometric Redshift Training Sets I: Efficient Compression of the Galaxy Color-Redshift Relation with UMAP
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Impact of Primordial Black Hole Dark Matter on Gas Properties at Very High Redshift: A Semi-Analytical Model
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The Impact of Foregrounds on Dark Ages Measurements with the Highly Redshifted 21 cm Line
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Putting Flat $Λ$CDM In The (Redshift) Bin
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Higher Semiadditive Algebraic K-Theory and Redshift
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Similar Items
-
Here There Be (Dusty) Monsters: High Redshift AGN are Dustier Than Their Hosts
by: Brooks, Madisyn, et al.
Published: (2024) -
The Emerging Black Hole Mass Function in the High-Redshift Universe
by: Jeon, Junehyoung, et al.
Published: (2025) -
Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot
by: Lambrides, Erini, et al.
Published: (2025) -
JWST & the Waz Arc I: Spatially Resolving the Physical Conditions within a Post-Starburst Galaxy at Redshift 5 with NIRSpec IFS
by: Hutchison, Taylor A., et al.
Published: (2025) -
Hunting for the First Explosions at the High-Redshift Frontier
by: Jeon, Junehyoung, et al.
Published: (2026)