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Astrometric Redshifts of Supernovae
Published 2024-01-01“…For a conservative choice of a 5 mas systematic uncertainty floor, we find that our redshift estimation is accurate at z < 0.6. We then combine our astrometric redshifts with both host-galaxy photometric redshifts and supernovae photometric (light-curve) redshifts and show that this considerably improves the overall redshift estimates. …”
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Demography of High-Redshift AGN
Published 2012-01-01“…High-redshift AGN holds the key to understanding early structure formation and to probe the Universe during its infancy. …”
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Use of Redshifts as Evidence of Dark Energy
Published 2025-06-01“…To make contact with observational data, the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>a</mi><mo>(</mo><mi>t</mi><mo>)</mo></mrow></semantics></math></inline-formula> function needs to be related to the observable <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>z</mi><mo>(</mo><mi>r</mi><mo>)</mo></mrow></semantics></math></inline-formula> function, redshift versus distance. Model fitting of data has shown that the equation that governs <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>z</mi><mo>(</mo><mi>r</mi><mo>)</mo></mrow></semantics></math></inline-formula> needs to contain a constant term, which has been identified as Einstein’s cosmological constant. …”
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HETDEX-LOFAR Spectroscopic Redshift Catalog
Published 2024-01-01Subjects: “…Redshift surveys…”
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Machine Learning–based Photometric Redshifts for Galaxies in the North Ecliptic Pole Wide Field: Catalogs of Spectroscopic and Photometric Redshifts
Published 2025-01-01Subjects: “…Redshift surveys…”
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Redshift and Photon Energy Attenuation Constant in Vacuum
Published 2024-06-01Subjects: “…redshift…”
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The cosmic timeline implied by the highest redshift quasars
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Early Enrichment Population Theory at High Redshift
Published 2025-01-01“…This population likely existed at high redshifts ( z ∼ 10), relics of which we posit exist today as dwarf galaxies. …”
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A Glimpse of the New Redshift Frontier through AS1063
Published 2025-01-01Subjects: “…High-redshift galaxies…”
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Spatiospectral properties of redshifted free electron laser radiation
Published 2025-04-01“…Free electron lasers (FELs) are advanced light sources delivering pulses with unprecedented intensity down to the hard x-ray range. Redshifted FEL represents a new scheme exploiting strongly chirped electron beams to emit tunable coherent radiation at wavelengths longer than the FEL's resonant condition. …”
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Searching for Low-redshift Hot Dust-obscured Galaxies
Published 2025-01-01“…Hot dust-obscured galaxies (Hot DOGs), discovered by the “W1W2 dropout” selection at high redshifts ( z ∼ 2–4), are a rare population of hyperluminous obscured quasars. …”
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Low-Redshift Observational Constraints on Dark Energy Cosmologies
Published 2023-10-01“…Applying the Markov chain Monte Carlo algorithm and using low-redshift observational data, we put cosmological constraints on dark energy cosmologies. …”
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Searching for Internal Absorption Signatures in High-redshift Blazars
Published 2025-01-01“…In this study, we select a sample of γ -ray detected FSRQs with high redshift ( z ≳ 3) to search for absorption features appearing at lower photon energies due to a substantial redshift. …”
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Gravitational Redshift as a Measure of Rapid Mass Increase
Published 2025-06-01Subjects: Get full text
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15
Reidentification of Redshifts of SDSS Galaxies Overlapped with Galactic Objects
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Primordial Non-Gaussianity Systematics from Redshift Mismatch with SPHEREx
Published 2025-01-01“…We simulate 500 SPHEREx-like galaxy density fields and divide the galaxies into redshift bins assuming Gaussian photometric redshift errors. …”
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The 2023 Flight of the Faint Intergalactic-medium Redshifted Emission Balloon
Published 2025-01-01“…The second iteration of the Faint Intergalactic-medium Redshifted Emission Balloon (FIREBall-2) is a UV multiobject spectrograph designed to detect emission from the circumgalactic and circumquasar medium at low redshifts ( z < 1). …”
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Inhomogeneous Dust Biases Photometric Redshifts and Stellar Masses for LSST
Published 2025-01-01“…Spectral energy distribution (SED) modeling is one of the main methods to estimate galaxy properties, such as photometric redshifts, z , and stellar masses, M _* , for extragalactic imaging surveys. …”
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Estimating the Masses of Supercluster-scale Filaments from Redshift Dispersions
Published 2024-01-01Subjects: Get full text
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The Emerging Black Hole Mass Function in the High-redshift Universe
Published 2025-01-01“…We find that both pathways can reproduce observations at z ∼ 5–6, but have distinct features at higher redshifts of z ∼ 10. Specifically, JWST observations have the potential to constrain the fraction of efficiently accreting (super-Eddington) SMBHs, as well as the existence and prevalence of heavy seeds, in particular through ultradeep observations of blank fields and/or gravitational lensing surveys. …”
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