We present the results of an unbiased search for Lyα emission from continuum-selected 5.6 4σ) emission lines using two different automated detection methods, free of any visual inspection biases. Applying these methods on photometrically-selected high-redshift candidates between 5.6 7 (140.3 ± 19.0Å).Astronom
We present a quantitative model of Lyα emission throughout cosmic history and determine the prospect...
Deep spectroscopic observations of z ≳ 6.5 galaxies have revealed a marked decline with increasing r...
Deep spectroscopic observations of z ≳ 6.5 galaxies have revealed a marked decline with increasing r...
We present the results of an unbiased search for Lyα emission from continuum-selected 5.6 < z <...
We present the results of an unbiased search for Lyα emission from continuum-selected 5.6 < z <...
open21siWe present the results of an unbiased search for Lyα emission from continuum-selected 5.6 &l...
We present U_(336)V_(606)J_(125)H_(160) follow-up Hubble Space Telescope (HST) observations of 16 z ...
We present the highest redshift detections of resolved Lyα emission, using Hubble Space Telescope (H...
We present U_(336)V_(606)J_(125)H_(160) follow-up Hubble Space Telescope (HST) observations of 16 z ...
University of Minnesota Ph.D. dissertation.August 2018. Major: Astrophysics. Advisor: Claudia Scarl...
Galaxies at high redshifts are a valuable tool for studying cosmic dawn, therefore it is crucial to ...
We have conducted a deep long-slit spectroscopic search for high-redshift (2.7 \u3c z \u3c 4.7) Lyα ...
We have conducted a deep long-slit spectroscopic search for high-redshift (2.7 \u3c z \u3c 4.7) Lyα ...
Galaxies at high redshifts are a valuable tool for studying cosmic dawn, therefore it is crucial to ...
We present a quantitative model of Lyα emission throughout cosmic history and determine the prospect...
We present a quantitative model of Lyα emission throughout cosmic history and determine the prospect...
Deep spectroscopic observations of z ≳ 6.5 galaxies have revealed a marked decline with increasing r...
Deep spectroscopic observations of z ≳ 6.5 galaxies have revealed a marked decline with increasing r...
We present the results of an unbiased search for Lyα emission from continuum-selected 5.6 < z <...
We present the results of an unbiased search for Lyα emission from continuum-selected 5.6 < z <...
open21siWe present the results of an unbiased search for Lyα emission from continuum-selected 5.6 &l...
We present U_(336)V_(606)J_(125)H_(160) follow-up Hubble Space Telescope (HST) observations of 16 z ...
We present the highest redshift detections of resolved Lyα emission, using Hubble Space Telescope (H...
We present U_(336)V_(606)J_(125)H_(160) follow-up Hubble Space Telescope (HST) observations of 16 z ...
University of Minnesota Ph.D. dissertation.August 2018. Major: Astrophysics. Advisor: Claudia Scarl...
Galaxies at high redshifts are a valuable tool for studying cosmic dawn, therefore it is crucial to ...
We have conducted a deep long-slit spectroscopic search for high-redshift (2.7 \u3c z \u3c 4.7) Lyα ...
We have conducted a deep long-slit spectroscopic search for high-redshift (2.7 \u3c z \u3c 4.7) Lyα ...
Galaxies at high redshifts are a valuable tool for studying cosmic dawn, therefore it is crucial to ...
We present a quantitative model of Lyα emission throughout cosmic history and determine the prospect...
We present a quantitative model of Lyα emission throughout cosmic history and determine the prospect...
Deep spectroscopic observations of z ≳ 6.5 galaxies have revealed a marked decline with increasing r...
Deep spectroscopic observations of z ≳ 6.5 galaxies have revealed a marked decline with increasing r...
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