Reproducing the kinematics of damped Lyman α systems by Bird, Simeon, Haehnelt, Martin, Neeleman, Marcel, Genel, Shy, Vogelsberger, Mark, Hernquist, Lars

“…We examine the kinematic structure of damped Lyman α systems (DLAs) in a series of cosmological hydrodynamic simulations using the AREPO code. …”
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Damped Lyman α absorbers as a probe of stellar feedback by Bird, Simeon, Vogelsberger, Mark, Haehnelt, Martin, Sijacki, Debora, Genel, Shy, Torrey, Paul, Springel, Volker, Hernquist, Lars

“…We examine the abundance, clustering and metallicity of Damped Lyman α Absorbers (DLAs) in a suite of hydrodynamic cosmological simulations using the moving mesh code arepo. …”
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The THESAN project: Lyman-α emission and transmission during the Epoch of Reionization by Smith, A, Kannan, R, Garaldi, E, Vogelsberger, M, Pakmor, R, Springel, V, Hernquist, L

“…ABSTRACT The visibility of high-redshift Lyman-alpha emitting galaxies (LAEs) provides important constraints on galaxy formation processes and the Epoch of Reionization (EoR). …”
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The THESAN project: Lyman-α emission and transmission during the Epoch of Reionization by Smith, Aaron Robin, Kannan, R, Garaldi, E, Vogelsberger, Mark, Pakmor, R, Springel, V, Hernquist, L

“…ABSTRACT The visibility of high-redshift Lyman-alpha emitting galaxies (LAEs) provides important constraints on galaxy formation processes and the Epoch of Reionization (EoR). …”
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Effect of magnetic seed fields on Lyman Alpha emission from distant quasars by Narayanan, Sruthi Annapoorny

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Lyman- α constraints on cosmic heating from dark matter annihilation and decay by Liu, Hongwan, Qin, Wenzer, Ridgway, Gregory W, Slatyer, Tracy R

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Tests of the levels of Lyman alpha which lead to a flattened absorption profile by Rogers, Alan E.E.

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The Sunburst Arc: Direct Lyman α escape observed in the brightest known lensed galaxy by Rivera-Thorsen, TE, Dahle, H, Gronke, M, Bayliss, M, Rigby, JR, Simcoe, R, Bordoloi, R, Turner, M, Furesz, G

“…The source reveals a characteristic triple-peaked Lyman α profile that has been predicted in various theoretical works, but to our knowledge has not been unambiguously observed previously. …”
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Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at z ≈ 2.67 by Hong, Sungryong, Dey, Arjun, Lee, Kyung-Soo, Orsi, Álvaro A, Gebhardt, Karl, Vogelsberger, Mark, Hernquist, Lars, Xue, Rui, Jung, Intae, Finklestein, Steven L, Tuttle, Sarah, Boylan-Kolchin, Michael

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PREDOMINANTLY LOW METALLICITIES MEASURED IN A STRATIFIED SAMPLE OF LYMAN LIMIT SYSTEMS AT Z = 3.7 by Cooksey, Kathy L., O’Meara, John M., Glidden, Ana, Cooper, Thomas Jared, Simcoe, Robert A.

“…We measured metallicities for 33 z = 3.4–4.2 absorption line systems drawn from a sample of H i-selected-Lyman limit systems (LLSs) identified in Sloan Digital Sky Survey (SDSS) quasar spectra and stratified based on metal line features. …”
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ETHOS – an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-α forest by Bose, Sownak, Vogelsberger, Mark, Zavala, Jesús, Pfrommer, Christoph, Cyr-Racine, Francis-Yan, Bohr, Sebastian, Bringmann, Torsten

“…In particular, we use the ETHOS framework to compare statistics of the Lyman-α forest in cold dark matter (CDM) with an alternative model in which the DM couples strongly with a relativistic species in the early universe. …”
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ETHOS – an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-α forest by Bose, Sownak, Vogelsberger, Mark, Zavala, Jesús, Pfrommer, Christoph, Cyr-Racine, Francis-Yan, Bohr, Sebastian, Bringmann, Torsten

“…In particular, we use the ETHOS framework to compare statistics of the Lyman-α forest in cold dark matter (CDM) with an alternative model in which the DM couples strongly with a relativistic species in the early universe. …”
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The cosmic ultraviolet baryon survey (CUBS) – III. Physical properties and elemental abundances of Lyman-limit systems at z by Zahedy, Fakhri S, Chen, Hsiao-Wen, Cooper, Thomas M, Boettcher, Erin, Johnson, Sean D, Rudie, Gwen C, Chen, Mandy C, Cantalupo, Sebastiano, Cooksey, Kathy L, Faucher-Giguère, Claude-André, Greene, Jenny E, Lopez, Sebastian, Mulchaey, John S, Penton, Steven V, Petitjean, Patrick, Putman, Mary E, Rafelski, Marc, Rauch, Michael, Schaye, Joop, Simcoe, Robert A, Walth, Gregory L

“…<jats:title>ABSTRACT</jats:title> <jats:p>We present a systematic investigation of physical conditions and elemental abundances in four optically thick Lyman-limit systems (LLSs) at z = 0.36–0.6 discovered within the Cosmic Ultraviolet Baryon Survey (CUBS). …”
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Experimental Studies of Neutral Particle Effects on Edge Transport Barriers in Tokamaks Using the Lyman-alpha Measurement Apparatus by Rosenthal, Aaron Michael

“…To better quantify the hydrogenic neutral particle source, a one-dimensional, absolutely calibrated pinhole camera system was installed on the DIII-D tokamak to measure edge Lyman-alpha (Ly-𝛼) emission. Ly-𝛼 emission from hydrogenic isotopes can be used to infer hydrogenic neutral density and ionization rate profiles. …”
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Tools, techniques, and early results in studies of 21 cm, Lyman-alpha, and H-alpha emission from the cosmic dawn by Neben, Abraham Richard

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The Cosmic Ultraviolet Baryon Survey (CUBS) – I. Overview and the diverse environments of Lyman limit systems at z &lt; 1 by Chen, Hsiao-Wen, Zahedy, Fakhri S, Boettcher, Erin, Cooper, Thomas M, Johnson, Sean D, Rudie, Gwen C, Chen, Mandy C, Walth, Gregory L, Cantalupo, Sebastiano, Cooksey, Kathy L, Faucher-Giguère, Claude-André, Greene, Jenny E, Lopez, Sebastian, Mulchaey, John S, Penton, Steven V, Petitjean, Patrick, Putman, Mary E, Rafelski, Marc, Rauch, Michael, Schaye, Joop, Simcoe, Robert A, Weiner, Benjamin J

“…CUBS QSOs are selected based on their NUV brightness to avoid biases against the presence of intervening Lyman limit systems (LLSs) at zabs &amp;lt; 1. We report five new LLSs of $\log \, N({\mathrm{ H} \,{\small I}})/{{\rm cm^{-2}}}\gtrsim 17.2$ over a total redshift survey path-length of $\Delta \, z_{\mathrm{ LL}}=9.3$, and a number density of $n(z)=0.43_{-0.18}^{+0.26}$. …”
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The Cosmic Ultraviolet Baryon Survey (CUBS) – I. Overview and the diverse environments of Lyman limit systems at z &lt; 1 by Chen, Hsiao-Wen, Zahedy, Fakhri S, Boettcher, Erin, Cooper, Thomas M, Johnson, Sean D, Rudie, Gwen C, Chen, Mandy C, Walth, Gregory L, Cantalupo, Sebastiano, Cooksey, Kathy L, Faucher-Giguère, Claude-André, Greene, Jenny E, Lopez, Sebastian, Mulchaey, John S, Penton, Steven V, Petitjean, Patrick, Putman, Mary E, Rafelski, Marc, Rauch, Michael, Schaye, Joop, Simcoe, Robert A., Weiner, Benjamin J

“…CUBS QSOs are selected based on their NUV brightness to avoid biases against the presence of intervening Lyman limit systems (LLSs) at zabs &amp;lt; 1. We report five new LLSs of $\log \, N({\mathrm{ H} \,{\small I}})/{{\rm cm^{-2}}}\gtrsim 17.2$ over a total redshift survey path-length of $\Delta \, z_{\mathrm{ LL}}=9.3$, and a number density of $n(z)=0.43_{-0.18}^{+0.26}$. …”
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The Cosmic Ultraviolet Baryon Survey (CUBS) – IV. The complex multiphase circumgalactic medium as revealed by partial Lyman limit systems by Cooper, Thomas J, Rudie, Gwen C, Chen, Hsiao-Wen, Johnson, Sean D, Zahedy, Fakhri S, Chen, Mandy C, Boettcher, Erin, Walth, Gregory L, Cantalupo, Sebastiano, Cooksey, Kathy L, Faucher-Giguère, Claude-André, Greene, Jenny E, Lopez, Sebastian, Mulchaey, John S, Penton, Steven V, Petitjean, Patrick, Putman, Mary E, Rafelski, Marc, Rauch, Michael, Schaye, Joop, Simcoe, Robert A

“…<jats:title>ABSTRACT</jats:title> <jats:p>We present a detailed study of two partial Lyman limit systems (pLLSs) of neutral hydrogen column density $N_\mathrm{H\, I}\approx (1-3)\times 10^{16}\, \mathrm{cm}^{-2}$ discovered at $z$ = 0.5 in the Cosmic Ultraviolet Baryon Survey (CUBS). …”
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Impact of gas spin and Lyman–Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse by Bhowmick, Aklant K, Blecha, Laura, Torrey, Paul, Kelley, Luke Zoltan, Vogelsberger, Mark, Nelson, Dylan, Weinberger, Rainer, Hernquist, Lars

“…In this work, we use cosmological zoom simulations to study systematically the impact of requiring: (1) low gas angular momentum (spin), and (2) a minimum incident Lyman–Werner (LW) flux in order to form BH seeds. …”
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Spectral measurements of hydrogen Lyman-alpha in the atmospheres of Venus and Jupiter using a sounding rocket and the Hubble Space Telescope by Corbin, Benjamin Andrew

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