_version_ 1866912723293437952
author Uzsoy, Ana Sofía M.
Dey, Arjun
Raichoor, Anand
Finkbeiner, Douglas P.
Ramakrishnan, Vandana
Lee, Kyoung-Soo
Gawiser, Eric
Aguilar, Jessica Nicole
Ahlen, Steven
Anand, Abhijeet
Bianchi, Davide
Brooks, David
Claybaugh, Todd
de la Macorra, Axel
Doel, Peter
Ferraro, Simone
Firestone, Nicole M.
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Guaita, Lucia
Gutierrez, Gaston
Herrera-Alcantar, Hiram K.
Hwang, Ho Seong
Ishak, Mustapha
Joyce, Dick
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Lahav, Ofer
Lamman, Claire
Landriau, Martin
Guillou, Laurent Le
Manera, Marc
Miquel, Ramon
Moustakas, John
Muñoz-Gutiérrez, Andrea
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Percival, Will
Poppett, Claire
Prada, Francisco
Pérez-Ràfols, Ignasi
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Seo, Hee-Jong
Silber, Joseph Harry
Song, Hyunmi
Sprayberry, David
Tarlé, Gregory
Weaver, Benjamin Alan
Zou, Hu
author_facet Uzsoy, Ana Sofía M.
Dey, Arjun
Raichoor, Anand
Finkbeiner, Douglas P.
Ramakrishnan, Vandana
Lee, Kyoung-Soo
Gawiser, Eric
Aguilar, Jessica Nicole
Ahlen, Steven
Anand, Abhijeet
Bianchi, Davide
Brooks, David
Claybaugh, Todd
de la Macorra, Axel
Doel, Peter
Ferraro, Simone
Firestone, Nicole M.
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Guaita, Lucia
Gutierrez, Gaston
Herrera-Alcantar, Hiram K.
Hwang, Ho Seong
Ishak, Mustapha
Joyce, Dick
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Lahav, Ofer
Lamman, Claire
Landriau, Martin
Guillou, Laurent Le
Manera, Marc
Miquel, Ramon
Moustakas, John
Muñoz-Gutiérrez, Andrea
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Percival, Will
Poppett, Claire
Prada, Francisco
Pérez-Ràfols, Ignasi
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Seo, Hee-Jong
Silber, Joseph Harry
Song, Hyunmi
Sprayberry, David
Tarlé, Gregory
Weaver, Benjamin Alan
Zou, Hu
contents Lyman-Alpha Emitters (LAEs) are star-forming galaxies with significant Ly$α$ emission and are often used as tracers of large-scale structure at high redshift. We explore the relationship between the Ly$α$ line profile and environmental density with spectroscopy from the Dark Energy Spectroscopic Instrument (DESI) of LAEs selected with narrow-band photometry through the One-hundred-deg$^2$ DECam Imaging in Narrowbands (ODIN) survey. We use LAE surface density maps in the N419 (z $\sim$ 2.45) and N501 (z $\sim$ 3.12) narrow bands to probe the relationship between local environmental density and the Ly$α$ line profile. In both narrow bands, we stack the LAE spectra in bins of environmental density and inside and outside of protocluster regions. The N501 data shows $\sim$15% higher Ly$α$ line luminosity for galaxies in protoclusters, suggesting increased star formation in these regions. However, the line luminosity is not appreciably greater in protocluster galaxies in the N419 band, suggesting a potential redshift evolution of this effect. The shape of the line profile itself does not vary with environmental density, suggesting that line shape changes are caused by local effects independent of a galaxy's environment. These data indicate a potential relationship between LAE local environmental density, ionized gas distribution, and Ly$α$ line luminosity.
format Preprint
id arxiv_https___arxiv_org_abs_2511_17498
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Effect of local environment on Ly$α$ line profile in DESI/ODIN LAEs
Uzsoy, Ana Sofía M.
Dey, Arjun
Raichoor, Anand
Finkbeiner, Douglas P.
Ramakrishnan, Vandana
Lee, Kyoung-Soo
Gawiser, Eric
Aguilar, Jessica Nicole
Ahlen, Steven
Anand, Abhijeet
Bianchi, Davide
Brooks, David
Claybaugh, Todd
de la Macorra, Axel
Doel, Peter
Ferraro, Simone
Firestone, Nicole M.
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Guaita, Lucia
Gutierrez, Gaston
Herrera-Alcantar, Hiram K.
Hwang, Ho Seong
Ishak, Mustapha
Joyce, Dick
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Lahav, Ofer
Lamman, Claire
Landriau, Martin
Guillou, Laurent Le
Manera, Marc
Miquel, Ramon
Moustakas, John
Muñoz-Gutiérrez, Andrea
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Percival, Will
Poppett, Claire
Prada, Francisco
Pérez-Ràfols, Ignasi
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Seo, Hee-Jong
Silber, Joseph Harry
Song, Hyunmi
Sprayberry, David
Tarlé, Gregory
Weaver, Benjamin Alan
Zou, Hu
Astrophysics of Galaxies
Lyman-Alpha Emitters (LAEs) are star-forming galaxies with significant Ly$α$ emission and are often used as tracers of large-scale structure at high redshift. We explore the relationship between the Ly$α$ line profile and environmental density with spectroscopy from the Dark Energy Spectroscopic Instrument (DESI) of LAEs selected with narrow-band photometry through the One-hundred-deg$^2$ DECam Imaging in Narrowbands (ODIN) survey. We use LAE surface density maps in the N419 (z $\sim$ 2.45) and N501 (z $\sim$ 3.12) narrow bands to probe the relationship between local environmental density and the Ly$α$ line profile. In both narrow bands, we stack the LAE spectra in bins of environmental density and inside and outside of protocluster regions. The N501 data shows $\sim$15% higher Ly$α$ line luminosity for galaxies in protoclusters, suggesting increased star formation in these regions. However, the line luminosity is not appreciably greater in protocluster galaxies in the N419 band, suggesting a potential redshift evolution of this effect. The shape of the line profile itself does not vary with environmental density, suggesting that line shape changes are caused by local effects independent of a galaxy's environment. These data indicate a potential relationship between LAE local environmental density, ionized gas distribution, and Ly$α$ line luminosity.
title Effect of local environment on Ly$α$ line profile in DESI/ODIN LAEs
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2511.17498