_version_ 1866911298139193344
author Napolitano, Lucas
Myers, Adam D.
Tedeschi, Adam
Anand, Abhijeet
Herrera-Alcantar, Hiram K.
Aguilar, Jessica
Ahlen, Steven
Bailey, Stephen
BenZvi, Segev
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cuceu, Andrei
de la Macorra, Axel
Dey, Arjun
Dey, Biprateep
Doel, Peter
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztanaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Guy, Julien
Joyce, Dick
Kremin, Anthony
Landriau, Martin
Guillou, Laurent Le
Manera, Marc
Meisner, Aaron
Miquel, Ramon
Moustakas, John
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Percival, Will
Prada, Francisco
Perez-Rafols, Ignasi
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Silber, Joesph Harry
Sprayberry, David
Tarle, Gregory
Weaver, Benjamin Alan
Zhou, Rongpu
Zou, Hu
author_facet Napolitano, Lucas
Myers, Adam D.
Tedeschi, Adam
Anand, Abhijeet
Herrera-Alcantar, Hiram K.
Aguilar, Jessica
Ahlen, Steven
Bailey, Stephen
BenZvi, Segev
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cuceu, Andrei
de la Macorra, Axel
Dey, Arjun
Dey, Biprateep
Doel, Peter
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztanaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Guy, Julien
Joyce, Dick
Kremin, Anthony
Landriau, Martin
Guillou, Laurent Le
Manera, Marc
Meisner, Aaron
Miquel, Ramon
Moustakas, John
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Percival, Will
Prada, Francisco
Perez-Rafols, Ignasi
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Silber, Joesph Harry
Sprayberry, David
Tarle, Gregory
Weaver, Benjamin Alan
Zhou, Rongpu
Zou, Hu
contents We present details regarding the construction of a composite spectrum of quasar (QSO) absorption line systems. In this composite spectrum we identify more than 70 absorption lines, and observe oxygen and hydrogen emission features at a higher signal-to-noise ratio than in any previous study. As the light from a distant quasar travels towards an observer, it may interact with the circumgalactic medium environment of an intervening galaxy, forming absorption lines. In order to maximize the signal of these absorption lines, we have selected a sample of 238,838 quasar spectra from the second data release of the Dark Energy Spectroscopic Instrument (DESI), each identified to have absorption lines resulting from such an interaction. By stacking these spectra in the restframe of the absorption, and calculating a median composite spectrum, we are able to isolate and enhance these absorption lines. We provide a full atlas of all detected absorption and emission lines as well as their fit centroids and equivalent width values. This atlas should aid in future studies investigating the compositions and physical conditions of these absorbers.
format Preprint
id arxiv_https___arxiv_org_abs_2512_02992
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The Composite Spectrum of QSO Absorption Line Systems in DESI DR2
Napolitano, Lucas
Myers, Adam D.
Tedeschi, Adam
Anand, Abhijeet
Herrera-Alcantar, Hiram K.
Aguilar, Jessica
Ahlen, Steven
Bailey, Stephen
BenZvi, Segev
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cuceu, Andrei
de la Macorra, Axel
Dey, Arjun
Dey, Biprateep
Doel, Peter
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztanaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Guy, Julien
Joyce, Dick
Kremin, Anthony
Landriau, Martin
Guillou, Laurent Le
Manera, Marc
Meisner, Aaron
Miquel, Ramon
Moustakas, John
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Percival, Will
Prada, Francisco
Perez-Rafols, Ignasi
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Schubnell, Michael
Silber, Joesph Harry
Sprayberry, David
Tarle, Gregory
Weaver, Benjamin Alan
Zhou, Rongpu
Zou, Hu
Astrophysics of Galaxies
We present details regarding the construction of a composite spectrum of quasar (QSO) absorption line systems. In this composite spectrum we identify more than 70 absorption lines, and observe oxygen and hydrogen emission features at a higher signal-to-noise ratio than in any previous study. As the light from a distant quasar travels towards an observer, it may interact with the circumgalactic medium environment of an intervening galaxy, forming absorption lines. In order to maximize the signal of these absorption lines, we have selected a sample of 238,838 quasar spectra from the second data release of the Dark Energy Spectroscopic Instrument (DESI), each identified to have absorption lines resulting from such an interaction. By stacking these spectra in the restframe of the absorption, and calculating a median composite spectrum, we are able to isolate and enhance these absorption lines. We provide a full atlas of all detected absorption and emission lines as well as their fit centroids and equivalent width values. This atlas should aid in future studies investigating the compositions and physical conditions of these absorbers.
title The Composite Spectrum of QSO Absorption Line Systems in DESI DR2
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2512.02992