Construction of the Damped Ly$α$ Absorber Catalog for DESI DR2 Ly$α$ BAO
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| Format: | Preprint |
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2025
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| author | Brodzeller, A. Wolfson, M. Santos, D. M. Ho, M. Tan, T. Pieri, M. M. Cuceu, A. Abdul-Karim, M. Aguilar, J. Ahlen, S. Anand, A. Andrade, U. Armengaud, E. Aviles, A. Bailey, S. Bault, A. Bianchi, D. Brooks, D. Canning, R. Casas, L. Charles, M. Chaussidon, E. Chaves-Montero, J. Chebat, D. Claybaugh, T. Dawson, K. S. de Belsunce, R. de la Macorra, A. de Mattia, A. Dey, Arjun Dey, Biprateep Doshi, M. Doel, P. Elbers, W. Ferraro, S. Font-Ribera, A. Forero-Romero, J. E. Garcia-Quintero, C. Garrison, L. H. Gaztañaga, E. Gontcho, S. Gontcho A Gonzalez-Morales, A. X. Green, D. Gutierrez, G. Guy, J. Hahn, C. Herbold, M. Herrera-Alcantar, H. K. Honscheid, K. Howlett, C. Huterer, D. Ishak, M. Juneau, S. Kehoe, R. Kisner, T. Kremin, A. Lahav, O. Lamman, C. Landriau, M. Goff, J. M. Le Guillou, L. Le Leauthaud, A. Levi, M. E. Li, Q. Manera, M. Martini, P. Meisner, A. Mena-Fernandez, J. Miquel, R. Moustakas, J. Muñoz-Gutiérrez, A. Myers, A. D. Nadathur, S. Napolitano, L. Noriega, H. E. Paillas, E. Palanque-Delabrouille, N. Percival, W. J. Poppett, C. Prada, F. Pérez-Ràfols, I. Ramírez-Pérez, C. Ravoux, C. Rohlf, J. Rossi, G. Sanchez, E. Schlegel, D. Schubnell, M. Sinigaglia, F. Sprayberry, D. Tarlé, G. Taylor, P. Turner, W. Walther, M. Weaver, B. A. Yèche, C. Zhou, R. Zou, H. Zou, S. |
| author_facet | Brodzeller, A. Wolfson, M. Santos, D. M. Ho, M. Tan, T. Pieri, M. M. Cuceu, A. Abdul-Karim, M. Aguilar, J. Ahlen, S. Anand, A. Andrade, U. Armengaud, E. Aviles, A. Bailey, S. Bault, A. Bianchi, D. Brooks, D. Canning, R. Casas, L. Charles, M. Chaussidon, E. Chaves-Montero, J. Chebat, D. Claybaugh, T. Dawson, K. S. de Belsunce, R. de la Macorra, A. de Mattia, A. Dey, Arjun Dey, Biprateep Doshi, M. Doel, P. Elbers, W. Ferraro, S. Font-Ribera, A. Forero-Romero, J. E. Garcia-Quintero, C. Garrison, L. H. Gaztañaga, E. Gontcho, S. Gontcho A Gonzalez-Morales, A. X. Green, D. Gutierrez, G. Guy, J. Hahn, C. Herbold, M. Herrera-Alcantar, H. K. Honscheid, K. Howlett, C. Huterer, D. Ishak, M. Juneau, S. Kehoe, R. Kisner, T. Kremin, A. Lahav, O. Lamman, C. Landriau, M. Goff, J. M. Le Guillou, L. Le Leauthaud, A. Levi, M. E. Li, Q. Manera, M. Martini, P. Meisner, A. Mena-Fernandez, J. Miquel, R. Moustakas, J. Muñoz-Gutiérrez, A. Myers, A. D. Nadathur, S. Napolitano, L. Noriega, H. E. Paillas, E. Palanque-Delabrouille, N. Percival, W. J. Poppett, C. Prada, F. Pérez-Ràfols, I. Ramírez-Pérez, C. Ravoux, C. Rohlf, J. Rossi, G. Sanchez, E. Schlegel, D. Schubnell, M. Sinigaglia, F. Sprayberry, D. Tarlé, G. Taylor, P. Turner, W. Walther, M. Weaver, B. A. Yèche, C. Zhou, R. Zou, H. Zou, S. |
| contents | We present the Damped Ly$α$ Toolkit for automated detection and characterization of Damped Ly$α$ absorbers (DLA) in quasar spectra. Our method uses quasar spectral templates with and without absorption from intervening DLAs to reconstruct observed quasar forest regions. The best-fitting model determines whether a DLA is present while estimating the redshift and \texttt{HI} column density. With an optimized quality cut on detection significance ($Δχ_{r}^2>0.03$), the technique achieves an estimated 80\% purity and 79\% completeness when evaluated on simulated spectra with S/N~$>2$ that are free of broad absorption lines (BAL). We provide a catalog containing candidate DLAs from the DLA Toolkit detected in DESI DR1 quasar spectra, of which 21,719 were found in S/N~$>2$ spectra with predicted $\log_{10} (N_\texttt{HI}) > 20.3$ and detection significance $Δχ_{r}^2 >0.03$. We compare the Damped Ly$α$ Toolkit to two alternative DLA finders based on a convolutional neural network (CNN) and Gaussian process (GP) models. We present a strategy for combining these three techniques to produce a high-fidelity DLA catalog from DESI DR2 for the Ly$α$ forest baryon acoustic oscillation measurement. The combined catalog contains 41,152 candidate DLAs with $\log_{10} (N_\texttt{HI}) > 20.3$ from quasar spectra with S/N~$>2$. We estimate this sample to be approximately 85\% pure and 79\% complete when BAL quasars are excluded. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2503_14740 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Construction of the Damped Ly$α$ Absorber Catalog for DESI DR2 Ly$α$ BAO Brodzeller, A. Wolfson, M. Santos, D. M. Ho, M. Tan, T. Pieri, M. M. Cuceu, A. Abdul-Karim, M. Aguilar, J. Ahlen, S. Anand, A. Andrade, U. Armengaud, E. Aviles, A. Bailey, S. Bault, A. Bianchi, D. Brooks, D. Canning, R. Casas, L. Charles, M. Chaussidon, E. Chaves-Montero, J. Chebat, D. Claybaugh, T. Dawson, K. S. de Belsunce, R. de la Macorra, A. de Mattia, A. Dey, Arjun Dey, Biprateep Doshi, M. Doel, P. Elbers, W. Ferraro, S. Font-Ribera, A. Forero-Romero, J. E. Garcia-Quintero, C. Garrison, L. H. Gaztañaga, E. Gontcho, S. Gontcho A Gonzalez-Morales, A. X. Green, D. Gutierrez, G. Guy, J. Hahn, C. Herbold, M. Herrera-Alcantar, H. K. Honscheid, K. Howlett, C. Huterer, D. Ishak, M. Juneau, S. Kehoe, R. Kisner, T. Kremin, A. Lahav, O. Lamman, C. Landriau, M. Goff, J. M. Le Guillou, L. Le Leauthaud, A. Levi, M. E. Li, Q. Manera, M. Martini, P. Meisner, A. Mena-Fernandez, J. Miquel, R. Moustakas, J. Muñoz-Gutiérrez, A. Myers, A. D. Nadathur, S. Napolitano, L. Noriega, H. E. Paillas, E. Palanque-Delabrouille, N. Percival, W. J. Poppett, C. Prada, F. Pérez-Ràfols, I. Ramírez-Pérez, C. Ravoux, C. Rohlf, J. Rossi, G. Sanchez, E. Schlegel, D. Schubnell, M. Sinigaglia, F. Sprayberry, D. Tarlé, G. Taylor, P. Turner, W. Walther, M. Weaver, B. A. Yèche, C. Zhou, R. Zou, H. Zou, S. Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies We present the Damped Ly$α$ Toolkit for automated detection and characterization of Damped Ly$α$ absorbers (DLA) in quasar spectra. Our method uses quasar spectral templates with and without absorption from intervening DLAs to reconstruct observed quasar forest regions. The best-fitting model determines whether a DLA is present while estimating the redshift and \texttt{HI} column density. With an optimized quality cut on detection significance ($Δχ_{r}^2>0.03$), the technique achieves an estimated 80\% purity and 79\% completeness when evaluated on simulated spectra with S/N~$>2$ that are free of broad absorption lines (BAL). We provide a catalog containing candidate DLAs from the DLA Toolkit detected in DESI DR1 quasar spectra, of which 21,719 were found in S/N~$>2$ spectra with predicted $\log_{10} (N_\texttt{HI}) > 20.3$ and detection significance $Δχ_{r}^2 >0.03$. We compare the Damped Ly$α$ Toolkit to two alternative DLA finders based on a convolutional neural network (CNN) and Gaussian process (GP) models. We present a strategy for combining these three techniques to produce a high-fidelity DLA catalog from DESI DR2 for the Ly$α$ forest baryon acoustic oscillation measurement. The combined catalog contains 41,152 candidate DLAs with $\log_{10} (N_\texttt{HI}) > 20.3$ from quasar spectra with S/N~$>2$. We estimate this sample to be approximately 85\% pure and 79\% complete when BAL quasars are excluded. |
| title | Construction of the Damped Ly$α$ Absorber Catalog for DESI DR2 Ly$α$ BAO |
| topic | Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2503.14740 |