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Peer-reviewedCC BY 4.0The Astrophysical Journal

Unveiling Hidden Lyman Alpha Emitters in the DESI DR1 Data

30 more authors
36 affiliations
  1. 1National Taiwan University
  2. 2Institute of Astronomy and Astrophysics
  3. 3University of California at Santa Cruz
  4. 4University of California Observatories
  5. 5University of Tokyo
  6. 6Division of Science
  7. 7Missouri University of Science and Technology
  8. 8Lawrence Berkeley National Laboratory
  9. 9Boston University
  10. 10Università degli Studi di Milano
  11. 11INAF-Osservatorio Astronomico di Brera
  12. 12University College London
  13. 13Universidad Nacional Autónoma de México
  14. 14University of Toronto
  15. 15University of Pittsburgh
  16. 16Institució Catalana de Recerca i Estudis Avançats
  17. 17Institut de Física d’Altes Energies (IFAE)
  18. 18Universidad de los Andes
  19. 19Institut d’Estudis Espacials de Catalunya (IEEC)
  20. 20University of Portsmouth
  21. 21Institute of Space Sciences
  22. 22University of Virginia
  23. 23Fermi National Accelerator Laboratory
  24. 24University of Texas at Austin
  25. 25NSF NOIRLab
  26. 26University of California
  27. 27Universitat Autònoma de Barcelona
  28. 28Siena University
  29. 29University of Waterloo
  30. 30Perimeter Institute for Theoretical Physics
  31. 31Instituto de Astrofísica de Andalucía (CSIC)
  32. 32Universitat Politècnica de Catalunya
  33. 33Sejong University
  34. 34CIEMAT
  35. 35University of Michigan
  36. 36Chinese Academy of Sciences

Abstract

We present an automatic method based on machine learning convolutional neural network (CNN) architecture to detect Ly α emitters (LAEs) hidden in the Data Release 1 spectroscopic data set of the Dark Energy Spectroscopic Instrument (DESI). Those LAEs mostly have incorrect redshift estimations because the current DESI pipeline is not designed to detect and measure the redshifts of galaxies at z > 2. To uncover those sources, we first visually inspect 4134 DESI spectra and construct a sample, consisting of both LAEs and non-LAEs, for training and testing the CNN-based model to (1) detect LAEs in DESI spectra and (2) determine their Ly α redshifts. The final model yields 95.2% purity and 95.9% completeness for detecting LAEs. We apply this model to approximately 2 × 10 ⁶ spectra of sources targeted as emission-line galaxies and detect 19,685 LAEs from z ∼ 2 to 3.5 within 12 minutes with a single GPU, illustrating the high efficiency of this model for identifying LAEs. The detected LAEs are mostly at the bright end of the luminosity function with Ly α luminosity L Ly α ≳ 10 ⁴³ erg s ⁻¹ . The high signal-to-noise composite spectrum of the detected LAEs further shows various spectral features, including P-Cygni profiles of metal lines and Mg ii emission lines, possible indicators of Lyman continuum escape fraction, revealing the rich astrophysical information in this LAE sample. Finally, this sample can be used to train and validate the pipelines for redshift determination of LAEs for the preparation of the DESI-II survey.

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BibTeX
@article{chan2026unveiling,
  title = {{Unveiling Hidden Lyman Alpha Emitters in the DESI DR1 Data}},
  author = {Jui-Kuan Chan and Ting-Wen Lan and J. Xavier Prochaska and Shun Saito and J. Aguilar and S. Ahlen and D. Bianchi and D. Brooks and A. Cuceu and A. de la Macorra and Biprateep Dey and P. Doel and A. Font-Ribera and J. E. Forero-Romero and E. Gaztañaga and Satya Gontcho A Gontcho and G. Gutierrez and C. Hahn and J. Jimenez and R. Joyce and S. Juneau and D. Kirkby and A. Kremin and M. Landriau and M. Manera and A. Meisner and R. Miquel and J. Moustakas and S. Nadathur and W. J. Percival and C. Poppett and F. Prada and I. Pérez-Ràfols and G. Rossi and E. Sanchez and D. Schlegel and M. Schubnell and J. Silber and D. Sprayberry and G. Tarlé and B. A. Weaver and H. Zou},
  journal = {The Astrophysical Journal},
  year = {2026},
  month = oct,
  doi = {10.3847/1538-4357/aeaa44},
  url = {https://iopscience.iop.org/article/10.3847/1538-4357/aeaa44},
  note = {CC BY 4.0},
}
RIS
TY  - JOUR
TI  - Unveiling Hidden Lyman Alpha Emitters in the DESI DR1 Data
AU  - Jui-Kuan Chan
AU  - Ting-Wen Lan
AU  - J. Xavier Prochaska
AU  - Shun Saito
AU  - J. Aguilar
AU  - S. Ahlen
AU  - D. Bianchi
AU  - D. Brooks
AU  - A. Cuceu
AU  - A. de la Macorra
AU  - Biprateep Dey
AU  - P. Doel
AU  - A. Font-Ribera
AU  - J. E. Forero-Romero
AU  - E. Gaztañaga
AU  - Satya Gontcho A Gontcho
AU  - G. Gutierrez
AU  - C. Hahn
AU  - J. Jimenez
AU  - R. Joyce
AU  - S. Juneau
AU  - D. Kirkby
AU  - A. Kremin
AU  - M. Landriau
AU  - M. Manera
AU  - A. Meisner
AU  - R. Miquel
AU  - J. Moustakas
AU  - S. Nadathur
AU  - W. J. Percival
AU  - C. Poppett
AU  - F. Prada
AU  - I. Pérez-Ràfols
AU  - G. Rossi
AU  - E. Sanchez
AU  - D. Schlegel
AU  - M. Schubnell
AU  - J. Silber
AU  - D. Sprayberry
AU  - G. Tarlé
AU  - B. A. Weaver
AU  - H. Zou
PY  - 2026
DA  - 2026/10/28
JO  - The Astrophysical Journal
DO  - 10.3847/1538-4357/aeaa44
UR  - https://iopscience.iop.org/article/10.3847/1538-4357/aeaa44
AB  - We present an automatic method based on machine learning convolutional neural network (CNN) architecture to detect Ly α emitters (LAEs) hidden in the Data Release 1 spectroscopic data set of the Dark Energy Spectroscopic Instrument (DESI). Those LAEs mostly have incorrect redshift estimations because the current DESI pipeline is not designed to detect and measure the redshifts of galaxies at z > 2. To uncover those sources, we first visually inspect 4134 DESI spectra and construct a sample, consisting of both LAEs and non-LAEs, for training and testing the CNN-based model to (1) detect LAEs in DESI spectra and (2) determine their Ly α redshifts. The final model yields 95.2% purity and 95.9% completeness for detecting LAEs. We apply this model to approximately 2 × 10 ⁶ spectra of sources targeted as emission-line galaxies and detect 19,685 LAEs from z ∼ 2 to 3.5 within 12 minutes with a single GPU, illustrating the high efficiency of this model for identifying LAEs. The detected LAEs are mostly at the bright end of the luminosity function with Ly α luminosity L Ly α ≳ 10 ⁴³ erg s ⁻¹ . The high signal-to-noise composite spectrum of the detected LAEs further shows various spectral features, including P-Cygni profiles of metal lines and Mg ii emission lines, possible indicators of Lyman continuum escape fraction, revealing the rich astrophysical information in this LAE sample. Finally, this sample can be used to train and validate the pipelines for redshift determination of LAEs for the preparation of the DESI-II survey.
SN  - 1538-4357
SN  - 0004-637X
ER  -