DESI Strong Lens Foundry II: DESI Spectroscopy for Strong Lens Candidates
Xiaosheng Huang, Jose Carlos Inchausti, Christopher J. Storfer, S. Tabares-Tarquinio, J. Moustakas, W. Sheu, S. Agarwal, M. Tamargo-Arizmendi, D. J. Schlegel, J. Aguilar, S. Ahlen, G. Aldering, S. Bailey, S. Banka, S. BenZvi, D. Bianchi, A. Bolton, D. Brooks, A. Cikota, T. Claybaugh, K. S. Dawson, A. de la Macorra, A. Dey, P. Doel, J. Edelstein, J. E. Forero-Romero, E. Gaztanaga, S. Gontcho A Gontcho, A. X. Gonzalez-Morales, A. Gu, K. Honscheid, M. Ishak, S. Juneau, R. Kehoe, T. Kisner, S. E. Koposov, K. J. Kwon, A. Lambert, M. Landriau, D. Lang, L. Le Guillou, M. E. Levi, J. Liu, A. Meisner, R. Miquel, A. D. Myers, S. Perlmutter, N. Palanque-Delabrouille, I. Perez-Rafols, C. Poppett, F. Prada, G. Rossi, D. Rubin, E. Sanchez, M. Schubnell, Y. Shu, E. Silver, D. Sprayberry, N. Suzuki, G. Tarle, B. A. Weaver, H. Zou
Published: 2025/9/22
Abstract
We present the Dark Energy Spectroscopic Instrument (DESI) Strong Lensing Secondary Target Program. This is a spectroscopic follow-up program for strong gravitational lens candidates found in the DESI Legacy Imaging Surveys footprint. Spectroscopic redshifts for the lenses and lensed source are crucial for lens modeling to obtain physical parameters. The spectroscopic catalog in this paper consists of 73 candidate systems from the DESI Early Data Release (EDR). We have confirmed 20 strong lensing systems and determined four to not be lenses. For the remaining systems, more spectroscopic data from ongoing and future observations will be presented in future publications. We discuss the implications of our results for lens searches with neural networks in existing and future imaging surveys as well as for lens modeling. This Strong Lensing Secondary Target Program is part of the DESI Strong Lens Foundry project, and this is Paper II of a series on this project.