Optimal 1D Ly$\alpha$ Forest Power Spectrum Estimation -- III. DESI early data
Naim G\"oksel Kara\c{c}ayl{\i}, Paul Martini, Julien Guy, Corentin, Ravoux, Marie Lynn Abdul-Karim, Eric Armengaud, Michael Walther, J. Aguilar,, S. Ahlen, S. Bailey, J. Bautista, S.F. Beltran, D. Brooks, L. Cabayol-Garcia,, S. Chabanier, E. Chaussidon, J. Chaves-Montero

TL;DR
This paper presents the first measurement of the 1D Lyα forest power spectrum using DESI early data, demonstrating the pipeline's accuracy and systematic error control, with implications for cosmology.
Contribution
It introduces the first quadratic maximum likelihood estimation of the Lyα forest power spectrum from DESI early data, including systematic error analysis and pipeline validation.
Findings
Successful measurement of $P_{\mathrm{1D}}$ with QMLE from DESI data
Validation of spectroscopic pipeline noise and resolution accuracy
Comparison with FFT-based methods for future analysis
Abstract
The one-dimensional power spectrum of the Ly forest provides important information about cosmological and astrophysical parameters, including constraints on warm dark matter models, the sum of the masses of the three neutrino species, and the thermal state of the intergalactic medium. We present the first measurement of with the quadratic maximum likelihood estimator (QMLE) from the Dark Energy Spectroscopic Instrument (DESI) survey early data sample. This early sample of quasars is already comparable in size to the largest previous studies, and we conduct a thorough investigation of numerous instrumental and analysis systematic errors to evaluate their impact on DESI data with QMLE. We demonstrate the excellent performance of the spectroscopic pipeline noise estimation and the impressive accuracy of the spectrograph resolution matrix…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Radio Astronomy Observations and Technology
