The Lyman- Forest from LBGs: First 3D Correlation Measurement with DESI and Prospects for Cosmology
arXiv:2507.21852 · doi:10.1088/1475-7516/2025/12/053
Abstract
The Lyman- (Ly) forest is a key tracer of large-scale structure at redshifts z > 2, traditionally studied using spectra of quasars. Here, we explore the viability Lyman Break Galaxies (LBGs) as alternative background sources for Ly forest studies. We analyze 4,151 Ly forest skewers extracted from LBG spectra obtained in the DESI pilot surveys in the COSMOS and XMM-LSS fields. We present the first measurement of the Ly forest auto-correlation function derived exclusively from LBG spectra, probing comoving separations up to 48 Mpc at an effective redshift of = 2.70. The measured signal is consistent with that from DESI DR2 quasar Ly forest spectra at a comparable redshift, validating LBGs as reliable background sources. We also measure the cross-correlation between the LBG Ly forest and 13,362 galaxy positions, showing that this observable serves as a sensitive diagnostic for galaxy redshift uncertainties and systematic offsets. Finally, using synthetic LBG spectra and Fisher forecasts, we show that a future wide-area survey over 5000 deg, targeting 1000 LBGs per deg at similar signal-to-noise than our dataset, could enable Ly forest baryon acoustic oscillation (BAO) measurements with 0.4% precision on the isotropic BAO scale and 1.3% on the anisotropic (Alcock-Paczynski) scale. Combining BAO with a Ly forest full-shape analysis improves the AP constraint to 0.6%. These results open a new path for precision cosmology at high redshift using dense LBG samples.
References in corpus (28)
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Baryon Acoustic Oscillations in the Ly-α forest of BOSS quasars
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- PolyChord: nested sampling for cosmology
- Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman- forests
- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument
- Target Selection and Validation of DESI Quasars
- The Robotic Multi-Object Focal Plane System of the Dark Energy Spectroscopic Instrument (DESI)
- Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-alpha forest
- DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- The DESI Survey Validation: Results from Visual Inspection of the Quasar Survey Spectra
- The VLT LBG Redshift Survey - III. The clustering and dynamics of Lyman-break galaxies at z ~ 3
- The SDSS-DR12 large-scale cross-correlation of Damped Lyman Alpha Systems with the Lyman Alpha Forest
- Performance of the Quasar Spectral Templates for the Dark Energy Spectroscopic Instrument
- Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
- Constraints on the cosmic expansion rate at redshift 2.3 from the Lyman- forest
- Second Data Release of the COSMOS Lyman-alpha Mapping and Tomographic Observation: The First 3D Maps of the Detailed Cosmic Web at 2.05<z<2.55
- CoLoRe: fast cosmological realisations over large volumes with multiple tracers
- The extended Baryon Oscillation Spectroscopic Survey: measuring the cross-correlation between the MgII flux transmission field and quasars and galaxies at
- The Alcock-Paczyński effect from Lyman- forest correlations: Analysis validation with synthetic data
- The ACCEL project: simulating Lyman- forest in large-volume hydrodynamical simulations
- ELG Spectroscopic Systematics Analysis of the DESI Data Release 1
- Synthetic spectra for Lyman- forest analysis in the Dark Energy Spectroscopic Instrument
- Measurement of the small-scale 3D Lyman- forest power spectrum
- High redshift LBGs from deep broadband imaging for future spectroscopic surveys
- Effective Opacity of the Intergalactic Medium from Galaxy Spectra Analysis