MM
M. Maus
astro-ph.COastro-ph.IMhep-exhep-phhep-th
On Valency
published · living versionsW_5mdbgr3b·v1 · currentpublished
DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
with DESI Collaboration, A. G. Adame, J. Aguilar, S. Ahlen +191
1 version
W_chhej67s·v1published
W_an52ar5m·v1published
Preprints & journals
17 papers in the corpus · 2022–2026DESI DR2 Results IV: Alcock-Paczyński Measurements from the Lyman Alpha Forest and Cosmological Constraints2607.27410v3 · A. G. Adame, J. Aguilar, S. Ahlen et al.2026 · 0 citationsarXiv
An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics2602.12343v2 · M. Maus, A. Baleato Lizancos, M. White et al.2026 · 2 citationsJCAP05(2026)078
Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy2601.16165v3 · Mikhail M. Ivanov, James M. Sullivan, Roger de Belsunce et al.2026 · 0 citationsarXiv
Enhancing DESI DR1 Full-Shape analyses using HOD-informed priors2504.10407v1 · Hanyu Zhang, Marco Bonici, Antoine Rocher et al.2025 · 9 citationsarXiv
Data Release 1 of the Dark Energy Spectroscopic Instrument2503.14745v2 · M. Abdul Karim, A. G. Adame, D. Aguado et al.2025 · 155 citationsarXivon Valency
DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars2411.12021v5 · A. G. Adame, J. Aguilar, S. Ahlen et al.2024 · 107 citationsJCAP, Volume 2025, Issue 09, id.008
DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements2411.12022v2 · A. G. Adame, J. Aguilar, S. Ahlen et al.2024 · 212 citationsJCAP 07 (2025) 028on Valency
Full Modeling and Parameter Compression Methods in configuration space for DESI 2024 and beyond2404.07268v2 · S. Ramirez-Solano, M. Icaza-Lizaola, H. E. Noriega et al.2024 · 20 citationsarXiv
Comparing Compressed and Full-modeling Analyses with FOLPS: Implications for DESI 2024 and beyond2404.07269v3 · H. E. Noriega, A. Aviles, H. Gil-Mar'in et al.2024 · 29 citationsarXiv
A comparison of effective field theory models of redshift space galaxy power spectra for DESI 2024 and future surveys2404.07272v4 · M. Maus, Y. Lai, H. E. Noriega et al.2024 · 41 citationsarXiv
A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond2404.07283v6 · Y. Lai, C. Howlett, M. Maus et al.2024 · 24 citationsarXiv
An analysis of parameter compression and full-modeling techniques with Velocileptors for DESI 2024 and beyond2404.07312v4 · M. Maus, S. Chen, M. White et al.2024 · 51 citationsarXiv
DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars2404.03000v1 · A. G. Adame, J. Aguilar, S. Ahlen et al.2024 · 323 citationsJCAP 04 (2025) 012on Valency
DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest2404.03001v4 · A. G. Adame, J. Aguilar, S. Ahlen et al.2024 · 272 citationsarXiv
DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations2404.03002v3 · A. G. Adame, J. Aguilar, S. Ahlen et al.2024 · 1,143 citationsJCAP 02 (2025) 021
A comparison of template vs. direct model fitting for redshift-space distortions in BOSS2302.07430v2 · Mark Maus, Shi-Fan Chen, Martin White2023 · 27 citationsarXiv
Accurate predictions from small boxes: variance suppression via the Zel'dovich approximation2205.15327v2 · Nickolas Kokron, Shi-Fan Chen, Martin White et al.2022 · 31 citationsarXiv
Career total: at least 28 works. 17 are in this corpus.
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