alphaFeedback
SA

S. Allam

astro-ph.COastro-ph.GAastro-ph.IM

On Valency

published · living versions
W_594umn73·v1 · currentpublished

Preprints & journals

12 papers in the corpus · 2017–2026
Dark Energy Survey: DESI-Independent Angular BAO Measurement2601.14864v2 · J. Mena-Fern'andez, S. Avila, A. Porredon et al.2026 · 2 citationsPhys. Rev. D 113, 123521 (2026)
Dark Energy Survey Year 6 Results: Galaxy-galaxy lensing2601.15175v2 · G. Giannini, G. Camacho-Ciurana, A. Whyley et al.2026 · 2 citationsPhysical Review D, Volume 113, Issue 10, id.103503, 30 pp, May 2026
Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample2509.07964v2 · G. Giannini, A. Alarcon, W. d'Assignies et al.2025 · 2 citationsPhysical Review D, Volume 114, Issue 2, id.023520, 35 pp, July 2026
Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset2402.10697v2 · J. Mena-Fern'andez, M. Rodr'iguez-Monroy, S. Avila et al.2024 · 14 citationsPhys. Rev. D 110, 063514 (2024)
The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset2401.02929v4 · T. M. C. Abbott, M. Acevedo, M. Aguena et al.2024 · 35 citationsThe Astrophysical Journal Letters (2024), 973(1), L14on Valency
Dark Energy Survey Year 1 Results: tomographic cross-correlations between DES galaxies and CMB lensing from SPT+Planck1810.02342v1 · Y. Omori, T. Giannantonio, A. Porredon et al.2018 · 52 citationsPhys. Rev. D 100, 043501 (2019)
Dark Energy Survey Year 1 Results: Cross-correlation between DES Y1 galaxy weak lensing and SPT+Planck CMB weak lensing1810.02441v1 · Y. Omori, E. Baxter, C. Chang et al.2018 · 30 citationsPhys. Rev. D 100, 043517 (2019)
DES Science Portal: Computing Photometric Redshifts1708.05643v3 · Julia Gschwend, Aurelio Carnero Rosell, Ricardo Ogando et al.2017 · 26 citations2018A&C....25...58G
Career total: 15 works. 12 are in this corpus.

Profile built from the corpus for this byline.

Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.