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20242026
most citedArchetype-Based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey

29 citations · 101 across the 32 of their papers we have counts for

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Showing 2024 · astro-ph.COShow all

13 papers · 2 filters

astro-ph.CO2024

Extensive analysis of reconstruction algorithms for DESI 2024 baryon acoustic oscillations

X. Chen, Z. Ding, E. Paillas +64

Reconstruction of the baryon acoustic oscillation (BAO) signal has been a standard procedure in BAO analyses over the past decade and has helped to improve the BAO parameter precis…

astro-ph.CO2024★ 1 cited

Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples

E. Chaussidon, C. Yèche, A. de Mattia +49

We analyse the large-scale clustering of the Luminous Red Galaxy (LRG) and Quasar (QSO) sample from the first data release (DR1) of the Dark Energy Spectroscopic Instrument (DESI).…

astro-ph.CO2024

A Sound Horizon-Free Measurement of in DESI 2024

E. A. Zaborowski, P. Taylor, K. Honscheid +53

The physical size of the sound horizon at recombination is a powerful source of information for early-time measurements of the Hubble constant , and many proposed solutions to…

astro-ph.CO2024

Measuring the Mean Free Path of HI Ionizing Photons at with DESI Y1 Quasars

Anning Gao, Jason X. Prochaska, Zheng Cai +31

The mean free path of ionizing photons () in the intergalactic medium (IGM) is a crucial quantity in modelling the ionization state of IGM and the extragalact…

astro-ph.CO2024★ 5 cited

Window convolution of the galaxy clustering bispectrum

Mike Shengbo Wang, Florian Beutler, J. Aguilar +25

In galaxy survey analysis, the observed clustering statistics do not directly match theoretical predictions but rather have been processed by a window function that arises from the…

astro-ph.CO2024★ 3 cited

Catalog-level blinding on the bispectrum for DESI-like galaxy surveys

S. Novell-Masot, H. Gil-Marín, L. Verde +28

We evaluate the performance of the catalog-level blind analysis technique (blinding) presented in Brieden et al. (2020) in the context of a fixed template power spectrum and bispec…

astro-ph.CO2024★ 14 cited

Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel'dovich observations with ACT and DESI photometric galaxies

B. Hadzhiyska, S. Ferraro, B. Ried Guachalla +70

Recent advances in cosmological observations have provided an unprecedented opportunity to investigate the distribution of baryons relative to the underlying matter. In this work,…

astro-ph.CO2024★ 1 cited

STag II: Classification of Serendipitous Supernovae Observed by Galaxy Redshift Surveys

W. Davison, D. Parkinson, S. BenZvi +32

With the number of supernovae observed expected to drastically increase thanks to large-scale surveys like the Dark Energy Spectroscopic Instrument (DESI), it is necessary that the…

astro-ph.CO2024★ 21 cited

Fiducial-Cosmology-dependent systematics for the DESI 2024 BAO Analysis

A. Pérez-Fernández, L. Medina-Varela, R. Ruggeri +61

When measuring the Baryon Acoustic Oscillations (BAO) scale from galaxy surveys, one typically assumes a fiducial cosmology when converting redshift measurements into comoving dist…

astro-ph.CO2024

The clustering of Lyman Alpha Emitting galaxies at z=2-3

M. White, A. Raichoor, Arjun Dey +52

We measure the clustering of Lyman Alpha Emitting galaxies (LAEs) selected from the One-hundred-square-degree DECam Imaging in Narrowbands (ODIN) survey, with spectroscopic follow-…

astro-ph.CO2024★ 3 cited

Blinding scheme for the scale-dependence bias signature of local primordial non-Gaussianity for DESI 2024

E. Chaussidon, A. de Mattia, C. Yèche +32

The next generation of spectroscopic surveys is expected to achieve an unprecedented level of accuracy in the measurement of cosmological parameters. To avoid confirmation bias and…

astro-ph.CO2024★ 29 cited

Archetype-Based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey

Abhijeet Anand, Julien Guy, Stephen Bailey +46

We present a computationally efficient galaxy archetype-based redshift estimation and spectral classification method for the Dark Energy Survey Instrument (DESI) survey. The DESI s…

astro-ph.CO2024

The Dark Energy Survey 5-year photometrically classified type Ia supernovae without host-galaxy redshifts

A. Möller, P. Wiseman, M. Smith +60

Current and future Type Ia Supernova (SN Ia) surveys will need to adopt new approaches to classifying SNe and obtaining their redshifts without spectra if they wish to reach their…