activity
20182026
most citedDynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements

62 citations · 290 across the 81 of their papers we have counts for

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Showing 2024Show all

23 papers · 1 filter

astro-ph.GA2024★ 1 cited

DESI Mg II Absorbers: Extinction Characteristics & Quasar Redshift Accuracy

Lucas Napolitano, Adam D. Myers, Vicky Fawcett +32

In this paper, we study how absorption-line systems affect the spectra and redshifts of quasars (QSOs), using catalogs of Mg II absorbers from the early data release (EDR) and firs…

astro-ph.CO2024★ 1 cited

Constraining the phase shift of relativistic species in DESI BAOs

Abbé M. Whitford, Hugo Rivera-Morales, Cullan Howlett +36

In the early Universe, neutrinos decouple quickly from the primordial plasma and propagate without further interactions. The impact of free-streaming neutrinos is to create a tempo…

astro-ph.GA2024

The first identification of Lyman Changing-look Quasars at high-redshift in DESI

Wei-Jian Guo, Zhiwei Pan, Małgorzata Siudek +38

We present two cases of Ly changing-look (CL) quasars (J1306 and J1512) along with two additional candidates (J1511 and J1602), all discovered serendipitously at through…

astro-ph.CO2024★ 6 cited

DESIVAST: A Catalog of Low-Redshift Voids using Data from the DESI DR1 Bright Galaxy Survey

Hernan Rincon, Segev BenZvi, Kelly Douglass +37

We present three separate void catalogs created using a volume-limited sample of the DESI Year 1 Bright Galaxy Survey. We use the algorithms VoidFinder and V2 to construct void cat…

astro-ph.CO2024

The Atacama Cosmology Telescope DR6 and DESI: Structure growth measurements from the cross-correlation of DESI Legacy Imaging galaxies and CMB lensing from ACT DR6 and Planck PR4

Frank J. Qu, Qianjun Hang, Gerrit Farren +51

We measure the growth of cosmic density fluctuations on large scales and across the redshift range through the cross-correlation of the ACT DR6 CMB lensing map and gala…

astro-ph.GA2024★ 1 cited

DESI Emission Line Galaxies: Unveiling the Diversity of [OII] Profiles and its Links to Star Formation and Morphology

Ting-Wen Lan, J. Xavier Prochaska, John Moustakas +34

We study the [OII] profiles of emission line galaxies (ELGs) from the Early Data Release of the Dark Energy Spectroscopic Instrument (DESI). To this end, we decompose and classify…

astro-ph.GA2024★ 18 cited

Exploring the interaction between the MW and LMC with a large sample of blue horizontal branch stars from the DESI survey

Amanda Byström, Sergey E. Koposov, Sophia Lilleengen +42

The Large Magellanic Cloud (LMC) is a Milky Way (MW) satellite that is massive enough to gravitationally attract the MW disc and inner halo, causing significant motion of the inner…

astro-ph.CO2024

Selection of high-redshift Lyman-Break Galaxies from broadband and wide photometric surveys

C. Payerne, W. d'Assignies Doumerg, C. Yèche +44

In this paper, we investigate the possibility of selecting high-redshift Lyman-Break Galaxies (LBG) using current and future broadband wide photometric surveys, such as UNIONS or t…

astro-ph.IM2024

ANNZ+: an enhanced photometric redshift estimation algorithm with applications on the PAU Survey

Imdad Mahmud Pathi, John Y. H. Soo, Mao Jie Wee +16

ANNZ is a fast and simple algorithm which utilises artificial neural networks (ANNs), it was known as one of the pioneers of machine learning approaches to photometric redshift est…

astro-ph.GA2024★ 9 cited

Stellar reddening map from DESI imaging and spectroscopy

Rongpu Zhou, Julien Guy, Sergey E. Koposov +54

We present new Galactic dust reddening maps of the high Galactic latitude sky using DESI imaging and spectroscopy. We directly measure the reddening of 2.6 million stars by compari…

astro-ph.CO2024

Detection of the large-scale tidal field with galaxy multiplet alignment in the DESI Y1 spectroscopic survey

Claire Lamman, Daniel Eisenstein, Jaime E. Forero-Romero +36

We explore correlations between the orientations of small galaxy groups, or "multiplets", and the large-scale gravitational tidal field. Using data from the Dark Energy Spectroscop…

astro-ph.CO2024★ 19 cited

Measuring using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference

Tanveer Karim, Sukhdeep Singh, Mehdi Rezaie +39

Measuring the growth of structure is a powerful probe for studying the dark sector, especially in light of the tension between primary CMB anisotropy and low-redshift surveys…

astro-ph.GA2024★ 3 cited

Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. II. Statistical Properties from the First Data Release

Wei-Jian Guo, Hu Zou, Claire L. Greenwell +33

We present the identification of changing-look active galactic nuclei (CL-AGNs) from the Dark Energy Spectroscopic Instrument First Data Release and Sloan Digital Sky Survey Data R…

astro-ph.GA2024★ 8 cited

DESI Massive Post-Starburst Galaxies at have compact structures and dense cores

Yunchong Zhang, David J. Setton, Sedona H. Price +33

Post-starburst galaxies (PSBs) are young quiescent galaxies that have recently experienced a rapid decrease in star formation, allowing us to probe the fast-quenching period of gal…

astro-ph.GA2024★ 4 cited

The PAU Survey: The quasar UV and Ly luminosity functions at

Alberto Torralba-Torregrosa, Pablo Renard, Daniele Spinoso +17

We present the Lyman- (Ly) and ultraviolet (UV) luminosity function (LF), in bins of redshift, of quasars selected in the Physics of the Accelerating Universe Survey (PAUS).…

astro-ph.GA2024★ 5 cited

AuriDESI: Mock Catalogues for the DESI Milky Way Survey

Namitha Kizhuprakkat, Andrew P. Cooper, Alexander H. Riley +31

The Dark Energy Spectroscopic Instrument Milky Way Survey (DESI MWS) will explore the assembly history of the Milky Way by characterising remnants of ancient dwarf galaxy accretion…

astro-ph.HE2024★ 1 cited

The MOST Hosts Survey: spectroscopic observation of the host galaxies of ~40,000 transients using DESI

Maayane T. Soumagnac, Peter Nugent, Robert A. Knop +54

We present the MOST Hosts survey (Multi-Object Spectroscopy of Transient Hosts). The survey is planned to run throughout the five years of operation of the Dark Energy Spectroscopi…

astro-ph.CO2024

Constraints on the spacetime variation of the fine-structure constant using DESI emission-line galaxies

Linhua Jiang, Zhiwei Pan, Jessica Nicole Aguilar +38

We present strong constraints on the spacetime variation of the fine-structure constant using the Dark Energy Spectroscopic Instrument (DESI). In this pilot work, we utilize $\…

astro-ph.CO2024★ 11 cited

High redshift LBGs from deep broadband imaging for future spectroscopic surveys

Vanina Ruhlmann-Kleider, Christophe Yèche, Christophe Magneville +60

Lyman break galaxies (LBGs) are promising probes for clustering measurements at high redshift, , a region only covered so far by Lyman- forest measurements. In this paper,…

astro-ph.GA2024★ 6 cited

Emission Line Predictions for Mock Galaxy Catalogues: a New Differentiable and Empirical Mapping from DESI

Ashod Khederlarian, Jeffrey A. Newman, Brett H. Andrews +43

We present a simple, differentiable method for predicting emission line strengths from rest-frame optical continua using an empirically-determined mapping. Extensive work has been…

astro-ph.CO2024

Redshift evolution and covariances for joint lensing and clustering studies with DESI Y1

Sihan Yuan, Chris Blake, Alex Krolewski +48

Galaxy-galaxy lensing (GGL) and clustering measurements from the Dark Energy Spectroscopic Instrument Year 1 (DESI Y1) dataset promise to yield unprecedented combined-probe tests o…

astro-ph.HE2024★ 10 cited

The rate of extreme coronal line emitting galaxies in the Sloan Digital Sky Survey and their relation to tidal disruption events

Joseph Callow, Or Graur, Peter Clark +27

High-ionization iron coronal lines (CLs) are a rare phenomenon observed in galaxy and quasi-stellar object spectra that are thought to be created by high-energy emission from activ…

astro-ph.CO2024★ 16 cited

Synthetic spectra for Lyman- forest analysis in the Dark Energy Spectroscopic Instrument

Hiram K. Herrera-Alcantar, Andrea Muñoz-Gutiérrez, Ting Tan +51

Synthetic data sets are used in cosmology to test analysis procedures, to verify that systematic errors are well understood and to demonstrate that measurements are unbiased. In th…