Работы, на которые ссылается эта работа

Работ: 141

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

Why your model parameter confidences might be too optimistic. Unbiased estimation of the inverse covariance matrix
J. Hartlap, P. Šimon, Peter Schneider
Статья2006Цитирований: 5
ABI
Dark Energy Survey Year 3 results: galaxy clustering and systematics treatment for lens galaxy samples
M. Rodríguez-Monroy, N. Weaverdyck, J. Elvin-Poole +97
Статья2022Цитирований: 5
ABI
Clustering in real space and in redshift space
Nick Kaiser
Статья1987Цитирований: 4
ABI
Без названия
ДругоеЦитирований: 4
ABI
Characterization of DESI fiber assignment incompleteness effect on 2-point clustering and mitigation methods for DR1 analysis
Davide Bianchi, M. Hanif, A. Carnero Rosell +52
СтатьяAdvanced Fluorescence Microscopy TechniquesJournal of Cosmology and Astroparticle Physics2025Цитирований: 4
ABI
An optimal FFT-based anisotropic power spectrum estimator
Nick Hand, Yin Li, Zachary Slepian +1
Статья2017Цитирований: 4
ABI
Без названия
ДругоеЦитирований: 4
ABI
Mitigating imaging systematics for DESI 2024 emission Line Galaxies and beyond
A. Rosado-Marin, A.J. Ross, Hee‐Jong Seo +55
СтатьяGalaxies: Formation, Evolution, PhenomenaJournal of Cosmology and Astroparticle Physics2025Цитирований: 4
ABI
Без названия
ДругоеЦитирований: 4
ABI
Mitigating contamination in LSS surveys: a comparison of methods
N. Weaverdyck, Dragan Huterer
Статья2021Цитирований: 4
ABI
Constraints on local primordial non-Gaussianity from large scale structure
Anže Slosar, Christopher Hirata, Uroš Seljak +2
Статья2008Цитирований: 3
ABI
Imprints of primordial non-Gaussianities on large-scale structure: Scale-dependent bias and abundance of virialized objects
Neal Dalal, Olivier Doré, Dragan Huterer +1
Статья2008Цитирований: 3
ABI
healpy: equal area pixelization and spherical harmonics transforms for data on the sphere in Python
A. Zonca, Leo Singer, Daniel Lenz +4
Статья2019Цитирований: 3
ABI
Performance of the Quasar Spectral Templates for the Dark Energy Spectroscopic Instrument
A. Brodzeller, Kyle Dawson, S. Bailey +44
Статья2023Цитирований: 3
ABI
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: anisotropic galaxy clustering in Fourier space
Florian Beutler, Hee‐Jong Seo, Shun Saito +20
Статья2016Цитирований: 3
ABI
Large-scale galaxy bias
Vincent Desjacques, Donghui Jeong, Fabian Schmidt
Статья2018Цитирований: 3
ABI
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: analysis of potential systematics
A.J. Ross, Will J. Percival, Ariel G. Sánchez +39
Статья2012Цитирований: 3
ABI
Forward modeling fluctuations in the DESI LRGs target sample using image simulations
H. Kong, A.J. Ross, K. Honscheid +50
СтатьяGamma-ray bursts and supernovaeJournal of Cosmology and Astroparticle Physics2025Цитирований: 3
ABI
Без названия
ДругоеЦитирований: 3
ABI
Ameliorating systematic uncertainties in the angular clustering of galaxies: a study using the SDSS-III
A.J. Ross, Shirley Ho, Antonio J. Cuesta +29
Статья2011Цитирований: 3
ABI
Improving galaxy clustering measurements with deep learning: analysis of the DECaLS DR7 data
Mehdi Rezaie, Hee‐Jong Seo, A.J. Ross +1
Статья2020Цитирований: 3
ABI
Removing imaging systematics from galaxy clustering measurements with <tt>Obiwan</tt>: application to the SDSS-IV extended Baryon Oscillation Spectroscopic Survey emission-line galaxy sample
H. Kong, Kaylan Burleigh, A.J. Ross +10
Статья2020Цитирований: 3
ABI
Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey – I: Catalogue preparation and systematic mitigation
Mehdi Rezaie, A.J. Ross, Hee‐Jong Seo +17
Статья2021Цитирований: 3
ABI
<i>Planck</i>2018 results
Y. Akrami, F. Arroja, M. Ashdown +97
Статья2019Цитирований: 3
ABI
Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey II: measurements in Fourier space with optimal weights
Eva-Maria Mueller, Mehdi Rezaie, Will J. Percival +12
Статья2022Цитирований: 3
ABI