Baryon acoustic oscillations in thin redshift shells from BOSS DR12 and eBOSS DR16 galaxies

被引:9
|
作者
Menote, Ranier [1 ]
Marra, Valerio [2 ,3 ,4 ,5 ]
机构
[1] Univ Fed Espirito Santo, PPGCosmo, BR-29075910 Vitoria, ES, Brazil
[2] Univ Fed Espirito Santo, Nucleo Astrofis & Cosmol, BR-29075910 Vitoria, ES, Brazil
[3] Univ Fed Espirito Santo, Dept Fis, BR-29075910 Vitoria, ES, Brazil
[4] INAF Osservatorio Astron Trieste, Via Tiepolo 11, I-34131 Trieste, Italy
[5] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy
基金
美国国家科学基金会; 美国安德鲁·梅隆基金会;
关键词
cosmological parameters; large-scale structure of Universe; cosmology: observations; cosmology: theory; SPECTROSCOPIC SURVEY; SYSTEMATICS; CATALOGS; LIGHT;
D O I
10.1093/mnras/stac847
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In an age of large astronomical data sets and severe cosmological tensions, the case for model independent analyses is compelling. We present a set of 14 baryon acoustic oscillations measurements in thin redshift shells with 3 per cent precision that were obtained by analysing BOSS DR12 and eBOSS DR16 galaxies in the redshift range 0.32 < z < 0.66. Thanks to the use of thin shells, the analysis is carried out using just redshifts and angles so that the fiducial model is only introduced when considering the mock catalogues, necessary for the covariance matrix estimation and the pipeline validation. We compare our measurements, with and without supernova data, to the corresponding constraints from Planck 2018, finding good compatibility. A Monte Python module for this likelihood is available at github.com/ranier137/angularBAO.
引用
收藏
页码:1600 / 1608
页数:9
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