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1 |
Material Type: Article
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Probing the growth of supermassive black holes at z > 6 with LOFARMonthly notices of the Royal Astronomical Society, 2006-12, Vol.373 (2), p.623-631 [Peer Reviewed Journal]2006 The Authors. Journal compilation © 2006 RAS 2006 ;2006 INIST-CNRS ;2006 The Authors. Journal compilation © 2006 RAS ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1111/j.1365-2966.2006.11003.x ;CODEN: MNRAA4Full text available |
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2 |
Material Type: Article
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New constraints on the linear growth rate using cosmic voids in the SDSS DR12 datasetsarXiv.org, 2019-032019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1903.05645Full text available |
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3 |
Material Type: Article
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An Accurate Fitting Function For Scale-dependent Growth Rate in Hu-Sawicki \(f(R)\) GravityarXiv.org, 2020-012020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1906.07683Full text available |
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4 |
Material Type: Article
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Perturbations in Tachyon Dark Energy and their Effect on Matter ClusteringarXiv.org, 2020-052020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1907.13309Full text available |
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5 |
Material Type: Article
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Validating the methodology for constraining the linear growth rate from clustering anisotropiesarXiv.org, 2020-032020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1909.08016Full text available |
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6 |
Material Type: Article
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Assessing non-linear models for galaxy clustering II: model validation and forecasts for Stage IV surveysarXiv.org, 2020-022020. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1905.05122Full text available |
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7 |
Material Type: Article
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A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voidsarXiv.org, 2018-102018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1805.09349Full text available |
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8 |
Material Type: Article
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The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space DistortionsarXiv.org, 2019-082019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1810.05183Full text available |
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9 |
Material Type: Article
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Synergies between radio, optical and microwave observations at high redshiftarXiv.org, 2019-062019. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1810.00911Full text available |
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10 |
Material Type: Article
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Modelling the environmental dependence of the growth ratearXiv.org, 2018-062018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1806.04684Full text available |
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11 |
Material Type: Article
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Growth of perturbations in dark energy parametrization scenariosarXiv.org, 2018-042018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1804.09886Full text available |
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12 |
Material Type: Article
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Deconstructing the neutrino mass constraint from galaxy redshift surveysarXiv.org, 2018-032018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1712.01857Full text available |
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13 |
Material Type: Article
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Information Content of the Angular Multipoles of Redshift-Space Galaxy BispectrumarXiv.org, 2016-122016. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1610.03488Full text available |
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14 |
Material Type: Article
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Limits on the growth rate of supermassive black holes at early cosmic epochsarXiv.org, 2017-092017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1709.04175Full text available |
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15 |
Material Type: Article
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Measuring the Universe with galaxy redshift surveysarXiv.org, 2018-032018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1803.10814Full text available |
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16 |
Material Type: Article
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Consistency of the growth rate in different environments with the 6dF Galaxy Survey: measurement of the void-galaxy and galaxy-galaxy correlation functionsarXiv.org, 2017-032017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1606.03092Full text available |
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17 |
Material Type: Article
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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2arXiv.org, 2018-012018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1801.03062Full text available |
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18 |
Material Type: Article
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Validating estimates of the growth rate of structure with modified gravity simulationsarXiv.org, 2016-112016. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1605.03965Full text available |
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19 |
Material Type: Article
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Measuring the growth rate of structure with Type IA Supernovae from LSSTarXiv.org, 2017-092017. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1708.08236Full text available |
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20 |
Material Type: Article
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Cosmological Forecasts for Combined and Next Generation Peculiar Velocity SurveysarXiv.org, 2016-092016. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;http://arxiv.org/licenses/nonexclusive-distrib/1.0 ;EISSN: 2331-8422 ;DOI: 10.48550/arxiv.1609.08247Full text available |