ORCID Profile
0000-0001-8820-673X
Current Organisation
University of Oxford
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Publisher: American Physical Society (APS)
Date: 08-07-2009
Publisher: Oxford University Press (OUP)
Date: 14-03-2018
DOI: 10.1093/MNRAS/STY551
Publisher: Oxford University Press (OUP)
Date: 12-08-2016
Publisher: American Astronomical Society
Date: 14-01-2011
Publisher: Oxford University Press (OUP)
Date: 19-07-2017
Publisher: American Physical Society (APS)
Date: 05-03-2013
Publisher: IOP Publishing
Date: 17-08-2010
Publisher: Cambridge University Press (CUP)
Date: 2017
DOI: 10.1017/PASA.2017.6
Abstract: Superluminous supernovae are beginning to be discovered at redshifts as early as the epoch of reionisation. A number of candidate mechanisms is reviewed, together with the discovery programmes.
Publisher: Oxford University Press (OUP)
Date: 23-06-2018
Publisher: American Physical Society (APS)
Date: 24-06-2010
Publisher: The Open Journal
Date: 26-06-2019
Publisher: Oxford University Press (OUP)
Date: 23-08-2017
Publisher: Oxford University Press (OUP)
Date: 17-12-2013
DOI: 10.1093/MNRAS/STS437
Publisher: EDP Sciences
Date: 2020
DOI: 10.1051/0004-6361/201936772
Abstract: We reanalyse the anisotropic galaxy clustering measurement from the Baryon Oscillation Spectroscopic Survey (BOSS), demonstrating that using the full shape information provides cosmological constraints that are comparable to other low-redshift probes. We find Ω m = 0.317 +0.015 −0.019 , σ 8 = 0.710±0.049, and h = 0.704 ± 0.024 for flat ΛCDM cosmologies using uninformative priors on Ω c h 2 , 100 θ MC , ln10 10 A s , and n s , and a prior on Ω b h 2 that is much wider than current constraints. We quantify the agreement between the Planck 2018 constraints from the cosmic microwave background and BOSS, finding the two data sets to be consistent within a flat ΛCDM cosmology using the Bayes factor as well as the prior-insensitive suspiciousness statistic. Combining two low-redshift probes, we jointly analyse the clustering of BOSS galaxies with weak lensing measurements from the Kilo-Degree Survey (KV450). The combination of BOSS and KV450 improves the measurement by up to 45%, constraining σ 8 = 0.702 ± 0.029 and S 8 = σ 8 Ω m /0.3 = 0.728 ± 0.026. Over the full 5D parameter space, the odds in favour of a single cosmology describing galaxy clustering, lensing, and the cosmic microwave background are 7 ± 2. The suspiciousness statistic signals a 2.1 ± 0.3 σ tension between the combined low-redshift probes and measurements from the cosmic microwave background.
Publisher: Oxford University Press (OUP)
Date: 04-06-2014
DOI: 10.1093/MNRAS/STU794
Publisher: Oxford University Press (OUP)
Date: 05-04-2018
DOI: 10.1093/MNRAS/STY859
Publisher: Oxford University Press (OUP)
Date: 05-12-2017
Publisher: Oxford University Press (OUP)
Date: 23-11-2017
Publisher: Oxford University Press (OUP)
Date: 04-10-2012
Publisher: Oxford University Press (OUP)
Date: 09-08-2016
Publisher: American Physical Society (APS)
Date: 25-04-2013
Publisher: American Psychological Association (APA)
Date: 03-2023
DOI: 10.1037/NEU0000850
Publisher: Oxford University Press (OUP)
Date: 31-10-2018
Publisher: Oxford University Press (OUP)
Date: 17-10-2017
Publisher: American Physical Society (APS)
Date: 19-06-2008
Publisher: Oxford University Press (OUP)
Date: 04-07-2017
Publisher: American Physical Society (APS)
Date: 04-06-2018
Publisher: American Physical Society (APS)
Date: 21-09-2011
Publisher: Oxford University Press (OUP)
Date: 02-11-2016
Publisher: Oxford University Press (OUP)
Date: 13-10-2015
Publisher: Oxford University Press (OUP)
Date: 31-12-2016
Publisher: American Physical Society (APS)
Date: 13-07-2012
Publisher: Oxford University Press (OUP)
Date: 26-04-2017
DOI: 10.1093/MNRAS/STX998
Publisher: Oxford University Press (OUP)
Date: 26-02-2016
DOI: 10.1093/MNRAS/STW447
Publisher: Elsevier BV
Date: 10-2009
Location: United Kingdom of Great Britain and Northern Ireland
No related grants have been discovered for Shahab Joudaki.