Can we really measure f NL from the galaxy power spectrum?

Monthly Notices of the Royal Astronomical Society: Letters

Volumn 425, Issue 1, 2012, Pages

  Roth, Nina ^a   Porciani, Cristiano ^a  

^a UNIVERSITY OF BONN   (Germany)

Author keywords

Cosmological parameters; Large scale structure of Universe; Methods: numerical

Indexed keywords

EID: 84869845829     PISSN: 17453933     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1745-3933.2012.01305.x     Document Type: Letter

References (22)

1. Bartolo N., Komatsu E., Matarrese S., Riotto A., 2004, Phys. Rep., 402, 103
2. Dalal N., Doré O., Huterer D., Shirokov A., 2008, Phys. Rev. D, 77, 123514
3. Desjacques V., Seljak U., 2010, Phys. Rev. D, 81, 023006
4. Giannantonio T., Porciani C., 2010, Phys. Rev. D, 81, 63530
5. Giannantonio T., Porciani C., Carron J., Amara A., Pillepich A., 2012, MNRAS, 422, 2854
6. Ivezic Z. et al., 2008, preprint (arXiv:0805.2366)
7. Jeffreys H., 1961, The Theory of Probability, 3rd edn. Oxford Univ. Press, Oxford
8. Kass R. E., 1993, Statistician, 42, 551
9. Komatsu E. et al., 2009, ApJS, 180, 330
10. Komatsu E. et al., 2011, ApJS, 192, 18
11. Laureijs R. et al., 2011, preprint (arXiv:1110.3193)
12. Matarrese S., Verde L., 2008, ApJ, 677, L77
13. Pillepich A., Porciani C., Hahn O., 2010, MNRAS, 402, 191
14. Pillepich A., Porciani C., Reiprich T. H., 2012, MNRAS, 422, 44
15. Predehl P. et al., 2010, Proc. SPIE, 7732, 23
16. Slosar A., Hirata C., Seljak U., Ho S., Padmanabhan N., 2008, J. Cosmol. Astropart. Phys., 8, 31
17. Smith K. M., LoVerde M., 2011, J. Cosmol. Astropart. Phys., 11, 9
18. Smith K. M., Ferraro S., LoVerde M., 2012, J. Cosmol. Astropart. Phys., 3, 32 (SFL12)
19. Springel V., 2005, MNRAS, 364, 1105
20. Trotta R., 2008, Contemporary Phys., 49, 71
21. Vielva P., Sanz J. L., 2010, MNRAS, 404, 895
22. Xia J.-Q., Baccigalupi C., Matarrese S., Verde L., Viel M., 2011, J. Cosmol. Astropart. Phys., 8, 33