Constraining Primordial Non-Gaussianity with High-Redshift Probes

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

16 pages, 8 figures, 1 table, Accepted for publication on JCAP

Scientific paper

10.1088/1475-7516/2010/08/013

We present an analysis of the constraints on the amplitude of primordial non-Gaussianity of local type described by the dimensionless parameter $f_{\rm NL}$. These constraints are set by the auto-correlation functions (ACFs) of two large scale structure probes, the radio sources from NRAO VLA Sky Survey (NVSS) and the quasar catalogue of Sloan Digital Sky Survey Release Six (SDSS DR6 QSOs), as well as by their cross-correlation functions (CCFs) with the cosmic microwave background (CMB) temperature map (Integrated Sachs-Wolfe effect). Several systematic effects that may affect the observational estimates of the ACFs and of the CCFs are investigated and conservatively accounted for. Our approach exploits the large-scale scale-dependence of the non-Gaussian halo bias. The derived constraints on {$f_{\rm NL}$} coming from the NVSS CCF and from the QSO ACF and CCF are weaker than those previously obtained from the NVSS ACF, but still consistent with them. Finally, we obtain the constraints on $f_{\rm NL}=53\pm25$ ($1\,\sigma$) and $f_{\rm NL}=58\pm24$ ($1\,\sigma$) from NVSS data and SDSS DR6 QSO data, respectively.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Constraining Primordial Non-Gaussianity with High-Redshift Probes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Constraining Primordial Non-Gaussianity with High-Redshift Probes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Constraining Primordial Non-Gaussianity with High-Redshift Probes will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-349911

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.