244 research outputs found
Including parameter dependence in the data and covariance for cosmological inference
The final step of most large-scale structure analyses involves the comparison
of power spectra or correlation functions to theoretical models. It is clear
that the theoretical models have parameter dependence, but frequently the
measurements and the covariance matrix depend upon some of the parameters as
well. We show that a very simple interpolation scheme from an unstructured mesh
allows for an efficient way to include this parameter dependence
self-consistently in the analysis at modest computational expense. We describe
two schemes for covariance matrices. The scheme which uses the geometric
structure of such matrices performs roughly twice as well as the simplest
scheme, though both perform very well.Comment: 17 pages, 4 figures, matches version published in JCA
Matched filtering with interferometric 21cm experiments
A new generation of interferometric instruments is emerging which aim to use
intensity mapping of redshifted cm radiation to measure the large-scale
structure of the Universe at over wide areas of sky. While these
instruments typically have limited angular resolution, they cover huge volumes
and thus can be used to provide large samples of rare objects. In this paper we
study how well such instruments could find spatially extended large-scale
structures, such as cosmic voids, using a matched filter formalism. Such a
formalism allows us to work in Fourier space, the natural space for
interferometers, and to study the impact of finite coverage, noise and
foregrounds on our ability to recover voids. We find that in the absence of
foregrounds such instruments would provide enormous catalogs of voids, with
high completeness, but that control of foregrounds is key to realizing this
goal.Comment: 14 pages, 8 figures, minor revisions to match version accepted by
MNRA
Constraints on local primordial non-Gaussianity from large scale structure
Recent work has shown that the local non-Gaussianity parameter f_NL induces a
scale-dependent bias, whose amplitude is growing with scale. Here we first
rederive this result within the context of peak-background split formalism and
show that it only depends on the assumption of universality of mass function,
assuming halo bias only depends on mass. We then use extended Press-Schechter
formalism to argue that this assumption may be violated and the scale dependent
bias will depend on other properties, such as merging history of halos. In
particular, in the limit of recent mergers we find the effect is suppressed.
Next we use these predictions in conjunction with a compendium of large scale
data to put a limit on the value of f_NL. When combining all data assuming that
halo occupation depends only on halo mass, we get a limit of -29 ~ (-65)< f_NL
< +70 ~(+93) at 95% (99.7%) confidence. While we use a wide range of datasets,
our combined result is dominated by the signal from the SDSS photometric quasar
sample. If the latter are modeled as recent mergers then the limits weaken to
-31 ~(-96) < f_NL < +70 ~ (+96) . These limits are comparable to the strongest
current limits from the WMAP 5 year analysis, with no evidence of a positive
signal in f_NL. While the method needs to be thoroughly tested against large
scale structure simulations with realistic quasar and galaxy formation models,
our results indicate that this is a competitive method relative to CMB and
should be further pursued both observationally and theoretically.Comment: 18 pages, 5 figures; v2 matches version accepted by JCAP, several
small changes in the text, added refs and fixed typo
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