We show how the massive data compression algorithm MOPED can be used to reduce, by orders of magnitude, the number of simulated data sets which are required to estimate the covariance matrix required for the analysis of Gaussian-distributed data. This is relevant when the covariance matrix cannot be calculated directly. The compression is especially valuable when the covariance matrix varies with the model parameters. In this case, it may be prohibitively expensive to run enough simulations to estimate the full covariance matrix throughout the parameter space. This compression may be particularly valuable for the next generation of weak lensing surveys, such as proposed for Euclid and Large Synoptic Survey Telescope, for which the number of...
In many astrophysical settings, covariance matrices of large data sets have to be determined empiric...
Data analysis in cosmology requires reliable covariance matrices. Covariance matrices derived from n...
In this paper, we propose a Gaussian Process (GP) emulator for the calculation both of tomographic w...
Albeit LCDM's fame as the concordance model, there are many interesting mysteries worth exploring, s...
Context. Future large scale cosmological surveys will provide huge data sets whose analysi...
The disconnected part of the power spectrum covariance matrix (also known as the "Gaussian" covarian...
International audienceThe covariance matrix Σ of non-linear clustering statistics that are measured ...
29 pags., 15 figs.The disconnected part of the power spectrum covariance matrix (also known as the >...
Upham, R.E., et al. (Euclid Consortium)An accurate covariance matrix is essential for obtaining reli...
Computation of covariance matrices from observed data is an important problem, as such matrices are ...
The final step of most large-scale structure analyses involves the comparison of power spectra or co...
Cosmological covariance matrices are fundamental for parameter inference, since they are responsible...
We present a method for radical linear compression of datasets where the data are dependent on some ...
With the ability to collect and store increasingly large datasets on modern computers comes the need...
Creating accurate and low-noise covariance matrices represents a formidable challenge in modern-day ...
In many astrophysical settings, covariance matrices of large data sets have to be determined empiric...
Data analysis in cosmology requires reliable covariance matrices. Covariance matrices derived from n...
In this paper, we propose a Gaussian Process (GP) emulator for the calculation both of tomographic w...
Albeit LCDM's fame as the concordance model, there are many interesting mysteries worth exploring, s...
Context. Future large scale cosmological surveys will provide huge data sets whose analysi...
The disconnected part of the power spectrum covariance matrix (also known as the "Gaussian" covarian...
International audienceThe covariance matrix Σ of non-linear clustering statistics that are measured ...
29 pags., 15 figs.The disconnected part of the power spectrum covariance matrix (also known as the >...
Upham, R.E., et al. (Euclid Consortium)An accurate covariance matrix is essential for obtaining reli...
Computation of covariance matrices from observed data is an important problem, as such matrices are ...
The final step of most large-scale structure analyses involves the comparison of power spectra or co...
Cosmological covariance matrices are fundamental for parameter inference, since they are responsible...
We present a method for radical linear compression of datasets where the data are dependent on some ...
With the ability to collect and store increasingly large datasets on modern computers comes the need...
Creating accurate and low-noise covariance matrices represents a formidable challenge in modern-day ...
In many astrophysical settings, covariance matrices of large data sets have to be determined empiric...
Data analysis in cosmology requires reliable covariance matrices. Covariance matrices derived from n...
In this paper, we propose a Gaussian Process (GP) emulator for the calculation both of tomographic w...