Automated Author ProfileMoretti, Chiara
Institute for Astronomy, The University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UK0000-0003-3314-8936
Moretti, Chiara
Current S-Index
Sum of Dataset Indices for all datasets
Average Dataset Index per Dataset
Average Dataset Index per dataset
Total Datasets
Total datasets for this author
Average FAIR Score
Average FAIR Score per dataset
Total Citations
Total citations to the author's datasets
Total Mentions
Total mentions of the author's datasets
S-Index Interpretation
The S-Index (Sharing Index) is a comprehensive metric that represents the cumulative impact of all your datasets. It is calculated as the sum of Dataset Index scores across all your claimed datasets.
What it means:
- A higher S-index indicates greater overall impact of your datasets relative to typical datasets in their fields of research
- The S-Index grows as you add more datasets or as existing datasets gain more citations and mentions
- It provides a single number to track your research data impact over time
Current S-Index: 1.8 (sum of 9 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
Includes measurements of the post-reconstruction BAO alpha parameters and their covariances, following the agreed upon datamodels.redshifts = [1.0, 1.2, 1.4, 1.65]parameters = { 'H0': 67.0, 'Omega_cdm0': 0.27, 'Omega_b0': 0.049, 'Omega_k0': 0.0, 'mnu': 0.0, 'w0': -1.0, 'wa': 0.0, 'ns': 0.96, 'As': 2.1e-9, 'gamma_MG': 0.545,}The measurements assumed fiducial cosmology = true cosmology, so alpha=1 for all values.
Authors
- Moretti, Chiara ;
- Gambardella, Giosuè ;
- Sarpa, Elena
Description: Includes multipoles of the 2PCF post-reconstruction from smin=0 Mpc/h to smax=200 Mpc/h with a linear binning of 1 Mpc/h, to be used with the blinding notebook. Uses 4 redshift bins, from z=0.9 to z=1.8, with width of Delta_z=(0.2, 0.2, 0.2, 0.3). The synthetic data were generated with the publicly available code BeXiCov, using the following parameters:parameters = { 'H0': 67.0, 'Omega_cdm0': 0.27, 'Omega_b0': 0.049, 'Omega_k0': 0.0, 'mnu': 0.0, 'w0': -1.0, 'wa': 0.0, 'ns': 0.96, 'As': 2.1e-9, 'gamma_MG': 0.545, 'b1': np.array([1.412, 1.769, 2.039, 2.496]),}
Authors
- Moretti, Chiara
Description: Includes multipoles of the 2PCF and 2PCF polar post-reconstruction from smin=0 Mpc/h to smax=200 Mpc/h with a linear binning of 1 Mpc/h, to be used with the blinding notebook. Uses 4 redshift bins, from z=0.9 to z=1.8, with width of Delta_z=(0.2, 0.2, 0.2, 0.3). The synthetic data were generated with the publicly available code BeXiCov, using the following parameters:parameters = { 'H0': 67.0, 'Omega_cdm0': 0.27, 'Omega_b0': 0.049, 'Omega_k0': 0.0, 'mnu': 0.0, 'w0': -1.0, 'wa': 0.0, 'ns': 0.96, 'As': 2.1e-9, 'gamma_MG': 0.545, 'b1': np.array([1.412, 1.769, 2.039, 2.496]),}
Authors
- Moretti, Chiara
Includes measurements of the post-reconstruction BAO alpha parameters and their covariances, following the agreed upon datamodels.redshifts = [1.0, 1.2, 1.4, 1.65]parameters = { 'H0': 67.0, 'Omega_cdm0': 0.27, 'Omega_b0': 0.049, 'Omega_k0': 0.0, 'mnu': 0.0, 'w0': -1.0, 'wa': 0.0, 'ns': 0.96, 'As': 2.1e-9, 'gamma_MG': 0.545,}The measurements assumed fiducial cosmology = true cosmology, so alpha=1 for all values.
Authors
- Moretti, Chiara ;
- Gambardella, Giosuè ;
- Sarpa, Elena
Description: Includes multipoles of the 2PCF and 2PCF polar post-reconstruction from smin=0 Mpc/h to smax=200 Mpc/h with a linear binning of 1 Mpc/h, to be used with the blinding notebook. Uses 4 redshift bins, from z=0.9 to z=1.8, with width of Delta_z=(0.2, 0.2, 0.2, 0.3). The synthetic data were generated with the publicly available code BeXiCov, using the following parameters:parameters = { 'H0': 67.0, 'Omega_cdm0': 0.27, 'Omega_b0': 0.049, 'Omega_k0': 0.0, 'mnu': 0.0, 'w0': -1.0, 'wa': 0.0, 'ns': 0.96, 'As': 2.1e-9, 'gamma_MG': 0.545, 'b1': np.array([1.412, 1.769, 2.039, 2.496]),}
Authors
- Moretti, Chiara
Description: Includes multipoles of the 2PCF post-reconstruction from smin=0 Mpc/h to smax=200 Mpc/h with a linear binning of 1 Mpc/h, to be used with the blinding notebook. Uses 4 redshift bins, from z=0.9 to z=1.8, with width of Delta_z=(0.2, 0.2, 0.2, 0.3). The synthetic data were generated with the publicly available code BeXiCov, using the following parameters:parameters = { 'H0': 67.0, 'Omega_cdm0': 0.27, 'Omega_b0': 0.049, 'Omega_k0': 0.0, 'mnu': 0.0, 'w0': -1.0, 'wa': 0.0, 'ns': 0.96, 'As': 2.1e-9, 'gamma_MG': 0.545, 'b1': np.array([1.412, 1.769, 2.039, 2.496]),}
Authors
- Moretti, Chiara
Includes measurements of the post-reconstruction BAO alpha parameters and their covariances.redshifts = [1.0, 1.2, 1.4, 1.65]parameters = { 'H0': 67.0, 'Omega_cdm0': 0.27, 'Omega_b0': 0.049, 'Omega_k0': 0.0, 'mnu': 0.0, 'w0': -1.0, 'wa': 0.0, 'ns': 0.96, 'As': 2.1e-9, 'gamma_MG': 0.545,}The measurements assumed fiducial cosmology = true cosmology, so alpha=1 for all values.
Authors
- Moretti, Chiara ;
- Gambardella, Giosuè ;
- Sarpa, Elena
Includes measurements of the post-reconstruction BAO alpha parameters and their covariances.redshifts = [1.0, 1.2, 1.4, 1.65]parameters = { 'H0': 67.0, 'Omega_cdm0': 0.27, 'Omega_b0': 0.049, 'Omega_k0': 0.0, 'mnu': 0.0, 'w0': -1.0, 'wa': 0.0, 'ns': 0.96, 'As': 2.1e-9, 'gamma_MG': 0.545,}The measurements assumed fiducial cosmology = true cosmology, so alpha=1 for all values.
Authors
- Moretti, Chiara ;
- Gambardella, Giosuè ;
- Sarpa, Elena
This is the main repository for a distributed data set associated with the paper ‘Euclid: Modelling massive neutrinos in cosmology — a code comparison’. This record holds the scripts needed for generating all figures and power spectra, as well as some demonstration scripts. All is governed by a Makefile, which can also be used to download further data records. The finished figures are included as well. This is a direct record of the GitHub repository jmd-dk/nucodecomp-data, created by Jeppe Dakin ([email protected]). To get started exploring the data, download and extract the ZIP file contained within this record, or clone the Git repository:
git clone https://github.com/jmd-dk/nucodecomp-data.gitAuthors
- Adamek, Julian ;
- Angulo, Raul E. ;
- Arnold, Christian ;
- Baldi, Marco ;
- Biagetti, Matteo ;
- Bose, Benjamin ;
- Carbone, Carmelita ;
- Castro, Tiago ;
- Dakin, Jeppe ;
- Dolag, Klaus ;
- Elbers, Willem ;
- Fidler, Christian ;
- Giocoli, Carlo ;
- Hannestad, Steen ;
- Hassani, Farbod ;
- Hernández-Aguayo, César ;
- Koyama, Kazuya ;
- Li, Baojiu ;
- Mauland, Renate ;
- Monaco, Pierluigi ;
- Moretti, Chiara ;
- Mota, David F. ;
- Partmann, Christian ;
- Parimbelli, Gabriele ;
- Potter, Douglas ;
- Schneider, Aurel ;
- Schulz, Sebastian ;
- Smith, Robert E. ;
- Springel, Volker ;
- Stadel, Joachim ;
- Tram, Thomas ;
- Viel, Matteo ;
- Villaescusa-Navarro, Francisco ;
- Winther, Hans A. ;
- Wright, Bill S. ;
- Zennaro, Matteo