Automated Organization ProfileHarvard Physics, Harvard Astronomy
Harvard Physics, Harvard Astronomy
Current S-Index
Sum of Dataset Indices for all datasets
Average Dataset Index per Dataset
Average Dataset Index per dataset
Total Datasets
Total datasets in this organization
Average FAIR Score
Average FAIR Score per dataset
Total Citations
Total citations to the organization's datasets
Total Mentions
Total mentions of the organization'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: 0.4 (sum of 1 dataset Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
Probabilistic catalog of the gamma-ray sky in the North Galactic Polar Cap (NGPC).<br><br>The dataset contains fair samples drawn from the catalog space consistent with the Fermi-LAT photon count data collected in the NGPC. <br><br>Available data fields are: <br>lgalpop0: galactic longitude in radians <br>bgalpop0: galactic latitude in radians<br>fluxpop0: flux density in 1/cm^2/s/sr/GeV in the 1-3 GeV energy bin<br>sindpop0: spectral index<br>meanpnts: mean number of point sources<br>fluxdistslop: log-log slope of the flux distribution function<br>bacp: normalizations of the isotropic and Fermi diffuse model templates in the PSF class 2 and the three energy bins, 0.3 GeV - 1 GeV, 1 GeV - 3, and 3 GeV - 10 GeV.<br>psfp: 5 parameters of the double king function for each energy bin.<br><br>All fields are two dimensional arrays, where the first dimension is the sample index and the second dimension is the parameter index. For the transdimensional fields, e.g., lgalpop0, bgalpop0, fluxpop0 and sindpop0, rows are padded with NaNs, which indicate the end of the parameter vector for the given sample.
Authors
- Daylan, Tansu ;
- K. N. Portillo, Stephen ;
- P. Finkbeiner, Douglas