Automated Organization ProfileThe William H. Miller III Department of Physics \& Astronomy, Bloomberg Center for Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA
The William H. Miller III Department of Physics \& Astronomy, Bloomberg Center for Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA
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: 2.4 (sum of 2 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
This deposit contains the full machine-readable tables for the accepted version of the manuscript, "The Panchromatic Hubble Andromeda Treasury XXI. The Legacy Resolved Stellar Photometry Catalog", submitted and accepted to the Astrophysical Journal Supplments. The specific files included in this deposit are the full version of Tables 1-3 in this manuscript:Table 1: Simplified table of PHAT photometry for easy use;Table 2: Simplified table of artificial star test results for easy use;Table 3: Summary of artificial star statistics as a function of brightness and stellar density.The .txt files are formatted according to the machine-readable standards adopted by the AAS Journals and CDS/Vizier. Documentation of this format can be found at these links:AAS Journals MRT overviewCDS/Vizier standardsThese files can be read in python using the astropy package or with the most recent version of TOPCAT (> Version 4.8). An example script for reading these files in astropy is given here: from astropy.table import Table data = Table.read("datafile3.txt", format="ascii.cds")In addition, a headerless, compressed TeX (&-delimited; "full_table.tex.xz") version of Table 1, and a header-only, dataless version of Table 1 ("datafile1_headeronly.txt") are provided to give users additional tools for dealing with this large dataset. The compression routine was applied using xz https://tukaani.org/xz/ with the encodingsxz -z -7 -T 0 full_table.texxz -z -9 -T 0 datafile1.txtThe Table 1 files on Zenodo were then split into smaller chunks to upload them to Zenodo using the GNU split routine. The full files can be recovered by recombining them before decompressing them. The list of related commands and the expected md5 hexidecimal checksums are given here:split --bytes=512M ../full_table.tex.xz full_table.tex.xz.split --bytes=512M ../datafile1.txt.xz datafile1.txt.xz.cat full_table.tex.xz.a > full_table.tex.xzcat datafile1.txt.xz.a* > datafile1.txt.xzMD5 (full_table.tex.xz) = 7f9195210bec61c08d04926ada4a021aMD5 (datafile1.txt.xz) = 63205fe1051e97f4e04380dd23469893Finally, those interested in generating their own cuts from the DOLPHOT quality parameters can access the full photometry tables, available at MAST as a High Level Science Product via doi.org/10.17909/T91S30
Authors
- Williams, Benjamin F. ;
- Durbin, Meredith ;
- Lang, Dustin ;
- Dalcanton, Julianne J. ;
- Dolphin, Andrew E. ;
- Smercina, Adam ;
- Yanchulova Merica-Jones, Petia ;
- Weisz, Daniel R. ;
- Bell, Eric F. ;
- Gilbert, Karoline M. ;
- Girardi, Leo ;
- Gordon, Karl ;
- Guhathakurta, Puragra ;
- Johnson, L. Clifton ;
- Lauer, Tod R. ;
- Seth, Anil ;
- Skillman, Evan
This deposit contains the full machine-readable tables for the accepted version of the manuscript, "The Panchromatic Hubble Andromeda Treasury XXI. The Legacy Resolved Stellar Photometry Catalog", submitted and accepted to the Astrophysical Journal Supplments. The specific files included in this deposit are the full version of Tables 1-3 in this manuscript:Table 1: Simplified table of PHAT photometry for easy use;Table 2: Simplified table of artificial star test results for easy use;Table 3: Summary of artificial star statistics as a function of brightness and stellar density.The .txt files are formatted according to the machine-readable standards adopted by the AAS Journals and CDS/Vizier. Documentation of this format can be found at these links:AAS Journals MRT overviewCDS/Vizier standardsThese files can be read in python using the astropy package or with the most recent version of TOPCAT (> Version 4.8). An example script for reading these files in astropy is given here: from astropy.table import Table data = Table.read("datafile3.txt", format="ascii.cds")In addition, a headerless, compressed TeX (&-delimited; "full_table.tex.xz") version of Table 1, and a header-only, dataless version of Table 1 ("datafile1_headeronly.txt") are provided to give users additional tools for dealing with this large dataset. The compression routine was applied using xz https://tukaani.org/xz/ with the encodingsxz -z -7 -T 0 full_table.texxz -z -9 -T 0 datafile1.txtThe Table 1 files on Zenodo were then split into smaller chunks to upload them to Zenodo using the GNU split routine. The full files can be recovered by recombining them before decompressing them. The list of related commands and the expected md5 hexidecimal checksums are given here:split --bytes=512M ../full_table.tex.xz full_table.tex.xz.split --bytes=512M ../datafile1.txt.xz datafile1.txt.xz.cat full_table.tex.xz.a > full_table.tex.xzcat datafile1.txt.xz.a* > datafile1.txt.xzMD5 (full_table.tex.xz) = 7f9195210bec61c08d04926ada4a021aMD5 (datafile1.txt.xz) = 63205fe1051e97f4e04380dd23469893Finally, those interested in generating their own cuts from the DOLPHOT quality parameters can access the full photometry tables, available at MAST as a High Level Science Product via doi.org/10.17909/T91S30
Authors
- Williams, Benjamin F. ;
- Durbin, Meredith ;
- Lang, Dustin ;
- Dalcanton, Julianne J. ;
- Dolphin, Andrew E. ;
- Smercina, Adam ;
- Yanchulova Merica-Jones, Petia ;
- Weisz, Daniel R. ;
- Bell, Eric F. ;
- Gilbert, Karoline M. ;
- Girardi, Leo ;
- Gordon, Karl ;
- Guhathakurta, Puragra ;
- Johnson, L. Clifton ;
- Lauer, Tod R. ;
- Seth, Anil ;
- Skillman, Evan