Automated Author ProfileSchlaufman, Kevin
Schlaufman, Kevin
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: 3.6 (sum of 2 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
Data products for the paper titled "Cloudy Mornings and Clear Evenings on a Giant Extrasolar World"The four files (FIREFLy.csv, Fu_spectrum.txt, Eureka_1.txt, and Eureka_2.txt) contain the reduced transmission spectrum of the morning and evening terminators of planet WASP-94A b.The file named "FIREFLy-spherical1D.csv" contains the extracted 1D spherical spectrum for WASP-94A b with FIREFLy. Atmospheric Retrieval ProductsThe zipped folder PICASO-1.5D includes retrieval samples from the 1.5D retrieval on the morning/evening spectrum of WASP-94A b. The best-fit model for each limb along with +-1/2 sigma constraints on the transmission spectrum of each limb is also included in this folder. The spectral samples for each limb are included too.The zipped folder PICASO-1D includes retrieval samples from the 1D retrieval on the spherical spectrum of WASP-94A b. The best-fit model along with +-1/2 sigma constraints on the transmission spectrum is also included in this folder. The spectral samples are included too.General Circulation Model ProductsWe have included products from the GCM modeling of WASP-94A b and haze optical depth profiles for the three other hot Jupiter GCMs included in our paper. These are included in the "GCM_products.zip" folder. The GCM modeling outputs from the UM GCM can be read and analyzed with the Iris analysis tool. The raw data is publicly available on the Mikulski Archive for Space Telescopes (MAST) server. The data were obtained through JWST Cycle 3 GO program #5924 (PI- Sing) and can be accessed through the MAST DOI- http://dx.doi.org/10.17909/eptp-qq05
Authors
- Mukherjee, Sagnick ;
- Sing, David ;
- Fu, Guangwei ;
- Stevenson, Kevin ;
- Schmidt, Stephen ;
- Baskett, Harry ;
- McCreery, Patrick ;
- Mayne, Nathan ;
- Zamyatina, Maria ;
- López-Morales, Mercedes ;
- Lustig-Yaeger, Jacob ;
- Allen, Natalie ;
- Lothringer, Joshua ;
- Bennett, Katherine ;
- Goyal, Jayesh ;
- Gascon, Carlos ;
- HÉBRARD, Éric ;
- Wang, Le-Chris ;
- Christie, Duncan ;
- Ramos Rosado, Lakeisha M. ;
- Schlaufman, Kevin ;
- May, Erin ;
- Mayorga, Laura ;
- Reggiani, Henrique ;
- Sotzen, Kristin Showalter ;
- Thorngren, Daniel ;
- Rustamkulov, Zafar ;
- Mak, Mei Ting
Data products for the paper titled "Cloudy Mornings and Clear Evenings on a Giant Extrasolar World"The four files (FIREFLy.csv, Fu_spectrum.txt, Eureka_1.txt, and Eureka_2.txt) contain the reduced transmission spectrum of the morning and evening terminators of planet WASP-94A b.The file named "FIREFLy-spherical1D.csv" contains the extracted 1D spherical spectrum for WASP-94A b with FIREFLy. Atmospheric Retrieval ProductsThe zipped folder PICASO-1.5D includes retrieval samples from the 1.5D retrieval on the morning/evening spectrum of WASP-94A b. The best-fit model for each limb along with +-1/2 sigma constraints on the transmission spectrum of each limb is also included in this folder. The spectral samples for each limb are included too.The zipped folder PICASO-1D includes retrieval samples from the 1D retrieval on the spherical spectrum of WASP-94A b. The best-fit model along with +-1/2 sigma constraints on the transmission spectrum is also included in this folder. The spectral samples are included too.General Circulation Model ProductsWe have included products from the GCM modeling of WASP-94A b and haze optical depth profiles for the three other hot Jupiter GCMs included in our paper. These are included in the "GCM_products.zip" folder. The GCM modeling outputs from the UM GCM can be read and analyzed with the Iris analysis tool. The raw data is publicly available on the Mikulski Archive for Space Telescopes (MAST) server. The data were obtained through JWST Cycle 3 GO program #5924 (PI- Sing) and can be accessed through the MAST DOI- http://dx.doi.org/10.17909/eptp-qq05
Authors
- Mukherjee, Sagnick ;
- Sing, David ;
- Fu, Guangwei ;
- Stevenson, Kevin ;
- Schmidt, Stephen ;
- Baskett, Harry ;
- McCreery, Patrick ;
- Mayne, Nathan ;
- Zamyatina, Maria ;
- López-Morales, Mercedes ;
- Lustig-Yaeger, Jacob ;
- Allen, Natalie ;
- Lothringer, Joshua ;
- Bennett, Katherine ;
- Goyal, Jayesh ;
- Gascon, Carlos ;
- HÉBRARD, Éric ;
- Wang, Le-Chris ;
- Christie, Duncan ;
- Ramos Rosado, Lakeisha M. ;
- Schlaufman, Kevin ;
- May, Erin ;
- Mayorga, Laura ;
- Reggiani, Henrique ;
- Sotzen, Kristin Showalter ;
- Thorngren, Daniel ;
- Rustamkulov, Zafar ;
- Mak, Mei Ting