Automated Author ProfileSmith, Peter
Arizona State University0000-0002-9946-5259
Smith, Peter
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: 3.9 (sum of 6 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
These are the processed data and outputs from the work presented in Panwar et al. 2025 : "The Roasting Marshmallows Program with IGRINS on Gemini South III: Seeing deeper into the metal depleted atmosphere of a gas-giant on the cusp of the hot to ultra-hot Jupiter transition", arXiv: https://arxiv.org/abs/2507.07204, and to be published in MNRAS. Please see the README file for more details on how to use the data products.
Authors
- Panwar, Vatsal ;
- Brogi, Matteo ;
- Kanumalla, Sai Krishna Teja ;
- Line, Michael ;
- Gandhi, Siddharth ;
- Smith, Peter ;
- Bean, Jacob ;
- PINO, Lorenzo ;
- Savel, Arjun ;
- Wardenier, Joost ;
- Cegla, Heather ;
- Beltz, Hayley ;
- Weiner Mansfield, Megan ;
- Sanchez, Jorge ;
- Desert, Jean-Michel ;
- Welbanks, Luis ;
- Parmentier, Vivien ;
- Kye, Changwoo ;
- Fortney, Jonathan ;
- de Azevedo Silva, Tomás
These are the processed data and outputs from the work presented in Panwar et al. 2025 : "The Roasting Marshmallows Program with IGRINS on Gemini South III: Seeing deeper into the metal depleted atmosphere of a gas-giant on the cusp of the hot to ultra-hot Jupiter transition", arXiv: https://arxiv.org/abs/2507.07204, and to be published in MNRAS. Please see the README file for more details on how to use the data products.
Authors
- Panwar, Vatsal ;
- Brogi, Matteo ;
- Kanumalla, Sai Krishna Teja ;
- Line, Michael ;
- Gandhi, Siddharth ;
- Smith, Peter ;
- Bean, Jacob ;
- PINO, Lorenzo ;
- Savel, Arjun ;
- Wardenier, Joost ;
- Cegla, Heather ;
- Beltz, Hayley ;
- Weiner Mansfield, Megan ;
- Sanchez, Jorge ;
- Desert, Jean-Michel ;
- Welbanks, Luis ;
- Parmentier, Vivien ;
- Kye, Changwoo ;
- Fortney, Jonathan ;
- de Azevedo Silva, Tomás
File NameDescriptionw121_1DRC_H2O_ONLY.txtSelf consistent, solar composition model spectrum with only H2O opacity.w121_1DRC_OH_ONLY.txtSelf consistent, solar composition model spectrum with only OH opacity.w121_1DRC_CO_ONLY.txtSelf consistent, solar composition model spectrum with only CO opacity.w121_1DRC_EVERYTHING.txtSelf consistent, solar composition model spectrum with all sources of opacity.pre_.picPre-eclipse data in data cuboid of shape N_order, N_frame, N_pixelpre_variance.picAssociated per-pixel variance for the pre-eclipse data.post_cube.picPost-eclipse data in data cuboid of shape N_order, N_frame, N_pixelpre_time_BJD.picAverage frame time in BJD for the pre-eclipse sequence.pre_rvel.picStellar radial velocity, including barycentric correction, per frame for the pre-eclipse sequence.post_ph.picOrbital phase per frame for the post-eclipse sequence.post_time_BJD.picAverage frame time in BJD for the post-eclipse sequence.post_rvel.picStellar radial velocity, including barycentric correction, per frame for the post-eclipse sequence
Authors
- Smith, Peter C. B. ;
- Sanchez, Jorge ;
- Line, Michael ;
- Rauscher, Emily ;
- Weiner Mansfield, Megan ;
- Kempton, Eliza M.-R. ;
- Savel, Arjun B. ;
- Wardenier, Joost P. ;
- Pino, Lorenzo ;
- Bean, Jacob ;
- Beltz, Hayley ;
- Panwar, Vatsal ;
- Brogi, Matteo ;
- Malsky, Isaac ;
- Fortney,, Jonathan ;
- Desert, Jean-Michel ;
- Pelletier, Stefan ;
- Parmentier, Vivien ;
- Kanumalla, Krishna ;
- Welbanks, Luis ;
- Meyer, Michael ;
- Monnier, John
File NameDescriptionw121_1DRC_H2O_ONLY.txtSelf consistent, solar composition model spectrum with only H2O opacity.w121_1DRC_OH_ONLY.txtSelf consistent, solar composition model spectrum with only OH opacity.w121_1DRC_CO_ONLY.txtSelf consistent, solar composition model spectrum with only CO opacity.w121_1DRC_EVERYTHING.txtSelf consistent, solar composition model spectrum with all sources of opacity.pre_.picPre-eclipse data in data cuboid of shape N_order, N_frame, N_pixelpre_variance.picAssociated per-pixel variance for the pre-eclipse data.post_cube.picPost-eclipse data in data cuboid of shape N_order, N_frame, N_pixelpre_time_BJD.picAverage frame time in BJD for the pre-eclipse sequence.pre_rvel.picStellar radial velocity, including barycentric correction, per frame for the pre-eclipse sequence.post_ph.picOrbital phase per frame for the post-eclipse sequence.post_time_BJD.picAverage frame time in BJD for the post-eclipse sequence.post_rvel.picStellar radial velocity, including barycentric correction, per frame for the post-eclipse sequence
Authors
- Smith, Peter C. B. ;
- Sanchez, Jorge ;
- Line, Michael ;
- Rauscher, Emily ;
- Weiner Mansfield, Megan ;
- Kempton, Eliza M.-R. ;
- Savel, Arjun B. ;
- Wardenier, Joost P. ;
- Pino, Lorenzo ;
- Bean, Jacob ;
- Beltz, Hayley ;
- Panwar, Vatsal ;
- Brogi, Matteo ;
- Malsky, Isaac ;
- Fortney,, Jonathan ;
- Desert, Jean-Michel ;
- Pelletier, Stefan ;
- Parmentier, Vivien ;
- Kanumalla, Krishna ;
- Welbanks, Luis ;
- Meyer, Michael ;
- Monnier, John
Supplementary material for A Combined Ground-based and JWST Atmospheric Retrieval Analysis: Both IGRINS and NIRSpec Agree The Atmosphere of WASP-77A b is Metal-Poor, accepted for publication in the Astronomical Journal 2023.
Authors
- Smith, Peter
Supplementary material for A Combined Ground-based and JWST Atmospheric Retrieval Analysis: Both IGRINS and NIRSpec Agree The Atmosphere of WASP-77A b is Metal-Poor, accepted for publication in the Astronomical Journal 2023.
Authors
- Smith, Peter