The James Webb Interferometer: Space-based Interferometric Detections of PDS 70 b and c at 4.8 μm
Article
Blakely, Dori, Johnstone, Doug, Cugno, Gabriele, Sivaramakrishnan, Anand, Tuthill, Peter, Dong, Ruobing, Pope, Benjamin J. S., Albert, Loic, Charles, Max, Cooper, Rachel A., Furio, Matthew De, Desdoigts, Louis, Doyon, Rene, Francis, Logan, Greenbaum, Alexandra, Lafrenière, David, Lloyd, James P., Meyer, Michael R., Pueyo, Laurent, ..., Vandal, Thomas. 2025. "The James Webb Interferometer: Space-based Interferometric Detections of PDS 70 b and c at 4.8 μm." The Astronomical Journal. 169 (3). https://doi.org/10.3847/1538-3881/ad9b94
| Article Title | The James Webb Interferometer: Space-based Interferometric Detections of PDS 70 b and c at 4.8 μm |
|---|---|
| ERA Journal ID | 1048 |
| Article Category | Article |
| Authors | Blakely, Dori, Johnstone, Doug, Cugno, Gabriele, Sivaramakrishnan, Anand, Tuthill, Peter, Dong, Ruobing, Pope, Benjamin J. S., Albert, Loic, Charles, Max, Cooper, Rachel A., Furio, Matthew De, Desdoigts, Louis, Doyon, Rene, Francis, Logan, Greenbaum, Alexandra, Lafrenière, David, Lloyd, James P., Meyer, Michael R., Pueyo, Laurent, Ray, Shrishmoy, Sanchez-Bermudez, Joel, Soulain, Anthony, Thatte, Deepashri, Thompson, William and Vandal, Thomas |
| Journal Title | The Astronomical Journal |
| Journal Citation | 169 (3) |
| Article Number | 137 |
| Number of Pages | 16 |
| Year | 2025 |
| Publisher | IOP Publishing |
| Place of Publication | United States |
| ISSN | 0004-6256 |
| 1538-3881 | |
| Digital Object Identifier (DOI) | https://doi.org/10.3847/1538-3881/ad9b94 |
| Web Address (URL) | https://iopscience.iop.org/article/10.3847/1538-3881/ad9b94 |
| Abstract | We observed the planet-hosting system PDS 70 with the James Webb Interferometer, JWST's aperture masking interferometric mode within NIRISS. Observing with the F480M filter centered at 4.8 mu m, we simultaneously fit geometrical models to the outer disk and the two known planetary companions. We redetect the protoplanets PDS 70 b and c at a signal-to-noise ratio (SNR) of 14.7 and 7.0, respectively. Our photometry of both PDS 70 b and c provides tentative evidence of mid-IR circumplanetary disk emission through fitting spectral energy distribution models to these new measurements and those found in the literature. We also newly detect emission within the disk gap at an SNR of similar to 4, a position angle of 220-15+10 @, and an unconstrained separation within similar to 200 mas. Follow-up observations will be needed to determine the nature of this emission. We place a 5 sigma upper limit of 208 +/- 10 mu Jy on the flux of the candidate PDS 70 d at 4.8 mu m, which indicates that if the previously observed emission at shorter wavelengths is due to a planet, this putative planet has a different atmospheric composition than PDS 70 b or c. Finally, we place upper limits on emission from any additional planets in the disk gap. We find an azimuthally averaged 5 sigma contrast upper limit >7 mag at separations greater than 110 mas. These are the deepest limits to date within similar to 250 mas at 4.8 mu m and the first space-based interferometric observations of this system. |
| Keywords | Protoplanetary disks ; Exoplanets |
| Contains Sensitive Content | Does not contain sensitive content |
| ANZSRC Field of Research 2020 | 5101. Astronomical sciences |
| Byline Affiliations | University of Victoria, Canada |
| NRC Herzberg Astronomy and Astrophysics, Canada | |
| University of Michigan, United States | |
| Space Telescope Science Institute, United States | |
| American Museum of Natural History, United States | |
| Johns Hopkins University, United States | |
| University of Sydney | |
| Peking University, China | |
| Centre for Astrophysics | |
| University of Queensland | |
| University of Montreal, Canada | |
| University of Texas at Austin, United States | |
| Leiden University, Netherlands | |
| Infrared Processing and Analysis Center (IPAC), United States | |
| Cornell University, United States | |
| National Autonomous University of Mexico, Mexico | |
| Max Planck Institute for Astronomy, Germany | |
| Grenoble Alpes University, France |
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