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pro vyhledávání: '"Baptista, Jay"'
Autor:
Kunimoto, Michelle, Vanderburg, Andrew, Huang, Chelsea X., Davis, M. Ryleigh, Affer, Laura, Cameron, Andrew Collier, Charbonneau, David, Cosentino, Rosario, Damasso, Mario, Dumusque, Xavier, Fiorenzano, A. F. Martnez, Ghedina, Adriano, Haywood, R. D., Lienhard, Florian, López-Morales, Mercedes, Mayor, Michel, Pepe, Francesco, Pinamonti, Matteo, Poretti, Ennio, Maldonado, Jesús, Rice, Ken, Sozzetti, Alessandro, Wilson, Thomas G., Udry, Stéphane, Baptista, Jay, Barkaoui, Khalid, Becker, Juliette, Benni, Paul, Bieryla, Allyson, Bosch-Cabot, Pau, Ciardi, David R., Collins, Karen A., Collins, Kevin I., Evans, Elise, Dupuy, Trent J., Goliguzova, Maria V., Guerra, Pere, Kraus, Adam, Lissauer, Jack J., Huber, Daniel, Murgas, Felipe, Palle, Enric, Quinn, Samuel N., Safonov, Boris S., Schwarz, Richard P., Shporer, Avi, Stassun, Keivan G., Jenkins, Jon M., Latham, David W., Ricker, George R., Seager, Sara, Vanderspek, Roland, Winn, Joshua, Essack, Zahra, Lewis, Hannah M., Rose, Mark E.
Publikováno v:
AJ, 166, 7 (2023)
We report the confirmation of three exoplanets transiting TOI-4010 (TIC-352682207), a metal-rich K dwarf observed by TESS in Sectors 24, 25, 52, and 58. We confirm these planets with HARPS-N radial velocity observations and measure their masses with
Externí odkaz:
http://arxiv.org/abs/2306.05308
Autor:
Baptista, Jay, Prochaska, J. Xavier, Mannings, Alexandra G., James, C. W., Shannon, R. M., Ryder, Stuart D., Deller, A. T., Scott, Danica R., Glowacki, Marcin, Tejos, Nicolas
The Macquart relation describes the correlation between the dispersion measure (DM) of fast radio bursts (FRBs) and the redshift $z$ of their host galaxies. The scatter of the Macquart relation is sensitive to the distribution of baryons in the inter
Externí odkaz:
http://arxiv.org/abs/2305.07022
Autor:
Baptista, Jay, Sanderson, Robyn, Huber, Dan, Wetzel, Andrew, Sameie, Omid, Boylan-Kolchin, Michael, Bailin, Jeremy, Hopkins, Philip F., Faucher-Giguere, Claude-Andre, Chakrabarti, Sukanya, Vargya, Drona, Panithanpaisal, Nondh, Arora, Arpit, Cunningham, Emily
The shape and orientation of dark matter (DM) halos are sensitive to the micro-physics of the DM particle, yet in many mass models, the symmetry axes of the Milky Way's DM halo are often assumed to be aligned with the symmetry axes of the stellar dis
Externí odkaz:
http://arxiv.org/abs/2211.16382
Autor:
Panithanpaisal, Nondh, Sanderson, Robyn E., Arora, Arpit, Cunningham, Emily C., Baptista, Jay
Recent studies have suggested that the Milky Way (MW)'s Dark Matter (DM) halo may be significantly tilted with respect to its central stellar disk, a feature that might be linked to its formation history. In this work, we demonstrate a method of cons
Externí odkaz:
http://arxiv.org/abs/2210.14983
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Akademický článek
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