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Articles 31 - 60 of 204
Full-Text Articles in Physical Sciences and Mathematics
Toi-2109: An Ultrahot Gas Giant On A 16 Hr Orbit, I. Wong, A. Shporer, G. Zhou, D. Kitzmann, T. D. Komacek, X. Tan, R. Tronsgaard, L. A. Buchhave, S. Vissapragada, M. Greklek-Mckeon, J. E. Rodriguez, J. P. Ahlers, S. N. Quinn, E. Furlan, S. B. Howell, A. Bieryla, K. Heng, H. A. Knutson, K. A. Collins, K. K. Mcleod, P. Berlind, P. Brown, M. L. Calkins, J. P. De Leon, E. Esparza-Borges, G. A. Esquerdo, A. Fukui, T. Gan, E. Girardin, C. L. Gnilka, M. Ikoma, Eric L.N. Jensen, J. Kielkopf, T. Kodama, S. Kurita, K. V. Lester, P. Lewin, G. Marino, F. Murgas, N. Narita, E. Pallé, R. P. Schwarz, K. G. Stassun, M. Tamura, N. Watanabe, B. Benneke, G. R. Ricker, D. W. Latham, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, D. A. Caldwell, W. Fong, C. X. Huang, I. Mireles, J. E. Schlieder, B. Shiao, J. N. Villaseñor
Toi-2109: An Ultrahot Gas Giant On A 16 Hr Orbit, I. Wong, A. Shporer, G. Zhou, D. Kitzmann, T. D. Komacek, X. Tan, R. Tronsgaard, L. A. Buchhave, S. Vissapragada, M. Greklek-Mckeon, J. E. Rodriguez, J. P. Ahlers, S. N. Quinn, E. Furlan, S. B. Howell, A. Bieryla, K. Heng, H. A. Knutson, K. A. Collins, K. K. Mcleod, P. Berlind, P. Brown, M. L. Calkins, J. P. De Leon, E. Esparza-Borges, G. A. Esquerdo, A. Fukui, T. Gan, E. Girardin, C. L. Gnilka, M. Ikoma, Eric L.N. Jensen, J. Kielkopf, T. Kodama, S. Kurita, K. V. Lester, P. Lewin, G. Marino, F. Murgas, N. Narita, E. Pallé, R. P. Schwarz, K. G. Stassun, M. Tamura, N. Watanabe, B. Benneke, G. R. Ricker, D. W. Latham, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, D. A. Caldwell, W. Fong, C. X. Huang, I. Mireles, J. E. Schlieder, B. Shiao, J. N. Villaseñor
Physics & Astronomy Faculty Works
We report the discovery of an ultrahot Jupiter with an extremely short orbital period of 0.67247414 ± 0.00000028 days (∼16 hr). The 1.347 ± 0.047 RJup planet, initially identified by the Transiting Exoplanet Survey Satellite (TESS) mission, orbits TOI-2109 (TIC 392476080)—a Teff ∼ 6500 K F-type star with a mass of 1.447 ± 0.077 M☉, a radius of 1.698 ± 0.060 R☉, and a rotational velocity of v sin i* = 81.9 ± 1.7 km s⁻¹. The planetary nature of TOI-2109b was confirmed through radial-velocity measurements, which yielded a planet mass of 5.02 …
Tess-Keck Survey. V. Twin Sub-Neptunes Transiting The Nearby G Star Hd 63935, N. Scarsdale, J. M. Akana Murphy, N. M. Batalha, I. J. M. Crossfield, C. D. Dressing, B. Fulton, A. W. Howard, D. Huber, H. Isaacson, S. R. Kane, E. A. Petigura, P. Robertson, A. Roy, L. M. Weiss, C. Beard, A. Behmard, A. Chontos, J. L. Christiansen, D. R. Ciardi, Z. R. Claytor, K. A. Collins, K. I. Collins, F. Dai, P. A. Dalba, D. Dragomir, T. Fetherolf, A. Fukui, S. Giacalone, E. J. Gonzales, M. L. Hill, L. A. Hirsch, Eric L.N. Jensen, M. R. Kosiarek, J. P. De Leon, J. Lubin, M. B. Lund, R. Luque, A. W. Mayo, T. Močnik, M. Mori, N. Narita, G. Nowak, E. Pallé, M. Rabus, L. J. Rosenthal, R. A. Rubenzahl, J. E. Schlieder, A. Shporer, K. G. Stassun, J. Twicken, G. Wang, D. A. Yahalomi, J. Jenkins, D. W. Latham, G. R. Ricker, S. Seager, R. Vanderspek, J. N. Winn
Tess-Keck Survey. V. Twin Sub-Neptunes Transiting The Nearby G Star Hd 63935, N. Scarsdale, J. M. Akana Murphy, N. M. Batalha, I. J. M. Crossfield, C. D. Dressing, B. Fulton, A. W. Howard, D. Huber, H. Isaacson, S. R. Kane, E. A. Petigura, P. Robertson, A. Roy, L. M. Weiss, C. Beard, A. Behmard, A. Chontos, J. L. Christiansen, D. R. Ciardi, Z. R. Claytor, K. A. Collins, K. I. Collins, F. Dai, P. A. Dalba, D. Dragomir, T. Fetherolf, A. Fukui, S. Giacalone, E. J. Gonzales, M. L. Hill, L. A. Hirsch, Eric L.N. Jensen, M. R. Kosiarek, J. P. De Leon, J. Lubin, M. B. Lund, R. Luque, A. W. Mayo, T. Močnik, M. Mori, N. Narita, G. Nowak, E. Pallé, M. Rabus, L. J. Rosenthal, R. A. Rubenzahl, J. E. Schlieder, A. Shporer, K. G. Stassun, J. Twicken, G. Wang, D. A. Yahalomi, J. Jenkins, D. W. Latham, G. R. Ricker, S. Seager, R. Vanderspek, J. N. Winn
Physics & Astronomy Faculty Works
We present the discovery of two nearly identically sized sub-Neptune transiting planets orbiting HD 63935, a bright (V = 8.6 mag), Sun-like (Teff = 5560 K) star at 49 pc. TESS identified the first planet, HD 63935 b (TOI-509.01), in Sectors 7 and 34. We identified the second signal (HD 63935 c) in Keck High Resolution Echelle Spectrometer and Lick Automated Planet Finder radial velocity data as part of our follow-up campaign. It was subsequently confirmed with TESS photometry in Sector 34 as TOI-509.02. Our analysis of the photometric and radial velocity data yielded a robust detection …
Toi-1518b: A Misaligned Ultra-Hot Jupiter With Iron In Its Atmosphere, S. H. C. Cabot, A. Bello-Arufe, J. M. Mendonça, R. Tronsgaard, I. Wong, G. Zhou, L. A. Buchhave, D. A. Fischer, K. G. Stassun, V. Antoci, D. Baker, A. A. Belinski, B. Benneke, L. G. Bouma, J. L. Christiansen, K. A. Collins, M. V. Goliguzova, S. Hagey, J. M. Jenkins, Eric L.N. Jensen, R. C. Kidwell Jr., D. Laloum, B. Massey, K. K. Mcleod, D. W. Latham, E. H. Morgan, G. Ricker, B. S. Safonov, J. E. Schlieder, S. Seager, A. Shporer, J. C. Smith, G. Srdoc, I. A. Strakhov, G. Torres, J. D. Twicken, R. Vanderspek, M. Vezie, J. N. Winn
Toi-1518b: A Misaligned Ultra-Hot Jupiter With Iron In Its Atmosphere, S. H. C. Cabot, A. Bello-Arufe, J. M. Mendonça, R. Tronsgaard, I. Wong, G. Zhou, L. A. Buchhave, D. A. Fischer, K. G. Stassun, V. Antoci, D. Baker, A. A. Belinski, B. Benneke, L. G. Bouma, J. L. Christiansen, K. A. Collins, M. V. Goliguzova, S. Hagey, J. M. Jenkins, Eric L.N. Jensen, R. C. Kidwell Jr., D. Laloum, B. Massey, K. K. Mcleod, D. W. Latham, E. H. Morgan, G. Ricker, B. S. Safonov, J. E. Schlieder, S. Seager, A. Shporer, J. C. Smith, G. Srdoc, I. A. Strakhov, G. Torres, J. D. Twicken, R. Vanderspek, M. Vezie, J. N. Winn
Physics & Astronomy Faculty Works
We present the discovery of TOI-1518b—an ultra-hot Jupiter orbiting a bright star (V = 8.95). The transiting planet is confirmed using high-resolution optical transmission spectra from EXPRES. It is inflated, with Rp = 1.875 ± 0.053 RJ, and exhibits several interesting properties, including a misaligned orbit (240.34 (+0.93)/(-0.98) degrees) and nearly grazing transit (b = 0.9036 (+0.0061)/(-0.0053)). The planet orbits a fast-rotating F0 host star (Teff ≃ 7300 K) in 1.9 days and experiences intense irradiation. Notably, the TESS data show a clear secondary eclipse with a depth of 364 ± 28 ppm …
The Magellan-Tess Survey. I. Survey Description And Midsurvey Results, J. Teske, S. X. Wang, A. Wolfgang, T. Gan, M. Plotnykov, D. J. Armstrong, R. P. Butler, B. Cale, J. D. Crane, W. Howard, Eric L.N. Jensen, N. Law, S. A. Shectman, P. Plavchan, D. Valencia, A. Vanderburg, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, V. Adibekyan, D. Barrado, S. C. C. Barros, Z. Benkhaldoun, D. J. A. Brown, E. M. Bryant, J. Burt, D. A. Caldwell, D. Charbonneau, R. Cloutier, K. A. Collins, K. I. Collins, K. D. Colon, D. M. Conti, O. D. S. Demangeon, J. D. Eastman, M. Elmufti, F. Feng, E. Flowers, N. M. Guerrero, S. Hojjatpanah, J. M. Irwin, G. Isopi, J. Lillo-Box, F. Mallia, B. Massey, M. Mori, S. E. Mullally, N. Narita, T. Nishiumi, A. Osborn, M. Paegert, J. P. De Leon, S. N. Quinn, M. Reefe, R. P. Schwarz, A. Shporer, A. Soubkiou, S. G. Sousa, C. Stockdale, P. A. Strøm, T.-G. Tan, J. Tang, P. Tenenbaum, P. J. Wheatley, J. Wittrock, D. A. Yahalomi, F. Zohrabi
The Magellan-Tess Survey. I. Survey Description And Midsurvey Results, J. Teske, S. X. Wang, A. Wolfgang, T. Gan, M. Plotnykov, D. J. Armstrong, R. P. Butler, B. Cale, J. D. Crane, W. Howard, Eric L.N. Jensen, N. Law, S. A. Shectman, P. Plavchan, D. Valencia, A. Vanderburg, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, V. Adibekyan, D. Barrado, S. C. C. Barros, Z. Benkhaldoun, D. J. A. Brown, E. M. Bryant, J. Burt, D. A. Caldwell, D. Charbonneau, R. Cloutier, K. A. Collins, K. I. Collins, K. D. Colon, D. M. Conti, O. D. S. Demangeon, J. D. Eastman, M. Elmufti, F. Feng, E. Flowers, N. M. Guerrero, S. Hojjatpanah, J. M. Irwin, G. Isopi, J. Lillo-Box, F. Mallia, B. Massey, M. Mori, S. E. Mullally, N. Narita, T. Nishiumi, A. Osborn, M. Paegert, J. P. De Leon, S. N. Quinn, M. Reefe, R. P. Schwarz, A. Shporer, A. Soubkiou, S. G. Sousa, C. Stockdale, P. A. Strøm, T.-G. Tan, J. Tang, P. Tenenbaum, P. J. Wheatley, J. Wittrock, D. A. Yahalomi, F. Zohrabi
Physics & Astronomy Faculty Works
Kepler revealed that roughly one-third of Sunlike stars host planets orbiting within 100 days and between the size of Earth and Neptune. How do these planets form, what are they made of, and do they represent a continuous population or multiple populations? To help address these questions, we began the Magellan-TESS Survey (MTS), which uses Magellan II/PFS to obtain radial velocity (RV) masses of 30 TESS-detected exoplanets and develops an analysis framework that connects observed planet distributions to underlying populations. In the past, small-planet RV measurements have been challenging to obtain due to host star faintness and low RV semiamplitudes …
Toi-3362b: A Proto Hot Jupiter Undergoing High-Eccentricity Tidal Migration, J. Dong, C. X. Huang, G. Zhou, R. I. Dawson, J. E. Rodriguez, J. D. Eastman, K. A. Collins, S. N. Quinn, A. Shporer, A. H. M. J. Triaud, S. Wang, T. Beatty, J. M. Jackson, K. I. Collins, L. Abe, O. Suarez, N. Crouzet, D. Mékarnia, G. Dransfield, Eric L.N. Jensen, C. Stockdale, K. Barkaoui, A. Heitzmann, D. J. Wright, B. C. Addison, R. A. Wittenmyer, J. Okumura, B. P. Bowler, J. Horner, S. R. Kane, J. Kielkopf, H. Liu, P. Plavchan, M. W. Mengel, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, J. L. Christiansen, M. Paegert
Toi-3362b: A Proto Hot Jupiter Undergoing High-Eccentricity Tidal Migration, J. Dong, C. X. Huang, G. Zhou, R. I. Dawson, J. E. Rodriguez, J. D. Eastman, K. A. Collins, S. N. Quinn, A. Shporer, A. H. M. J. Triaud, S. Wang, T. Beatty, J. M. Jackson, K. I. Collins, L. Abe, O. Suarez, N. Crouzet, D. Mékarnia, G. Dransfield, Eric L.N. Jensen, C. Stockdale, K. Barkaoui, A. Heitzmann, D. J. Wright, B. C. Addison, R. A. Wittenmyer, J. Okumura, B. P. Bowler, J. Horner, S. R. Kane, J. Kielkopf, H. Liu, P. Plavchan, M. W. Mengel, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, J. L. Christiansen, M. Paegert
Physics & Astronomy Faculty Works
High-eccentricity tidal migration is a possible way for giant planets to be placed in short-period orbits. If this happens often, one would expect to catch proto hot Jupiters on highly elliptical orbits undergoing high-eccentricity tidal migration. As of yet, few such systems have been discovered. Here, we introduce TOI-3362b (TIC-464300749b), an 18.1 day, 5 MJup planet orbiting a main-sequence F-type star that is likely undergoing high-eccentricity tidal migration. The orbital eccentricity is 0.815 (+0.023)/(-0.032). With a semimajor axis of 0.153 (+0.002)/(-0.003) au, the planet's orbit is expected to shrink to a final orbital radius of 0.051 (+0.008)/(-0.006) au after …
Hd 183579b: A Warm Sub-Neptune Transiting A Solar Twin Detected By Tess, T. Gan, M. Bedell, S. X. Wang, D. Foreman-Mackey, J. Meléndez, S. Mao, K. G. Stassun, S. B. Howell, C. Ziegler, R. A. Wittenmyer, C. Hellier, K. A. Collins, A. Shporer, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, B. C. Addison, S. Ballard, T. Barclay, J. L. Bean, B. P. Bowler, C. Briceño, I. J. M. Crossfield, J. Dittman, J. Horner, Eric L.N. Jensen, S. R. Kane, J. Kielkopf, L. Kreidberg, N. Law, A. W. Mann, M. W. Mengel, E. D. Morgan, J. Okumura, H. P. Osborn, M. Paegert, P. Plavchan, R. P. Schwarz, B. Shiao, J. C. Smith, L. Spina, C. G. Tinney, G. Torres, J. D. Twicken, M. Vezie, G. Wang, D. J. Wright, H. Zhang
Hd 183579b: A Warm Sub-Neptune Transiting A Solar Twin Detected By Tess, T. Gan, M. Bedell, S. X. Wang, D. Foreman-Mackey, J. Meléndez, S. Mao, K. G. Stassun, S. B. Howell, C. Ziegler, R. A. Wittenmyer, C. Hellier, K. A. Collins, A. Shporer, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, B. C. Addison, S. Ballard, T. Barclay, J. L. Bean, B. P. Bowler, C. Briceño, I. J. M. Crossfield, J. Dittman, J. Horner, Eric L.N. Jensen, S. R. Kane, J. Kielkopf, L. Kreidberg, N. Law, A. W. Mann, M. W. Mengel, E. D. Morgan, J. Okumura, H. P. Osborn, M. Paegert, P. Plavchan, R. P. Schwarz, B. Shiao, J. C. Smith, L. Spina, C. G. Tinney, G. Torres, J. D. Twicken, M. Vezie, G. Wang, D. J. Wright, H. Zhang
Physics & Astronomy Faculty Works
We report the discovery and characterization of a transiting warm sub-Neptune planet around the nearby bright (V = 8.75 mag, K = 7.15 mag) solar twin HD 183579, delivered by the Transiting Exoplanet Survey Satellite (TESS). The host star is located 56.8 ± 0.1 pc away with a radius of R* = 0.97 ± 0.02 R⊙ and a mass of M* = 1.03 ± 0.05 M⊙. We confirm the planetary nature by combining space and ground-based photometry, spectroscopy, and imaging. We find that HD 183579b (TOI-1055b) has a radius of Rp …
Toi-431/Hip 26013: A Super-Earth And A Sub-Neptune Transiting A Bright, Early K Dwarf, With A Third Rv Planet, A. Osborn, D. J. Armstrong, B. Cale, R. Brahm, R. A. Wittenmyer, F. Dai, I. J. M. Crossfield, E. M. Bryant, V. Adibekyan, R. Cloutier, K. A. Collins, E. Delgado Mena, M. Fridlund, C. Hellier, S. B. Howell, G. W. King, J. Lillo-Box, J. Otegi, S. Sousa, K. G. Stassun, E. C. Matthews, C. Ziegler, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, J. S. Acton, B. C. Addison, D. R. Anderson, S. Ballard, D. Barrado, S. C. C. Barros, N. Batalha, D. Bayliss, T. Barclay, B. Benneke, J. Berberian Jr., F. Bouchy, B. P. Bowler, C. Briceño, C. J. Burke, M. R. Burleigh, S. L. Casewell, D. Ciardi, K. I. Collins, B. F. Cooke, O. D. S. Demangeon, R. F. Díaz, C. Dorn, D. Dragomir, C. Dressing, X. Dumusque, N. Espinoza, P. Figueira, B. Fulton, E. Furlan, E. Gaidos, C. Geneser, S. Gill, M. R. Road, E. J. Gonzales, V. Gorjian, M. N. Günther, R. Helled, B. A. Henderson, T. Henning, A. Hogan, S. Hojjatpanah, J. Horner, A. W. Howard, S. Hoyer, D. Huber, H. Isaacson, J. S. Jenkins, Eric L.N. Jensen, A. Jordán, A. R. Kane, R. C. Kidwell Jr., J. Kielkopf, N. Law, M. Lendl, M. Lund, R. A. Matson, A. W. Mann, J. Mccormac, M. W. Mengel, F. Y. Morales, L. D. Nielsen, J. Okumura, H. P. Osborn, E. A. Petigura, P. Plavchan, D. Pollacco, E. V. Quintana, L. Raynard, P. Robertson, M. E. Rose, A. Roy, M. Reefe, A. Santerne, N. C. Santos, P. Sarkis, J. Schlieder, R. P. Schwarz, N. J. Scott, A. Shporer, A. M. S. Smith, C. Stibbard, C. Stockdale, P. A. Strøm, J. D. Twicken, T.-G. Tan, A. Tanner, J. Teske, R. H. Tilbrook, C. G. Tinney, S. Udry, J. N. Villaseñor, J. I. Vines, S. X. Wang, L. M. Weiss, R. G. West, P. J. Wheatley, D. J. Wright, H. Zhang, F. Zohrabi
Toi-431/Hip 26013: A Super-Earth And A Sub-Neptune Transiting A Bright, Early K Dwarf, With A Third Rv Planet, A. Osborn, D. J. Armstrong, B. Cale, R. Brahm, R. A. Wittenmyer, F. Dai, I. J. M. Crossfield, E. M. Bryant, V. Adibekyan, R. Cloutier, K. A. Collins, E. Delgado Mena, M. Fridlund, C. Hellier, S. B. Howell, G. W. King, J. Lillo-Box, J. Otegi, S. Sousa, K. G. Stassun, E. C. Matthews, C. Ziegler, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, J. S. Acton, B. C. Addison, D. R. Anderson, S. Ballard, D. Barrado, S. C. C. Barros, N. Batalha, D. Bayliss, T. Barclay, B. Benneke, J. Berberian Jr., F. Bouchy, B. P. Bowler, C. Briceño, C. J. Burke, M. R. Burleigh, S. L. Casewell, D. Ciardi, K. I. Collins, B. F. Cooke, O. D. S. Demangeon, R. F. Díaz, C. Dorn, D. Dragomir, C. Dressing, X. Dumusque, N. Espinoza, P. Figueira, B. Fulton, E. Furlan, E. Gaidos, C. Geneser, S. Gill, M. R. Road, E. J. Gonzales, V. Gorjian, M. N. Günther, R. Helled, B. A. Henderson, T. Henning, A. Hogan, S. Hojjatpanah, J. Horner, A. W. Howard, S. Hoyer, D. Huber, H. Isaacson, J. S. Jenkins, Eric L.N. Jensen, A. Jordán, A. R. Kane, R. C. Kidwell Jr., J. Kielkopf, N. Law, M. Lendl, M. Lund, R. A. Matson, A. W. Mann, J. Mccormac, M. W. Mengel, F. Y. Morales, L. D. Nielsen, J. Okumura, H. P. Osborn, E. A. Petigura, P. Plavchan, D. Pollacco, E. V. Quintana, L. Raynard, P. Robertson, M. E. Rose, A. Roy, M. Reefe, A. Santerne, N. C. Santos, P. Sarkis, J. Schlieder, R. P. Schwarz, N. J. Scott, A. Shporer, A. M. S. Smith, C. Stibbard, C. Stockdale, P. A. Strøm, J. D. Twicken, T.-G. Tan, A. Tanner, J. Teske, R. H. Tilbrook, C. G. Tinney, S. Udry, J. N. Villaseñor, J. I. Vines, S. X. Wang, L. M. Weiss, R. G. West, P. J. Wheatley, D. J. Wright, H. Zhang, F. Zohrabi
Physics & Astronomy Faculty Works
We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photometry and radial velocities (RVs). We estimate the stellar rotation period to be 30.5 ± 0.7 d using archival photometry and RVs. Transiting Exoplanet Survey Satellite (TESS) objects of Interest (TOI)-431 b is a super-Earth with a period of 0.49 d, a radius of 1.28 ± 0.04 R⊕, a mass of 3.07 ± 0.35 M⊕, and a density of 8.0 ± 1.0 g cm⁻³; TOI-431 d is a sub-Neptune with a period of 12.46 d, a radius of 3.29 ± 0.09 …
Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths With Earth-Like Compositions, T. Hirano, J. H. Livingston, A. Fukui, N. Narita, H. Harakawa, H. T. Ishikawa, K. Miyakawa, T. Kimura, A. Nakayama, N. Fujita, Y. Hori, K. G. Stassun, A. Bieryla, C. Cadieux, D. R. Ciardi, K. A. Collins, M. Ikoma, A. Vanderburg, T. Barclay, C. E. Brasseur, J. P. De Leon, J. P. Doty, R. Doyon, E. Esparza-Borges, G. A. Esquerdo, E. Furlan, E. Gaidos, E. J. Gonzales, K. Hodapp, S. B. Howell, K. Isogai, S. Jacobson, J. M. Jenkins, Eric L.N. Jensen, K. Kawauchi, T. Kotani, T. Kudo, S. Kurita, T. Kurokawa, N. Kusakabe, M. Kuzuhara, D. Lafrenière, D. W. Latham, B. Massey, M. Mori, F. Murgas, J. Nishikawa, T. Nishiumi, M. Omiya, M. Paegert, E. Palle, H. Parviainen, S. N. Quinn, G. R. Ricker, R. P. Schwarz, S. Seager, M. Tamura, P. Tenenbaum, Y. Terada, R. K. Vanderspek, S. Vievard, N. Watanabe, J. N. Winn
Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths With Earth-Like Compositions, T. Hirano, J. H. Livingston, A. Fukui, N. Narita, H. Harakawa, H. T. Ishikawa, K. Miyakawa, T. Kimura, A. Nakayama, N. Fujita, Y. Hori, K. G. Stassun, A. Bieryla, C. Cadieux, D. R. Ciardi, K. A. Collins, M. Ikoma, A. Vanderburg, T. Barclay, C. E. Brasseur, J. P. De Leon, J. P. Doty, R. Doyon, E. Esparza-Borges, G. A. Esquerdo, E. Furlan, E. Gaidos, E. J. Gonzales, K. Hodapp, S. B. Howell, K. Isogai, S. Jacobson, J. M. Jenkins, Eric L.N. Jensen, K. Kawauchi, T. Kotani, T. Kudo, S. Kurita, T. Kurokawa, N. Kusakabe, M. Kuzuhara, D. Lafrenière, D. W. Latham, B. Massey, M. Mori, F. Murgas, J. Nishikawa, T. Nishiumi, M. Omiya, M. Paegert, E. Palle, H. Parviainen, S. N. Quinn, G. R. Ricker, R. P. Schwarz, S. Seager, M. Tamura, P. Tenenbaum, Y. Terada, R. K. Vanderspek, S. Vievard, N. Watanabe, J. N. Winn
Physics & Astronomy Faculty Works
We present observations of two bright M dwarfs (TOI-1634 and TOI-1685: J = 9.5–9.6) hosting ultra-short-period (USP) planets identified by the TESS mission. The two stars are similar in temperature, mass, and radius (Teff ≈ 3500 K, M⋆ ≈ 0.45–0.46 M⊙, and R⋆ ≈ 0.45–0.46 R⊙), and the planets are both super-Earth size (1.25 R⊕ < Rp < 2.0 R⊕). For both systems, light curves from ground-based photometry exhibit planetary transits, whose depths are consistent with those from the TESS photometry. We also refine the transit ephemerides based on the ground-based …
Toi-1231 B: A Temperate, Neptune-Sized Planet Transiting The Nearby M3 Dwarf Nltt 24399, J. A. Burt, D. Dragomir, P. Mollière, A. Youngblood, A. García Muñoz, J. Mccann, L. Kreidberg, C. X. Huang, K. A. Collins, J. D. Eastman, L. Abe, J. M. Almenara, I. J. M. Crossfield, C. Ziegler, J. E. Rodriguez, E. E. Mamajek, K. G. Stassun, S. P. Halverson, S. Villanueva Jr., R. P. Butler, S. X. Wang, R. P. Schwarz, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, A. Agabi, X. Bonfils, D. Ciardi, M. Cointepas, J. D. Crane, N. Crouzet, G. Dransfield, F. Feng, E. Furlan, T. Guillot, A. F. Gupta, S. B. Howell, Eric L.N. Jensen, N. Law, A. W. Mann, W. Marie-Sainte, R. A. Matson, E. C. Matthews, D. Mékarnia, J. Pepper, N. Scott, S. A. Shectman, J. E. Schlieder, F.-X. Schmider, D. J. Stevens, J. K. Teske, A. H. M. J. Triaud, D. Charbonneau, Z. K. Berta-Thompson, C. J. Burke, T. Daylan, T. Barclay, B. Wohler, C. E. Brasseur
Toi-1231 B: A Temperate, Neptune-Sized Planet Transiting The Nearby M3 Dwarf Nltt 24399, J. A. Burt, D. Dragomir, P. Mollière, A. Youngblood, A. García Muñoz, J. Mccann, L. Kreidberg, C. X. Huang, K. A. Collins, J. D. Eastman, L. Abe, J. M. Almenara, I. J. M. Crossfield, C. Ziegler, J. E. Rodriguez, E. E. Mamajek, K. G. Stassun, S. P. Halverson, S. Villanueva Jr., R. P. Butler, S. X. Wang, R. P. Schwarz, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, A. Agabi, X. Bonfils, D. Ciardi, M. Cointepas, J. D. Crane, N. Crouzet, G. Dransfield, F. Feng, E. Furlan, T. Guillot, A. F. Gupta, S. B. Howell, Eric L.N. Jensen, N. Law, A. W. Mann, W. Marie-Sainte, R. A. Matson, E. C. Matthews, D. Mékarnia, J. Pepper, N. Scott, S. A. Shectman, J. E. Schlieder, F.-X. Schmider, D. J. Stevens, J. K. Teske, A. H. M. J. Triaud, D. Charbonneau, Z. K. Berta-Thompson, C. J. Burke, T. Daylan, T. Barclay, B. Wohler, C. E. Brasseur
Physics & Astronomy Faculty Works
We report the discovery of a transiting, temperate, Neptune-sized exoplanet orbiting the nearby (d = 27.5 pc), M3V star TOI-1231 (NLTT 24399, L 248-27, 2MASS J10265947-5228099). The planet was detected using photometric data from the Transiting Exoplanet Survey Satellite and followed up with observations from the Las Cumbres Observatory and the Antarctica Search for Transiting ExoPlanets program. Combining the photometric data sets, we find that the newly discovered planet has a radius of 3.65 (+0.16)/(-0.15) R⊕ and an orbital period of 24.246 days. Radial velocity measurements obtained with the Planet Finder Spectrograph on the Magellan Clay telescope confirm …
Toi-674b: An Oasis In The Desert Of Exo-Neptunes Transiting A Nearby M Dwarf, F. Murgas, N. Astudillo-Defru, X. Bonfils, I. Crossfield, J. M. Almenara, J. Livingston, K. G. Stassun, J. Korth, J. Orell-Miquel, G. Morello, J. D. Eastman, J. J. Lissauer, S. R. Kane, F. Y. Morales, M. W. Werner, V. Gorjian, B. Benneke, D. Dragomir, E. C. Matthews, S. B. Howell, D. Ciardi, E. Gonzales, R. Matson, C. Beichman, J. Schlieder, K. A. Collins, K. I. Collins, Eric L.N. Jensen, P. Evans, F. J. Pozuelos, M. Gillon, E. Jehin, K. Barkaoui, E. Artigau, F. Bouchy, D. Charbonneau, X. Delfosse, R. F. Díaz, R. Doyon, P. Figueira, T. Forveille, C. Lovis, C. Melo, G. Gaisné, F. Pepe, N. C. Santos, D. Ségransan, S. Udry, R. F. Goeke, A. M. Levine, E. V. Quintana, N. M. Guerrero, I. Mireles, D. A. Caldwell, P. Tenenbaum, C. E. Brasseur, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. Winn, J. M. Jenkins
Toi-674b: An Oasis In The Desert Of Exo-Neptunes Transiting A Nearby M Dwarf, F. Murgas, N. Astudillo-Defru, X. Bonfils, I. Crossfield, J. M. Almenara, J. Livingston, K. G. Stassun, J. Korth, J. Orell-Miquel, G. Morello, J. D. Eastman, J. J. Lissauer, S. R. Kane, F. Y. Morales, M. W. Werner, V. Gorjian, B. Benneke, D. Dragomir, E. C. Matthews, S. B. Howell, D. Ciardi, E. Gonzales, R. Matson, C. Beichman, J. Schlieder, K. A. Collins, K. I. Collins, Eric L.N. Jensen, P. Evans, F. J. Pozuelos, M. Gillon, E. Jehin, K. Barkaoui, E. Artigau, F. Bouchy, D. Charbonneau, X. Delfosse, R. F. Díaz, R. Doyon, P. Figueira, T. Forveille, C. Lovis, C. Melo, G. Gaisné, F. Pepe, N. C. Santos, D. Ségransan, S. Udry, R. F. Goeke, A. M. Levine, E. V. Quintana, N. M. Guerrero, I. Mireles, D. A. Caldwell, P. Tenenbaum, C. E. Brasseur, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. Winn, J. M. Jenkins
Physics & Astronomy Faculty Works
Context. The NASA mission TESS is currently doing an all-sky survey from space to detect transiting planets around bright stars. As part of the validation process, the most promising planet candidates need to be confirmed and characterized using follow-up observations. Aims. In this article, our aim is to confirm the planetary nature of the transiting planet candidate TOI-674b using spectroscopic and photometric observations. Methods. We use TESS, Spitzer, ground-based light curves, and HARPS spectrograph radial velocity measurements to establish the physical properties of the transiting exoplanet candidate TOI-674b. We perform a joint fit of the light …
Toi-2076 And Toi-1807: Two Young, Comoving Planetary Systems Within 50 Pc Identified By Tess That Are Ideal Candidates For Further Follow Up, C. Hedges, A. Hughes, G. Zhou, T. J. David, J. Becker, S. Giacalone, A. Vanderburg, J. E. Rodriguez, A. Bieryla, C. Wirth, S. Atherton, T. Fetherolf, K. A. Collins, A. M. Price-Whelan, M. Bedell, S. N. Quinn, T. Gan, G. R. Ricker, D. W. Latham, R. K. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, J. F. Kielkopf, R. P. Schwarz, C. D. Dressing, E. J. Gonzales, I. J. M. Crossfield, E. C. Matthews, Eric L.N. Jensen, E. Furlan, C. L. Gnilka, S. B. Howell, K. V. Lester, N. J. Scott, D. L. Feliz, M. B. Lund, R. J. Siverd, D. J. Stevens, N. Narita, A. Fukui, F. Murgas, E. Palle, P. J. Sutton, K. G. Stassun, L. G. Bouma, M. Vezie, J. N. Villaseñor, E. V. Quintana, J. C. Smith
Toi-2076 And Toi-1807: Two Young, Comoving Planetary Systems Within 50 Pc Identified By Tess That Are Ideal Candidates For Further Follow Up, C. Hedges, A. Hughes, G. Zhou, T. J. David, J. Becker, S. Giacalone, A. Vanderburg, J. E. Rodriguez, A. Bieryla, C. Wirth, S. Atherton, T. Fetherolf, K. A. Collins, A. M. Price-Whelan, M. Bedell, S. N. Quinn, T. Gan, G. R. Ricker, D. W. Latham, R. K. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, J. F. Kielkopf, R. P. Schwarz, C. D. Dressing, E. J. Gonzales, I. J. M. Crossfield, E. C. Matthews, Eric L.N. Jensen, E. Furlan, C. L. Gnilka, S. B. Howell, K. V. Lester, N. J. Scott, D. L. Feliz, M. B. Lund, R. J. Siverd, D. J. Stevens, N. Narita, A. Fukui, F. Murgas, E. Palle, P. J. Sutton, K. G. Stassun, L. G. Bouma, M. Vezie, J. N. Villaseñor, E. V. Quintana, J. C. Smith
Physics & Astronomy Faculty Works
We report the discovery of two planetary systems around comoving stars: TOI-2076 (TIC 27491137) and TOI-1807 (TIC 180695581). TOI-2076 is a nearby (41.9 pc) multiplanetary system orbiting a young (204 ± 50 Myr), bright (K = 7.115 in TIC v8.1) start. TOI-1807 hosts a single transiting planet and is similarly nearby (42.58 pc), similarly young (180 ± 40 Myr ), and bright. Both targets exhibit significant, periodic variability due to starspots, characteristic of their young ages. Using photometric data collected by TESS we identify three transiting planets around TOI-2076 with radii of Rb = 3.3 ± 0.04 R …
Discovery Of A Young Low-Mass Brown Dwarf Transiting A Fast-Rotating F-Type Star By The Galactic Plane Exoplanet (Gpx) Survey, P. Benni, A. Y. Burdanov, V. V. Krushinsky, A. Bonfanti, G. Hébrard, J. M. Almenara, S. Dalal, O. D. S. Demangeon, M. Tsantaki, J. Pepper, K. G. Stassun, A. Vanderburg, A. Belinski, F. Kashaev, K. Barkaoui, T. Kim, W. Kang, K. Antonyuk, V. V. Dyachenko, D. A. Tastegaev, A. Beskakotov, A. A. Mitrofanova, F. J. Pozuelos, E. D. Kuznetsov, A. Popov, F. Kieger, P. A. Wilson, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. M. Jenkins, E. Sokov, I. Sokova, A. Marchini, R. Papini, F. Salvaggio, M. Banfi, Ö. Baştürk, Ş. Torun, S. Yalçinkaya, K. Ivanov, G. Valyavin, E. Jehin, M. Gillon, E. Pakštienė, V.-P. Hentunen, S. Shadick, M. Bretton, A. Wünsche, J. Garlitz, Y. Jongen, D. Molina, E. Girardin, F. Grau Horta, R. Naves, Z. Benkhaldoun, M. D. Joner, M. Spencer, A. Bieryla, D. J. Stevens, Eric L.N. Jensen, K. A. Collins, D. Charbonneau, E. V. Quintana, S. E. Mullally, C. E. Henze
Discovery Of A Young Low-Mass Brown Dwarf Transiting A Fast-Rotating F-Type Star By The Galactic Plane Exoplanet (Gpx) Survey, P. Benni, A. Y. Burdanov, V. V. Krushinsky, A. Bonfanti, G. Hébrard, J. M. Almenara, S. Dalal, O. D. S. Demangeon, M. Tsantaki, J. Pepper, K. G. Stassun, A. Vanderburg, A. Belinski, F. Kashaev, K. Barkaoui, T. Kim, W. Kang, K. Antonyuk, V. V. Dyachenko, D. A. Tastegaev, A. Beskakotov, A. A. Mitrofanova, F. J. Pozuelos, E. D. Kuznetsov, A. Popov, F. Kieger, P. A. Wilson, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. M. Jenkins, E. Sokov, I. Sokova, A. Marchini, R. Papini, F. Salvaggio, M. Banfi, Ö. Baştürk, Ş. Torun, S. Yalçinkaya, K. Ivanov, G. Valyavin, E. Jehin, M. Gillon, E. Pakštienė, V.-P. Hentunen, S. Shadick, M. Bretton, A. Wünsche, J. Garlitz, Y. Jongen, D. Molina, E. Girardin, F. Grau Horta, R. Naves, Z. Benkhaldoun, M. D. Joner, M. Spencer, A. Bieryla, D. J. Stevens, Eric L.N. Jensen, K. A. Collins, D. Charbonneau, E. V. Quintana, S. E. Mullally, C. E. Henze
Physics & Astronomy Faculty Works
We announce the discovery of GPX-1 b, a transiting brown dwarf with a mass of 19.7 ± 1.6 MJup and a radius of 1.47 ± 0.10 RJup, the first substellar object discovered by the Galactic Plane eXoplanet (GPX) survey. The brown dwarf transits a moderately bright (V = 12.3 mag) fast-rotating F-type star with a projected rotational velocity v sin i* 40 ± 10km s⁻¹. We use the isochrone placement algorithm to characterize the host star, which has effective temperature 7000 ± 200 K, mass 1.68 ± 0.10 M⊙, radius 1.56 ± 0.10 …
Populating The Brown Dwarf And Stellar Boundary: Five Stars With Transiting Companions Near The Hydrogen-Burning Mass Limit, N. Grieves, F. Bouchy, M. Lendl, T. Carmichael, I. Mireles, A. Shporer, K. K. Mcleod, K. A. Collins, R. Brahm, K. G. Stassun, S. Gill, L. G. Bouma, T. Guillot, M. Cointepas, L. A. Dos Santos, S. L. Casewell, J. M. Jenkins, T. Henning, L. D. Nielsen, A. Psaridi, S. Udry, D. Ségransan, J. D. Eastman, G. Zhou, L. Abe, A. Agabi, G. Bakos, D. Charbonneau, K. I. Collins, K. D. Colon, N. Crouzet, G. Dransfield, P. Evans, R. F. Goeke, R. Hart, J. M. Irwin, Eric L.N. Jensen, A. Jordán, J. F. Kielkopf, D. W. Latham, W. Marie-Sainte, D. Mékarnia, P. Nelson, S. N. Quinn, D. J. Radford, D. R. Rodriguez, P. Rowden, F.–X. Schmider, R. P. Schwarz, J. C. Smith, C. Stockdale, O. Suarez, T.-G. Tan, A. H. M. J. Triaud, W. Waalkes, G. Wingham
Populating The Brown Dwarf And Stellar Boundary: Five Stars With Transiting Companions Near The Hydrogen-Burning Mass Limit, N. Grieves, F. Bouchy, M. Lendl, T. Carmichael, I. Mireles, A. Shporer, K. K. Mcleod, K. A. Collins, R. Brahm, K. G. Stassun, S. Gill, L. G. Bouma, T. Guillot, M. Cointepas, L. A. Dos Santos, S. L. Casewell, J. M. Jenkins, T. Henning, L. D. Nielsen, A. Psaridi, S. Udry, D. Ségransan, J. D. Eastman, G. Zhou, L. Abe, A. Agabi, G. Bakos, D. Charbonneau, K. I. Collins, K. D. Colon, N. Crouzet, G. Dransfield, P. Evans, R. F. Goeke, R. Hart, J. M. Irwin, Eric L.N. Jensen, A. Jordán, J. F. Kielkopf, D. W. Latham, W. Marie-Sainte, D. Mékarnia, P. Nelson, S. N. Quinn, D. J. Radford, D. R. Rodriguez, P. Rowden, F.–X. Schmider, R. P. Schwarz, J. C. Smith, C. Stockdale, O. Suarez, T.-G. Tan, A. H. M. J. Triaud, W. Waalkes, G. Wingham
Physics & Astronomy Faculty Works
We report the discovery of five transiting companions near the hydrogen-burning mass limit in close orbits around main sequence stars originally identified by the Transiting Exoplanet Survey Satellite (TESS) as TESS objects of interest (TOIs): TOI-148, TOI-587, TOI-681, TOI-746, and TOI-1213. Using TESS and ground-based photometry as well as radial velocities from the CORALIE, CHIRON, TRES, and FEROS spectrographs, we found the companions have orbital periods between 4.8 and 27.2 days, masses between 77 and 98 MJup, and radii between 0.81 and 1.66 RJup. These targets have masses near the uncertain lower limit of hydrogen core …
Tic 454140642: A Compact, Coplanar, Quadruple-Lined Quadruple Star System Consisting Of Two Eclipsing Binaries, V. B. Kostov, B. P. Powell, G. Torres, T. Borkovits, S. A. Rappaport, A. Tokovinin, P. Zasche, D. Anderson, T. Barclay, P. Berlind, P. Brown, M. L. Calkins, K. A. Collins, K. I. Collins, D. M. Conti, G. A. Esquerdo, C. Hellier, Eric L.N. Jensen, J. Kamler, E. Kruse, D. W. Latham, M. Mašek, F. Murgas, G. Olmschenk, J. A. Orosz, A. Pál, E. Palle, R. P. Schwarz, C. Stockdale, D. Tamayo, R. Uhlař, W. F. Welsh, R. West
Tic 454140642: A Compact, Coplanar, Quadruple-Lined Quadruple Star System Consisting Of Two Eclipsing Binaries, V. B. Kostov, B. P. Powell, G. Torres, T. Borkovits, S. A. Rappaport, A. Tokovinin, P. Zasche, D. Anderson, T. Barclay, P. Berlind, P. Brown, M. L. Calkins, K. A. Collins, K. I. Collins, D. M. Conti, G. A. Esquerdo, C. Hellier, Eric L.N. Jensen, J. Kamler, E. Kruse, D. W. Latham, M. Mašek, F. Murgas, G. Olmschenk, J. A. Orosz, A. Pál, E. Palle, R. P. Schwarz, C. Stockdale, D. Tamayo, R. Uhlař, W. F. Welsh, R. West
Physics & Astronomy Faculty Works
We report the discovery of a compact, coplanar, quadruple-lined, eclipsing quadruple star system from Transiting Exoplanet Survey Satellite data, TIC 454140642, also known as TYC 0074-01254-1. The target was first detected in Sector 5 with a 30-minute cadence in full-frame images and then observed in Sector 32 with a 2-minute cadence. The light curve exhibits two sets of primary and secondary eclipses with periods of PA = 13.624 days (binary A) and PB = 10.393 days (binary B). Analysis of archival and follow-up data shows clear eclipse-timing variations and divergent radial velocities, indicating dynamical interactions between the two …
Toi-1634 B: An Ultra-Short-Period Keystone Planet Sitting Inside The M-Dwarf Radius Valley, R. Cloutier, D. Charbonneau, K. G. Stassun, F. Murgas, A. Mortier, R. Massey, J. J. Lissauer, D. W. Latham, J. Irwin, R. D. Haywood, P. Guerra, E. Girardin, S. A. Giacalone, P. Bosch-Cabot, A. Bieryla, J. Winn, C. A. Watson, R. Vanderspek, S. Udry, M. Tamura, A. Sozzetti, A. Shporer, D. Ségransan, S. Seager, A. B. Savel, D. Sasselov, M. Rose, G. Ricker, K. Rice, E. V. Quintana, S. N. Quinn, G. Piotto, D. Phillips, F. Pepe, M. Pedani, H. Parviainen, E. Palle, N. Narita, E. Molinari, G. Micela, S. Mcdermott, M. Mayor, R. A. Matson, A. F. Martinez Fiorenzano, C. Lovis, M. López-Morales, N. Kusakabe, Eric L.N. Jensen, J. M. Jenkins, C. X. Huang, S. B. Howell, A. Harutyunyan, G. Fűrész, A. Fukui, G. A. Esquerdo, E. Esparza-Borges, X. Dumusque, C. D. Dressing, L. Di Fabrizio, K. A. Collins, A. Collier Cameron, J. L. Christiansen, M. Cecconi, L. A. Buchhave, W. Boschin, G. Andreuzzi
Toi-1634 B: An Ultra-Short-Period Keystone Planet Sitting Inside The M-Dwarf Radius Valley, R. Cloutier, D. Charbonneau, K. G. Stassun, F. Murgas, A. Mortier, R. Massey, J. J. Lissauer, D. W. Latham, J. Irwin, R. D. Haywood, P. Guerra, E. Girardin, S. A. Giacalone, P. Bosch-Cabot, A. Bieryla, J. Winn, C. A. Watson, R. Vanderspek, S. Udry, M. Tamura, A. Sozzetti, A. Shporer, D. Ségransan, S. Seager, A. B. Savel, D. Sasselov, M. Rose, G. Ricker, K. Rice, E. V. Quintana, S. N. Quinn, G. Piotto, D. Phillips, F. Pepe, M. Pedani, H. Parviainen, E. Palle, N. Narita, E. Molinari, G. Micela, S. Mcdermott, M. Mayor, R. A. Matson, A. F. Martinez Fiorenzano, C. Lovis, M. López-Morales, N. Kusakabe, Eric L.N. Jensen, J. M. Jenkins, C. X. Huang, S. B. Howell, A. Harutyunyan, G. Fűrész, A. Fukui, G. A. Esquerdo, E. Esparza-Borges, X. Dumusque, C. D. Dressing, L. Di Fabrizio, K. A. Collins, A. Collier Cameron, J. L. Christiansen, M. Cecconi, L. A. Buchhave, W. Boschin, G. Andreuzzi
Physics & Astronomy Faculty Works
Studies of close-in planets orbiting M dwarfs have suggested that the M-dwarf radius valley may be well explained by distinct formation timescales between enveloped terrestrials and rocky planets that form at late times in a gas-depleted environment. This scenario is at odds with the picture that close-in rocky planets form with a primordial gaseous envelope that is subsequently stripped away by some thermally driven mass-loss process. These two physical scenarios make unique predictions of the rocky/enveloped transition's dependence on orbital separation such that studying the compositions of planets within the M-dwarf radius valley may be able to establish the dominant …
Warm Jupiters In Tess Full-Frame Images: A Catalog And Observed Eccentricity Distribution For Year 1, J. Dong, C. X. Huang, R. I. Dawson, D. Foreman-Mackey, K. A. Collins, S. N. Quinn, J. J. Lissauer, T. Beatty, B. Quarles, L. Sha, A. Shporer, Z. Guo, S. R. Kane, L. Abe, K. Barkaoui, Z. Benkhaldoun, R. Brahm, F. Bouchy, T. W. Carmichael, K. I. Collins, D. M. Conti, N. Crouzet, G. Dransfield, P. Evans, T. Gan, M. Ghachoui, M. Gillon, N. Grieves, T. Guillot, C. Hellier, E. Jehin, Eric L.N. Jensen, A. Jordán, J. Kamler, J. F. Kielkopf, D. Mékarnia, L. D. Nielsen, F. J. Pozuelos, D. J. Radford, F.-X. Schmider, R. P. Schwarz, C. Stockdale, T.-G. Tan, M. Timmermans, A. H. M. J. Triaud, G. Wang, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, I. Mireles, D. A. Yahalomi, E. H. Morgan, M. Vezie, E. V. Quintana, M. E. Rose, J. C. Smith, B. Shiao
Warm Jupiters In Tess Full-Frame Images: A Catalog And Observed Eccentricity Distribution For Year 1, J. Dong, C. X. Huang, R. I. Dawson, D. Foreman-Mackey, K. A. Collins, S. N. Quinn, J. J. Lissauer, T. Beatty, B. Quarles, L. Sha, A. Shporer, Z. Guo, S. R. Kane, L. Abe, K. Barkaoui, Z. Benkhaldoun, R. Brahm, F. Bouchy, T. W. Carmichael, K. I. Collins, D. M. Conti, N. Crouzet, G. Dransfield, P. Evans, T. Gan, M. Ghachoui, M. Gillon, N. Grieves, T. Guillot, C. Hellier, E. Jehin, Eric L.N. Jensen, A. Jordán, J. Kamler, J. F. Kielkopf, D. Mékarnia, L. D. Nielsen, F. J. Pozuelos, D. J. Radford, F.-X. Schmider, R. P. Schwarz, C. Stockdale, T.-G. Tan, M. Timmermans, A. H. M. J. Triaud, G. Wang, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, I. Mireles, D. A. Yahalomi, E. H. Morgan, M. Vezie, E. V. Quintana, M. E. Rose, J. C. Smith, B. Shiao
Physics & Astronomy Faculty Works
Warm Jupiters—defined here as planets larger than 6 Earth radii with orbital periods of 8–200 days—are a key missing piece in our understanding of how planetary systems form and evolve. It is currently debated whether Warm Jupiters form in situ, undergo disk or high-eccentricity tidal migration, or have a mixture of origin channels. These different classes of origin channels lead to different expectations for Warm Jupiters' properties, which are currently difficult to evaluate due to the small sample size. We take advantage of the Transiting Exoplanet Survey Satellite (TESS) survey and systematically search for Warm Jupiter candidates around main-sequence host …
An Ultra-Short-Period Transiting Super-Earth Orbiting The M3 Dwarf Toi-1685, P. Bluhm, E. Pallé, K. Molaverdikhani, J. Kemmer, A. P. Hatzes, D. Kossakowski, S. Stock, J. A. Caballero, J. Lillo-Box, V. J. S. Béjar, M. G. Soto, P. J. Amado, P. Brown, C. Cadieux, R. Cloutier, K. A. Collins, K. I. Collins, M. Cortés-Contreras, R. Doyon, S. Dreizler, N. Espinoza, A. Fukui, E. González-Álvarez, T. Henning, K. Horne, S. V. Jeffers, J. M. Jenkins, Eric L.N. Jensen, A. Kaminski, J. F. Kielkopf, N. Kusakabe, M. Kürster, D. Lafrenière, R. Luque, F. Murgas, D. Montes, J. C. Morales, N. Narita, V. M. Passegger, A. Quirrenbach, P. Schöfer, S. Reffert, A. Reiners, I. Ribas, G. R. Ricker, S. Seager, A. Schweitzer, R. P. Schwarz, M. Tamura, T. Trifonov, R. Vanderspek, J. Winn, M. Zechmeister, M. R. Zapatero Osorio
An Ultra-Short-Period Transiting Super-Earth Orbiting The M3 Dwarf Toi-1685, P. Bluhm, E. Pallé, K. Molaverdikhani, J. Kemmer, A. P. Hatzes, D. Kossakowski, S. Stock, J. A. Caballero, J. Lillo-Box, V. J. S. Béjar, M. G. Soto, P. J. Amado, P. Brown, C. Cadieux, R. Cloutier, K. A. Collins, K. I. Collins, M. Cortés-Contreras, R. Doyon, S. Dreizler, N. Espinoza, A. Fukui, E. González-Álvarez, T. Henning, K. Horne, S. V. Jeffers, J. M. Jenkins, Eric L.N. Jensen, A. Kaminski, J. F. Kielkopf, N. Kusakabe, M. Kürster, D. Lafrenière, R. Luque, F. Murgas, D. Montes, J. C. Morales, N. Narita, V. M. Passegger, A. Quirrenbach, P. Schöfer, S. Reffert, A. Reiners, I. Ribas, G. R. Ricker, S. Seager, A. Schweitzer, R. P. Schwarz, M. Tamura, T. Trifonov, R. Vanderspek, J. Winn, M. Zechmeister, M. R. Zapatero Osorio
Physics & Astronomy Faculty Works
Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated planets, can be studied by characterizing the ultra-short-period planet population, which the TESS mission is particularly well suited to discover. Here, we report on the follow-up of a transit signal detected in the TESS sector 19 photometric time series of the M3.0 V star TOI-1685 (2MASS J04342248+4302148). We confirm the planetary nature of the transit signal, which has a period of Pb = 0.6691403−0.0000021+0.0000023 d, using precise radial velocity measurements taken with the CARMENES spectrograph. From the joint photometry and radial velocity analysis, we estimate the …
Mass And Density Of The Transiting Hot And Rocky Super-Earth Lhs 1478 B (Toi-1640 B), M. G. Soto, G. Anglada-Escudé, S. Dreizler, K. Molaverdikhani, J. Kemmer, C. Rodríguez-López, J. Lillo-Box, E. Pallé, N. Espinoza, J. A. Caballero, A. Quirrenbach, I. Ribas, A. Reiners, N. Narita, T. Hirano, P. J. Amado, V. J. S. Béjar, P. Bluhm, C. J. Burke, D. A. Caldwell, D. Charbonneau, R. Cloutier, K. A. Collins, M. Cortés-Contreras, E. Girardin, P. Guerra, H. Harakawa, A. P. Hatzes, J. Irwin, J. M. Jenkins, Eric L.N. Jensen, K. Kawauchi, T. Kotani, T. Kudo, M. Kunimoto, M. Kuzuhara, D. W. Latham, D. Montes, J. C. Morales, M. Mori, R. P. Nelson, M. Omiya, S. Pedraz, V. M. Passegger, B. V. Rackham, A. Rudat, J. E. Schlieder, P. Schöfer, A. Schweitzer, A. Selezneva, C. Stockdale, M. Tamura, T. Trifonov, R. Vanderspek, D. Watanabe
Mass And Density Of The Transiting Hot And Rocky Super-Earth Lhs 1478 B (Toi-1640 B), M. G. Soto, G. Anglada-Escudé, S. Dreizler, K. Molaverdikhani, J. Kemmer, C. Rodríguez-López, J. Lillo-Box, E. Pallé, N. Espinoza, J. A. Caballero, A. Quirrenbach, I. Ribas, A. Reiners, N. Narita, T. Hirano, P. J. Amado, V. J. S. Béjar, P. Bluhm, C. J. Burke, D. A. Caldwell, D. Charbonneau, R. Cloutier, K. A. Collins, M. Cortés-Contreras, E. Girardin, P. Guerra, H. Harakawa, A. P. Hatzes, J. Irwin, J. M. Jenkins, Eric L.N. Jensen, K. Kawauchi, T. Kotani, T. Kudo, M. Kunimoto, M. Kuzuhara, D. W. Latham, D. Montes, J. C. Morales, M. Mori, R. P. Nelson, M. Omiya, S. Pedraz, V. M. Passegger, B. V. Rackham, A. Rudat, J. E. Schlieder, P. Schöfer, A. Schweitzer, A. Selezneva, C. Stockdale, M. Tamura, T. Trifonov, R. Vanderspek, D. Watanabe
Physics & Astronomy Faculty Works
One of the main objectives of the Transiting Exoplanet Survey Satellite (TESS) mission is the discovery of small rocky planets around relatively bright nearby stars. Here, we report the discovery and characterization of the transiting super-Earth planet orbiting LHS 1478 (TOI-1640). The star is an inactive red dwarf (J ~ 9.6 mag and spectral type m3 V) with mass and radius estimates of 0.20 ± 0.01M⊙ and 0.25 ± 0.01R⊙, respectively, and an effective temperature of 3381 ± 54 K. It was observed by TESS in four sectors. These data revealed a transit-like feature with a period of 1.949 days. …
Hot Planets Around Cool Stars – Two Short-Period Mini-Neptunes Transiting The Late K-Dwarf Toi-1260, I. Y. Georgieva, C. M. Persson, O. Barragán, G. Nowak, M. Fridlund, D. Locci, E. Palle, R. Luque, I. Carleo, D. Gandolfi, S. R. Kane, J. Korth, K. G. Stassun, J. Livingston, E. C. Matthews, K. A. Collins, S. B. Howell, L. M. Serrano, S. Albrecht, A. Bieryla, C. E. Brasseur, D. Ciardi, W. D. Cochran, K. D. Colon, I. J. M. Crossfield, S. Csizmadia, H. J. Deeg, M. Esposito, E. Furlan, T. Gan, E. Goffo, E. Gonzales, S. Grziwa, E. W. Guenther, P. Guerra, T. Hirano, J. M. Jenkins, Eric L.N. Jensen, P. Kabáth, E. Knudstrup, K. W. F. Lam, D. W. Latham, A. M. Levine, R. A. Matson, S. Mcdermott, H. L. M. Osborne, M. Paegert, S. N. Quinn, S. Redfield, G. R. Ricker, J. E. Schlieder, N. J. Scott, S. Seager, A. M. S. Smith, P. Tenenbaum, J. D. Twicken, R. Vanderspek, V. Van Eylen, J. N. Winn
Hot Planets Around Cool Stars – Two Short-Period Mini-Neptunes Transiting The Late K-Dwarf Toi-1260, I. Y. Georgieva, C. M. Persson, O. Barragán, G. Nowak, M. Fridlund, D. Locci, E. Palle, R. Luque, I. Carleo, D. Gandolfi, S. R. Kane, J. Korth, K. G. Stassun, J. Livingston, E. C. Matthews, K. A. Collins, S. B. Howell, L. M. Serrano, S. Albrecht, A. Bieryla, C. E. Brasseur, D. Ciardi, W. D. Cochran, K. D. Colon, I. J. M. Crossfield, S. Csizmadia, H. J. Deeg, M. Esposito, E. Furlan, T. Gan, E. Goffo, E. Gonzales, S. Grziwa, E. W. Guenther, P. Guerra, T. Hirano, J. M. Jenkins, Eric L.N. Jensen, P. Kabáth, E. Knudstrup, K. W. F. Lam, D. W. Latham, A. M. Levine, R. A. Matson, S. Mcdermott, H. L. M. Osborne, M. Paegert, S. N. Quinn, S. Redfield, G. R. Ricker, J. E. Schlieder, N. J. Scott, S. Seager, A. M. S. Smith, P. Tenenbaum, J. D. Twicken, R. Vanderspek, V. Van Eylen, J. N. Winn
Physics & Astronomy Faculty Works
We present the discovery and characterization of two sub-Neptunes in close orbits, as well as a tentative outer planet of a similar size, orbiting TOI-1260 – a low metallicity K6 Vdwarf star. Photometry from TESS yields radii of Rb = 2.33 ± 0.10 R⊕ and Rc = 2.82 ± 0.15 R⊕, and periods of 3.13 and 7.49 days for TOI-1260 b and TOI-1260 c, respectively. We combined the TESS data with a series of ground-based follow-up observations to characterize the planetary system. From HARPS-N high-precision radial velocities we obtain Mb =8.6+1.4−1.5 M⊕ and Mc =11.8+3.4−3.2 M⊕. The star is moderately …
Chandra Grating Spectroscopy Of Embedded Wind Shock X-Ray Emission From O Stars Shows Low Plasma Temperatures And Significant Wind Absorption, David H. Cohen, V. Vaughn Parts, Graham M. Doskoch , '20, Jiaming Wang , '22, V. Petit, M. A. Leutenegger, M. Gagné
Chandra Grating Spectroscopy Of Embedded Wind Shock X-Ray Emission From O Stars Shows Low Plasma Temperatures And Significant Wind Absorption, David H. Cohen, V. Vaughn Parts, Graham M. Doskoch , '20, Jiaming Wang , '22, V. Petit, M. A. Leutenegger, M. Gagné
Physics & Astronomy Faculty Works
We present a uniform analysis of six examples of embedded wind shock (EWS) O star X-ray sources observed at high resolution with the Chandra grating spectrometers. By modelling both the hot plasma emission and the continuum absorption of the soft X-rays by the cool, partially ionized bulk of the wind we derive the temperature distribution of the shock-heated plasma and the wind mass-loss rate of each star. We find a similar temperature distribution for each star’s hot wind plasma, consistent with a power-law differential emission measure, dlogEMdlogT, with a slope a little steeper than −2, up to temperatures of only …
Precise Transit And Radial-Velocity Characterization Of A Resonant Pair: The Warm Jupiter Toi-216c And Eccentric Warm Neptune Toi-216b, R. I. Dawson, C. X. Huang, R. Brahm, K. A. Collins, M. J. Hobson, A. Jordán, J. Dong, J. Korth, T. Trifonov, L. Abe, A. Agabi, I. Bruni, R. P. Butler, M. Barbieri, K. I. Collins, D. M. Conti, J. D. Crane, N. Crouzet, G. Dransfield, P. Evans, N. Espinoza, T. Gan, T. Guillot, T. Henning, J. J. Lissauer, Eric L. N. Jensen, W. M. Sainte, D. Mékarnia, G. Myers, S. Nandakumar, H. M. Relles, P. Sarkis, P. Torres, S. Shectman, F.-X. Schmider, A. Shporer, C. Stockdale, J. Teske, A. H. M. J. Triaud, S. X. Wang, C. Ziegler, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. Winn, J. M. Jenkins, L. G. Bouma, J. A. Burt, D. Charbonneau, A. M. Levine, S. Mcdermott, B. Mclean, M. E. Rose, A. Vanderburg, B. Wohler
Precise Transit And Radial-Velocity Characterization Of A Resonant Pair: The Warm Jupiter Toi-216c And Eccentric Warm Neptune Toi-216b, R. I. Dawson, C. X. Huang, R. Brahm, K. A. Collins, M. J. Hobson, A. Jordán, J. Dong, J. Korth, T. Trifonov, L. Abe, A. Agabi, I. Bruni, R. P. Butler, M. Barbieri, K. I. Collins, D. M. Conti, J. D. Crane, N. Crouzet, G. Dransfield, P. Evans, N. Espinoza, T. Gan, T. Guillot, T. Henning, J. J. Lissauer, Eric L. N. Jensen, W. M. Sainte, D. Mékarnia, G. Myers, S. Nandakumar, H. M. Relles, P. Sarkis, P. Torres, S. Shectman, F.-X. Schmider, A. Shporer, C. Stockdale, J. Teske, A. H. M. J. Triaud, S. X. Wang, C. Ziegler, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. Winn, J. M. Jenkins, L. G. Bouma, J. A. Burt, D. Charbonneau, A. M. Levine, S. Mcdermott, B. Mclean, M. E. Rose, A. Vanderburg, B. Wohler
Physics & Astronomy Faculty Works
TOI-216 hosts a pair of warm, large exoplanets discovered by the TESS mission. These planets were found to be in or near the 2:1 resonance, and both of them exhibit transit timing variations (TTVs). Precise characterization of the planets' masses and radii, orbital properties, and resonant behavior can test theories for the origins of planets orbiting close to their stars. Previous characterization of the system using the first six sectors of TESS data suffered from a degeneracy between planet mass and orbital eccentricity. Radial-velocity measurements using HARPS, FEROS, and the Planet Finder Spectrograph break that degeneracy, and an expanded TTV …
A Hot Mini-Neptune In The Radius Valley Orbiting Solar Analogue Hd 110113, H. P. Osborn, D. J. Armstrong, V. Adibekyan, K. A. Collins, E. Delgado-Mena, S. B. Howell, C. Hellier, G. W. King, J. Lillo-Box, L. D. Nielsen, J. F. Otegi, N. C. Santos, C. Ziegler, D. R. Anderson, C. Briceño, C. Burke, D. Bayliss, D. Barrado, E. M. Bryant, D. J. A. Brown, S. C. C. Barros, F. Bouchy, D. A. Caldwell, D. M. Conti, R. F. Díaz, D. Dragomir, M. Deleuil, O. D. S. Demangeon, C. Dorn, T. Daylan, P. Figueira, R. Helled, S. Hoyer, J. M. Jenkins, Eric L.N. Jensen, D. W. Latham, N. Law, D. R. Louie, A. W. Mann, A. Osborn, D. L. Pollacco, D. R. Rodriguez, B. V. Rackham, G. Ricker, N. J. Scott, S. G. Sousa, S. Seager, K. G. Stassun, J. C. Smith, P. Strøm, S. Udry, J. Villaseñor, R. Vanderspek, R. West, P. J. Wheatley, J. N. Winn
A Hot Mini-Neptune In The Radius Valley Orbiting Solar Analogue Hd 110113, H. P. Osborn, D. J. Armstrong, V. Adibekyan, K. A. Collins, E. Delgado-Mena, S. B. Howell, C. Hellier, G. W. King, J. Lillo-Box, L. D. Nielsen, J. F. Otegi, N. C. Santos, C. Ziegler, D. R. Anderson, C. Briceño, C. Burke, D. Bayliss, D. Barrado, E. M. Bryant, D. J. A. Brown, S. C. C. Barros, F. Bouchy, D. A. Caldwell, D. M. Conti, R. F. Díaz, D. Dragomir, M. Deleuil, O. D. S. Demangeon, C. Dorn, T. Daylan, P. Figueira, R. Helled, S. Hoyer, J. M. Jenkins, Eric L.N. Jensen, D. W. Latham, N. Law, D. R. Louie, A. W. Mann, A. Osborn, D. L. Pollacco, D. R. Rodriguez, B. V. Rackham, G. Ricker, N. J. Scott, S. G. Sousa, S. Seager, K. G. Stassun, J. C. Smith, P. Strøm, S. Udry, J. Villaseñor, R. Vanderspek, R. West, P. J. Wheatley, J. N. Winn
Physics & Astronomy Faculty Works
We report the discovery of HD 110113 b (TESS object of interest-755.01), a transiting mini-Neptune exoplanet on a 2.5-d orbit around the solar-analogue HD 110113 (Teff = 5730 K). Using TESS photometry and High Accuracy Radial velocity Planet Searcher (HARPS) radial velocities gathered by the NCORES program, we find that HD 110113 b has a radius of 2.05 ± 0.12 R⊕ and a mass of 4.55 ± 0.62 M⊕. The resulting density of 2.90+0.75−0.59 g cm−3 is significantly lower than would be expected from a pure-rock world; therefore HD 110113 b must be a mini-Neptune with a significant volatile atmosphere. …
Tic 168789840: A Sextuply Eclipsing Sextuple Star System, B. P. Powell, V. B. Kostov, S. A. Rappaport, T. Borkovits, P. Zasche, A. Tokovinin, E. Kruse, D. W. Latham, B. T. Montet, Eric L.N. Jensen, R. Jayaraman, K. A. Collins, M. Mašek, C. Hellier, P. Evans, T.-G. Tan, J. E. Schlieder, G. Torres, A. P. Smale, A. H. Friedman, T. Barclay, R. Gagliano, E. V. Quintana, T. L. Jacobs, E. A. Gilbert, M. H. Kristiansen, K. D. Colón, D. M. Lacourse, G. Olmschenk, M. Omohundro, J. D. Schnittman, H. M. Schwengeler, R. K. Barry, I. A. Terentev, P. Boyd, A. R. Schmitt, S. M. Quinn, A. Vanderburg, E. Palle, J. Armstrong, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, D. A. Caldwell, B. Wohler, B. Shiao, C. J. Burke, T. Daylan, J. Villaseñor
Tic 168789840: A Sextuply Eclipsing Sextuple Star System, B. P. Powell, V. B. Kostov, S. A. Rappaport, T. Borkovits, P. Zasche, A. Tokovinin, E. Kruse, D. W. Latham, B. T. Montet, Eric L.N. Jensen, R. Jayaraman, K. A. Collins, M. Mašek, C. Hellier, P. Evans, T.-G. Tan, J. E. Schlieder, G. Torres, A. P. Smale, A. H. Friedman, T. Barclay, R. Gagliano, E. V. Quintana, T. L. Jacobs, E. A. Gilbert, M. H. Kristiansen, K. D. Colón, D. M. Lacourse, G. Olmschenk, M. Omohundro, J. D. Schnittman, H. M. Schwengeler, R. K. Barry, I. A. Terentev, P. Boyd, A. R. Schmitt, S. M. Quinn, A. Vanderburg, E. Palle, J. Armstrong, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, D. A. Caldwell, B. Wohler, B. Shiao, C. J. Burke, T. Daylan, J. Villaseñor
Physics & Astronomy Faculty Works
We report the discovery of a sextuply eclipsing sextuple star system from TESS data, TIC 168789840, also known as TYC 7037-89-1, the first known sextuple system consisting of three eclipsing binaries. The target was observed in Sectors 4 and 5 during Cycle 1, with lightcurves extracted from TESS Full Frame Image data. It was also previously observed by the WASP survey and ASAS-SN. The system consists of three gravitationally bound eclipsing binaries in a hierarchical structure of an inner quadruple system with an outer binary subsystem. Follow-up observations from several different observatories were conducted as a means of determining additional …
Tess Delivers Five New Hot Giant Planets Orbiting Bright Stars From The Full-Frame Images, J. E. Rodriguez, S. N. Quinn, G. Zhou, A. Vanderburg, L. D. Nielsen, R. A. Wittenmyer, R. Brahm, P. A. Reed, C. X. Huang, S. Vach, D. R. Ciardi, R. J. Oelkers, K. G. Stassun, C. Hellier, B. S. Gaudi, J. D. Eastman, K. A. Collins, A. Bieryla, S. Christian, D. W. Latham, I. Carleo, D. J. Wright, E. Matthews, E. J. Gonzales, C. Ziegler, C. D. Dressing, S. B. Howell, T.-G. Tan, J. Wittrock, P. Plavchan, K. K. Mcleod, D. Baker, G. Wang, D. J. Radford, R. P. Schwarz, M. Esposito, G. R. Ricker, R. K. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, B. Addison, D. R. Anderosn, T. Barclay, T. G. Beatty, P. Berlind, F. Bouchy, M. Bowen, B. P. Bowler, C. E. Brasseur, C. Briceño, D. A. Caldwell, M. L. Calkins, S. Cartwright, P. Chaturvedi, G. Chaverot, S. Chimaladinne, J. L. Christiansen, K. I. Collins, I. J. M. Crossfield, K. Eastridge, N. Espinoza, G. A. Esquerdo, D. L. Felix, T. Fenske, W. Fong, T. Gan, S. Giacalone, H. Gill, L. Gordon, A. Granados, N. Grieves, E. W. Guenther, N. Guerrero, T. Henning, C. E. Henze, K. Hesse, M. J. Hobson, J. Horner, D. J. James, Eric L. N. Jensen, M. Jimenez, A. Jordán, S. R. Kane, J. Kielkopf, K. Kim, R. B. Kuhn, N. Latouf, N. M. Law, A. M. Levine, M. B. Lund, A. W. Mann, S. Mao, R. A. Matson, M. W. Mengel, J. Mink, P. Newman, T. O’Dwyer, J. Okumura, E. Palle, J. Pepper, E. V. Quintana, P. Sarkis, A. B. Savel, J. E. Schlieder, C. Schnaible, A. Shporer, R. Sefako, J. V. Seidel, R. J. Siverd, B. Skinner, M. Stalport, D. J. Stevens, C. Stibbards, C. G. Tinney, R. G. West, D. A. Yahalomi, H. Zhang
Tess Delivers Five New Hot Giant Planets Orbiting Bright Stars From The Full-Frame Images, J. E. Rodriguez, S. N. Quinn, G. Zhou, A. Vanderburg, L. D. Nielsen, R. A. Wittenmyer, R. Brahm, P. A. Reed, C. X. Huang, S. Vach, D. R. Ciardi, R. J. Oelkers, K. G. Stassun, C. Hellier, B. S. Gaudi, J. D. Eastman, K. A. Collins, A. Bieryla, S. Christian, D. W. Latham, I. Carleo, D. J. Wright, E. Matthews, E. J. Gonzales, C. Ziegler, C. D. Dressing, S. B. Howell, T.-G. Tan, J. Wittrock, P. Plavchan, K. K. Mcleod, D. Baker, G. Wang, D. J. Radford, R. P. Schwarz, M. Esposito, G. R. Ricker, R. K. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, B. Addison, D. R. Anderosn, T. Barclay, T. G. Beatty, P. Berlind, F. Bouchy, M. Bowen, B. P. Bowler, C. E. Brasseur, C. Briceño, D. A. Caldwell, M. L. Calkins, S. Cartwright, P. Chaturvedi, G. Chaverot, S. Chimaladinne, J. L. Christiansen, K. I. Collins, I. J. M. Crossfield, K. Eastridge, N. Espinoza, G. A. Esquerdo, D. L. Felix, T. Fenske, W. Fong, T. Gan, S. Giacalone, H. Gill, L. Gordon, A. Granados, N. Grieves, E. W. Guenther, N. Guerrero, T. Henning, C. E. Henze, K. Hesse, M. J. Hobson, J. Horner, D. J. James, Eric L. N. Jensen, M. Jimenez, A. Jordán, S. R. Kane, J. Kielkopf, K. Kim, R. B. Kuhn, N. Latouf, N. M. Law, A. M. Levine, M. B. Lund, A. W. Mann, S. Mao, R. A. Matson, M. W. Mengel, J. Mink, P. Newman, T. O’Dwyer, J. Okumura, E. Palle, J. Pepper, E. V. Quintana, P. Sarkis, A. B. Savel, J. E. Schlieder, C. Schnaible, A. Shporer, R. Sefako, J. V. Seidel, R. J. Siverd, B. Skinner, M. Stalport, D. J. Stevens, C. Stibbards, C. G. Tinney, R. G. West, D. A. Yahalomi, H. Zhang
Physics & Astronomy Faculty Works
We present the discovery and characterization of five hot and warm Jupiters—TOI-628 b (TIC 281408474; HD 288842), TOI-640 b (TIC 147977348), TOI-1333 b (TIC 395171208, BD+47 3521A), TOI-1478 b (TIC 409794137), and TOI-1601 b (TIC 139375960)—based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The five planets were identified from the full-frame images and were confirmed through a series of photometric and spectroscopic follow-up observations by the TESS Follow-up Observing Program Working Group. The planets are all Jovian size (RP = 1.01–1.77 RJ) and have masses that range from 0.85 to 6.33 MJ. The host stars of these systems …
A Nearby Transiting Rocky Exoplanet That Is Suitable For Atmospheric Investigation, T. Trifonov, J. A. Caballero, J. C. Morales, A. Seifahrt, I. Ribas, A. Reiners, J. L. Bean, R. Luque, H. Parviainen, E. Pallé, S. Stock, M. Zechmeister, P. J. Amado, G. Anglada-Escudé, M. Azzaro, T. Barclay, V. J. S. Béjar, P. Bluhm, N. Casasayas-Barris, C. Cifuentes, K. A. Collins, K. I. Collins, M. Cortés-Contreras, J. De Leon, S. Dreizler, C. D. Dressing, E. Esparza-Borges, N. Espinoza, M. Fausnaugh, A. Fukui, A. P. Hatzes, C. Hellier, T. Henning, C. E. Henze, E. Herrero, S. V. Jeffers, J. M. Jenkins, Eric L.N. Jensen, A. Kaminski, D. Kasper, D. Kossakowski, M. Kürster, M. Lafarga, D. W. Latham, A. W. Mann, K. Molaverdikhani, D. Montes, B. T. Montet, F. Murgas, N. Narita, M. Oshagh, V. M. Passegger, D. Pollacco, S. N. Quinn, A. Quirrenbach, G. R. Ricker, C. Rodríguez López, J. Sanz-Forcada, R. P. Schwarz, A. Schweitzer, S. Seager, A. Shporer, M. Stangret, J. Stürmer, T. G. Tan, P. Tenenbaum, J. D. Twicken, R. Vanderspek, J. N. Winn
A Nearby Transiting Rocky Exoplanet That Is Suitable For Atmospheric Investigation, T. Trifonov, J. A. Caballero, J. C. Morales, A. Seifahrt, I. Ribas, A. Reiners, J. L. Bean, R. Luque, H. Parviainen, E. Pallé, S. Stock, M. Zechmeister, P. J. Amado, G. Anglada-Escudé, M. Azzaro, T. Barclay, V. J. S. Béjar, P. Bluhm, N. Casasayas-Barris, C. Cifuentes, K. A. Collins, K. I. Collins, M. Cortés-Contreras, J. De Leon, S. Dreizler, C. D. Dressing, E. Esparza-Borges, N. Espinoza, M. Fausnaugh, A. Fukui, A. P. Hatzes, C. Hellier, T. Henning, C. E. Henze, E. Herrero, S. V. Jeffers, J. M. Jenkins, Eric L.N. Jensen, A. Kaminski, D. Kasper, D. Kossakowski, M. Kürster, M. Lafarga, D. W. Latham, A. W. Mann, K. Molaverdikhani, D. Montes, B. T. Montet, F. Murgas, N. Narita, M. Oshagh, V. M. Passegger, D. Pollacco, S. N. Quinn, A. Quirrenbach, G. R. Ricker, C. Rodríguez López, J. Sanz-Forcada, R. P. Schwarz, A. Schweitzer, S. Seager, A. Shporer, M. Stangret, J. Stürmer, T. G. Tan, P. Tenenbaum, J. D. Twicken, R. Vanderspek, J. N. Winn
Physics & Astronomy Faculty Works
Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability. Combining radial velocity (RV) and transit data provides additional information on exoplanet physical properties. We detect a transiting rocky planet with an orbital period of 1.467 days around the nearby red dwarf star Gliese 486. The planet Gliese 486 b is 2.81 Earth masses and 1.31 Earth radii, with uncertainties of 5%, as determined from RV data and photometric light curves. The host star is at a distance of ~8.1 parsecs, has a J-band magnitude of ~7.2, and is observable from both hemispheres of Earth. On …
Tess Discovery Of A Super-Earth And Three Sub-Neptunes Hosted By The Bright, Sun-Like Star Hd 108236, T. Daylan, K. Pinglé, J. Wright, M. N. Günther, K. G. Stassun, S. R. Kane, A. Vanderburg, D. Jontof-Hutter, J. E. Rodriguez, A. Shporer, C. X. Huang, T. Mikal-Evans, M. Badenas-Agusti, K. A. Collins, B. V. Rackham, S. N. Quinn, R. Cloutier, K. I. Collins, P. Guerra, Eric L.N. Jensen, J. F. Kielkopf, B. Massey, R. P. Schwarz, D. Charbonneau, J. J. Lissauer, J. M. Irwin, Ö Baştürk, B. Fulton, A. Soubkiou, B. Zouhair, S. B. Howell, C. Ziegler, C. Briceño, N. Law, A. W. Mann, N. Scott, E. Furlan, D. R. Ciardi, R. Matson, C. Hellier, D. R. Anderson, R. P. Butler, J. D. Crane, J. K. Teske, S. A. Shectman, M. H. Kristiansen, I. A. Terentev, H. M. Schwengeler, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, Z. K. Berta-Thompson, L. G. Bouma, W. Fong, G. Furesz, C. E. Henze, E. H. Morgan, E. Quintana, E. B. Ting, J. D. Twicken
Tess Discovery Of A Super-Earth And Three Sub-Neptunes Hosted By The Bright, Sun-Like Star Hd 108236, T. Daylan, K. Pinglé, J. Wright, M. N. Günther, K. G. Stassun, S. R. Kane, A. Vanderburg, D. Jontof-Hutter, J. E. Rodriguez, A. Shporer, C. X. Huang, T. Mikal-Evans, M. Badenas-Agusti, K. A. Collins, B. V. Rackham, S. N. Quinn, R. Cloutier, K. I. Collins, P. Guerra, Eric L.N. Jensen, J. F. Kielkopf, B. Massey, R. P. Schwarz, D. Charbonneau, J. J. Lissauer, J. M. Irwin, Ö Baştürk, B. Fulton, A. Soubkiou, B. Zouhair, S. B. Howell, C. Ziegler, C. Briceño, N. Law, A. W. Mann, N. Scott, E. Furlan, D. R. Ciardi, R. Matson, C. Hellier, D. R. Anderson, R. P. Butler, J. D. Crane, J. K. Teske, S. A. Shectman, M. H. Kristiansen, I. A. Terentev, H. M. Schwengeler, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, Z. K. Berta-Thompson, L. G. Bouma, W. Fong, G. Furesz, C. E. Henze, E. H. Morgan, E. Quintana, E. B. Ting, J. D. Twicken
Physics & Astronomy Faculty Works
We report the discovery and validation of four extrasolar planets hosted by the nearby, bright, Sun-like (G3V) star HD 108236 using data from the Transiting Exoplanet Survey Satellite (TESS). We present transit photometry, reconnaissance, and precise Doppler spectroscopy, as well as high-resolution imaging, to validate the planetary nature of the objects transiting HD 108236, also known as the TESS Object of Interest (TOI) 1233. The innermost planet is a possibly rocky super-Earth with a period of ${3.79523}_{-0.00044}^{+0.00047}$days and has a radius of 1.586 ± 0.098 R⊕. The outer planets are sub-Neptunes, with potential gaseous envelopes, having radii of ${2.068}_{-0.091}^{+0.10}$R⊕, 2.72 …
Tess Hunt For Young And Maturing Exoplanets (Thyme). Iv. Three Small Planets Orbiting A 120 Myr Old Star In The Pisces–Eridanus Stream, E. R. Newton, A. W. Mann, A. L. Kraus, J. H. Livingston, A. Vanderburg, J. L. Curtis, P. C. Thao, K. Hawkins, M. L. Wood, A. C. Rizzuto, A. Soubkiou, B. M. Tofflemire, G. Zhou, I. J. M. Crossfield, L. A. Pearce, K. A. Collins, D. M. Conti, T.-G. Tan, S. Villanueva, A. Spencer, D. Dragomir, S. M. Quinn, Eric L.N. Jensen, K. I. Collins, C. Stockdale, R. Cloutier, C. Hellier, Z. Benkhaldoun, C. Ziegler, C. Briceño, N. Law, B. Benneke, J. L. Christiansen, V. Gorjian, S. R. Kane, L. Kreidberg, F. Y. Morales, M. W. Werner, J. D. Twicken, A. M. Levine, D. R. Ciardi, N. M. Guerrero, K. Hesse, E. V. Quintana, B. Shiao, J. C. Smith, G. Torres, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, D. W. Latham
Tess Hunt For Young And Maturing Exoplanets (Thyme). Iv. Three Small Planets Orbiting A 120 Myr Old Star In The Pisces–Eridanus Stream, E. R. Newton, A. W. Mann, A. L. Kraus, J. H. Livingston, A. Vanderburg, J. L. Curtis, P. C. Thao, K. Hawkins, M. L. Wood, A. C. Rizzuto, A. Soubkiou, B. M. Tofflemire, G. Zhou, I. J. M. Crossfield, L. A. Pearce, K. A. Collins, D. M. Conti, T.-G. Tan, S. Villanueva, A. Spencer, D. Dragomir, S. M. Quinn, Eric L.N. Jensen, K. I. Collins, C. Stockdale, R. Cloutier, C. Hellier, Z. Benkhaldoun, C. Ziegler, C. Briceño, N. Law, B. Benneke, J. L. Christiansen, V. Gorjian, S. R. Kane, L. Kreidberg, F. Y. Morales, M. W. Werner, J. D. Twicken, A. M. Levine, D. R. Ciardi, N. M. Guerrero, K. Hesse, E. V. Quintana, B. Shiao, J. C. Smith, G. Torres, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn, J. M. Jenkins, D. W. Latham
Physics & Astronomy Faculty Works
Young exoplanets can offer insight into the evolution of planetary atmospheres, compositions, and architectures. We present the discovery of the young planetary system TOI 451 (TIC 257605131, Gaia DR2 4844691297067063424). TOI 451 is a member of the 120 Myr old Pisces–Eridanus stream (Psc–Eri). We confirm membership in the stream with its kinematics, its lithium abundance, and the rotation and UV excesses of both TOI 451 and its wide-binary companion, TOI 451 B (itself likely an M-dwarf binary). We identified three candidate planets transiting in the Transiting Exoplanet Survey Satellite data and followed up the signals with photometry from Spitzer and …
The Tess-Keck Survey. Ii. An Ultra-Short-Period Rocky Planet And Its Siblings Transiting The Galactic Thick-Disk Star Toi-561, L. M. Weiss, F. Dai, D. Huber, J. M. Brewer, K. A. Collins, D. R. Ciardi, E. C. Matthews, C. Ziegler, S. B. Howell, N. M. Batalha, I. J. M. Crossfield, C. Dressing, B. Fulton, A. W. Howard, H. Isaacson, S. R. Kane, E. A. Petigura, P. Robertson, A. Roy, R. A. Rubenzahl, J. D. Twicken, Z. R. Claytor, K. G. Stassun, M. G. Macdougall, A. Chontos, S. Giacalone, P. A. Dalba, T. Mocnik, M. L. Hill, C. Beard, J. M. Akana Murphy, L. J. Rosenthal, A. Behmard, J. Van Zandt, J. Lubin, M. R. Kosiarek, M. B. Lund, J. L. Christiansen, R. A. Matson, C. A. Beichman, J. E. Schlieder, E. J. Gonzales, C. Briceño, N. Law, A. W. Mann, K. I. Collins, P. Evans, A. Fukui, Eric L.N. Jensen, F. Murgas, N. Narita, E. Palle, H. Parviainen, R. P. Schwarz, T.-G. Tan, J. S. Acton, P. Eigmüller, J. Jenkins, G. Ricker, S. Seager, J. N. Winn
The Tess-Keck Survey. Ii. An Ultra-Short-Period Rocky Planet And Its Siblings Transiting The Galactic Thick-Disk Star Toi-561, L. M. Weiss, F. Dai, D. Huber, J. M. Brewer, K. A. Collins, D. R. Ciardi, E. C. Matthews, C. Ziegler, S. B. Howell, N. M. Batalha, I. J. M. Crossfield, C. Dressing, B. Fulton, A. W. Howard, H. Isaacson, S. R. Kane, E. A. Petigura, P. Robertson, A. Roy, R. A. Rubenzahl, J. D. Twicken, Z. R. Claytor, K. G. Stassun, M. G. Macdougall, A. Chontos, S. Giacalone, P. A. Dalba, T. Mocnik, M. L. Hill, C. Beard, J. M. Akana Murphy, L. J. Rosenthal, A. Behmard, J. Van Zandt, J. Lubin, M. R. Kosiarek, M. B. Lund, J. L. Christiansen, R. A. Matson, C. A. Beichman, J. E. Schlieder, E. J. Gonzales, C. Briceño, N. Law, A. W. Mann, K. I. Collins, P. Evans, A. Fukui, Eric L.N. Jensen, F. Murgas, N. Narita, E. Palle, H. Parviainen, R. P. Schwarz, T.-G. Tan, J. S. Acton, P. Eigmüller, J. Jenkins, G. Ricker, S. Seager, J. N. Winn
Physics & Astronomy Faculty Works
We report the discovery of TOI-561, a multiplanet system in the galactic thick disk that contains a rocky, ultra-short-period planet. This bright (V = 10.2) star hosts three small transiting planets identified in photometry from the NASA TESS mission: TOI-561 b (TOI-561.02, P = 0.44 days, Rp = 1.45 ± 0.11 R⊕), c (TOI-561.01, P = 10.8 days, Rp = 2.90 ± 0.13 R⊕), and d (TOI-561.03, P = 16.3 days, Rp = 2.32 ± 0.16 R⊕). The star is chemically ([Fe/H] = −0.41 ± 0.05, [α/Fe] = +0.23 ± 0.05) and kinematically consistent with the galactic thick-disk population, making …
Toi-954 B And K2-329 B: Short-Period Saturn-Mass Planets That Test Whether Irradiation Leads To Inflation, L. Sha, C. X. Huang, A. Shporer, J. E. Rodriguez, A. Vanderburg, R. Brahm, J. Hagelberg, E. C. Matthews, C. Ziegler, J. H. Livingston, K. G. Stassun, D. J. Wright, J. D. Crane, N. Espinoza, F. Bouchy, G. Á. Bakos, K. A. Collins, G. Zhou, A. Bieryla, J. D. Hartman, R. A. Wittenmyer, L. D. Nielsen, P. Plavchan, D. Bayliss, P. Sarkis, T.-G. Tan, R. Cloutier, L. Mancini, A. Jordán, S. Wang, T. Henning, N. Narita, K. Penev, J. K. Teske, S. R. Kane, A. W. Mann, B. C. Addison, M. Tamura, J. Horner, M. Barbieri, J. A. Burt, M. R. Díaz, I. J. M. Crossfield, D. Dragomir, H. Drass, A. D. Feinstein, H. Zhang, R. Hart, J. F. Kielkopf, Eric L.N. Jensen, B. T. Montet, G. Ottoni, R. P. Schwarz, F. Rojas, D. Nespral, P. Torres, M. W. Mengel, S. Udry, A. Zapata, E. Snoddy, J. Okumura, G. R. Ricker, R. K. Vanderspek, D. W. Latham, J. N. Winn, S. Seager, J. M. Jenkins, K. D. Colón, C. E. Henze, A. Krishnamurthy, E. B. Ting, M. Vezie, S. Villanueva
Toi-954 B And K2-329 B: Short-Period Saturn-Mass Planets That Test Whether Irradiation Leads To Inflation, L. Sha, C. X. Huang, A. Shporer, J. E. Rodriguez, A. Vanderburg, R. Brahm, J. Hagelberg, E. C. Matthews, C. Ziegler, J. H. Livingston, K. G. Stassun, D. J. Wright, J. D. Crane, N. Espinoza, F. Bouchy, G. Á. Bakos, K. A. Collins, G. Zhou, A. Bieryla, J. D. Hartman, R. A. Wittenmyer, L. D. Nielsen, P. Plavchan, D. Bayliss, P. Sarkis, T.-G. Tan, R. Cloutier, L. Mancini, A. Jordán, S. Wang, T. Henning, N. Narita, K. Penev, J. K. Teske, S. R. Kane, A. W. Mann, B. C. Addison, M. Tamura, J. Horner, M. Barbieri, J. A. Burt, M. R. Díaz, I. J. M. Crossfield, D. Dragomir, H. Drass, A. D. Feinstein, H. Zhang, R. Hart, J. F. Kielkopf, Eric L.N. Jensen, B. T. Montet, G. Ottoni, R. P. Schwarz, F. Rojas, D. Nespral, P. Torres, M. W. Mengel, S. Udry, A. Zapata, E. Snoddy, J. Okumura, G. R. Ricker, R. K. Vanderspek, D. W. Latham, J. N. Winn, S. Seager, J. M. Jenkins, K. D. Colón, C. E. Henze, A. Krishnamurthy, E. B. Ting, M. Vezie, S. Villanueva
Physics & Astronomy Faculty Works
We report the discovery of two short-period Saturn-mass planets, one transiting the G subgiant TOI-954 (TIC 44792534, V = 10.343, T = 9.78) observed in TESS sectors 4 and 5 and one transiting the G dwarf K2-329 (EPIC 246193072, V = 12.70, K = 10.67) observed in K2 campaigns 12 and 19. We confirm and characterize these two planets with a variety of ground-based archival and follow-up observations, including photometry, reconnaissance spectroscopy, precise radial velocity, and high-resolution imaging. Combining all available data, we find that TOI-954 b has a radius of ${0.852}_{-0.062}^{+0.053}\,{R}_{{\rm{J}}}$and a mass of ${0.174}_{-0.017}^{+0.018}$MJ and is in a …
A Planetary System With Two Transiting Mini-Neptunes Near The Radius Valley Transition Around The Bright M Dwarf Toi-776, R. Luque, L. M. Serrano, K. Molaverdikhani, M. C. Nixon, J. H. Livingston, E. W. Guenther, E. Pallé, N. Madhusudhan, G. Nowak, J. Korth, W. D. Cochran, T. Hirano, P. Chaturvedi, E. Goffo, S. Albrecht, O. Barragán, C. Briceño, J. Cabrera, D. Charbonneau, R. Cloutier, K. A. Collins, K. I. Collins, K. D. Colón, J. M. Crossfield, S. Csizmadia, F. Dai, H. J. Deeg, M. Esposito, M. Fridlund, D. Gandolfi, I. Georgieva, A. Glidden, R. F. Goeke, S. Grziwa, A. P. Hatzes, C. E. Henze, S. B. Howell, J. Irwin, J. M. Jenkins, Eric L.N. Jensen, P. Kábath, R. C. Kidwell Jr., J. F. Kielkopf, E. Knudstrup, K. W. F. Lam, D. W. Latham, J. J. Lissauer, A. W. Mann, E. C. Matthews, I. Mireles, N. Narita, M. Paegert, C. M. Persson, S. Redfield, G. R. Ricker, F. Rodler, J. E. Schlieder, N. J. Scott, S. Seager, J. Šubjak, T. G. Tan, E. B. Ting, R. Vanderspek, V. Van Eylen, J. N. Winn, C. Ziegler
A Planetary System With Two Transiting Mini-Neptunes Near The Radius Valley Transition Around The Bright M Dwarf Toi-776, R. Luque, L. M. Serrano, K. Molaverdikhani, M. C. Nixon, J. H. Livingston, E. W. Guenther, E. Pallé, N. Madhusudhan, G. Nowak, J. Korth, W. D. Cochran, T. Hirano, P. Chaturvedi, E. Goffo, S. Albrecht, O. Barragán, C. Briceño, J. Cabrera, D. Charbonneau, R. Cloutier, K. A. Collins, K. I. Collins, K. D. Colón, J. M. Crossfield, S. Csizmadia, F. Dai, H. J. Deeg, M. Esposito, M. Fridlund, D. Gandolfi, I. Georgieva, A. Glidden, R. F. Goeke, S. Grziwa, A. P. Hatzes, C. E. Henze, S. B. Howell, J. Irwin, J. M. Jenkins, Eric L.N. Jensen, P. Kábath, R. C. Kidwell Jr., J. F. Kielkopf, E. Knudstrup, K. W. F. Lam, D. W. Latham, J. J. Lissauer, A. W. Mann, E. C. Matthews, I. Mireles, N. Narita, M. Paegert, C. M. Persson, S. Redfield, G. R. Ricker, F. Rodler, J. E. Schlieder, N. J. Scott, S. Seager, J. Šubjak, T. G. Tan, E. B. Ting, R. Vanderspek, V. Van Eylen, J. N. Winn, C. Ziegler
Physics & Astronomy Faculty Works
We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8.5 mag, M = 0.54 ± 0.03 M ⊙) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combining the TESS photometry with HARPS radial velocities, as well as ground-based follow-up transit observations from the MEarth and LCOGT telescopes, for the inner planet, TOI-776 b, we measured a period of P b = 8.25 d, a radius of R b = 1.85 ± 0.13 R ⊕, and a mass of M b = 4.0 ± 0.9 …