Browsing by Author "Jenkins, J."

Now showing 1 - 12 of 12
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    An eccentric companion at the edge of the brown dwarf desert orbiting the 2.4 M-circle dot giant star HIP 67537
    (2017) Jones Fernández, Matías Ignacio; Brahm Scott, Rafael; Wittenmyer, R.; Drass, Holger; Jenkins, J.; Melo, C.; Vos, J.; Rojo, P.
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    Fibrin-Targeted Magnetic Resonance Imaging Allows In Vivo Quantification of Thrombus Fibrin Content and Identifies Thrombi Amenable for Thrombolysis
    (2014) Andía Kohnenkampf, Marcelo Edgardo; Saha, P.; Jenkins, J.; Modarai, B.; Wiethoff, A.; Phinikaridou, A.; Grover, S.; Patel, A.
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    Four new planets around giant stars and the mass-metallicity correlation of planet-hosting stars
    (2016) Jones Fernández, Matías Ignacio; Jenkins, J.; Brahm, R.; Wittenmyer, R; Olivares, F.; Melo, C.; Rojo, P.; Jordán Colzani, Andrés Cristóbal; Drass, Holger; Butler, R.; Wang, L.
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    Giant planets around two intermediate-mass evolved stars and confirmation of the planetary nature of HIP 67851c
    (2015) Jones Fernández, Matías Ignacio; Jenkins, J.; Rojo, P.; Olivares, F.; Melo, C.
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    HATS-71b : A Giant Planet Transiting an M3 Dwarf Star in TESS Sector 1
    (2020) Bakos, G. A.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm Scott, Rafael; Csubry, Z.; Espinoza, N.; Hartman, J. D.; Jordán Colzani, Andrés Cristóbal; Rabus, Markus; Henning, T.; Mancini, L.; Penev, K.; Sarkis, P.; Suc, V.; de Val-Borro, M.; Zhou, G.; Butler, R. P.; Crane, J.; Durkan, S.; Shectman, S.; Kim, J.; Lazar, J.; Papp, I.; Sari, P.; Ricker, G.; Vanderspek, R.; Latham, D. W.; Seager, S.; Winn, J. N.; Jenkins, J.; Chacon, A. D.; Furesz, G.; Goeke, B.; Li, J.; Quinn, S.; Quintana, E. V.; Tenenbaum, P.; Teske, J.; Vezie, M.; Yu, L.; Stockdale, C.; Evans, P.; Relles, H. M.
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    HD 207897 b: A dense sub-Neptune transiting a nearby and bright K-type star
    (2022) Heidari, N.; Boisse, I; Orell-Miquel, J.; Hebrard, G.; Acuna, L.; Hara, N. C.; Lillo-Box, J.; Eastman, J. D.; Arnold, L.; Astudillo-Defru, N.; Adibekyan, V; Bieryla, A.; Bonfils, X.; Bouchy, F.; Barclay, T.; Brasseur, C. E.; Borgniet, S.; Bourrier, V; Buchhave, L.; Behmard, A.; Beard, C.; Batalha, N. M.; Courcol, B.; Cortes-Zuleta, P.; Collins, K.; Carmona, A.; Crossfield, I. J. M.; Chontos, A.; Delfosse, X.; Dalal, S.; Deleuil, M.; Demangeon, O. D. S.; Diaz, R. F.; Dumusque, X.; Daylan, T.; Dragomir, D.; Mena, E. Delgado; Dressing, C.; Dai, F.; Dalba, P. A.; Ehrenreich, D.; Forveille, T.; Fulton, B.; Fetherolf, T.; Gaisne, G.; Giacalone, S.; Riazi, N.; Hoyer, S.; Hobson, M. J.; Howard, A. W.; Huber, D.; Hill, M. L.; Hirsch, L. A.; Isaacson, H.; Jenkins, J.; Kane, S. R.; Kiefer, F.; Luque, R.; Latham, D. W.; Lubin, J.; Lopez, T.; Mousis, O.; Moutou, C.; Montagnier, G.; Mignon, L.; Mayo, A.; Mocnik, T.; Murphy, J. M. A.; Palle, E.; Pepe, F.; Petigura, E. A.; Rey, J.; Ricker, G.; Robertson, P.; Roy, A.; Rubenzahl, R. A.; Rosenthal, L. J.; Santerne, A.; Santos, N. C.; Sousa, S. G.; Stassun, K. G.; Stalport, M.; Scarsdale, N.; Strom, P. A.; Seager, S.; Segransan, D.; Tenenbaum, P.; Tronsgaard, R.; Udry, S.; Vanderspek, R.; Vakili, F.; Winn, J.; Weiss, L. M.
    We present the discovery and characterization of a transiting sub-Neptune that orbits the nearby (28 pc) and bright (V = 8.37) K0V star HD 207897 (TOI-1611) with a 16.20-day period. This discovery is based on photometric measurements from the Transiting Exoplanet Survey Satellite mission and radial velocity (RV) observations from the SOPHIE, Automated Planet Finder, and HIRES high-precision spectrographs. We used EXOFASTv2 to model the parameters of the planet and its host star simultaneously, combining photometric and RV data to determine the planetary system parameters. We show that the planet has a radius of 2.50 +/- 0.08 R-E and a mass of either 14.4 +/- 1.6 M-E or 15.9 +/- 1.6 M-E with nearly equal probability. The two solutions correspond to two possibilities for the stellar activity period. The density accordingly is either 5.1 +/- 0.7 g cm(-3) or 5.5(-0.7)(+0.8) g cm(-3), making it one of the relatively rare dense sub-Neptunes. The existence of this dense planet at only 0.12 AU from its host star is unusual in the currently observed sub-Neptune (2 < R-E < 4) population. The most likely scenario is that this planet has migrated to its current position.
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    New planetary systems from the Calan-Hertfordshire Extrasolar Planet Search
    (2017) Jenkins, J.; Jones, H.; Tuomi, M.; Díaz, Marco A.; Cordero, J.; Aguayo, A.; Pantoja, B.; Arriagada, P.; Brahm Scott, Rafael; Jones Fernández, Matías Ignacio; Mahu, R.; Rojo, P.; Soto, M.; Ivanyuk O.; Becerra Yoma N.; Day-Jones A.; Ruiz M.; Pavlenko Y.; Barnes J.; Murgas F.; Pinfield, D.; López-Morales, M.
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    New spectroscopic binary companions of giant stars and updated metallicity distribution for binary systems
    (2016) Bluhm, P.; Jones Fernández, Matías Ignacio; Vanzi, Leonardo; Soto, M.; Voss, J.; Wittenmyer, R.; Drass, Holger; Jenkins, J.; Olivares, F.; Mennickent, R.; Vuckovic, M.; Rojo, P.; Melo, C.
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    Pan genome of the phytoplankton Emiliania underpins its global distribution
    (2013) Read, Betsy A.; Kegel, Jessica; Klute, Mary J.; Kuo, Alan; Lefebvre, Stephane C.; Maumus, Florian; Mayer, Christoph; Miller, John; Monier, Adam; Salamov, Asaf; Young, Jeremy; Aguilar, Maria; Claverie, Jean-Michel; Frickenhaus, Stephan; Gonzalez, Karina; Herman, Emily K.; Lin, Yao-Cheng; Napier, Johnathan; Ogata, Hiroyuki; Sarno, Analissa F.; Shmutz, Jeremy; Schroeder, Declan; de Vargas, Colomban; Verret, Frederic; von Dassow, Peter; Valentin, Klaus; Van de Peer, Yves; Wheeler, Glen; Dacks, Joel B.; Delwiche, Charles F.; Dyhrman, Sonya T.; Gloeckner, Gernot; John, Uwe; Richards, Thomas; Worden, Alexandra Z.; Zhang, Xiaoyu; Grigoriev, Igor V.; Allen, Andrew E.; Bidle, Kay; Borodovsky, M.; Bowler, C.; Brownlee, Colin; Cock, J. Mark; Elias, Marek; Gladyshev, Vadim N.; Groth, Marco; Guda, Chittibabu; Hadaegh, Ahmad; Iglesias-Rodriguez, Maria Debora; Jenkins, J.; Jones, Bethan M.; Lawson, Tracy; Leese, Florian; Lindquist, Erika; Lobanov, Alexei; Lomsadze, Alexandre; Malik, Shehre-Banoo; Marsh, Mary E.; Mackinder, Luke; Mock, Thomas; Mueller-Roeber, Bernd; Pagarete, Antonio; Parker, Micaela; Probert, Ian; Quesneville, Hadi; Raines, Christine; Rensing, Stefan A.; Riano-Pachon, Diego Mauricio; Richier, Sophie; Rokitta, Sebastian; Shiraiwa, Yoshihiro; Soanes, Darren M.; van der Giezen, Mark; Wahlund, Thomas M.; Williams, Bryony; Wilson, Willie; Wolfe, Gordon; Wurch, Louie L.
    Coccolithophores have influenced the global climate for over 200 million years(1). These marine phytoplankton can account for 20 per cent of total carbon fixation in some systems(2). They form blooms that can occupy hundreds of thousands of square kilometres and are distinguished by their elegantly sculpted calcium carbonate exoskeletons (coccoliths), rendering them visible from space(3). Although coccolithophores export carbon in the form of organic matter and calcite to the sea floor, they also release CO2 in the calcification process. Hence, they have a complex influence on the carbon cycle, driving either CO2 production or uptake, sequestration and export to the deep ocean(4). Here we report the first haptophyte reference genome, from the coccolithophore Emiliania huxleyi strain CCMP1516, and sequences from 13 additional isolates. Our analyses reveal a pan genome (core genes plus genes distributed variably between strains) probably supported by an atypical complement of repetitive sequence in the genome. Comparisons across strains demonstrate that E. huxleyi, which has long been considered a single species, harbours extensive genome variability reflected in different metabolic repertoires. Genome variability within this species complex seems to underpin its capacity both to thrive in habitats ranging from the equator to the subarctic and to form large-scale episodic blooms under a wide variety of environmental conditions.
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    Precision radial velocities of 15 M5-M9 dwarfs
    (2014) Barnes, J.; Jenkins, J.; Jones, H.; Jeffers, S.; Rojo, P.; Arriagada, P.; Jordán Colzani, Andrés Cristóbal; Minniti, D.
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    THE. PAN-PACIFIC. PLANET. SEARCH. IV. TWO. SUPER-JUPITERS. IN. A. 3:5 RESONANCE. ORBITING. THE. GIANT. STAR. HD. 33844
    (2016) Wittenmyer, R.; Johnson, J.; Butler, R.; Horner, J.; Wang, L.; Robertson, P.; Jones Fernández, Matías Ignacio; Jenkins, J.; Brahm, R.; Tinney, C.; Mengel, M.; Clark, J.
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    TOI-150b and TOI-163b : two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ
    (2019) Kossakowski, D.; Espinoza, N.; Brahm Scott, Rafael; Jordán Colzani, Andrés Cristóbal; Henning, T.; Rojas, F.; Kurster, M.; Sarkis, P.; Schlecker, M.; Pozuelos, F. J.; Barkaoui, K.; Jehin, E.; Gillon, M.; Matthews, E.; Horch, E. P.; Ciardi, D. R.; Rossfield, I. J. M.; Gonzales, E.; Howell, S. B.; Matson, R.; Schlieder, J.; Jenkins, J.; Ricker, G.; Seager, S.; Winn, J. N.; Li, J.; Rose, M. E.; Smith, J. C.; Dynes, S.; Morgan, E.; Villaseñor, J. N.; Charbonneau, D.; Jaffe, T.; Yu, L.; Bakos, G.; Bhatti, W.; Bouchy, F.; Collins, K. A.; Collins, K. I.; Csubry, Z.; Evans, P.; Jensen, E. L. N.; Lovis, C.; Marmier, M.; Nielsen, L. D.; Osip, D.; Pepe, F.; Relles, H. M.; Segransan, D.; Shporer, A.; Stockdale, C.; Suc, V.; Turner, O.; Udry, S.