Zobrazeno 1 - 10 of 60 pro vyhledávání: '"Fortney JJ"'
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The JWST Early-release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 μm Spectrum of the Planetary-mass Companion VHS 1256-1257 b
Autor: Miles, BE, Biller, BA, Patapis, P, Worthen, K, Rickman, E, Hoch, KKW, Skemer, A, Perrin, MD, Whiteford, N, Chen, CH, Sargent, B, Mukherjee, S, Morley, CV, Moran, SE, Bonnefoy, M, Petrus, S, Carter, AL, Choquet, E, Hinkley, S, Ward-Duong, K, Leisenring, JM, Millar-Blanchaer, MA, Pueyo, L, Ray, S, Sallum, S, Stapelfeldt, KR, Stone, JM, Wang, JJ, Absil, O, Balmer, WO, Boccaletti, A, Bonavita, M, Booth, M, Bowler, BP, Chauvin, G, Christiaens, V, Currie, T, Danielski, C, Fortney, JJ, Girard, JH, Grady, CA, Greenbaum, AZ, Henning, T, Hines, DC, Janson, M, Kalas, P, Kammerer, J, Kennedy, GM, Kenworthy, MA, Kervella, P, Lagage, PO, Lew, BWP, Liu, MC, Macintosh, B, Marino, S, Marley, MS, Marois, C, Matthews, EC, Matthews, BC, Mawet, D, McElwain, MW, Metchev, S, Meyer, MR, Molliere, P, Pantin, E, Quirrenbach, A, Rebollido, I, Ren, BB, Schneider, G, Vasist, M, Wyatt, MC, Zhou, Y, Briesemeister, ZW, Bryan, ML, Calissendorff, P, Cantalloube, F, Cugno, G, De Furio, M, Dupuy, TJ, Factor, SM, Faherty, JK, Fitzgerald, MP, Franson, K, Gonzales, EC, Hood, CE, Howe, AR, Kraus, AL, Kuzuhara, M, Lagrange, AM, Lawson, K, Lazzoni, C, Liu, P, Llop-Sayson, J, Lloyd, JP, Martinez, RA, Mazoyer, J, Quanz, SP, Redai, JA, Samland, M, Schlieder, JE
We present the highest fidelity spectrum to date of a planetary-mass object. VHS 1256 b is a M Jup widely separated (∼8″, a = 150 au), young, planetary-mass companion that shares photometric colors and spectroscopic features with the directly ima
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::209474dbf87b7c226483f5fb8f578585
https://www.repository.cam.ac.uk/handle/1810/347876
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The transiting exoplanet community early release science program for JWST
Autor: Bean, JL, Stevenson, KB, Batalha, NM, Berta-Thompson, Z, Kreidberg, L, Crouzet, N, Benneke, B, Line, MR, Sing, DK, Wakeford, HR, Knutson, HA, Kempton, EMR, Désert, JM, Crossfield, I, Batalha, NE, De Wit, J, Parmentier, V, Harrington, J, Moses, JI, Lopez-Morales, M, Alam, MK, Blecic, J, Bruno, G, Carter, AL, Chapman, JW, Decin, L, Dragomir, D, Evans, TM, Fortney, JJ, Fraine, JD, Gao, P, Muñoz, AG, Gibson, NP, Goyal, JM, Heng, K, Hu, R, Kendrew, S, Kilpatrick, BM, Krick, J, Lagage, PO, Lendl, M, Louden, T, Madhusudhan, N, Mandell, AM, Mansfield, M, May, EM, Morello, G, Morley, CV, Nikolov, N, Redfield, S, Roberts, JE, Schlawin, E, Spake, JJ, Todorov, KO, Tsiaras, A, Venot, O, Waalkes, WC, Wheatley, PJ, Zellem, RT, Angerhausen, D, Barrado, D, Carone, L, Casewell, SL, Cubillos, PE, Damiano, M, Borro, MDV, Drummond, B, Edwards, B, Endl, M, Espinoza, N, France, K, Gizis, JE, Greene, TP, Henning, TK, Hong, Y, Ingalls, JG, Iro, N, Irwin, PGJ, Kataria, T, Lahuis, F, Leconte, J, Lillo-Box, J, Lines, S, Lothringer, JD, Mancini, L, Marchis, F, Mayne, N, Palle, E, Rauscher, E, Roudier, G, Shkolnik, EL, Southworth, J, Swain, MR, Taylor, J, Teske, J, Tinetti, G, Tremblin, P, Tucker, GS, Boekel, RV, Waldmann, IP
The James Webb Space Telescope (JWST) presents the opportunity to transform our understanding of planets and the origins of life by revealing the atmospheric compositions, structures, and dynamics of transiting exoplanets in unprecedented detail. How
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::419c9125f068fd373340cd15f98cbeed
https://www.repository.cam.ac.uk/handle/1810/316352
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Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager
Autor: Macintosh, B, Graham, JR, Barman, T, De Rosa, RJ, Konopacky, Q, Marley, MS, Marois, C, Nielsen, EL, Pueyo, L, Rajan, A, Rameau, J, Saumon, D, Wang, JJ, Patience, J, Ammons, M, Arriaga, P, Artigau, E, Beckwith, S, Brewster, J, Bruzzone, S, Bulger, J, Burningham, B, Burrows, AS, Chen, C, Chiang, E, Chilcote, JK, Dawson, RI, Dong, R, Doyon, R, Draper, ZH, Duchêne, G, Esposito, TM, Fabrycky, D, Fitzgerald, MP, Follette, KB, Fortney, JJ, Gerard, B, Goodsell, S, Greenbaum, AZ, Hibon, P, Hinkley, S, Cotton, TH, Hung, LW, Ingraham, P, Johnson-Groh, M, Kalas, P, Lafreniere, D, Larkin, JE, Lee, J, Line, M, Long, D, Maire, J, Marchis, F, Matthews, BC, Max, CE, Metchev, S, Millar-Blanchaer, MA, Mittal, T, Morley, CV, Morzinski, KM, Murray-Clay, R, Oppenheimer, R, Palmer, DW, Patel, R, Perrin, MD, Poyneer, LA, Rafikov, RR, Rantakyrö, FT, Rice, EL, Rojo, P, Rudy, AR, Ruffio, JB, Ruiz, MT, Sadakuni, N, Saddlemyer, L, Salama, M, Savransky, D, Schneider, AC, Sivaramakrishnan, A, Song, I, Soummer, R, Thomas, S, Vasisht, G
Publikováno v: Macintosh, B; Graham, JR; Barman, T; De Rosa, RJ; Konopacky, Q; Marley, MS; et al.(2015). Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager. Science, 350(6256), 64-67. doi: 10.1126/science.aac5891. UCLA: Retrieved from: http://www.escholarship.org/uc/item/5rg522fk
Directly detecting thermal emission from young extrasolar planets allows measurement of their atmospheric compositions and luminosities, which are influenced by their formation mechanisms. Using the Gemini Planet Imager, we discovered a planet orbiti
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od_______325::410add22b0dad023b77946cf0623e63c
http://www.escholarship.org/uc/item/5rg522fk
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3.6 AND 4.5 μm PHASE CURVES OF THE HIGHLY IRRADIATED ECCENTRIC HOT JUPITER WASP-14b
Autor: Wong, I, Knutson, HA, Lewis, NK, Kataria, T, Burrows, A, Fortney, JJ, Schwartz, J, Agol, E, Cowan, NB, Deming, D, Désert, JM, Fulton, BJ, Howard, AW, Langton, J, Laughlin, G, Showman, AP, Todorov, K
Publikováno v: The Astrophysical Journal, vol 811, iss 2
Astrophysical Journal, vol 811, iss 2
Wong, I; Knutson, HA; Lewis, NK; Kataria, T; Burrows, A; Fortney, JJ; et al.(2015). 3.6 and 4.5 μm PHASE CURVES of the HIGHLY IRRADIATED ECCENTRIC HOT JUPITER WASP-14b. Astrophysical Journal, 811(2). doi: 10.1088/0004-637X/811/2/122. UC Santa Cruz: Retrieved from: http://www.escholarship.org/uc/item/35s7v6mg
© 2015. The American Astronomical Society. All rights reserved.. We present full-orbit phase curve observations of the eccentric (e ∼ 0.08) transiting hot Jupiter WASP-14b obtained in the 3.6 and 4.5 μm bands using the Spitzer Space Telescope. We
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::75a0edf8478483ce32dd4bd19b358653
https://escholarship.org/uc/item/35s7v6mg
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The LEECH Exoplanet Imaging Survey. Further constraints on the planet architecture of the HR 8799 system (vol 576, pg A133, 2015)
Autor: Maire, A-L, Skemer, AJ, Hinz, PM, Desidera, S, Esposito, S, Gratton, R, Marzari, F, Skrutskie, MF, Biller, BA, Defrere, D, Bailey, VP, Leisenring, JM, Apai, D, Bonnefoy, M, Brandner, W, Buenzli, E, Claudi, RU, Close, LM, Crepp, JR, De Rosa, RJ, Eisner, JA, Fortney, JJ, Henning, T, Hofmann, K-H, Kopytova, TG, Males, JR, Mesa, D, Morzinski, KM, Oza, A, Patience, J, Pinna, E, Rajan, A, Schertl, D, Schlieder, JE, Su, KYL, Vaz, A, Ward-Duong, K, Weigelt, G, Woodward, CE
Publikováno v: ASTRONOMY & ASTROPHYSICS, vol 579
Maire, A-L; Skemer, AJ; Hinz, PM; Desidera, S; Esposito, S; Gratton, R; et al.(2015). The LEECH Exoplanet Imaging Survey. Further constraints on the planet architecture of the HR 8799 system (vol 576, pg A133, 2015). ASTRONOMY & ASTROPHYSICS, 579. doi: 10.1051/0004-6361/201425185e. UC Santa Cruz: Retrieved from: http://www.escholarship.org/uc/item/9tq0m0n8
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::05d3c151ae6da59d6f4dbb63980ef55f
https://escholarship.org/uc/item/9tq0m0n8
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Low False Positive Rate of Kepler Candidates Estimated From A Combination Of Spitzer And Follow-Up Observations
Autor: Désert, JM, Charbonneau, D, Torres, G, Fressin, F, Ballard, S, Bryson, ST, Knutson, HA, Batalha, NM, Borucki, WJ, Brown, TM, Deming, D, Ford, EB, Fortney, JJ, Gilliland, RL, Latham, DW, Seager, S
Publikováno v: The Astrophysical Journal, vol 804, iss 1
Désert, JM; Charbonneau, D; Torres, G; Fressin, F; Ballard, S; Bryson, ST; et al.(2015). Low false positive rate of kepler candidates estimated from a combination of spitzer and follow-up observations. Astrophysical Journal, 804(1). doi: 10.1088/0004-637X/804/1/59. UC Santa Cruz: Retrieved from: http://www.escholarship.org/uc/item/4c70v4mf
Astrophysical Journal, vol 804, iss 1
© 2015. The American Astronomical Society. All rights reserved.. NASA's Kepler mission has provided several thousand transiting planet candidates during the 4 yr of its nominal mission, yet only a small subset of these candidates have been confirmed
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::185b500c56e3d2aeacdd53fd39284641
https://resolver.caltech.edu/CaltechAUTHORS:20150605-135723176
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