Zobrazeno 1 - 10
of 55
pro vyhledávání: '"Kennedy, GM"'
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
https://www.repository.cam.ac.uk/handle/1810/347876
Autor:
Lovell, JB, Marino, S, Wyatt, MC, Kennedy, GM, MacGregor, MA, Stapelfeldt, K, Dent, B, Krist, J, Matrà, L, Kral, Q, Panić, O, Pearce, TD, Wilner, D
We present Atacama Large Millimetre/sub-Millimetre Array (ALMA) 1.3 and 0.86 mm observations of the nearby (17.34 pc) F9V star q1 Eri (HD 10647, HR 506). This system, with age ∼1.4 Gyr, hosts a ∼2 au radial velocity planet and a debris disc with
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::7ac4b349d606a62497d78644240762a9
https://eprints.whiterose.ac.uk/179294/1/Lovell.pdf
https://eprints.whiterose.ac.uk/179294/1/Lovell.pdf
Autor:
Lovell, JB, Wyatt, MC, Ansdell, M, Kama, M, Kennedy, GM, Manara, CF, Marino, S, Matrà, L, Rosotti, G, Tazzari, M, Testi, L, Williams, JP
Class III stars are those in star forming regions without large non-photospheric infrared emission, suggesting recent dispersal of their protoplanetary discs. We observed 30 class III stars in the 1–3 Myr Lupus region with ALMA at ∼856μm, result
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be2234468bdc4b89575470c1c966d810
Autor:
Stone, J. M., Ertel, S, Defrere, D, Hinz, P, Mennesson, B, Kennedy, GM, Danchi, WC, Gelino, C, Hill, JM, Hoffmann, WF, Mazoyer, J, Rieke, G, Shannon, A, Stapelfeldt, K, Spalding, E, Stone, JM, Vaz, A, Weinberger, AJ, Willems, P, Absil, O, Arbo, P, Bailey, VP, Beichman, C, Bryden, G, Downey, EC, Durney, O, Esposito, S, Gaspar, A, Grenz, P, Haniff, CA, Leisenring, JM, Marion, L, McMahon, TJ, Millan-Gabet, R, Montoya, M, Morzinski, KM, Perera, S, Pinna, E, Pott, JU, Power, J, Puglisi, A, Roberge, A, Serabyn, E, Skemer, AJ, Su, KYL, Vaitheeswaran, V, Wyatt, MC
The Large Binocular Telescope Interferometer (LBTI) enables nulling interferometric observations across the N band (8 to 13 um) to suppress a star's bright light and probe for faint circumstellar emission. We present and statistically analyze the res
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dad15c77b9491dc7d431a6d73a9b2b1f
Autor:
Boyajian, TS, Alonso, R, Ammerman, A, Armstrong, D, Ramos, AA, Barkaoui, K, Beatty, TG, Benkhaldoun, Z, Benni, P, Bentley, RO, Berdyugin, A, Berdyugina, S, Bergeron, S, Bieryla, A, Blain, MG, Blanco, AC, Bodman, EHL, Boucher, A, Bradley, M, Brincat, SM, Brink, TG, Briol, J, Brown, DJA, Budaj, J, Burdanov, A, Cale, B, Carbo, MA, Garcia, RC, Clark, WJ, Clayton, GC, Clem, JL, Coker, PH, Cook, EM, Copperwheat, CM, Curtis, JL, Cutri, RM, Cseh, B, Cynamon, CH, Daniels, AJ, Davenport, JRA, Deeg, HJ, Lorenzo, RD, Jaeger, TD, Desrosiers, JB, Dolan, J, Dowhos, DJ, Dubois, F, Durkee, R, Dvorak, S, Easley, L, Edwards, N, Ellis, TG, Erdelyi, E, Ertel, S, Farfán, RG, Farihi, J, Filippenko, AV, Foxell, E, Gandolfi, D, Garcia, F, Giddens, F, Gillon, M, González-Carballo, JL, González-Fernández, C, Hernández, JIG, Graham, KA, Greene, KA, Gregorio, J, Hallakoun, N, Hanyecz, O, Harp, GR, Henry, GW, Herrero, E, Hildbold, CF, Hinzel, D, Holgado, G, Ignácz, B, Ilyin, I, Ivanov, VD, Jehin, E, Jermak, HE, Johnston, S, Kafka, S, Kalup, C, Kardasis, E, Kaspi, S, Kennedy, GM, Kiefer, F, Kielty, CL, Kessler, D, Kiiskinen, H, Killestein, TL, King, RA, Kollar, V, Korhonen, H, Kotnik, C, Könyves-Tóth, R, Kriskovics, L, Krumm, N, Krushinsky, V
We present a photometric detection of the first brightness dips of the unique variable star KIC 8462852 since the end of the Kepler space mission in 2013 May. Our regular photometric surveillance started in October 2015, and a sequence of dipping beg
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a3527c3026058ba0ce9a387b74912d43
https://www.repository.cam.ac.uk/handle/1810/273962
https://www.repository.cam.ac.uk/handle/1810/273962
Resolved observations of millimetre-sized dust, tracing larger planetesimals, have pinpointed the location of 26 Edgeworth-Kuiper belt analogs. We report that a belt's distance $R$ to its host star correlates with the star's luminosity $L_{\star}$, f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e92ef483d16cc43e18095d51320545af
https://www.repository.cam.ac.uk/handle/1810/278184
https://www.repository.cam.ac.uk/handle/1810/278184
Autor:
Kennedy, GM, Matrà, L, Facchini, S, Milli, J, Panić, O, Price, D, Wilner, DJ, Wyatt, MC, Yelverton, BM
Nearly all young stars are initially surrounded by ‘protoplanetary’ disks of gas and dust, and in the case of single stars at least 30% of these disks go on to form planets1. The process of protoplanetary disk formation can result in initial misa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::dc7afc281b8ae583eff29ff9aa0bec8b
https://eprints.whiterose.ac.uk/154449/1/1901.05018.pdf
https://eprints.whiterose.ac.uk/154449/1/1901.05018.pdf
Autor:
Matra, L, MacGregor, MA, Kalas, P, Wyatt, MC, Kennedy, GM, Wilner, DJ, Duchene, G, Hughes, AM, Pan, M, Shannon, A, Clampin, M, Fitzgerald, MP, Graham, JR, Holland, WS, Panić, O, Su, KYL
Recent ALMA observations present mounting evidence for the presence of exocometary gas released within Kuiper belt analogues around nearby main sequence stars. This represents a unique opportunity to study their ice reservoir at the younger ages when
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______109::854f5ed305bf131ac25e41a1734cb0d1
https://www.repository.cam.ac.uk/handle/1810/269756
https://www.repository.cam.ac.uk/handle/1810/269756
Autor:
Matrà, L, MacGregor, MA, Kalas, P, Wyatt, MC, Kennedy, GM, Wilner, DJ, Duchene, G, Hughes, AM, Pan, M, Shannon, A, Clampin, M, Fitzgerald, MP, Graham, JR, Holland, WS, Panić, O, Su, KYL
Recent Atacama Large Millimeter/submillimeter Array observations present mounting evidence for the presence of exocometary gas released within Kuiper Belt analogs around nearby main-sequence stars. This represents a unique opportunity to study their
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::7e59d16a6bd0b2abc6097774d8f41c8f
https://eprints.whiterose.ac.uk/127813/1/Fom2_paper.pdf
https://eprints.whiterose.ac.uk/127813/1/Fom2_paper.pdf
A decade of surveys has hinted at a possible higher occurrence rate of debris discs in systems hosting low mass planets. This could be due to common favourable forming conditions for rocky planets close in and planetesimals at large radii. In this pa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______109::0835cbe1f2ffeabb41543ee6c61687d0
https://www.repository.cam.ac.uk/handle/1810/265840
https://www.repository.cam.ac.uk/handle/1810/265840