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pro vyhledávání: '"Clarke, F"'
Autor:
Pereira-Santaella, M., Rigopoulou, D., Magdis, G. E., Thatte, N., Alonso-Herrero, A., Clarke, F., Farrah, D., García-Burillo, S., Hogan, L., Morris, S., Rodrigues, M., Huang, J. -S., Tecza, M.
The extreme infrared (IR) luminosity of local luminous and ultra-luminous IR galaxies (U/LIRGs; 11 < log LIR /Lsun < 12 and log LIR /Lsun > 12, respectively) is mainly powered by star-formation processes triggered by mergers or interactions. While U/
Externí odkaz:
http://arxiv.org/abs/1904.13267
Akademický článek
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Autor:
Neichel, B., Fusco, T., Sauvage, J. -F., Correia, C., Dohlen, K., El-Hadi, K., Blanco, L., Schwartz, N., Clarke, F., Thatte, N., Tecza, M., Paufique, J., Vernet, J., Louarn, M. Le, Hammersley, P., Gach, J. -L., Pascal, S., Vola, P., Petit, C., Conan, J. -M., Carlotti, A., Verinaud, C., Schnetler, H., Bryson, I., Morris, T., Myers, R., Hugot, E., Gallie, A.
HARMONI is a visible and NIR integral field spectrograph, providing the E-ELT's core spectroscopic capability at first light. HARMONI will work at the diffraction limit of the E-ELT, thanks to a Classical and a Laser Tomographic AO system. In this pa
Externí odkaz:
http://arxiv.org/abs/1805.11931
Autor:
Bowles, N. E., Snodgrass, C., Gibbings, A, Sanchez, J. P., Arnold, J. A., Eccleston, P., Andert, T., Probst, A., Naletto, G., Vandaele, A. C., de Leon, J., Nathues, A., Thomas, I. R., Thomas, N., Jorda, L., Da Deppo, V., Haack, H., Green, S. F., Carry, B., Hanna, K. L. Donaldson, Jorgensen, J. Leif, Kereszturi, A., DeMeo, F. E., Patel, M. R., Davies, J. K., Clarke, F., Kinch, K., Guilbert-Lepoutre, A., Agarwal, J., Rivkin, A. S., Pravec, P., Fornasier, S., Granvik, M., Jones, R. H., Murdoch, N., Joy, K. H., Pascale, E., Tecza, M., Barnes, J. M., Licandro, J., Greenhagen, B. T., Calcutt, S. B., Marriner, C. M., Warren, T., Tosh, I.
CASTAway is a mission concept to explore our Solar System's main asteroid belt. Asteroids and comets provide a window into the formation and evolution of our Solar System and the composition of these objects can be inferred from space-based remote se
Externí odkaz:
http://arxiv.org/abs/1710.10191
Autor:
Kendrew, S., Zieleniewski, S., Houghton, R. C. W., Thatte, N., Devriendt, J., Tecza, M., Clarke, F., O'Brien, K., Häussler, B.
We present a study into the capabilities of integrated and spatially resolved integral field spectroscopy of galaxies at z=2-4 with the future HARMONI spectrograph for the European Extremely Large Telescope (E-ELT) using the simulation pipeline, HSIM
Externí odkaz:
http://arxiv.org/abs/1602.06983
Autor:
Zieleniewski, S., Thatte, N., Kendrew, S., Houghton, R. C. W., Swinbank, A. M., Tecza, M., Clarke, F., Fusco, T.
We present HSIM: a dedicated pipeline for simulating observations with the HARMONI integral field spectrograph on the European Extremely Large Telescope. HSIM takes high spectral and spatial resolution input data-cubes, encoding physical descriptions
Externí odkaz:
http://arxiv.org/abs/1508.04441
Autor:
Clarke, F.
Chapter one provides a brief overview of the physics of ultra cool dwarfs, and discusses relevant observation to date. Of particular import is an understanding of their atmospheric physics. The cool temperatures (2500K) of their atmospheres are condu
Externí odkaz:
http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.597743
Autor:
Houghton, R. C. W., Davies, Roger L., D'Eugenio, F., Scott, N., Thatte, N., Clarke, F., Tecza, M., Salter, G. S., Fogarty, L. M. R., Goodsall, T.
We present integral-field spectroscopy of 27 galaxies in the Coma cluster observed with the Oxford SWIFT spectrograph, exploring the kinematic morphology-density relationship in a cluster environment richer and denser than any in the ATLAS3D survey.
Externí odkaz:
http://arxiv.org/abs/1308.6581