Zobrazeno 1 - 10
of 37
pro vyhledávání: '"J. M. Herreros"'
Autor:
A. Wahbi, A. Tsolakis, J. M. Herreros, S. Zeraati-Rezaei, O. Doustdar, P. J. Millington, A. Raj
Publikováno v:
Johnson Matthey Technology Review. 67:171-185
The main challenges of compressed natural gas (CNG) engine fuelling in terms of methane abatement in the aftertreatment system are addressed in this study using differently loaded platinum group metal (pgm) catalysts. A dual-fuel injection strategy o
Autor:
G. Brinklow, J. M. Herreros, S. Zeraati Rezaei, O. Doustdar, A. Tsolakis, A. Kolpin, P. Millington
Publikováno v:
International Journal of Environmental Science and Technology.
Transport sector decarbonisation is leading to increased demand for electrified powertrains including hybrid vehicles. The presence of an internal combustion engine and electric motor offer multiple performance and efficiency advantages. However, cha
Autor:
A. Bueno, J. Sánchez-Capuchino, Fraser Clarke, Matthias Tecza, I. Bryson, Niranjan Thatte, Elvio Hernández, J. M. Herreros
Publikováno v:
SPIE Proceedings.
HARMONI is a visible and near-infrared (0.47μm to 2.5μm) integral field spectrometer providing the E-ELT's core spectroscopic capability. It will provide ~32000 simultaneous spectra of a rectangular field of view at four foreseen different spatial
Autor:
Pere L. Palle, G. Grec, N. Pétrou, Joergen Christensen-Dalsgaard, M. Charra, T. Foglizzo, C. Régulo, T. Roca Cortés, J. M. Herreros, F. Baudin, M. Lazrek, Roger K. Ulrich, J. M. Robillot, Eric Fossat, Luca Bertello, H. Dzitko, M. Decaudin, A. H. Gabriel, Sarbani Basu, Rafael A. García, C. Renaud, Patrick Boumier, J. Charra, Sylvaine Turck-Chièze
Publikováno v:
Solar Physics. 175:207-226
GOLF in-flight commissioning and calibration was carried out during the first four months, most of which represented the cruise phase of SOHO towards its final LI orbit. The initial performance of GOLF is shown to be within the design specification,
Autor:
J. L. Cano de Diego, E. Blackhurst, Jose Alberto Rubino-Martin, Angel Mediavilla, Keith Grainge, F. Gómez-Reñasco, Michael P. Hobson, Rubén Sanquirce, Bruno Maffei, Alberto Vizcargüenaga, Gaizka Murga, Mark McCulloch, P. Vielva, J. M. Herreros, Beatriz Aja, Clive Dickinson, G. A. Herrera, D. Herran, R. J. Davis, R. B. Barreiro, M. López-Caniego, B. E. Arriaga, Enrique Villa, Rafael Rebolo-López, Ricardo Génova-Santos, R. Fernandez-Cobos, F. J. Casas, J. Luis Ruiz, Alicia Gomez, V. Sanchez de la Rosa, M. Aguiar-González, Eduardo Artal, Simon J. Melhuish, Stuart Harper, David Gómez Ortiz, Anthony Lasenby, Carlos H. López-Caraballo, E. Martínez-González, T. Viera-Curbelo, Roger J. Hoyland, Javier Ariño, L. de la Fuente, Giampaolo Pisano, C. Gomez, Lucio Piccirillo, Robert A. Watson, A. Vega-Moreno, J. Cagigas
Publikováno v:
Proceedings of SPIE, 2012, 8452, 845233
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI, Amsterdam, 2012
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
University of Manchester-PURE
Digital.CSIC. Repositorio Institucional del CSIC
instname
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VI, Amsterdam, 2012
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
University of Manchester-PURE
Digital.CSIC. Repositorio Institucional del CSIC
instname
Trabajo presentado a la conferencia: "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IV" (Poster session) celebrada en Amsterdam (Holanda) el 1 de julio de 2012.-- et al.
The QUIJOTE-CMB project has been
The QUIJOTE-CMB project has been
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::311e8df3d85c50eba65ff81e233f3069
http://hdl.handle.net/10261/109140
http://hdl.handle.net/10261/109140
Autor:
Lucio Piccirillo, Jose M. Diego, Bruno Maffei, M. Aguiar, Enrique Martinez-Gonzalez, R. D. Davies, Robert A. Watson, T. Viera-Curbelo, Juan Luis Cano, J. V. Terán, Simon J. Melhuish, Anthony Lasenby, Roger J. Hoyland, Richard D. E. Saunders, Michael L. Brown, A. E. Pelaez Santos, E. Blackhurst, Mark McCulloch, J. M. Herreros, Richard A. Battye, R. Fernandez-Cobos, Ricardo Génova-Santos, Beatriz Aja, L. de la Fuente, F. Gómez-Reñasco, V. Sanchez de la Rosa, R. J. Davis, David Ortiz, Angel Mediavilla, Giampaolo Pisano, Carlos H. López-Caraballo, D. Herranz, Clive Dickinson, Simon Harper, Rafael Rebolo, Keith Grainge, R. B. Barreiro, Paul F. Scott, Eduardo Artal, F. J. Casas, Michael P. Hobson, P. Vielva, Jose Alberto Rubino-Martin, M. López-Caniego, Enrique Villa, A. Vega-Moreno, J. Cagigas
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Proceedings of SPIE, 2012, 8444, 84442Y
Ground-based and Airborne Telescopes IV, Amsterdam, 2012
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
University of Manchester-PURE
instname
Proceedings of SPIE, 2012, 8444, 84442Y
Ground-based and Airborne Telescopes IV, Amsterdam, 2012
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
University of Manchester-PURE
Trabajo presentado a la conferencia: "Ground-based and Airborne Telescopes IV" (Poster session: Concepts for future telescopes) celebrada en Amsterdam (Holanda) el 1 de julio de 2012.-- et al.
The QUIJOTE (Q-U-I JOint Tenerife) CMB Experiment wi
The QUIJOTE (Q-U-I JOint Tenerife) CMB Experiment wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fea7a37f0ca451149248d645ea88df5b
http://hdl.handle.net/10261/109135
http://hdl.handle.net/10261/109135
Autor:
Nuno C. Santos, C. Lovis, Rafael Rebolo, Denis Mégevand, P. Di Marcantonio, A. Cabral, Francesco Pepe, Filippo Maria Zerbi, Stefano Cristiani, J. M. Herreros, Paolo Spanò
Publikováno v:
SPIE Proceedings.
ESPRESSO, a very high-resolution, high-efficiency, ultra-high stability, fiber-fed, cross-dispersed echelle spectrograph located in the Combined-Coude focus of the VLT, has been designed to detect exo-planets with unprecedented radial velocity accura
Autor:
Paolo Di Marcantonio, Filippo Maria Zerbi, Gerardo Avila, Nuno C. Santos, André Moitinho, António Amorim, Francesco Pepe, J. M. Herreros, Alexandre Cabral, João Coelho, Stefano Cristiani, Jorge Lima, Pedro Carvas, Rafael Rebolo, Denis Mégevand, José Manuel Rebordão, Christophe Lovis
Publikováno v:
SPIE Proceedings.
The first purpose of ESPRESSO is to develop a competitive, innovative high-resolution spectrograph to fully exploit the potentiality of the Very Large Telescope (VLT) of the European Southern Observatory and to allow new science. It is thus important
Autor:
M. Bersanelli, N. Mandolesi, R. C. Butler, A. Mennella, F. Villa, B. Aja, E. Artal, E. Artina, C. Baccigalupi, M. Balasini, G. Baldan, A. Banday, P. Bastia, P. Battaglia, T. Bernardino, E. Blackhurst, L. Boschini, C. Burigana, G. Cafagna, B. Cappellini, F. Cavaliere, F. Colombo, G. Crone, F. Cuttaia, O. D'Arcangelo, L. Danese, R. D. Davies, R. J. Davis, L. De Angelis, G. C. De Gasperis, L. De La Fuente, A. De Rosa, G. De Zotti, M. C. Falvella, F. Ferrari, R. Ferretti, L. Figini, S. Fogliani, C. Franceschet, E. Franceschi, T. Gaier, S. Garavaglia, F. Gomez, K. Gorski, A. Gregorio, P. Guzzi, J. M. Herreros, S. R. Hildebrandt, R. Hoyland, N. Hughes, M. Janssen, P. Jukkala, D. Kettle, V. H. Kilpiä, M. Laaninen, P. M. Lapolla, C. R. Lawrence, D. Lawson, J. P. Leahy, R. Leonardi, P. Leutenegger, S. Levin, P. B. Lilje, S. R. Lowe, P. M. Lubin, D. Maino, M. Malaspina, M. Maris, J. Marti-Canales, E. Martinez-Gonzalez, A. Mediavilla, P. Meinhold, M. Miccolis, G. Morgante, P. Natoli, R. Nesti, L. Pagan, C. Paine, B. Partridge, J. P. Pascual, F. Pasian, D. Pearson, M. Pecora, F. Perrotta, P. Platania, M. Pospieszalski, T. Poutanen, M. Prina, R. Rebolo, N. Roddis, J. A. Rubiño-Martin, M. J. Salmon, M. Sandri, M. Seiffert, R. Silvestri, A. Simonetto, P. Sjoman, G. F. Smoot, C. Sozzi, L. Stringhetti, E. Taddei, J. Tauber, L. Terenzi, M. Tomasi, J. Tuovinen, L. Valenziano, J. Varis, N. Vittorio, L. A. Wade, A. Wilkinson, F. Winder, A. Zacchei, A. Zonca
Publikováno v:
Bersanelli, M, Mandolesi, N, Butler, R C, Tuovinen, J, Varis, J & et al. 2010, ' Planck pre-launch status : Design and description of the Low Frequency Instrument ', Astronomy and Astrophysics, vol. 520 . https://doi.org/10.1051/0004-6361/200912853
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 520, pp.A4. ⟨10.1051/0004-6361/200912853⟩
Astronomy and Astrophysics, 520, A4.
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
Astronomy and Astrophysics, 2010, 520, A4.
Astronomy and Astrophysics-A&A, 2010, 520, pp.A4. ⟨10.1051/0004-6361/200912853⟩
Astronomy & astrophysics
520 (2010): A4. doi:10.1051/0004-6361/200912853
info:cnr-pdr/source/autori:M. Bersanelli1,2; N. Mandolesi3; R. C. Butler3; A. Mennella1,2; F. Villa3; B. Aja4; E. Artal4; E. Artina5; C. Baccigalupi6,15; M. Balasini5; G. Baldan5; A. Banday7,32; P. Bastia5; P. Battaglia5; T. Bernardino8; E. Blackhurst9; L. Boschini5; C. Burigana3; G. Cafagna5; B. Cappellini1,2; F. Cavaliere1; F. Colombo5; G. Crone10; F. Cuttaia3; O. D Arcangelo11; L. Danese6; R. D. Davies9; R. J. Davis9; L. De Angelis12; G. C. De Gasperis13; L. De La Fuente4; A. De Rosa3; G. De Zotti14; M. C. Falvella12; F. Ferrari5; R. Ferretti5; L. Figini11; S. Fogliani15; C. Franceschet1; E. Franceschi3; T. Gaier16; S. Garavaglia11; F. Gomez17; K. Gorski16; A. Gregorio18; P. Guzzi5; J. M. Herreros17; S. R. Hildebrandt17; R. Hoyland17; N. Hughes19; M. Janssen16; P. Jukkala19; D. Kettle9; V. H. Kilpiä19; M. Laaninen20; P. M. Lapolla5; C. R. Lawrence16; D. Lawson9; J. P. Leahy9; R. Leonardi21; P. Leutenegger5; S. Levin16; P. B. Lilje22; S. R. Lowe9; P. M. Lubin21; D.Maino1; M. Malaspina3; M. Maris15; J. Marti-Canales10; E. Martinez-Gonzalez8; A. Mediavilla4; P. Meinhold21; M. Miccolis5; G. Morgante3; P. Natoli13; R. Nesti23; L. Pagan5; C. Paine16; B. Partridge24; J. P. Pascual4; F. Pasian15; D. Pearson16; M. Pecora5; F. Perrotta15,6; P. Platania11; M. Pospieszalski25; T. Poutanen26,27,28; M. Prina16; R. Rebolo17; N. Roddis9; J. A. Rubiño-Martin17; M. J. Salmon8; M. Sandri3; M. Seiffert16; R. Silvestri5; A. Simonetto11; P. Sjoman19; G. F. Smoot29; C. Sozzi11; L. Stringhetti3; E. Taddei5; J. Tauber30; L. Terenzi3; M. Tomasi1; J. Tuovinen31; L. Valenziano3; J. Varis31; N. Vittorio13; L. A. Wade16; A. Wilkinson9; F.Winder9; A. Zacchei15; and A. Zonca1,2/titolo:Planck pre-launch status: Design and description of the Low Frequency Instrument/doi:10.1051%2F0004-6361%2F200912853/rivista:Astronomy & astrophysics (Print)/anno:2010/pagina_da:A4/pagina_a:/intervallo_pagine:A4/volume:520
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 520, pp.A4. ⟨10.1051/0004-6361/200912853⟩
Astronomy and Astrophysics, 520, A4.
UCrea Repositorio Abierto de la Universidad de Cantabria
Universidad de Cantabria (UC)
Astronomy and Astrophysics, 2010, 520, A4.
Astronomy and Astrophysics-A&A, 2010, 520, pp.A4. ⟨10.1051/0004-6361/200912853⟩
Astronomy & astrophysics
520 (2010): A4. doi:10.1051/0004-6361/200912853
info:cnr-pdr/source/autori:M. Bersanelli1,2; N. Mandolesi3; R. C. Butler3; A. Mennella1,2; F. Villa3; B. Aja4; E. Artal4; E. Artina5; C. Baccigalupi6,15; M. Balasini5; G. Baldan5; A. Banday7,32; P. Bastia5; P. Battaglia5; T. Bernardino8; E. Blackhurst9; L. Boschini5; C. Burigana3; G. Cafagna5; B. Cappellini1,2; F. Cavaliere1; F. Colombo5; G. Crone10; F. Cuttaia3; O. D Arcangelo11; L. Danese6; R. D. Davies9; R. J. Davis9; L. De Angelis12; G. C. De Gasperis13; L. De La Fuente4; A. De Rosa3; G. De Zotti14; M. C. Falvella12; F. Ferrari5; R. Ferretti5; L. Figini11; S. Fogliani15; C. Franceschet1; E. Franceschi3; T. Gaier16; S. Garavaglia11; F. Gomez17; K. Gorski16; A. Gregorio18; P. Guzzi5; J. M. Herreros17; S. R. Hildebrandt17; R. Hoyland17; N. Hughes19; M. Janssen16; P. Jukkala19; D. Kettle9; V. H. Kilpiä19; M. Laaninen20; P. M. Lapolla5; C. R. Lawrence16; D. Lawson9; J. P. Leahy9; R. Leonardi21; P. Leutenegger5; S. Levin16; P. B. Lilje22; S. R. Lowe9; P. M. Lubin21; D.Maino1; M. Malaspina3; M. Maris15; J. Marti-Canales10; E. Martinez-Gonzalez8; A. Mediavilla4; P. Meinhold21; M. Miccolis5; G. Morgante3; P. Natoli13; R. Nesti23; L. Pagan5; C. Paine16; B. Partridge24; J. P. Pascual4; F. Pasian15; D. Pearson16; M. Pecora5; F. Perrotta15,6; P. Platania11; M. Pospieszalski25; T. Poutanen26,27,28; M. Prina16; R. Rebolo17; N. Roddis9; J. A. Rubiño-Martin17; M. J. Salmon8; M. Sandri3; M. Seiffert16; R. Silvestri5; A. Simonetto11; P. Sjoman19; G. F. Smoot29; C. Sozzi11; L. Stringhetti3; E. Taddei5; J. Tauber30; L. Terenzi3; M. Tomasi1; J. Tuovinen31; L. Valenziano3; J. Varis31; N. Vittorio13; L. A. Wade16; A. Wilkinson9; F.Winder9; A. Zacchei15; and A. Zonca1,2/titolo:Planck pre-launch status: Design and description of the Low Frequency Instrument/doi:10.1051%2F0004-6361%2F200912853/rivista:Astronomy & astrophysics (Print)/anno:2010/pagina_da:A4/pagina_a:/intervallo_pagine:A4/volume:520
21 páginas, 23 figuras, 13 tablas.-- et al.
In this paper we present the Low Frequency Instrument (LFI), designed and developed as part of the Planck space mission, the ESA programme dedicated to precision imaging of the cosmic microwave backgr
In this paper we present the Low Frequency Instrument (LFI), designed and developed as part of the Planck space mission, the ESA programme dedicated to precision imaging of the cosmic microwave backgr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e99b320d118ac1421c113af1c138ec0
https://cris.vtt.fi/en/publications/49f325b5-4fd2-40f0-abe3-6287a775d2e1
https://cris.vtt.fi/en/publications/49f325b5-4fd2-40f0-abe3-6287a775d2e1
Autor:
Rafael Rebolo, Denis Mégevand, Paolo Di Marcantonio, Alexandre Cabral, Filippo Maria Zerbi, Stefano Cristiani, Nuno C. Santos, J. M. Herreros, Christophe Lovis, Francesco Pepe
ESPRESSO is a high-resolution, highly stable spectrograph for the VLT. It will inherit and enhance most capabilities from HARPS and UVES, combining both stability and efficiency. The main science driver will be the detection and characterization of E
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d939ef9d8d07a300aab509983a676cd2