Zobrazeno 1 - 10
of 641
pro vyhledávání: '"Delorme, J"'
Autor:
Costes, J. C., Xuan, J. W., Vigan, A., Wang, J., D'Orazi, V., Mollière, P., Baker, A., Bartos, R., Blake, G. A., Calvin, B., Cetre, S., Delorme, J., Doppmann, G., Echeveri, D., Finnerty, L., Fitzgerald, M. P., Hsu, C., Jovanovic, N., Lopez, R., Mawet, D., Morris, E., Pezzato, J., Phillips, C. L., Ruffio, J., Sappey, B., Schneeberger, A., Schofield, T., Skemer, A. J., Wallace, J. K.
Publikováno v:
A&A 686, A294 (2024)
Context. High-resolution spectroscopy has the potential to drive a better understanding of the atmospheric composition, physics, and dynamics of young exoplanets and brown dwarfs, bringing clear insights into the formation channel of individual objec
Externí odkaz:
http://arxiv.org/abs/2404.11523
Enhanced high-dispersion coronagraphy with KPIC phase II: design, assembly and status of sub-modules
Autor:
Jovanovic, N., Calvin, B., Porter, M., Schofield, T., Wang, J., Roberts, M., Ruane, G., Wallace, J. K., Bartos, R., Pezzato, J., Colborn, J., Delorme, J. R., Echeverri, D., Mawet, D., Bond, C. Z., Cetre, S., Lilley, S., Ragland, S., Wizinowich, P., Jensen-Clem, R.
The Keck Planet Imager and Characterizer (KPIC) is a purpose-built instrument for high-dispersion coronagraphy in the K and L bands on Keck. This instrument will provide the first high resolution (R$>$30,000) spectra of known directly imaged exoplane
Externí odkaz:
http://arxiv.org/abs/2012.06638
Autor:
Jovanovic, N., Delorme, J. R., Bond, C. Z., Cetre, S., Mawet, D., Echeverri, D., Wallace, J. K., Bartos, R., Lilley, S., Ragland, S., Ruane, G., Wizinowich, P., Chun, M., Wang, J., Fitzgerald, M., Matthews, K., Pezzato, J., Calvin, B., Millar-Blanchaer, M., Martin, E. C., Wetherell, E., Wang, E., Jacobson, S., Warmbier, E., Lockhart, C., Hall, D., Jensen-Clem, R., McEwen, E.
The Keck Planet Imager and Characterizer (KPIC) is an upgrade to the Keck II adaptive optics system enabling high contrast imaging and high-resolution spectroscopic characterization of giant exoplanets in the mid-infrared (2-5 microns). The KPIC inst
Externí odkaz:
http://arxiv.org/abs/1909.04541
Autor:
Mazin, B., Artigau, É., Bailey, V., Baranec, C., Beichman, C., Benneke, B., Birkby, J., Brandt, T., Chilcote, J., Chun, M., Close, L., Currie, T., Crossfield, I., Dekany, R., Delorme, J. R., Dong, C., Dong, R., Doyon, R., Dressing, C., Fitzgerald, M., Fortney, J., Frazin, R., Gaidos, E., Guyon, O., Hashimoto, J., Hillenbrand, L., Howard, A., Jensen-Clem, R., Jovanovic, N., Kotani, T., Kawahara, H., Konopacky, Q., Knutson, H., Liu, M., Lu, J., Lozi, J., Macintosh, B., Males, J., Marley, M., Marois, C., Mawet, D., Meeker, S., Millar-Blanchaer, M., Mondal, S., Bose, S. N., Murakami, N., Murray-Clay, R., Narita, N., Pyo, T. S., Roberts, L., Ruane, G., Serabyn, G., Shields, A., Skemer, A., Simard, L., Stelter, D., Tamura, M., Troy, M., Vasisht, G., Wallace, J. K., Wang, J., Wright, S.
Over the past three decades instruments on the ground and in space have discovered thousands of planets outside the solar system. These observations have given rise to an astonishingly detailed picture of the demographics of short-period planets, but
Externí odkaz:
http://arxiv.org/abs/1905.04275
Autor:
Jovanovic, N., Ruane, G., Echeverri, D., Delorme, J. R., Mawet, D., Fucik, J., Wallace, J. K., Coker, C., Delacroix, A., Levraud, N., Llop~Sayson, J. D., Wang, J., Riddle, R., Millar-Blanchaer, M. A.
Publikováno v:
SPIE, paper 10702-159, 2018
The High Contrast spectroscopy testbed for Segmented Telescopes (HCST) is being developed at Caltech. It aims at addressing the technology gap for future exoplanet imagers and providing the U.S. community with an academic facility to test components
Externí odkaz:
http://arxiv.org/abs/1807.07020
Autor:
Delorme, J. R., N'Diaye, M., Galicher, R., Dohlen, K., Baudoz, P., Caillat, A., Rousset, G., Soummer, R., Dupuis, O.
Publikováno v:
A&A 592, A119 (2016)
Specific high contrast imaging instruments are mandatory to characterize circumstellar disks and exoplanets around nearby stars. Coronagraphs are commonly used in these facilities to reject the diffracted light of an observed star and enable the dire
Externí odkaz:
http://arxiv.org/abs/1605.08523
Publikováno v:
A&A 588, A136 (2016)
High contrast imaging and spectroscopy provide unique constraints for exoplanet formation models as well as for planetary atmosphere models. But this can be challenging because of the planet-to-star small angular separation and high flux ratio. Recen
Externí odkaz:
http://arxiv.org/abs/1601.07748
Autor:
Jackson, Kathryn J., Schmidt, Dirk, Vernet, Elise, Wizinowich, P., Bouchez, A., Marin, E., Cetre, S., Chin, J., Correia, C., van Dam, M., Delorme, J.-R., Gers, L., Guthery, C., Karkar, S., Kwok, S., Lilley, S., Lyke, J., Richards, P., Service, M., Steiner, J., Surendran, A., Tsubota, K., Wetherell, E., Bottom, M., Dekany, R., Ghez, A., Hinz, P., Liu, M., Lu, J., Jensen-Clem, R., Millar-Blanchaer, M., Peretz, E., Sallum, S., Treu, T., Wright, S.
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13097 Issue: 1 p130970K-130970K-16, 12966047p
Publikováno v:
Eur.Phys.J. A8 (2000) 283-289
This paper is devoted to the evaluation of the pionic scalar density at finite temperature and baryonic density. We express the latter effect in terms of the nuclear response evaluated in the random phase approxima- tion. We discuss the density and t
Externí odkaz:
http://arxiv.org/abs/nucl-th/9912012
The apparent anomaly in the ratio of muon to electron atmospheric neutrinos first observed by Kamiokande and IMB has been confirmed by Super-Kamiokande and Soudan-2. The experimental analysis, including the asymmetry in the zenithal distributions of
Externí odkaz:
http://arxiv.org/abs/hep-ph/9906449