Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Magnone, Kenneth"'
Autor:
Konopacky, Quinn M., Baker, Ashley D., Mawet, Dimitri, Fitzgerald, Michael P., Jovanovic, Nemanja, Beichman, Charles, Ruane, Garreth, Bertz, Rob, Terada, Hiroshi, Dekany, Richard, Lingvay, Larry, Kassis, Marc, Anderson, David, Tamura, Motohide, Benneke, Bjorn, Beatty, Thomas, Do, Tuan, Nishiyama, Shogo, Plavchan, Peter, Wang, Jason, Wang, Ji, Burgasser, Adam, Ruffio, Jean-Baptiste, Zhang, Huihao, Brown, Aaron, Fucik, Jason, Gibbs, Aidan, Gibson, Rose, Halverson, Sam, Johnson, Christopher, Karkar, Sonia, Kotani, Takayuki, Kress, Evan, Leifer, Stephanie, Magnone, Kenneth, Maire, Jerome, Pahuja, Rishi, Porter, Michael, Roberts, Mitsuko, Sappey, Ben, Thorne, Jim, Wang, Eric, Artigau, Etienne, Blake, Geoffrey A., Canalizo, Gabriela, Chen, Guo, Doppmann, Greg, Doyon, Rene, Dressing, Courtney, Fang, Min, Greene, Thomas, Herczeg, Greg, Hillenbrand, Lynne, Howard, Andrew, Kane, Stephen, Kataria, Tiffany, Kempton, Eliza, Knutson, Heather, Lafreniere, David, Liu, Chao, Metchev, Stanimir, Millar-Blanchaer, Max, Narita, Norio, Pandey, Gajendra, Rajaguru, S. P., Robertson, Paul, Salyk, Colette, Sato, Bunei, Schlawin, Evertt, Sengupta, Sujan, Sivarani, Thirupathi, Skidmore, Warren, Vasisht, Gautam, Yasui, Chikako, Zhang, Hui
HISPEC is a new, high-resolution near-infrared spectrograph being designed for the W.M. Keck II telescope. By offering single-shot, R=100,000 between 0.98 - 2.5 um, HISPEC will enable spectroscopy of transiting and non-transiting exoplanets in close
Externí odkaz:
http://arxiv.org/abs/2309.11050
Autor:
Skemer, Andrew, Stelter, R. Deno, Sallum, Stephanie, MacDonald, Nicholas, Kupke, Renate, Ratliffe, Christopher, Banyal, Ravinder, Hasan, Amirul, Varshney, Hari Mohan, Surya, Arun, Prakash, Ajin, Thirupathi, Sivarani, Sethuraman, Ramya, V., Govinda K., Fitzgerald, Michael P., Wang, Eric, Kassis, Marc, Absil, Olivier, Alvarez, Carlos, Batalha, Natasha, Boucher, Marc-Andre, Bourgenot, Cyril, Brandt, Timothy, Briesemeister, Zackery, de Kleer, Katherine, de Pater, Imke, Deich, William, Divakar, Devika, Filion, Guillaume, Gauvin, Etienne, Gonzales, Michael, Greene, Thomas, Hinz, Philip, Jensen-Clem, Rebecca, Johnson, Christopher, Kain, Isabel, Kruglikov, Gabriel, Lach, Mackenzie, Landry, Jean-Thomas, Li, Jialin, Liu, Michael C., Lyke, James, Magnone, Kenneth, Marin, Eduardo, Martin, Emily C., Martinez, Raquel A., Mawet, Dimitri, Miles, Brittany, Sandford, Dale, Sheehan, Patrick, Sohn, Ji Man, Stone, Jordan
We present the design of SCALES (Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy) a new 2-5 micron coronagraphic integral field spectrograph under construction for Keck Observatory. SCALES enables low-resolution (R~50) spectroscopy,
Externí odkaz:
http://arxiv.org/abs/2208.10721
Autor:
Cosens, Maren, Wright, Shelley A., Brown, Aaron, Fitzgerald, Michael, Johnson, Chris, Jones, Tucker, Kassis, Marc, Kress, Evan, Kupke, Renate, Larkin, James E., Magnone, Kenneth, McGurk, Rosalie, Rundquist, Nils-Erik, Sohn, Ji Man, Wang, Eric, Wiley, James, Yeh, Sherry
Publikováno v:
Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 12184-224 (July 2022)
Liger is a next-generation near-infrared imager and integral field spectrograph (IFS) planned for the W.M. Keck Observatory. Liger is designed to take advantage of improved adaptive optics (AO) from the Keck All-Sky Precision Adaptive Optics (KAPA) u
Externí odkaz:
http://arxiv.org/abs/2208.07938
Autor:
Rundquist, Nils, Zonca, Andrea, Surya, Arun, Wright, Shelley A., Brown, Aaron, Cosens, Maren, Fitzgerald, Michael, Johnson, Chris, Kassis, Marc, Kupke, Renate, Lanclos, Kyle, Larkin, James E., Magnone, Kenneth, McGurk, Rosalie, Sohn, Ji Man, Walth, Gregory, Wiley, James, Yeh, Sherry
Publikováno v:
Proc. SPIE 12189, Software and Cyberinfrastructure for Astronomy VII, 12189-62 (July 2022)
Liger is a second generation near-infrared imager and integral field spectrograph (IFS) for the W. M. Keck Observatory that will utilize the capabilities of the Keck All-sky Precision Adaptive-optics (KAPA) system. Liger operates at a wavelength rang
Externí odkaz:
http://arxiv.org/abs/2208.07937
Autor:
Wiley, James, Brown, Aaron, Kupke, Renate, Cosens, Maren, Wright, Shelley A., Fitzgerald, Michael, Johnson, Chris, Jones, Tucker, Kassis, Marc, Kress, Evan, Larkin, James E., Magnone, Kenneth, McGurk, Rosalie, Rundquist, Nils, Wang, Eric, Yeh, Sherry
Publikováno v:
Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 12184-230 (July 2022)
Liger is an adaptive optics (AO) fed imager and integral field spectrograph (IFS) designed to take advantage of the Keck All-sky Precision Adaptive-optics (KAPA) upgrade for the W.M. Keck Observatory. We present the design and analysis of the imager
Externí odkaz:
http://arxiv.org/abs/2208.07936
Autor:
Delorme, Jacques-Robert, Jovanovic, Nemanja, Echeverri, Daniel, Mawet, Dimitri, Wallace, J. Kent, Bartos, Randall D., Cetre, Sylvain, Wizinowich, Peter, Ragland, Sam, Lilley, Scott, Wetherell, Edward, Doppmann, Greg, Wang, Jason J., Morris, Evan C., Ruffio, Jean-Baptiste, Martin, Emily C., Fitzgerald, Michael P., Ruane, Garreth, Schofield, Tobias, Suominen, Nick, Calvin, Benjamin, Wang, Eric, Magnone, Kenneth, Johnson, Christopher, Sohn, Ji Man, Lopez, Ronald A., Bond, Charlotte Z., Pezzato, Jacklyn, Sayson, Jorge Llop, Chun, Mark, Skemer, Andrew J.
The Keck Planet Imager and Characterizer (KPIC) is a purpose-built instrument to demonstrate new technological and instrumental concepts initially developed for the exoplanet direct imaging field. Located downstream of the current Keck II adaptive op
Externí odkaz:
http://arxiv.org/abs/2107.12556
Autor:
Martin, Emily C., Fitzgerald, Michael P., McLean, Ian S., Doppmann, Gregory, Kassis, Marc, Aliado, Ted, Canfield, John, Johnson, Chris, Kress, Evan, Lanclos, Kyle, Magnone, Kenneth, Sohn, Ji Man, Wang, Eric, Weiss, Jason
NIRSPEC is a 1-5 micron echelle spectrograph in use on the Keck II Telescope since 1999. The spectrograph is capable of both moderate (R~2,000) and high (R~25,000) resolution observations and has been a workhorse instrument across many astronomical f
Externí odkaz:
http://arxiv.org/abs/1808.06024
Autor:
Larkin, James E., Chilcote, Jeffrey K., Aliado, Theodore, Bauman, Brian J., Brims, George, Canfield, John M., Cardwell, Andrew, Dillon, Daren, Doyon, René, Dunn, Jennifer, Fitzgerald, Michael P., Graham, James R., Goodsell, Stephen, Hartung, Markus, Hibon, Pascale, Ingraham, Patrick, Johnson, Christopher A, Kress, Evan, Konopacky, Quinn M., Macintosh, Bruce A., Magnone, Kenneth G., Maire, Jérôme, McLean, Ian S., Palmer, David, Perrin, Marshall D., Quiroz, Carlos, Rantakyrö, Fredrik, Sadakuni, Naru, Saddlemyer, Leslie, Serio, Andrew, Thibault, Simon, Thomas, Sandrine J., Vallee, Philippe, Weiss, Jason L.
The Gemini Planet Imager (GPI) is a complex optical system designed to directly detect the self-emission of young planets within two arcseconds of their host stars. After suppressing the starlight with an advanced AO system and apodized coronagraph,
Externí odkaz:
http://arxiv.org/abs/1407.2314
Akademický článek
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Autor:
Evans, Christopher J., Bryant, Julia J., Motohara, Kentaro, Skemer, Andrew J., Stelter, R. Deno, Sallum, Stephanie, MacDonald, Nicholas, Kupke, Renate, Ratliff, Christopher, Banyal, Ravinder, Hasan, Amirul, Varshney, Hari Mohan, Surya, Arun, Prakaesh, Ajin, Thirupathi, Sivarani, Sethuram, Ramya, K.V., Govinda, Fitzgerald, Michael P., Wang, Eric, Kassis, Marc, Absil, Olivier, Alvarez, Carlos, Batalha, Natasha, Boucher, Marc-André, Bourgenot, Cyril, Brandt, Timothy, Briesemeister, Zackery, de Kleer, Katherine, de Pater, Imke, Deich, William, Divakar, Devika, Filion, Guillaume, Gauvin, Étienne, Gonzales, Michael, Greene, Thomas, Hinz, Philip, Jensen-Clem, Rebecca, Johnson, Christopher, Kain, Isabel, Kruglikov, Gabriel, Lach, Mackenzie, Landry, Jean-Thomas, Li, Jialin, Liu, Michael C., Lyke, James, Magnone, Kenneth, Marin, Eduardo, Martin, Emily, Martinez, Raquel, Mawet, Dimitri, Miles, Brittany, Sandford, Dale, Sheehan, Patrick, Sohn, Ji Man, Stone, Jordan
Publikováno v:
Proceedings of SPIE; August 2022, Vol. 12184 Issue: 1 p121840I-121840I-19, 12062180p