Zobrazeno 1 - 10
of 70
pro vyhledávání: '"Serio, Andrew"'
Autor:
Chilcote, Jeffrey, Pueyo, Laurent, Rosa, Robert J. De, Vargas, Jeffrey, Macintosh, Bruce, Bailey, Vanessa P., Barman, Travis, Bauman, Brian, Bruzzone, Sebastian, Bulger, Joanna, Burrows, Adam S., Cardwell, Andrew, Chen, Christine H., Cotten, Tara, Dillon, Daren, Doyon, Rene, Draper, Zachary H., Duchêne, Gaspard, Dunn, Jennifer, Erikson, Darren, Fitzgerald, Michael P., Follette, Katherine B., Gavel, Donald, Goodsell, Stephen J., Graham, James R., Greenbaum, Alexandra Z., Hartung, Markus, Hibon, Pascale, Hung, Li-Wei, Ingraham, Patrick, Kalas, Paul, Konopacky, Quinn, Larkin, James E., Maire, Jérôme, Marchis, Franck, Marley, Mark S., Marois, Christian, Metchev, Stanimir, Millar-Blanchaer, Maxwell A., Morzinski, Katie M., Nielsen, Eric L., Norton, Andrew, Oppenheimer, Rebecca, Palmer, David, Patience, Jennifer, Perrin, Marshall, Poyneer, Lisa, Rajan, Abhijith, Rameau, Julien, Rantakyrö, Fredrik T., Sadakuni, Naru, Saddlemyer, Leslie, Savransky, Dmitry, Schneider, Adam C., Serio, Andrew, Sivaramakrishnan, Anand, Song, Inseok, Soummer, Remi, Thomas, Sandrine, Wallace, J. Kent, Wang, Jason J., Ward-Duong, Kimberly, Wiktorowicz, Sloane, Wolff, Schuyler
Using the Gemini Planet Imager located at Gemini South, we measured the near-infrared (1.0-2.4 mu m) spectrum of the planetary companion to the nearby, young star beta. Pictoris. We compare the spectrum obtained with currently published model grids a
Externí odkaz:
http://hdl.handle.net/10150/623806
http://arizona.openrepository.com/arizona/handle/10150/623806
http://arizona.openrepository.com/arizona/handle/10150/623806
Autor:
Chilcote, Jeffrey, Pueyo, Laurent, De Rosa, Robert J., Vargas, Jeffrey, Macintosh, Bruce, Bailey, Vanessa P., Barman, Travis, Bauman, Brian, Bruzzone, Sebastian, Bulger, Joanna, Burrows, Adam S., Cardwell, Andrew, Chen, Christine H., Cotten, Tara, Dillon, Daren, Doyon, Rene, Draper, Zachary H., Duchêne, Gaspard, Dunn, Jennifer, Erikson, Darren, Fitzgerald, Michael P., Follette, Katherine B., Gavel, Donald, Goodsell, Stephen J., Graham, James R., Greenbaum, Alexandra Z., Hartung, Markus, Hibon, Pascale, Hung, Li-Wei, Ingraham, Patrick, Kalas, Paul, Konopacky, Quinn, Larkin, James E., Maire, Jérôme, Marchis, Franck, Marley, Mark S., Marois, Christian, Metchev, Stanimir, Millar-Blanchaer, Maxwell A., Morzinski, Katie M., Nielsen, Eric L., Norton, Andrew, Oppenheimer, Rebecca, Palmer, David, Patience, Jennifer, Perrin, Marshall, Poyneer, Lisa, Rajan, Abhijith, Rameau, Julien, Rantakyrö, Fredrik T., Sadakuni, Naru, Saddlemyer, Leslie, Savransky, Dmitry, Schneider, Adam C., Serio, Andrew, Sivaramakrishnan, Anand, Song, Inseok, Soummer, Remi, Thomas, Sandrine, Wallace, J. Kent, Wang, Jason J., Ward-Duong, Kimberly, Wiktorowicz, Sloane, Wolff, Schuyler
Using the Gemini Planet Imager (GPI) located at Gemini South, we measured the near-infrared (1.0-2.4 micron) spectrum of the planetary companion to the nearby, young star $\beta$ Pictoris. We compare the spectrum obtained with currently published mod
Externí odkaz:
http://arxiv.org/abs/1703.00011
Autor:
Wang, Jason J., Graham, James R., Pueyo, Laurent, Nielsen, Eric L., Millar-Blanchaer, Max, De Rosa, Robert J., Kalas, Paul, Ammons, S. Mark, Bulger, Joanna, Cardwell, Andrew, Chen, Christine, Chiang, Eugene, Chilcote, Jeffrey K., Doyon, René, Draper, Zachary H., Duchêne, Gaspard, Esposito, Thomas M., Fitzgerald, Michael P., Goodsell, Stephen J., Greenbaum, Alexandra Z., Hartung, Markus, Hibon, Pascale, Hinkley, Sasha, Hung, Li-Wei, Ingraham, Patrick, Larkin, James E., Macintosh, Bruce, Maire, Jerome, Marchis, Franck, Marois, Christian, Matthews, Brenda C., Morzinski, Katie M., Oppenheimer, Rebecca, Patience, Jenny, Perrin, Marshall D., Rajan, Abhijith, Rantakyrö, Fredrik T., Sadakuni, Naru, Serio, Andrew, Sivaramakrishnan, Anand, Soummer, Rémi, Thomas, Sandrine, Ward-Duong, Kimberly, Wiktorowicz, Sloane J., Wolff, Schuyler G.
We present Gemini Planet Imager (GPI) observations of AU Microscopii, a young M dwarf with an edge-on, dusty debris disk. Integral field spectroscopy and broadband imaging polarimetry were obtained during the commissioning of GPI. In our broadband im
Externí odkaz:
http://arxiv.org/abs/1508.04765
Autor:
Hartung, Markus, Hayward, Tom, Saddlemyer, Les, Poyneer, Lisa, Cardwell, Andrew, Cavedoni, Chas, Cho, Myung, Chilcote, Jeffrey K., Collins, Paul, Dillon, Darren, Galvez, Ramon, Gausachs, Gaston, Goodsell, Stephen, Guesalaga, Andres, Hibon, Pascal, Larkin, James, Macintosh, Bruce, Palmer, Dave, Sadakuni, Naru, Savransky, Dmitry, Serio, Andrew, Rantakyro, Fredrik, Wallace, Kent
The Gemini Planet Imager (GPI) entered on-sky commissioning and had its first-light at the Gemini South (GS) telescope in November 2013. GPI is an extreme adaptive optics (XAO), high-contrast imager and integral-field spectrograph dedicated to the di
Externí odkaz:
http://arxiv.org/abs/1407.7893
Autor:
Chilcote, Jeffrey, Barman, Travis, Fitzgerald, Michael P., Graham, James R., Larkin, James E., Macintosh, Bruce, Bauman, Brian, Burrows, Adam S., Cardwell, Andrew, De Rosa, Robert J., Dillon, Daren, Doyon, Rene, Dunn, Jennifer, Erikson, Darren, Gavel, Donald, Goodsell, Stephen J., Hartung, Markus, Hibon, Pascale, Ingraham, Patrick, Kalas, Paul, Konopacky, Quinn, Maire, Jérôme, Marchis, Franck, Marley, Mark S., Marois, Christian, Millar-Blanchaer, Max, Morzinski, Katie, Norton, Andrew, Oppenheimer, B. R., Palmer, David, Patience, Jennifer, Perrin, Marshall D., Poyneer, Lisa, Pueyo, Laurent, Rantakyrö, Fredrik, Sadakuni, Naru, Saddlemyer, Leslie, Savransky, Dmitry, Serio, Andrew, Sivaramakrishnan, Anand, Song, Inseok, Soummer, Remi, Thomas, Sandrine, Wallace, J. Kent, Wiktorowicz, Sloane J., Wolff, Schuyler
Using the recently installed Gemini Planet Imager (GPI), we have taken the first H-band spectrum of the planetary companion to the nearby young star beta Pictoris. GPI is designed to image and provide low-resolution spectra of Jupiter sized, self-lum
Externí odkaz:
http://arxiv.org/abs/1407.4469
Autor:
Sadakuni, Naru, Macintosh, Bruce A., Palmer, David W., Poyneer, Lisa A., Max, Claire E., Savransky, Dmitry, Thomas, Sandrine J., Cardwell, Andrew, Goodsell, Stephen, Hartung, Markus, Hibon, Pascale, Rantakyrö, Fredrik, Serio, Andrew, team, with the GPI
The Gemini Planet Imager (GPI) is a new facility, extreme adaptive optics (AO), coronagraphic instrument, currently being integrated onto the 8-meter Gemini South telescope, with the ultimate goal of directly imaging extrasolar planets. To achieve th
Externí odkaz:
http://arxiv.org/abs/1407.2316
Autor:
Savransky, Dmitry, Thomas, Sandrine J., Poyneer, Lisa A., Dunn, Jennifer, Macintosh, Bruce A., Sadakuni, Naru, Dillon, Daren, Goodsell, Stephen J., Hartung, Markus, Hibon, Pascale, Rantakyrö, Fredrik, Cardwell, Andrew, Serio, Andrew, team, with the GPI
The Gemini Planet Imager (GPI) is a next-generation, facility instrument currently being commissioned at the Gemini South observatory. GPI combines an extreme adaptive optics system and integral field spectrograph (IFS) with an apodized-pupil Lyot co
Externí odkaz:
http://arxiv.org/abs/1407.2313
Autor:
Hibon, Pascale, Thomas, Sandrine, Dunn, Jennifer, Atwood, Jenny, Saddlemyer, Les, Sadakuni, Naru, Goodsell, Stephen, Macintosh, Bruce, Graham, James, Perrin, Marshall, Rantakyrö, Fredrik, Fesquet, Vincent, Serio, Andrew, Quiroz, Carlos, Cardwell, Andrew, Gausachs, Gaston, Savransky, Dmitry, Kerley, Dan, Hartung, Markus, Galvez, Ramon, Hardie, Kayla
An Atmospheric Dispersion Corrector (ADC) uses a double-prism arrangement to nullify the vertical chromatic dispersion introduced by the atmosphere at non-zero zenith distances. The ADC installed in the Gemini Planet Imager (GPI) was first tested in
Externí odkaz:
http://arxiv.org/abs/1407.2315
Autor:
Greenbaum, Alexandra Z., Cheetham, Anthony, Sivaramakrishnan, Anand, Tuthill, Peter, Norris, Barnaby, Pueyo, Laurent, Sadakuni, Naru, Rantakyrö, Fredrik, Hibon, Pascale, Goodsell, Stephen, Hartung, Markus, Serio, Andrew, Cardwell, Andrew, Poyneer, Lisa, Macintosh, Bruce, Savransky, Dmitry, Perrin, Marshall D., Wolff, Schuyler, Ingraham, Patrick, Thomas, Sandrine, team, with the GPI
The Gemini Planet Imager (GPI) Extreme Adaptive Optics Coronograph contains an interferometric mode: a 10-hole non-redundant mask (NRM) in its pupil wheel. GPI operates at $Y, J, H$, and $K$ bands, using an integral field unit spectrograph (IFS) to o
Externí odkaz:
http://arxiv.org/abs/1407.2310
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