Zobrazeno 1 - 6
of 6
pro vyhledávání: '"team, with the GPI"'
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:
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:
Wang, Jason J., Rajan, Abhijith, Graham, James R., Savransky, Dmitry, Ingraham, Patrick J., Ward-Duong, Kimberly, Patience, Jennifer, De Rosa, Robert J., Bulger, Joanna, Sivaramakrishnan, Anand, Perrin, Marshall D., Thomas, Sandrine J., Sadakuni, Naru, Greenbaum, Alexandra Z., Pueyo, Laurent, Marois, Christian, Oppenheimer, Ben R., Kalas, Paul, Cardwell, Andrew, Goodsell, Stephen, Hibon, Pascale, Rantakyrö, Fredrik T., team, with the GPI
The Gemini Planet Imager (GPI) combines extreme adaptive optics, an integral field spectrograph, and a high performance coronagraph to directly image extrasolar planets in the near-infrared. Because the coronagraph blocks most of the light from the s
Externí odkaz:
http://arxiv.org/abs/1407.2308
Autor:
Draper, Zachary H., Marois, Christian, Wolff, Schuyler, Perrin, Marshall, Ingraham, Patrick, Ruffio, Jean-Baptiste, Rantakyrö, Fredrik T., Hartung, Markus, Goodsell, Stephen J., team, with the GPI
The Gemini Planet Imager (GPI) is an instrument designed to directly image planets and circumstellar disks from 0.9 to 2.5 microns (the $YJHK$ infrared bands) using high contrast adaptive optics with a lenslet-based integral field spectrograph. We de
Externí odkaz:
http://arxiv.org/abs/1407.2309
Autor:
Wolff, Schuyler G., Perrin, Marshall D., Maire, Jérôme, Ingraham, Patrick J., Rantakyrö, Fredrik T., Hibon, Pascale, team, with the GPI
We present the wavelength calibration for the lenslet-based Integral Field Spectrograph (IFS) that serves as the science instrument for the Gemini Planet Imager (GPI). The GPI IFS features a 2.7" x 2.7" field of view and a 190 x 190 lenslet array (14
Externí odkaz:
http://arxiv.org/abs/1407.2304