Zobrazeno 1 - 10
of 1 688
pro vyhledávání: '"Lloyd, James"'
Autor:
Blakely, Dori, Johnstone, Doug, Cugno, Gabriele, Sivaramakrishnan, Anand, Tuthill, Peter, Dong, Ruobing, Pope, Benjamin J. S., Albert, Loïc, Charles, Max, Cooper, Rachel A., De Furio, Matthew, Desdoigts, Louis, Doyon, René, Francis, Logan, Greenbaum, Alexandra Z., Lafrenière, David, Lloyd, James P., Meyer, Michael R., Pueyo, Laurent, Ray, Shrishmoy, Sánchez-Bermúdez, Joel, Soulain, Anthony, Thatte, Deepashri, Vandal, Thomas
We observed the planet-hosting system PDS 70 with the James Webb Interferometer, JWST's Aperture Masking Interferometric (AMI) mode within NIRISS. Observing with the F480M filter centered at 4.8 $\mu$m, we simultaneously fit a geometric model to the
Externí odkaz:
http://arxiv.org/abs/2404.13032
Autor:
Petrus, Simon, Whiteford, Niall, Patapis, Polychronis, Biller, Beth A., Skemer, Andrew, Hinkley, Sasha, Suárez, Genaro, Lueber, Anna, Palma-Bifani, Paulina, Stone, Jordan M., Vos, Johanna M., Morley, Caroline V., Tremblin, Pascal, Charnay, Benjamin, Helling, Christiane, Miles, Brittany E., Carter, Aarynn L., Wang, Jason J., Janson, Markus, Gonzales, Eileen C., Sutlieff, Ben, Hoch, Kielan K. W., Bonnefoy, Mickaël, Chauvin, Gaël, Absil, Olivier, Balmer, William O., Boccaletti, Anthony, Bonavita, Mariangela, Booth, Mark, Bowler, Brendan P., Briesemeister, Zackery W., Bryan, Marta L., Calissendorff, Per, Cantalloube, Faustine, Chen, Christine H., Choquet, Elodie, Christiaens, Valentin, Cugno, Gabriele, Currie, Thayne, Danielski, Camilla, De Furio, Matthew, Dupuy, Trent J., Factor, Samuel M., Faherty, Jacqueline K., Fitzgerald, Michael P., Fortney, Jonathan J., Franson, Kyle, Girard, Julien H., Grady, Carol A., Henning, Thomas, Hines, Dean C., Hood, Callie E., Howe, Alex R., Kalas, Paul, Kammerer, Jens, Kennedy, Grant M., Kenworthy, Matthew A., Kervella, Pierre, Kim, Minjae, Kitzmann, Daniel, Kraus, Adam L., Kuzuhara, Masayuki, Lagage, Pierre-Olivier, Lagrange, Anne-Marie, Lawson, Kellen, Lazzoni, Cecilia, Leisenring, Jarron M., Lew, Ben W. P., Liu, Michael C., Liu, Pengyu, Llop-Sayson, Jorge, Lloyd, James P., Macintosh, Bruce, Mâlin, Mathilde, Manjavacas, Elena, Marino, Sebastián, Marley, Mark S., Marois, Christian, Martinez, Raquel A., Matthews, Elisabeth C., Matthews, Brenda C., Mawet, Dimitri, Mazoyer, Johan, McElwain, Michael W., Metchev, Stanimir, Meyer, Michael R., Millar-Blanchaer, Maxwell A., Mollière, Paul, Moran, Sarah E., Mukherjee, Sagnick, Pantin, Eric, Perrin, Marshall D., Pueyo, Laurent, Quanz, Sascha P., Quirrenbach, Andreas, Ray, Shrishmoy, Rebollido, Isabel, Redai, Jea Adams, Ren, Bin B., Rickman, Emily, Sallum, Steph, Samland, Matthias, Sargent, Benjamin, Schlieder, Joshua E., Stapelfeldt, Karl R., Tamura, Motohide, Tan, Xianyu, Theissen, Christopher A., Uyama, Taichi, Vasist, Malavika, Vigan, Arthur, Wagner, Kevin, Ward-Duong, Kimberly, Wolff, Schuyler G., Worthen, Kadin, Wyatt, Mark C., Ygouf, Marie, Zurlo, Alice, Zhang, Xi, Zhang, Keming, Zhan, Zhoujian, Zhou, Yifan
The unprecedented medium-resolution (R~1500-3500) near- and mid-infrared (1-18um) spectrum provided by JWST for the young (140+/-20Myr) low-mass (12-20MJup) L-T transition (L7) companion VHS1256b gives access to a catalogue of molecular absorptions.
Externí odkaz:
http://arxiv.org/abs/2312.03852
Autor:
Ray, Shrishmoy, Sallum, Steph, Hinkley, Sasha, Sivamarakrishnan, Anand, Cooper, Rachel, Kammerer, Jens, Greebaum, Alexandra Z., Thatte, Deepashri, Lazzoni, Cecilia, Tokovinin, Andrei, de Furio, Matthew, Factor, Samuel, Meyer, Michael, Stone, Jordan M., Carter, Aarynn, Biller, Beth, Skemer, Andrew, Suarez, Genaro, Leisenring, Jarron M., Perrin, Marshall D., Kraus, Adam L., Absil, Olivier, Balmer, William O., Bonnefoy, Mickael, Bryan, Marta L., Betti, Sarah K., Boccaletti, Anthony, Bonavita, Mariangela, Booth, Mark, Bowler, Brendan P., Briesemeister, Zackery W., Cantalloube, Faustine, Chauvin, Gael, Christiaens, Valentin, Cugno, Gabriele, Currie, Thayne, Danielski, Camilla, Dupuy, Trent J., Faherty, Jacqueline K., Chen, Christine H., Calissendorff, Per, Choquet, Elodie, Fitzgerald, Michael P., Fortney, Jonathan J., Franson, Kyle, Girard, Julien H., Grady, Carol A., Gonzales, Eileen C., Henning, Thomas, Hines, Dean C., Hoch, Kielan K. W., Hood, Callie E., Howe, Alex R., Janson, Markus, Kalas, Paul, Kennedy, Grant M., Kenworthy, Matthew A., Kervella, Pierre, Kitzmann, Daniel, Kuzuhara, Masayuki, Lagrange, Anne-Marie, Lagage, Pierre-Olivier, Lawson, Kellen, Lew, Ben W. P., Liu, Michael C., Liu, Pengyu, Llop-Sayson, Jorge, Lloyd, James P., Lueber, Anna, Macintosh, Bruce, Manjavacas, Elena, Marino, Sebastian, Marley, Mark S., Marois, Christian, Martinez, Raquel A., Matthews, Brenda C., Matthews, Elisabeth C., Mawet, Dimitri, Mazoyer, Johan, McElwain, Michael W., Metchev, Stanimir, Miles, Brittany E., Millar-Blanchaer, Maxwell A., Molliere, Paul, Moran, Sarah E., Morley, Caroline V., Mukherjee, Sagnick, Palma-Bifani, Paulina, Pantin, Eric, Patapis, Polychronis, Petrus, Simon, Pueyo, Laurent, Quanz, Sascha P., Quirrenbach, Andreas, Rebollido, Isabel, Redai, Jea Adams, Ren, Bin B., Rickman, Emily, Samland, Matthias, Sargent, B. A., Schlieder, Joshua E., Schneider, Glenn, Stapelfeldt, Karl R., Sutlieff, Ben J., Tamura, Motohide, Tan, Xianyu, Theissen, Christopher A., Uyama, Taichi, Vigan, Arthur, Vasist, Malavika, Vos, Johanna M., Wagner, Kevin, Wang, Jason J., Ward-Duong, Kimberly, Whiteford, Niall, Wolff, Schuyler G., Worthen, Kadin, Wyatt, Mark C., Ygouf, Marie, Zhang, Xi, Zhang, Keming, Zhang, Zhoujian, Zhou, Yifan
We present aperture masking interferometry (AMI) observations of the star HIP 65426 at $3.8\,\rm{\mu m}$ as a part of the JWST Direct Imaging Early Release Science (ERS) program obtained using the Near Infrared Imager and Slitless Spectrograph (NIRIS
Externí odkaz:
http://arxiv.org/abs/2310.11508
Autor:
Sallum, Steph, Ray, Shrishmoy, Kammerer, Jens, Sivaramakrishnan, Anand, Cooper, Rachel, Greebaum, Alexandra Z., Thatte, Deepashri, de Furio, Matthew, Factor, Samuel, Meyer, Michael, Stone, Jordan M., Carter, Aarynn, Biller, Beth, Hinkley, Sasha, Skemer, Andrew, Suarez, Genaro, Leisenring, Jarron M., Perrin, Marshall D., Kraus, Adam L., Absil, Olivier, Balmer, William O., Bonnefoy, Mickael, Bryan, Marta L., Betti, Sarah K., Boccaletti, Anthony, Bonavita, Mariangela, Booth, Mark, Bowler, Brendan P., Briesemeister, Zackery W., Cantalloube, Faustine, Chauvin, Gael, Christiaens, Valentin, Cugno, Gabriele, Currie, Thayne, Danielski, Camilla, Dupuy, Trent J., Faherty, Jacqueline K., Chen, Christine H., Calissendorff, Per, Choquet, Elodie, Fitzgerald, Michael P., Fortney, Jonathan J., Franson, Kyle, Girard, Julien H., Grady, Carol A., Gonzales, Eileen C., Henning, Thomas, Hines, Dean C., Hoch, Kielan K. W., Hood, Callie E., Howe, Alex R., Janson, Markus, Kalas, Paul, Kennedy, Grant M., Kenworthy, Matthew A., Kervella, Pierre, Kitzmann, Daniel, Kuzuhara, Masayuki, Lagrange, Anne-Marie, Lagage, Pierre-Olivier, Lawson, Kellen, Lazzoni, Cecilia, Lew, Ben W. P., Liu, Michael C., Liu, Pengyu, Llop-Sayson, Jorge, Lloyd, James P., Lueber, Anna, Macintosh, Bruce, Manjavacas, Elena, Marino, Sebastian, Marley, Mark S., Marois, Christian, Martinez, Raquel A., Matthews, Brenda C., Matthews, Elisabeth C., Mawet, Dimitri, Mazoyer, Johan, McElwain, Michael W., Metchev, Stanimir, Miles, Brittany E., Millar-Blanchaer, Maxwell A., Molliere, Paul, Moran, Sarah E., Morley, Caroline V., Mukherjee, Sagnick, Palma-Bifani, Paulina, Pantin, Eric, Patapis, Polychronis, Petrus, Simon, Pueyo, Laurent, Quanz, Sascha P., Quirrenbach, Andreas, Rebollido, Isabel, Redai, Jea Adams, Ren, Bin B., Rickman, Emily, Samland, Matthias, Sargent, B. A., Schlieder, Joshua E., Schneider, Glenn, Stapelfeldt, Karl R., Sutlieff, Ben J., Tamura, Motohide, Tan, Xianyu, Theissen, Christopher A., Uyama, Taichi, Vigan, Arthur, Vasist, Malavika, Vos, Johanna M., Wagner, Kevin, Wang, Jason J., Ward-Duong, Kimberly, Whiteford, Niall, Wolff, Schuyler G., Worthen, Kadin, Wyatt, Mark C., Ygouf, Marie, Zhang, Xi, Zhang, Keming, Zhang, Zhoujian, Zhou, Yifan, Zurlo, Alice
We present a performance analysis for the aperture masking interferometry (AMI) mode on board the James Webb Space Telescope Near Infrared Imager and Slitless Spectrograph (JWST/NIRISS). Thanks to self-calibrating observables, AMI accesses inner work
Externí odkaz:
http://arxiv.org/abs/2310.11499
Autor:
Kammerer, Jens, Cooper, Rachel A., Vandal, Thomas, Thatte, Deepashri, Martinache, Frantz, Sivaramakrishnan, Anand, Chaushev, Alexander, Stolker, Tomas, Lloyd, James P., Albert, Loïc, Doyon, René, Sallum, Steph, Perrin, Marshall D., Pueyo, Laurent, Mérand, Antoine, Gallenne, Alexandre, Greenbaum, Alexandra, Sanchez-Bermudez, Joel, Blakely, Dori, Johnstone, Doug, Volk, Kevin, Martel, Andre, Goudfrooij, Paul, Meyer, Michael R., Willott, Chris J., De Furio, Matthew, Dang, Lisa, Radica, Michael, Noirot, Gaël
Kernel phase imaging (KPI) enables the direct detection of substellar companions and circumstellar dust close to and below the classical (Rayleigh) diffraction limit. We present a kernel phase analysis of JWST NIRISS full pupil images taken during th
Externí odkaz:
http://arxiv.org/abs/2210.17528
Autor:
Sivaramakrishnan, Anand, Tuthill, Peter, Lloyd, James P., Greenbaum, Alexandra Z., Thatte, Deepashri, Cooper, Rachel A., Vandal, Thomas, Kammerer, Jens, Sanchez-Bermudez, Joel, Pope, Benjamin J. S., Blakely, Dori, Albert, Loïc, Cook, Neil J., Johnstone, Doug, Martel, André R., Volk, Kevin, Soulain, Anthony, Artigau, Étienne, Lafrenière, David, Willott, Chris J., Parmentier, Sébastien, Ford, K. E. Saavik, McKernan, Barry, Vila, M. Begoña, Rowlands, Neil, Doyon, René, Desdoigts, Louis, Fullerton, Alexander W., De Furio, Matthew, Goudfrooij, Paul, Holfeltz, Sherie T., LaMassa, Stephanie, Maszkiewicz, Michael, Meyer, Michael R., Perrin, Marshall D., Pueyo, Laurent, Sahlmann, Johannes, Sohn, Sangmo Tony, Teixeira, Paula S.
The James Webb Space Telescope's Near Infrared Imager and Slitless Spectrograph (JWST-NIRISS) flies a 7-hole non-redundant mask (NRM), the first such interferometer in space, operating at 3-5 \micron~wavelengths, and a bright limit of $\simeq 4$ magn
Externí odkaz:
http://arxiv.org/abs/2210.17434
Autor:
Miles, Brittany E., Biller, Beth A., Patapis, Polychronis, Worthen, Kadin, Rickman, Emily, Hoch, Kielan K. W., Skemer, Andrew, Perrin, Marshall D., Whiteford, Niall, Chen, Christine H., Sargent, B., Mukherjee, Sagnick, Morley, Caroline V., Moran, Sarah E., Bonnefoy, Mickael, Petrus, Simon, Carter, Aarynn L., Choquet, Elodie, Hinkley, Sasha, Ward-Duong, Kimberly, Leisenring, Jarron M., Millar-Blanchaer, Maxwell A., Pueyo, Laurent, Ray, Shrishmoy, Stapelfeldt, Karl R., Stone, Jordan M., Wang, Jason J., Absil, Olivier, Balmer, William O., Boccaletti, Anthony, Bonavita, Mariangela, Booth, Mark, Bowler, Brendan P., Chauvin, Gael, Christiaens, Valentin, Currie, Thayne, Danielski, Camilla, Fortney, Jonathan J., Girard, Julien H., Greenbaum, Alexandra Z., Henning, Thomas, Hines, Dean C., Janson, Markus, Kalas, Paul, Kammerer, Jens, Kenworthy, Matthew A., Kervella, Pierre, Lagage, Pierre-Olivier, Lew, Ben W. P., Liu, Michael C., Macintosh, Bruce, Marino, Sebastian, Marley, Mark S., Marois, Christian, Matthews, Elisabeth C., Matthews, Brenda C., Mawet, Dimitri, McElwain, Michael W., Metchev, Stanimir, Meyer, Michael R., Molliere, Paul, Pantin, Eric, Rebollido, Andreas Quirrenbachm Isabel, Ren, Bin B., Vasist, Malavika, Wyatt, Mark C., Zhou, Yifan, Briesemeister, Zackery W., Bryan, Marta L., Calissendorff, Per, Catalloube, Faustine, Cugno, Gabriele, De Furio, Matthew, Dupuy, Trent J., Factor, Samuel M., Faherty, Jacqueline K., Fitzgerald, Michael P., Franson, Kyle, Gonzales, Eileen C., Hood, Callie E., Howe, Alex R., Kraus, Adam L., Kuzuhara, Masayuki, Lawson, Kellen, Lazzoni, Cecilia, Liu, Pengyu, Llop-Sayson, Jorge, Lloyd, James P., Martinez, Raquel A., Mazoyer, Johan, Quanz, Sascha P., Redai, Jea Adams, Samland, Matthias, Schlieder, Joshua E., Tamura, Motohide, Tan, Xianyu, Uyama, Taichi, Vigan, Arthur, Vos, Johanna M., Wagner, Kevin, Wolff, Schuyler G., Ygouf, Marie, Zhang, Keming, Zhang, Zhoujian
We present the highest fidelity spectrum to date of a planetary-mass object. VHS 1256 b is a $<$20 M$_\mathrm{Jup}$ widely separated ($\sim$8\arcsec, a = 150 au), young, planetary-mass companion that shares photometric colors and spectroscopic featur
Externí odkaz:
http://arxiv.org/abs/2209.00620
Autor:
Carter, Aarynn L., Hinkley, Sasha, Kammerer, Jens, Skemer, Andrew, Biller, Beth A., Leisenring, Jarron M., Millar-Blanchaer, Maxwell A., Petrus, Simon, Stone, Jordan M., Ward-Duong, Kimberly, Wang, Jason J., Girard, Julien H., Hines, Dean C., Perrin, Marshall D., Pueyo, Laurent, Balmer, William O., Bonavita, Mariangela, Bonnefoy, Mickael, Chauvin, Gael, Choquet, Elodie, Christiaens, Valentin, Danielski, Camilla, Kennedy, Grant M., Matthews, Elisabeth C., Miles, Brittany E., Patapis, Polychronis, Ray, Shrishmoy, Rickman, Emily, Sallum, Steph, Stapelfeldt, Karl R., Whiteford, Niall, Zhou, Yifan, Absil, Olivier, Boccaletti, Anthony, Booth, Mark, Bowler, Brendan P., Chen, Christine H., Currie, Thayne, Fortney, Jonathan J., Grady, Carol A., Greenbaum, Alexandra Z., Henning, Thomas, Hoch, Kielan K. W., Janson, Markus, Kalas, Paul, Kenworthy, Matthew A., Kervella, Pierre, Kraus, Adam L., Lagage, Pierre-Olivier, Liu, Michael C., Macintosh, Bruce, Marino, Sebastian, Marley, Mark S., Marois, Christian, Matthews, Brenda C., Mawet, Dimitri, McElwain, Michael W., Metchev, Stanimir, Meyer, Michael R., Molliere, Paul, Moran, Sarah E., Morley, Caroline V., Mukherjee, Sagnick, Pantin, Eric, Quirrenbach, Andreas, Rebollido, Isabel, Ren, Bin B., Schneider, Glenn, Vasist, Malavika, Worthen, Kadin, Wyatt, Mark C., Briesemeister, Zackery W., Bryan, Marta L., Calissendorff, Per, Cantalloube, Faustine, Cugno, Gabriele, De Furio, Matthew, Dupuy, Trent J., Factor, Samuel M., Faherty, Jacqueline K., Fitzgerald, Michael P., Franson, Kyle, Gonzales, Eileen C., Hood, Callie E., Howe, Alex R., Kuzuhara, Masayuki, Lagrange, Anne-Marie, Lawson, Kellen, Lazzoni, Cecilia, Lew, Ben W. P., Liu, Pengyu, Llop-Sayson, Jorge, Lloyd, James P., Martinez, Raquel A., Mazoyer, Johan, Palma-Bifani, Paulina, Quanz, Sascha P., Redai, Jea Adams, Samland, Matthias, Schlieder, Joshua E., Tamura, Motohide, Tan, Xianyu, Uyama, Taichi, Vigan, Arthur, Vos, Johanna M., Wagner, Kevin, Wolff, Schuyler G., Ygouf, Marie, Zhang, Xi, Zhang, Keming, Zhang, Zhoujian
We present JWST Early Release Science (ERS) coronagraphic observations of the super-Jupiter exoplanet, HIP 65426 b, with the Near-Infrared Camera (NIRCam) from 2-5 $\mu$m, and with the Mid-Infrared Instrument (MIRI) from 11-16 $\mu$m. At a separation
Externí odkaz:
http://arxiv.org/abs/2208.14990