Zobrazeno 1 - 10
of 7 643
pro vyhledávání: '"Meyër, Michael A."'
Autor:
Bowens, Rory, Leisenring, Jarron, Meyer, Michael R., Tobin, Taylor L., Miller, Alyssa L., Monnier, John D., Viges, Eric, Hoffmann, Bill, Montoya, Manny, Durney, Olivier, West, Grant, Morzinski, Katie, Forrest, William, McMurtry, Craig
We present results from commissioning observations of the mid-IR instrument, MIRAC-5, on the 6.5-m MMT telescope. MIRAC-5 is a novel ground-based instrument that utilizes a state-of-the-art GeoSnap (2 - 13 microns) HgCdTe detector with adaptive optic
Externí odkaz:
http://arxiv.org/abs/2412.10189
Autor:
Smith, Peter C. B., Sanchez, Jorge A., Line, Michael R., Rauscher, Emily, Mansfield, Megan Weiner, Kempton, Eliza M. -R., Savel, Arjun, Wardenier, Joost P., Pino, Lorenzo, Bean, Jacob L., Beltz, Hayley, Panwar, Vatsal, Brogi, Matteo, Malsky, Isaac, Fortney, Jonathan, Desert, Jean-Michel, Pelletier, Stefan, Parmentier, Vivien, Kanumalla, Krishna, Welbanks, Luis, Meyer, Michael, Monnier, John
A primary goal of exoplanet science is to measure the atmospheric composition of gas giants in order to infer their formation and migration histories. Common diagnostics for planet formation are the atmospheric metallicity ([M/H]) and the carbon-to-o
Externí odkaz:
http://arxiv.org/abs/2410.19017
Autor:
Beichman, Charles, Bryden, Geoffrey, Llop-Sayson, Jorge, Ygouf, Marie, Greenbaum, Alexandra, Leisenring, Jarron, Gaspar, Andras, Krist, John, Rieke, George, Wolff, Schuyler, Su, Kate, Hodapp, Klaus, Meyer, Michael, Kelly, Doug, Boyer, Martha, Johnstone, Doug, Horner, Scott, Rieke, Marcia
The most prominent of the IRAS debris disk systems, $\alpha$ Lyrae (Vega), at a distance of 7.7 pc, has been observed by both the NIRCam and MIRI instruments on the James Webb Space Telescope (JWST). This paper describes NIRCam coronagraphic observat
Externí odkaz:
http://arxiv.org/abs/2410.16551
Autor:
Cesario, Lorenzo, Lichtenberg, Tim, Alei, Eleonora, Carrión-González, Óscar, Dannert, Felix A., Defrère, Denis, Ertel, Steve, Fortier, Andrea, Muñoz, A. García, Glauser, Adrian M., Hansen, Jonah T., Helled, Ravit, Huber, Philipp A., Ireland, Michael J., Kammerer, Jens, Laugier, Romain, Lillo-Box, Jorge, Menti, Franziska, Meyer, Michael R., Noack, Lena, Quanz, Sascha P., Quirrenbach, Andreas, Rugheimer, Sarah, van der Tak, Floris, Wang, Haiyang S., Anger, Marius, Balsalobre-Ruza, Olga, Bhattarai, Surendra, Braam, Marrick, Castro-González, Amadeo, Cockell, Charles S., Constantinou, Tereza, Cugno, Gabriele, Davoult, Jeanne, Güdel, Manuel, Hernitschek, Nina, Hinkley, Sasha, Itoh, Satoshi, Janson, Markus, Johansen, Anders, Jones, Hugh R. A., Kane, Stephen R., van Kempen, Tim A., Kislyakova, Kristina G., Korth, Judith, Kovacevic, Andjelka B., Kraus, Stefan, Kuiper, Rolf, Mathew, Joice, Matsuo, Taro, Miguel, Yamila, Min, Michiel, Navarro, Ramon, Ramirez, Ramses M., Rauer, Heike, Ricketti, Berke Vow, Romagnolo, Amedeo, Schlecker, Martin, Sneed, Evan L., Squicciarini, Vito, Stassun, Keivan G., Tamura, Motohide, Viudez-Moreiras, Daniel, Wordsworth, Robin D., Collaboration, the LIFE
Publikováno v:
A&A 692, A172 (2024)
The increased brightness temperature of young rocky protoplanets during their magma ocean epoch makes them potentially amenable to atmospheric characterization to distances from the solar system far greater than thermally equilibrated terrestrial exo
Externí odkaz:
http://arxiv.org/abs/2410.13457
Autor:
Gouellec, Valentin J. M. Le, Lew, Ben W. P., Greene, Thomas P., Johnstone, Doug, Gusdorf, Antoine, Francis, Logan, DeWitt, Curtis, Meyer, Michael, Tychoniec, Łukasz, van Dishoeck, Ewine F., Barsony, Mary, Hodapp, Klaus W., Robberto, Massimo
The near-infrared (NIR) emission of the youngest protostars still needs to be characterized to better understand the evolution of their accretion and ejection activity. We analyze James Webb Space Telescope NIRSpec 1.7 -- 5.3 $\mu$m observations of t
Externí odkaz:
http://arxiv.org/abs/2410.11095
Autor:
De Furio, Matthew, Meyer, Michael R., Greene, Thomas, Hodapp, Klaus, Johnstone, Doug, Leisenring, Jarron, Rieke, Marcia, Robberto, Massimo, Roellig, Thomas, Cugno, Gabriele, Fiorellino, Eleonora, Manara, Carlo, Raileanu, Roberta, van Terwisga, Sierk
A successful theory of star formation should predict the number of objects as a function of their mass produced through star-forming events. Previous studies in star-forming regions and the solar neighborhood identify a mass function increasing from
Externí odkaz:
http://arxiv.org/abs/2409.04624
Autor:
Langeveld, Adam B., Scholz, Aleks, Mužić, Koraljka, Jayawardhana, Ray, Capela, Daniel, Albert, Loïc, Doyon, René, Flagg, Laura, de Furio, Matthew, Johnstone, Doug, Lafrèniere, David, Meyer, Michael
The discovery and characterization of free-floating planetary-mass objects (FFPMOs) is fundamental to our understanding of star and planet formation. Here we report results from an extremely deep spectroscopic survey of the young star cluster NGC1333
Externí odkaz:
http://arxiv.org/abs/2408.12639
Autor:
Carter, Aarynn L., Bowens-Rubin, Rachel, Calissendorff, Per, Kammerer, Jens, Li, Yiting, Meyer, Michael R., Booth, Mark, Factor, Samuel M., Franson, Kyle, Gaidos, Eric, Leisenring, Jarron M., Lew, Ben W. P., Martinez, Raquel A., Rebollido, Isabel, Rickman, Emily, Sutlieff, Ben J., Ward-Duong, Kimberly, Zhang, Zhoujian
We advocate for a large scale imaging survey of nearby young moving groups and star-forming regions to directly detect exoplanets over an unexplored range of masses, ages and orbits. Discovered objects will be identified early enough in JWST's lifeti
Externí odkaz:
http://arxiv.org/abs/2408.07722
Autor:
Monnier, John D., Jain, Prachet, Kalluri, Shashank, Cutler, James, D'Amico, Simone, Lightsey, Glenn, Pogorelyuk, Leonid, Vasisht, Gautam, Cahoy, Kerri, Meyer, Michael
We present the concept for STARI: STarlight Acquisition and Reflection toward Interferometry. If launched, STARI will be the first mission to control a 3-D CubeSat formation to the few mm-level, reflect starlight over 10s to 100s of meters from one s
Externí odkaz:
http://arxiv.org/abs/2408.03925
Autor:
Funke, Lars, Ilchen, Markus, Dingel, Kristina, Mazza, Tommaso, Mullins, Terence, Otto, Thorsten, Rivas, Daniel E., Savio, Sara, Serkez, Svitozar, Walter, Peter, Wieland, Niclas, Wülfing, Lasse, Bari, Sadia, Boll, Rebecca, Braune, Markus, Calegari, Francesca, De Fanis, Alberto, Decking, Winfried, Duensing, Andreas, Düsterer, Stefan, Egun, Felix, Ehresmann, Arno, Erk, Benjamin, de Lima, Danilo Enoque Ferreira, Galler, Andreas, Geloni, Gianluca, Grünert, Jan, Guetg, Marc, Grychtol, Patrik, Hans, Andreas, Held, Arne, Hindriksson, Ruda, Jahnke, Till, Laksman, Joakim, Larsson, Mats, Liu, Jia, Marangos, Jon P., Marder, Lutz, Meier, David, Meyer, Michael, Mirian, Najmeh, Ott, Christian, Passow, Christopher, Pfeifer, Thomas, Rupprecht, Patrick, Schletter, Albert, Schmidt, Philipp, Scholz, Frank, Schott, Simon, Schneidmiller, Evgeny, Sick, Bernhard, Tiedtke, Kai, Usenko, Sergey, Wanie, Vincent, Wurzer, Markus, Yurkov, Mikhail, Zhaunerchyk, Vitali, Helml, Wolfram
Attosecond X-ray pulses are the key to studying electron dynamics at their natural timescale in specifically targeted electronic states. They promise to build the conceptual bridge between physical and chemical photo-reaction processes. Free-electron
Externí odkaz:
http://arxiv.org/abs/2408.03858