Zobrazeno 1 - 10
of 10 065
pro vyhledávání: '"Suess A"'
Autor:
Miller, Tim B., Suess, Katherine A., Setton, David J., Price, Sedona H., Labbe, Ivo, Bezanson, Rachel, Brammer, Gabriel, Cutler, Sam E., Furtak, Lukas J., Leja, Joel, Pan, Richard, Wang, Bingjie, Weaver, John R., Whitaker, Katherine E., Dayal, Pratika, de Graaff, Anna, Feldmann, Robert, Greene, Jenny E., Fujimoto, S., Maseda, Michael V., Nanayakkara, Themiya, Nelson, Erica J., van Dokkum, Pieter, Zitrin, Adi
We study the rest-frame optical and ultraviolet morphology of galaxies in the first billion years of the Universe. Using JWST data from the UNCOVER and MegaScience surveys targeting the lensing cluster Abell 2744 we present multi-band morphological m
Externí odkaz:
http://arxiv.org/abs/2412.06957
Autor:
Labbe, Ivo, Greene, Jenny E., Matthee, Jorryt, Treiber, Helena, Kokorev, Vasily, Miller, Tim B., Kramarenko, Ivan, Setton, David J., Ma, Yilun, Goulding, Andy D., Bezanson, Rachel, Naidu, Rohan P., Williams, Christina C., Atek, Hakim, Brammer, Gabriel, Cutler, Sam E., Chemerynska, Iryna, Cloonan, Aidan P., Dayal, Pratika, de Graaff, Anna, Fudamoto, Yoshinobu, Fujimoto, Seiji, Furtak, Lukas J., Glazebrook, Karl, Heintz, Kasper E., Leja, Joel, Marchesini, Danilo, Nanayakkara, Themiya, Nelson, Erica J., Oesch, Pascal A., Pan, Richard, Price, Sedona H., Shivaei, Irene, Sobral, David, Suess, Katherine A., van Dokkum, Pieter, Wang, Bingjie, Weaver, John R., Whitaker, Katherine E., Zitrin, Adi
We present a detailed exploration of the most optically-luminous Little Red Dot ($L_{H\alpha}=10^{44}$erg/s, $L_V=10^{45}$erg/s, F444W=22AB) found to date. Located in the Abell 2744 field, source A744-45924 was observed by NIRSpec/PRISM with ultradee
Externí odkaz:
http://arxiv.org/abs/2412.04557
Autor:
Serha, Rostyslav O., Voronov, Andrey A., Schmoll, David, Klingbeil, Rebecca, Knauer, Sebastian, Koraltan, Sabri, Pribytova, Ekaterina, Lindner, Morris, Reimann, Timmy, Dubs, Carsten, Abert, Claas, Verba, Roman, Urbánek, Michal, Suess, Dieter, Chumak, Andrii V.
Quantum magnonics aims to exploit the quantum mechanical properties of magnons for nanoscale quantum information technologies. Ferrimagnetic yttrium iron garnet (YIG), which offers the longest magnon lifetimes, is a key material typically grown on ga
Externí odkaz:
http://arxiv.org/abs/2412.02827
Autor:
Voronov, Andrey A., Santos, Marcos Cuervo, Bruckner, Florian, Suess, Dieter, Chumak, Andrii V., Abert, Claas
The inverse design approach in magnonics exploits the wave nature of magnons and machine learning to develop novel logical devices with unique functionalities that exceed the capabilities of analytical methods. Despite its potential in analog, Boolea
Externí odkaz:
http://arxiv.org/abs/2411.19109
Autor:
Zenbaa, Noura, Majcen, Fabian, Abert, Claas, Bruckner, Florian, Mauser, Norbert J., Schrefl, Thomas, Wang, Qi, Suess, Dieter, Chumak, Andrii V.
Magnonic logic gates represent a crucial step toward realizing fully magnonic data processing systems without reliance on conventional electronic or photonic elements. Recently, a universal and reconfigurable inverse-design device has been developed,
Externí odkaz:
http://arxiv.org/abs/2411.17546
Autor:
Schmoll, David, Voronov, Andrey A., Serha, Rostslav O., Slobodianiuk, Denys, Levchenko, Khrystyna O., Abert, Claas, Knauer, Sebastian, Suess, Dieter, Verba, Roman, Chumak, Andrii V.
Magnons have inspired potential applications in modern quantum technologies and hybrid quantum systems due to their intrinsic nonlinearity, nanoscale scalability, and a unique set of experimentally accessible parameters for manipulating their dispers
Externí odkaz:
http://arxiv.org/abs/2411.13414
Autor:
Abert, Claas, Bruckner, Florian, Voronov, Andrey, Lang, Martin, Pathak, Swapneel Amit, Holt, Samuel, Kraft, Robert, Allayarov, Ruslan, Flauger, Peter, Koraltan, Sabri, Schrefl, Thomas, Chumak, Andrii, Fangohr, Hans, Suess, Dieter
We present NeuralMag, a flexible and high-performance open-source Python library for micromagnetic simulations. NeuralMag leverages modern machine learning frameworks, such as PyTorch and JAX, to perform efficient tensor operations on various paralle
Externí odkaz:
http://arxiv.org/abs/2411.11725
Autor:
Setton, David J., Greene, Jenny E., de Graaff, Anna, Ma, Yilun, Leja, Joel, Matthee, Jorryt, Bezanson, Rachel, Boogaard, Leindert A., Cleri, Nikko J., Katz, Harley, Labbe, Ivo, Maseda, Michael V., McConachie, Ian, Miller, Tim B., Price, Sedona H., Suess, Katherine A., van Dokkum, Pieter, Wang, Bingjie, Weibel, Andrea, Whitaker, Katherine E., Williams, Christina C.
Among the most puzzling early discoveries of JWST are "Little Red Dots" -- compact red sources that host broad Balmer emission lines and, in many cases, exhibit a "V shaped" change in slope in the rest-optical. The physical properties of Little Red D
Externí odkaz:
http://arxiv.org/abs/2411.03424
Autor:
Naidu, Rohan P., Matthee, Jorryt, Kramarenko, Ivan, Weibel, Andrea, Brammer, Gabriel, Oesch, Pascal A., Lechner, Peter, Furtak, Lukas J., Di Cesare, Claudia, Torralba, Alberto, Kotiwale, Gauri, Bezanson, Rachel, Bouwens, Rychard J., Chandra, Vedant, Claeyssens, Adélaïde, Danhaive, A. Lola, Frebel, Anna, de Graaff, Anna, Greene, Jenny E., Heintz, Kasper E., Ji, Alexander P., Kashino, Daichi, Katz, Harley, Labbe, Ivo, Leja, Joel, Li, Yijia, Maseda, Michael V., Richard, Johan, Shivaei, Irene, Simcoe, Robert A., Sobral, David, Suess, Katherine A., Tacchella, Sandro, Williams, Christina C.
Dwarf galaxies hold the key to crucial frontiers of astrophysics, however, their faintness renders spectroscopy challenging. Here we present the JWST Cycle 2 survey, All the Little Things (ALT, PID 3516), which is designed to seek late-forming Pop II
Externí odkaz:
http://arxiv.org/abs/2410.01874
Autor:
Lorenz, Brian, Kriek, Mariska, Shapley, Alice E., Sanders, Ryan L., Coil, Alison L., Leja, Joel, Mobasher, Bahram, Nelson, Erica, Price, Sedona H., Reddy, Naveen A., Runco, Jordan N., Suess, Katherine A., Shivaei, Irene, Siana, Brian, Weisz, Daniel R.
We examine star-formation and dust properties for a sample of 660 galaxies at $1.37\leq z\leq 2.61$ in the MOSDEF survey by dividing them into groups with similarly-shaped spectral energy distributions (SEDs). For each group, we combine the galaxy ph
Externí odkaz:
http://arxiv.org/abs/2409.18179