Zobrazeno 1 - 10
of 44 491
pro vyhledávání: '"Katherine, E"'
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:
Stange, Katherine E.
These notes cover and expand upon the material for two summer schools: The first, which was held at CIRM, Marseille, France, July 10-14, 2023, as part of "Renormalization and Visualization for packing, billiard and surfaces", was titled "Number theor
Externí odkaz:
http://arxiv.org/abs/2412.02050
Autor:
Mun, Marcie, Wisnioski, Emily, Harborne, Katherine E., Lagos, Claudia D. P., Valenzuela, Lucas M., Remus, Rhea-Silvia, Mendel, J. Trevor, Battisti, Andrew J., Ellison, Sara L., Foster, Caroline, Bravo, Matias, Brough, Sarah, Croom, Scott M., Gao, Tianmu, Grasha, Kathryn, Gupta, Anshu, Mai, Yifan, Mailvaganam, Anilkumar, Muller, Eric G. M., Sharma, Gauri, Sweet, Sarah M., Taylor, Edward N., Zafar, Tayyaba
We investigate the internal and external mechanisms that regulate and quench star formation (SF) in galaxies at $z \sim 0.3$ using MAGPI observations and the EAGLE, Magneticum, and IllustrisTNG cosmological simulations. Using SimSpin to generate mock
Externí odkaz:
http://arxiv.org/abs/2411.17882
Autor:
Smith, D. Hudson, Nisbet, Noah, Ehrett, Carl, Tica, Cristina I., Atwell, Madeline M., Weisensee, Katherine E.
Environmental and individualistic variables affect the rate of human decomposition in complex ways. These effects complicate the estimation of the postmortem interval (PMI) based on observed decomposition characteristics. In this work, we develop a g
Externí odkaz:
http://arxiv.org/abs/2411.09802
Autor:
Cheng, Yingjie, Giavalisco, Mauro, Backhaus, Bren E., Bhatawdekar, Rachana, Cleri, Nikko J., Costantin, Luca, Daddi, Emanuele, Dickinson, Mark, Finkelstein, Steven L., Hirschmann, Michaela, Holwerda, Benne W., Koekemoer, Anton M., Lucas, Ray A., Pacucci, Fabio, Pérez-González, Pablo G., Rodighiero, Giulia, Seillé, Lise-Marie, Whitaker, Katherine E., Yung, L. Y. Aaron, Haro, Pablo Arrabal, Bagley, Micaela B., Kartaltepe, Jeyhan S., Papovich, Casey, Pirzkal, Nor
Over the past decades, a population of galaxies invisible in optical/near-infrared, but bright at longer wavelengths, have been identified through color selections. These so-called optically faint/dark galaxies are considered to be massive quiescent
Externí odkaz:
http://arxiv.org/abs/2411.08100
Autor:
Kavuri, Gautam A., Palfree, Jasper, Reddy, Dileep V., Zhang, Yanbao, Bienfang, Joshua C., Mazurek, Michael D., Alhejji, Mohammad A., Siddiqui, Aliza U., Cavanagh, Joseph M., Dalal, Aagam, Abellán, Carlos, Amaya, Waldimar, Mitchell, Morgan W., Stange, Katherine E., Beale, Paul D., Brandão, Luís T. A. N., Booth, Harold, Peralta, René, Nam, Sae Woo, Mirin, Richard P., Stevens, Martin J., Knill, Emanuel, Shalm, Lynden K.
The unpredictability of random numbers is fundamental to both digital security and applications that fairly distribute resources. However, existing random number generators have limitations-the generation processes cannot be fully traced, audited, an
Externí odkaz:
http://arxiv.org/abs/2411.05247
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:
Borkiewicz, Kalina, Jensen, Eric, Miao, Yiwen, Levy, Stuart, Naiman, J. P., Carpenter, Jeff, Isaacs, Katherine E.
Quantifying the global reach of planetarium dome shows presents significant challenges due to the lack of standardized viewership tracking mechanisms across diverse planetarium venues. We present an analysis of the global impact of dome shows, presen
Externí odkaz:
http://arxiv.org/abs/2411.08045
Autor:
Allen, Natalie, Oesch, Pascal A., Toft, Sune, Matharu, Jasleen, McPartland, Conor J. R., Weibel, Andrea, Brammer, Gabe, Bowler, Rebecca A. A., Ito, Kei, Gottumukkala, Rashmi, Rizzo, Francesca, Valentino, Francesco, Varadaraj, Rohan G., Weaver, John R., Whitaker, Katherine E.
The evolution of galaxy sizes in different wavelengths provides unique insights on galaxy build-up across cosmic epochs. Such measurements can now finally be done at $z>3$ thanks to the exquisite spatial resolution and multi-wavelength capability of
Externí odkaz:
http://arxiv.org/abs/2410.16354