Zobrazeno 1 - 10
of 404
pro vyhledávání: '"Wilkins, Stephen M"'
Autor:
Maltz, Maxwell G. A., Thomas, Peter A., Lovell, Christoper C., Roper, William J., Vijayan, Aswin P., Irodotou, Dimitrios, Liao, Shihong, Seeyave, Louise T. C., Wilkins, Stephen M.
Understanding the galaxy-halo relationship is not only key for elucidating the interplay between baryonic and dark matter, it is essential for creating large mock galaxy catalogues from N-body simulations. High-resolution hydrodynamical simulations a
Externí odkaz:
http://arxiv.org/abs/2410.24082
Autor:
Taylor, Anthony J., Finkelstein, Steven L., Kocevski, Dale D., Jeon, Junehyoung, Bromm, Volker, Amorin, Ricardo O., Haro, Pablo Arrabal, Backhaus, Bren E., Bagley, Micaela B., Bañados, Eduardo, Bhatawdekar, Rachana, Brooks, Madisyn, Calabro, Antonello, Ortiz, Oscar A. Chavez, Cheng, Yingjie, Cleri, Nikko J., Cole, Justin W., Davis, Kelcey, Dickinson, Mark, Donnan, Callum, Dunlop, James S., Ellis, Richard S., Fernandez, Vital, Fontana, Adriano, Fujimoto, Seiji, Giavalisco, Mauro, Grazian, Andrea, Guo, Jingsong, Hathi, Nimish P., Holwerda, Benne W., Hirschmann, Michaela, Inayoshi, Kohei, Kartaltepe, Jeyhan S., Khusanova, Yana, Koekemoer, Anton M., Kokorev, Vasily, Larson, Rebecca L., Leung, Gene C. K., Lucas, Ray A., McLeod, Derek J., Napolitano, Lorenzo, Onoue, Masafusa, Pacucci, Fabio, Papovich, Casey, Pérez-González, Pablo G., Pirzkal, Nor, Somerville, Rachel S., Trump, Jonathan R., Wilkins, Stephen M., Yung, L. Y. Aaron, Zhang, Haowen
We present a sample of 50 H-alpha detected broad-line active galactic nuclei (BLAGN) at redshifts 3.5
Externí odkaz:
http://arxiv.org/abs/2409.06772
Autor:
Punyasheel, Paurush, Vijayan, Aswin P., Greve, Thomas R., Roper, William J., Algera, Hiddo, Gillman, Steven, Gullberg, Bitten, Irodotou, Dimitrios, Lovell, Christopher C., Seeyave, Louise T. C., Thomas, Peter A., Wilkins, Stephen M.
We use the First Light And Reionisation Epoch Simulations (FLARES) to study the evolution of the rest-frame ultraviolet (UV) and far-infrared (FIR) sizes for a statistical sample of massive ($\gtrsim10^{9}$M$_{\odot}$) high redshift galaxies (z $\in$
Externí odkaz:
http://arxiv.org/abs/2408.11037
Autor:
Rose, Caitlin, Kartaltepe, Jeyhan S., Snyder, Gregory F., Huertas-Company, Marc, Yung, L. Y. Aaron, Haro, Pablo Arrabal, Bagley, Micaela B., Bisigello, Laura, Calabrò, Antonello, Cleri, Nikko J., Dickinson, Mark, Ferguson, Henry C., Finkelstein, Steven L., Fontana, Adriano, Grazian, Andrea, Grogin, Norman A., Holwerda, Benne W., Iyer, Kartheik G., Kewley, Lisa J., Kirkpatrick, Allison, Kocevski, Dale D., Koekemoer, Anton M., Lotz, Jennifer M., Lucas, Ray A., Napolitan, Lorenzo, Papovich, Casey, Pentericci, Laura, Pérez-González, Pablo G., Pirzkal, Nor, Ravindranath, Swara, Somerville, Rachel S., Straughn, Amber N., Trump, Jonathan R., Wilkins, Stephen M., Yang, Guang
A crucial yet challenging task in galaxy evolution studies is the identification of distant merging galaxies, a task which suffers from a variety of issues ranging from telescope sensitivities and limitations to the inherently chaotic morphologies of
Externí odkaz:
http://arxiv.org/abs/2407.21279
Autor:
Conselice, Christopher J., Adams, Nathan, Harvey, Thomas, Austin, Duncan, Ferreira, Leonardo, Ormerod, Katherine, Duan, Qiao, Trussler, James, Li, Qiong, Juodzbalis, Ignas, Westcott, Lewi, Harris, Honor, Seeyave, Louise T. C., Bluck, Asa F. L., Windhorst, Rogier A., Bhatawdekar, Rachana, Coe, Dan, Cohen, Seth H., Cheng, Cheng, Driver, Simon P., Frye, Brenda, Furtak, Lukas J., Grogin, Norman A., Hathi, Nimish P., Holwerda, Benne W., Jansen, Rolf A., Koekemoer, Anton M., Marshall, Madeline A., Nonino, Mario, Robotham, Aaron, Summers, Jake, Wilkins, Stephen M., Willmer, Christopher N. A., Yan, Haojing, Zitrin, Adi
We present in this paper the discovery, properties, and a catalog of 1165 high redshift $6.5 < z < 18$ galaxies found in deep JWST NIRCam imaging from the GTO PEARLS survey combined with data from JWST public fields. We describe our bespoke homogeneo
Externí odkaz:
http://arxiv.org/abs/2407.14973
Autor:
Adamo, Angela, Atek, Hakim, Bagley, Micaela B., Bañados, Eduardo, Barrow, Kirk S. S., Berg, Danielle A., Bezanson, Rachel, Bradač, Maruša, Brammer, Gabriel, Carnall, Adam C., Chisholm, John, Coe, Dan, Dayal, Pratika, Eisenstein, Daniel J., Eldridge, Jan J., Ferrara, Andrea, Fujimoto, Seiji, de Graaff, Anna, Habouzit, Melanie, Hutchison, Taylor A., Kartaltepe, Jeyhan S., Kassin, Susan A., Kriek, Mariska, Labbé, Ivo, Maiolino, Roberto, Marques-Chaves, Rui, Maseda, Michael V., Mason, Charlotte, Matthee, Jorryt, McQuinn, Kristen B. W., Meynet, Georges, Naidu, Rohan P., Oesch, Pascal A., Pentericci, Laura, Pérez-González, Pablo G., Rigby, Jane R., Roberts-Borsani, Guido, Schaerer, Daniel, Shapley, Alice E., Stark, Daniel P., Stiavelli, Massimo, Strom, Allison L., Vanzella, Eros, Wang, Feige, Wilkins, Stephen M., Williams, Christina C., Willott, Chris J., Wylezalek, Dominika, Nota, Antonella
With stunning clarity, JWST has revealed the Universe's first billion years. The scientific community is analyzing a wealth of JWST imaging and spectroscopic data from that era, and is in the process of rewriting the astronomy textbooks. Here, 1.5 ye
Externí odkaz:
http://arxiv.org/abs/2405.21054
Autor:
Austin, Duncan, Conselice, Christopher J., Adams, Nathan J., Harvey, Thomas, Duan, Qiao, Trussler, James, Li, Qiong, Juodzbalis, Ignas, Ormerod, Katherine, Ferreira, Leonardo, Westcott, Lewi, Harris, Honor, Wilkins, Stephen M., Bhatawdekar, Rachana, Caruana, Joseph, Coe, Dan, Cohen, Seth H., Driver, Simon P., D'Silva, Jordan C. J., Frye, Brenda, Furtak, Lukas J., Grogin, Norman A., Hathi, Nimish P., Holwerda, Benne W., Jansen, Rolf A., Koekemoer, Anton M., Marshall, Madeline A., Nonino, Mario, Ortiz III, Rafael, Pirzkal, Nor, Robotham, Aaron, Ryan Jr., Russell E., Summers, Jake, Willmer, Christopher N. A., Windhorst, Rogier A., Yan, Haojing, Zackrisson, Erik
We present an analysis of rest-frame UV continuum slopes, $\beta$, using a sample of 1011 galaxies at $6.5
Externí odkaz:
http://arxiv.org/abs/2404.10751
Autor:
Kocevski, Dale D., Finkelstein, Steven L., Barro, Guillermo, Taylor, Anthony J., Calabrò, Antonello, Laloux, Brivael, Buchner, Johannes, Trump, Jonathan R., Leung, Gene C. K., Yang, Guang, Dickinson, Mark, Pérez-González, Pablo G., Pacucci, Fabio, Inayoshi, Kohei, Somerville, Rachel S., McGrath, Elizabeth J., Akins, Hollis B., Bagley, Micaela B., Bisigello, Laura, Bowler, Rebecca A. A., Carnall, Adam, Casey, Caitlin M., Cheng, Yingjie, Cleri, Nikko J., Costantin, Luca, Cullen, Fergus, Davis, Kelcey, Donnan, Callum T., Dunlop, James S., Ellis, Richard S., Ferguson, Henry C., Fujimoto, Seiji, Fontana, Adriano, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Hathi, Nimish P., Hirschmann, Michaela, Huertas-Company, Marc, Holwerda, Benne W., Illingworth, Garth, Juneau, Stéphanie, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Li, Wenxiu, Lucas, Ray A., Magee, Dan, Mason, Charlotte, McLeod, Derek J., McLure, Ross J., Napolitano, Lorenzo, Papovich, Casey, Pirzkal, Nor, Rodighiero, Giulia, Santini, Paola, Wilkins, Stephen M., Yung, L. Y. Aaron
We present a sample of 341 "little red dots" (LRDs) spanning the redshift range $z\sim2-11$ using data from the CEERS, PRIMER, JADES, UNCOVER and NGDEEP surveys. These sources are likely heavily-reddened AGN that trace a previously-hidden phase of du
Externí odkaz:
http://arxiv.org/abs/2404.03576
Autor:
Wilkins, Stephen M., Kuusisto, Jussi K., Irodotou, Dimitrios, Liao, Shihong, Lovell, Christopher C., Soininen, Sonja, Berger, Sabrina C., Newman, Sophie L., Roper, William J., Seeyave, Louise T. C., Thomas, Peter A., Vijayan, Aswin P.
Understanding the co-evolution of super-massive black holes (SMBHs) and their host galaxies remains a key challenge of extragalactic astrophysics, particularly the earliest stages at high-redshift. However, studying SMBHs at high-redshift with cosmol
Externí odkaz:
http://arxiv.org/abs/2404.02815
In recent years the James Webb Space Telescope has enabled the frontier of observational galaxy formation to push to ever higher redshift, deep within cosmic dawn. However, what is high-redshift, and when was cosmic dawn? While widely used, these ter
Externí odkaz:
http://arxiv.org/abs/2403.20144