Zobrazeno 1 - 10
of 54
pro vyhledávání: '"Seeyave, Louise"'
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:
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:
Trussler, James, Conselice, Christopher, Adams, Nathan, Austin, Duncan, Caruana, Joseph, Harvey, Tom, Li, Qiong, Lovell, Christopher, Seeyave, Louise, Vijayan, Aswin, Wilkins, Stephen
We develop a photometric search method for identifying smouldering galaxies at $5< z < 8$, which are defined to have weak emission lines and thus generally have low specific star formation rates and may even be in a state of (temporary) quiescence. T
Externí odkaz:
http://arxiv.org/abs/2404.07163
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
Autor:
Wilkins, Stephen M., Turner, Jack C., Bagley, Micaela B., Finkelstein, Steven L., Amorín, Ricardo O., Hautefort, Adrien Aufan Stoffels D, Behroozi, Peter, Bhatawdekar, Rachana, Dekel, Avishai, Donnellan, James, Drakos, Nicole E., Fortuni, Flaminia, Hathi, Nimish P., Hirschmann, Michaela, Holwerda, Benne W., Irodotou, Dimitrios, Koekemoer, Anton M., Lovell, Christopher C., Merlin, Emiliano, Roper, Will J., Seeyave, Louise T. C., Vijayan, Aswin P., Yung, L. Y. Aaron
The wavelength-coverage and sensitivity of JWST now enables us to probe the rest-frame UV - optical spectral energy distributions (SEDs) of galaxies at high-redshift ($z>4$). From these SEDs it is, in principle, through SED fitting possible to infer
Externí odkaz:
http://arxiv.org/abs/2311.08065
Autor:
Seeyave, Louise T. C., Wilkins, Stephen M., Kuusisto, Jussi K., Lovell, Christopher C., Irodotou, Dimitrios, Simmonds, Charlotte, Vijayan, Aswin P., Thomas, Peter A., Roper, William J., Byrne, Conor M., Jones, Gareth T., Turner, Jack C., Conselice, Christopher J.
The history of reionisation is highly dependent on the ionising properties of high-redshift galaxies. It is therefore important to have a solid understanding of how the ionising properties of galaxies are linked to physical and observable quantities.
Externí odkaz:
http://arxiv.org/abs/2305.18174
Autor:
Wilkins, Stephen M., Lovell, Christopher C., Irodotou, Dimitrios, Vijayan, Aswin P., Vikaeus, Anton, Zackrisson, Erik, Caruana, Joseph, Stanway, Elizabeth R., Conselice, Christopher J., Seeyave, Louise T. C., Roper, William J., Chworowsky, Katherine, Finkelstein, Steven L.
With the successful launch and commissioning of JWST we are now able to routinely spectroscopically probe the rest-frame optical emission of galaxies at $z>6$ for the first time. Amongst the most useful spectral diagnostics used in the optical is the
Externí odkaz:
http://arxiv.org/abs/2305.18175
Autor:
Vijayan, Aswin P., Thomas, Peter A., Lovell, Christopher C., Wilkins, Stephen M., Greve, Thomas R., Irodotou, Dimitrios, Roper, William J., Seeyave, Louise T. C.
Using the First Light And Reionisation Epoch Simulations (${\rm F{\small LARES}}$), a suite of hydrodynamical simulations we explore the consequences of a realistic model for star--dust geometry on the observed properties of galaxies. We find that th
Externí odkaz:
http://arxiv.org/abs/2303.04177
Autor:
Wilkins, Stephen M., Lovell, Christopher C., Vijayan, Aswin P., Irodotou, Dimitrios, Adams, Nathan J., Roper, William J., Caruana, Joseph, Matthee, Jorryt, Seeyave, Louise T. C., Conselice, Christopher J., Pérez-González, Pablo G., Turner, Jack C., Donnellan, James M. S.
JWST has now made it possible to probe the rest-frame optical line emission of high-redshift galaxies extending to z~9, and potentially beyond. To aid in the interpretation of these emerging constraints, in this work we explore predictions for [OIII]
Externí odkaz:
http://arxiv.org/abs/2301.13038
Autor:
Thomas, Peter A., Lovell, Christopher C., Maltz, Maxwell G. A., Vijayan, Aswin P., Wilkins, Stephen M., Irodotou, Dimitrios, Roper, William J., Seeyave, Louise
Upcoming deep galaxy surveys with JWST will probe galaxy evolution during the epoch of reionisation (EoR, $5\leq z\leq10$) over relatively compact areas (e.g. $\sim$ 300\,arcmin$^2$ for the JADES GTO survey). It is therefore imperative that we unders
Externí odkaz:
http://arxiv.org/abs/2301.09510