Zobrazeno 1 - 10
of 237
pro vyhledávání: '"Finlator, Kristian"'
Autor:
Heintz, Kasper E., Bennett, Jake S., Oesch, Pascal A., Sneppen, Albert, Rennehan, Douglas, Witstok, Joris, Smit, Renske, Vejlgaard, Simone, Terp, Chamilla, Koca, Umran S., Brammer, Gabriel B., Finlator, Kristian, Hayes, Matthew J., Sijacki, Debora, Naidu, Rohan P., Matthee, Jorryt, Valentino, Francesco, Tanvir, Nial R., Jakobsson, Páll, Laursen, Peter, Watson, Darach J., Davé, Romeel, Keating, Laura C., Covelo-Paz, Alba
Galaxy clusters are the most massive, gravitationally-bound structures in the Universe, emerging through hierarchical structure formation of large-scale dark matter and baryon overdensities. Early galaxy ``proto-clusters'' are believed to be importan
Externí odkaz:
http://arxiv.org/abs/2407.06287
How do galaxies of different luminosities contribute to the metal absorber populations of varying species and strength? We present our analysis of the predicted metal contributions from galaxies as observed in quasar absorption line spectra during th
Externí odkaz:
http://arxiv.org/abs/2405.00177
We implement a treatment of Helium {\sc ii} absorption and re-emission into the \TD cosmological simulations to study its impact on the metagalactic ultraviolet background (UVB) in three dimensions. By comparing simulations with and without He {\sc i
Externí odkaz:
http://arxiv.org/abs/2404.00193
Autor:
Wu, Yunjing, Cai, Zheng, Li, Jianan, Finlator, Kristian, Neeleman, Marcel, Prochaska, J. Xavier, Emonts, Bjorn H. C., Zhang, Shiwu, Wang, Feige, Yang, Jinyi, Wang, Ran, Fan, Xiaohui, Xu, Dandan, Golden-Marx, Emmet, Keating, Laura C., Hennawi, Joseph F.
We report the first statistical analyses of [CII] and dust continuum observations in six strong OI absorber fields at the end of the reionization epoch obtained by the Atacama Large Millimeter/Submillimeter Array (ALMA). Combined with one [CII] emitt
Externí odkaz:
http://arxiv.org/abs/2310.03796
Autor:
Wu, Yunjing, Wang, Feige, Cai, Zheng, Fan, Xiaohui, Finlator, Kristian, Yang, Jinyi, Hennawi, Joseph F., Sun, Fengwu, Champagne, Jaclyn B., Lin, Xiaojing, Li, Zihao, Chen, Zuyi, Bañados, Eduardo, Becker, George D., Bosman, Sarah E. I., Bruzual, Gstavo, Charlot, Stephane, Chen, Hsiao-Wen, Chevallard, Jacopo, Eilers, Anna-Christina, Farina, Emanuele Paolo, Jin, Xiangyu, Jun, Hyunsung D., Kakiichi, Koki, Li, Mingyu, Liu, Weizhe, Pudoka, Maria A., Tee, Wei Leong, Xie, Zhang-Liang, Zou, Siwei
The launch of ${\it JWST}$ opens a new window for studying the connection between metal-line absorbers and galaxies at the end of the Epoch of Reionization (EoR). Previous studies have detected absorber-galaxy pairs in limited quantities through grou
Externí odkaz:
http://arxiv.org/abs/2309.16757
Probing the Metal Enrichment of the Intergalactic Medium at z = 5–6 Using the Hubble Space Telescope
We test the galactic outflow model by probing associated galaxies of four strong intergalactic C IV absorbers at z = 5-6 using the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) ramp narrowband filters. The four strong C IV absorbers
Externí odkaz:
http://hdl.handle.net/10150/626049
http://arizona.openrepository.com/arizona/handle/10150/626049
http://arizona.openrepository.com/arizona/handle/10150/626049
Autor:
Simons, Raymond C., Papovich, Casey, Momcheva, Ivelina G., Brammer, Gabriel, Estrada-Carpenter, Vicente, Finkelstein, Steven L., Gosmeyer, Catherine M., Matharu, Jasleen, Trump, Jonathan R., Backhaus, Bren E., Cheng, Yingjie, Cleri, Nikko J., Ferguson, Henry C., Finlator, Kristian, Giavalisco, Mauro, Ji, Zhiyuan, Jung, Intae, Lotz, Jennifer M., O'Brien, Rosalia, Skelton, Rosalind E., Tilvi, Vithal, Weiner, Benjamin
We present an overview of the CANDELS Lyman-a Emission At Reionization (CLEAR) survey. CLEAR is a 130 orbit program of the Hubble Space Telescope using the Wide Field Camera 3 (WFC3) IR G102 grism. CLEAR targets 12 pointings divided between the GOODS
Externí odkaz:
http://arxiv.org/abs/2303.09570
Publikováno v:
Astrophys. J. 941 (2022) 180-190
It has been well established in the local universe that galaxy properties differ based on the large-scale environment in which they reside. As luminous Lyman-alpha nebulae have been shown to trace overdense environments at z~2-3, comparing the proper
Externí odkaz:
http://arxiv.org/abs/2301.02755
A growing population of metal absorbers are observed at z>5, many showing strong evolution in incidence approaching the epoch of hydrogen reionization. Follow-up surveys examining fields around these metals have resulted in galaxy detections but the
Externí odkaz:
http://arxiv.org/abs/2211.07313
ALMA reveals extended cool gas and hot ionized outflows in a typical star-forming galaxy at $z=7.13$
Autor:
Akins, Hollis, Fujimoto, Seiji, Finlator, Kristian, Watson, Darach, Knudsen, Kirsten, Richard, Johan, Bakx, Tom, Hashimoto, Takuya, Inoue, Akio, Matsuo, Hiroshi, Michalowski, Michal, Tamura, Yoichi
We present spatially-resolved morphological properties of [CII] 158 $\mu$m, [OIII] 88 $\mu$m, dust, and rest-frame ultraviolet (UV) continuum emission for A1689-zD1, a strongly lensed, sub-L* galaxy at $z=7.13$, by utilizing deep Atacama Large Millim
Externí odkaz:
http://arxiv.org/abs/2206.06939