Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Oliver, Sebastian"'
Publikováno v:
In The Knee March 2024 47:139-150
To ChatGPT, or not to ChatGPT: Navigating the paradoxes of generative AI in the advertising industry
Autor:
Osadchaya, Elena, Marder, Ben, Yule, Jennifer A., Yau, Amy, Lavertu, Laura, Stylos, Nikolaos, Oliver, Sebastian, Angell, Rob, Regt, Anouk de, Gao, Liyu, Qi, Kang, Zhang, Will Zhiyuan, Zhang, Yiwei, Li, Jiayuan, AlRabiah, Sara
Publikováno v:
In Business Horizons
Akademický článek
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Akademický článek
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Autor:
Pitchford, Lura K., Hatziminaoglou, Evanthia, Feltre, Anna, Farrah, Duncan, Clarke, Charlotte, Harris, Kathryn, Hurley, Peter, Oliver, Sebastian, Page, Mathew, Wang, Lingyu
We explore the relationship between active galactic nuclei and star formation in a sample of 513 optically luminous type 1 quasars up to redshifts of $\sim$4 hosting extremely high star formation rates (SFRs). The quasars are selected to be individua
Externí odkaz:
http://arxiv.org/abs/1607.06459
Autor:
Harris, Kathryn, Farrah, Duncan, Schulz, Bernhard, Hatziminaoglou, Evanthia, Viero, Marco, Anderson, Nick, Bethermin, Matthieu, Chapman, Scott, Clements, David L., Cooray, Asantha, Efstathiou, Andreas, Feltre, Anne, Hurley, Peter, Ibar, Eduardo, Lacy, Mark, Oliver, Sebastian, Page, Mathew J., Perez-Fournon, Ismael, Petty, Sara M., Pitchford, Lura K., Rigopoulou, Dimitra, Scott, Douglas, Symeonidis, Myrto, Vieira, Joaquin, Wang, Lingyu
We investigate the relation between star formation rates ($\dot{M}_{s}$) and AGN properties in optically selected type 1 quasars at $2
Externí odkaz:
http://arxiv.org/abs/1602.02755
Autor:
Marder, Ben, Oliver, Sebastian, Yau, Amy, Lavertu, Laura, Perier, Claire, Frank, Mats, Cowan, Kirsten
Publikováno v:
In The International Journal of Management Education March 2021 19(1)
Autor:
Shupe, David L., Rowan-Robinson, Michael, Lonsdale, Carol J., Masci, Frank, Evans, Tracey, Fang, Fan, Oliver, Sebastian, Vaccari, Mattia, Rodighiero, Giulia, Padgett, Deborah, Surace, Jason A., Xu, C. Kevin, Berta, Stefano, Pozzi, Francesca, Franceschini, Alberto, Babbedge, Thomas, Gonzales-Solares, Eduardo, Siana, Brian D., Farrah, Duncan, Frayer, David T., Smith, H. E., Polletta, Maria, Owen, Frazer, Perez-Fournon, Ismael
This paper presents galaxy source counts at 24 microns in the six Spitzer Wide-field InfraRed Extragalactic (SWIRE) fields. The source counts are compared to counts in other fields, and to model predictions that have been updated since the launch of
Externí odkaz:
http://arxiv.org/abs/0711.2026
Autor:
Kawada, Mitsunobu, Baba, Hajime, Barthel, Peter D., Clements, David, Cohen, Martin, Doi, Yasuo, Figueredo, Elysandra, Fujiwara, Mikio, Goto, Tomotsugu, Hasegawa, Sunao, Hibi, Yasunori, Hirao, Takanori, Hiromoto, Norihisa, Jeong, Woong-Seob, Kaneda, Hidehiro, Kawai, Toshihide, Kawamura, Akiko, Kester, Do, Kii, Tsuneo, Kobayashi, Hisato, Kwon, Suk Minn, Lee, Hyung Mok, Makiuti, Sin'itirou, Matsuo, Hiroshi, Matsuura, Shuji, Müller, Thomas G., Murakami, Noriko, Nagata, Hirohisa, Nakagawa, Takao, Narita, Masanao, Noda, Manabu, Oh, Sang Hoon, Okada, Yoko, Okuda, Haruyuki, Oliver, Sebastian, Ootsubo, Takafumi, Pak, Soojong, Park, Yong-Sun, Pearson, Chris P., Rowan-Robinson, Michael, Saito, Toshinobu, Salama, Alberto, Sato, Shinji, Savage, Richard S., Serjeant, Stephen, Shibai, Hiroshi, Shirahata, Mai, Sohn, Jungjoo, Suzuki, Toyoaki, Takagi, Toshinobu, Takahashi, Hidenori, Thomson, Matthew, Usui, Fumihiko, Verdugo, Eva, Watabe, Toyoki, White, Glenn J., Wang, Lingyu, Yamamura, Issei, Yamamuchi, Chisato, Yasuda, Akiko
The Far-Infrared Surveyor (FIS) is one of two focal plane instruments on the AKARI satellite. FIS has four photometric bands at 65, 90, 140, and 160 um, and uses two kinds of array detectors. The FIS arrays and optics are designed to sweep the sky wi
Externí odkaz:
http://arxiv.org/abs/0708.3004
Autor:
Glazebrook, Karl, Verma, Aprajita, Boyle, Brian, Oliver, Sebastian, Mann, Robert G., Monbleau, Davienne
Publikováno v:
Astron.J.131:2383-2393,2006
We present a deep photometric (B- and R-band) catalog and an associated spectroscopic redshift survey conducted in the vicinity of the Hubble Deep Field South. The spectroscopy yields 53 extragalactic redshifts in the range 0
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601112