Zobrazeno 1 - 10
of 4 081
pro vyhledávání: '"P. Ogle"'
Autor:
Liu, Weizhe, Veilleux, Sylvain, Sankar, Swetha, Rupke, David S. N., Zakamska, Nadia L., Wylezalek, Dominika, Vayner, Andrey, Bertemes, Caroline, Chen, Yu-Ching, Ishikawa, Yuzo, Greene, Jenny E., Heckman, Timothy, Liu, Guilin, Chen, Hsiao-Wen, Lutz, Dieter, Johnson, Sean D., Nesvadba, Nicole P. H., Ogle, Patrick, Diachenko, Nadiia, Goulding, Andy D., Hainline, Kevin N., Hamann, Fred, Lim, Hui Xian Grace, Lützgendorf, Nora, Mainieri, Vincenzo, McCrory, Ryan, Murphree, Grey, Sturm, Eckhard, Whitesell, Lillian
Quasar feedback may play a key role in the evolution of massive galaxies. The dust-reddened quasar, F2M110648.35$+$480712 at $z = 0.4352$ is one of the few cases at its redshift that exhibits powerful quasar feedback through bipolar outflows. Our new
Externí odkaz:
http://arxiv.org/abs/2410.14291
Autor:
Otter, Justin Atsushi, Alatalo, Katherine, Rowlands, Kate, McDermid, Richard M., Davis, Timothy A., Federrath, Christoph, French, K. Decker, Heckman, Timothy, Ogle, Patrick, Kakkad, Darshan, Luo, Yuanze, Nyland, Kristina, Tripathi, Akshat, Patil, Pallavi, Petric, Andreea, Smercina, Adam, Skarbinski, Maya, Lanz, Lauranne, Larson, Kristin, Appleton, Philip N., Aalto, Susanne, Olander, Gustav, Sazonova, Elizaveta, Smith, J. D. T.
We present Gemini near-infrared integral field spectrograph (NIFS) K-band observations of the central 400 pc of NGC 1266, a nearby (D$\approx$30 Mpc) post-starburst galaxy with a powerful multi-phase outflow and a shocked ISM. We detect 7 H$_2$ ro-vi
Externí odkaz:
http://arxiv.org/abs/2409.17319
The modern power grid has seen a rise in the integration of non-linear loads, presenting a significant concern for operators. These loads introduce unwanted harmonics, leading to potential issues such as overheating and improper functioning of circui
Externí odkaz:
http://arxiv.org/abs/2407.21259
Autor:
Solimano, M., González-López, J., Aravena, M., Pampliega, B. Alcalde, Assef, R. J., Béthermin, M., Boquien, M., Bovino, S., Casey, C. M., Cassata, P., da Cunha, E., Davies, R. L., De Looze, I., Ding, X., Díaz-Santos, T., Faisst, A. L., Ferrara, A., Fisher, D. B., Förster-Schreiber, N. M., Fujimoto, S., Ginolfi, M., Gruppioni, C., Guaita, L., Hathi, N., Herrera-Camus, R., Ibar, E., Inami, H., Jones, G. C., Koekemoer, A. M., Lee, L., Li, J., Liu, D., Liu, Z., Molina, J., Ogle, P., Posses, A. C., Pozzi, F., Relaño, M., Riechers, D. A., Romano, M., Spilker, J., Sulzenauer, N., Telikova, K., Vallini, L., Vasan, K. G. C., Veilleux, S., Vergani, D., Villanueva, V., Wang, W., Yan, L., Zamorani, G.
We present new JWST/NIRSpec IFU observations of the J1000+0234 system at $z=4.54$, the dense core of a galaxy protocluster hosting a massive, dusty star forming galaxy (DSFG) with a low luminosity radio counterpart. The new data reveals two extended,
Externí odkaz:
http://arxiv.org/abs/2407.13020
Autor:
P. N. Appleton, P. Guillard, Bjorn Emonts, Francois Boulanger, Aditya Togi, William T. Reach, Kathleen Alatalo, M. Cluver, T. Diaz Santos, P.-A. Duc, S. Gallagher, P. Ogle, E. O’Sullivan, K. Voggel, C. K. Xu
Publikováno v:
The Astrophysical Journal, Vol 951, Iss 2, p 104 (2023)
We combine James Webb Space Telescope (JWST) and Hubble Space Telescope imaging with Atacama Large Millimeter Array CO(2–1) spectroscopy to study the highly turbulent multiphase intergalactic medium (IGM) in Stephan’s Quintet on 25–150 pc scale
Externí odkaz:
https://doaj.org/article/d6c0761fe52f44b58477ed20c48f67ea
Autor:
Ren, Bin B., Fogarty, Kevin, Debes, John H., Meyer, Eileen T., Mo, Youbin, Mawet, Dimitri, Perrin, Marshall D., Ogle, Patrick M., Sahlmann, Johannes
The close-in regions of bright quasars' host galaxies have been difficult to image due to the overwhelming light from the quasars. With coronagraphic observations in visible light using the Space Telescope Imaging Spectrograph (STIS) on the Hubble Sp
Externí odkaz:
http://arxiv.org/abs/2402.09505
One of the primary impediments hindering the widespread acceptance of autonomous vehicles (AVs) among pedestrians is their limited comprehension of AVs. This study employs virtual reality (VR) to provide pedestrians with an immersive environment for
Externí odkaz:
http://arxiv.org/abs/2401.02339
Autor:
Ogle, Patrick M., Lopez, Ivan E., Reynaldi, Victoria, Togi, Aditya, Rich, R. Michael, Roman, Javier, Caceres, Osmin, Zhuofu, Li, Donnelly, Grant, Smith, J. D. T., Appleton, Philip N., Lanz, Lauranne
Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud AGN. The inner 2.6 kpc of the galaxy appears to be overrun by shocks from the radio jet cocoon. G
Externí odkaz:
http://arxiv.org/abs/2312.01936
The prototypical powerful FR \Romannum{2} radio galaxy Cygnus A fits extremely well into the quasar/radio galaxy unified model: high polarization with an angle almost perpendicular to the radio jet and polarized flux showing broad permitted lines. It
Externí odkaz:
http://arxiv.org/abs/2310.19401
Autor:
Young, Jason, Pope, Alexandra, Sajina, Anna, Yan, Lin, Goncalves, Thiago S, Eleazer, Miriam, Alberts, Stacey, Armus, Lee, Bonato, Matteo, Dale, Daniel A., Farrah, Duncan, Ferkinhoff, Carl, Hayward, Christopher C., McKinney, Jed, Murphy, Eric J., Nesvadba, Nicole, Ogle, Patrick, Sajkov, Leonid, Veilleux, Sylvain
We present JWST/MIRI/MRS observations of an infrared luminous disk galaxy, FLS1, at z=0.54. With a lookback time of 5 Gyr, FLS1 is chronologically at the midpoint between the peak epoch of star formation and the present day. The MRS data provide maps
Externí odkaz:
http://arxiv.org/abs/2310.06900