Zobrazeno 1 - 10
of 918
pro vyhledávání: '"BROWN, Michael J."'
Autor:
Bird, Robert E., Pretti, Giuliano, Coombs, William M., Augarde, Charles E., Sharif, Yaseen U., Brown, Michael J., Carter, Gareth, Macdonald, Catriona, Johnson, Kirstin
Accurate and robust modelling of large deformation three dimensional contact interaction is an important area of engineering, but it is also challenging from a computational mechanics perspective. This is particularly the case when there is significa
Externí odkaz:
http://arxiv.org/abs/2412.01565
Autor:
Martínez-Ramírez, L. N., Rivera, G. Calistro, Lusso, Elisabeta, Bauer, F. E., Nardini, Emanuele, Buchner, Johannes, Brown, Michael J. I., Pineda, Juan C. B., Temple, Matthew J., Banerji, Manda, Stalevski, M., Hennawi, Joseph F.
We present new frontiers in the modelling of the spectral energy distributions (SED) of active galaxies by introducing the radio-to-X-ray fitting capabilities of the publicly available Bayesian code AGNfitter. The new code release, called AGNfitter-r
Externí odkaz:
http://arxiv.org/abs/2405.12111
Autor:
Prathap, Jahang, Hopkins, Andrew M., Robotham, Aaron S. G., Bellstedt, Sabine, Afonso, José, Ahmed, Ummee T., Bilicki, Maciej, Bremer, Malcolm N., Brough, Sarah, Brown, Michael J. I., Gordon, Yjan, Holwerda, Benne W., Leahy, Denis, López-Sánchez, Ángel R., Marvil, Joshua R., Mukherjee, Tamal, Prandoni, Isabella, Shabala, Stanislav S., Vernstrom, Tessa, Zafar, Tayyaba
We propose a new method for identifying active galactic nuclei (AGN) in low mass ($\rm M_*\leq10^{10}M_\odot$) galaxies. This method relies on spectral energy distribution (SED) fitting to identify galaxies whose radio flux density has an excess over
Externí odkaz:
http://arxiv.org/abs/2402.11817
All very massive early-type galaxies contain supermassive blackholes but are these blackholes all sufficiently active to produce detectable radio continuum sources? We have used the 887.5~MHz Rapid ASKAP Continuum Survey DR1 to measure the radio emis
Externí odkaz:
http://arxiv.org/abs/2311.15456
Autor:
Bianchin, Marina, U, Vivian, Song, Yiqing, Lai, Thomas S. -Y., Remigio, Raymond P., Barcos-Munoz, Loreto, Diaz-Santos, Tanio, Armus, Lee, Inami, Hanae, Larson, Kirsten L., Evans, Aaron S., Boker, Torsten, Kader, Justin A., Linden, Sean T., Charmandaris, Vassilis, Malkan, Matthew A., Rich, Jeff, Bohn, Thomas, Medling, Anne M., Stierwalt, Sabrina, Mazzarella, Joseph M., Law, David R., Privon, George C., Aalto, Susanne, Appleton, Philip, Brown, Michael J. I., Buiten, Victorine A., Finnerty, Luke, Hayward, Christopher C., Howell, Justin, Iwasawa, Kazushi, Kemper, Francisca, Marshall, Jason, McKinney, Jed, Muller-Sanchez, Francisco, Murphy, Eric J., van der Werf, Paul P., Sanders, David B., Surace, Jason
We present new JWST-NIRSpec IFS data for the luminous infrared galaxy NGC7469: a nearby (70.6Mpc) active galaxy with a Sy 1.5 nucleus that drives a highly ionized gas outflow and a prominent nuclear star-forming ring. Using the superb sensitivity and
Externí odkaz:
http://arxiv.org/abs/2308.00209
GOALS-JWST: Small neutral grains and enhanced 3.3 micron PAH emission in the Seyfert galaxy NGC 7469
Autor:
Lai, Thomas S. -Y., Armus, Lee, Bianchin, Marina, Diaz-Santos, Tanio, Linden, Sean T., Privon, George C., Inami, Hanae, U, Vivian, Bohn, Thomas, Evans, Aaron S., Larson, Kirsten L., Hensley, Brandon S., Smith, J. -D. T., Malkan, Matthew A., Song, Yiqing, Stierwalt, Sabrina, van der Werf, Paul P., McKinney, Jed, Aalto, Susanne, Buiten, Victorine A., Rich, Jeff, Charmandaris, Vassilis, Appleton, Philip, Barcos-Munoz, Loreto, Boker, Torsten, Finnerty, Luke, Kader, Justin A., Law, David R., Brown, Michael J. I., Hayward, Christopher C., Howell, Justin, Iwasawa, Kazushi, Kemper, Francisca, Marshall, Jason, Mazzarella, Joseph M., Muller-Sanchez, Francisco, Murphy, Eric J., Sanders, David, Surace, Jason
We present James Webb Space Telescope (JWST) Near Infrared Spectrograph (NIRSpec) integral-field spectroscopy of the nearby luminous infrared galaxy, NGC 7469. We take advantage of the high spatial/spectral resolution and wavelength coverage of JWST
Externí odkaz:
http://arxiv.org/abs/2307.15169
Autor:
Alatalo, Katherine, Bitsakis, Theodoros, Lanz, Lauranne, Lacy, Mark, Brown, Michael J. I., French, K. Decker, Ciesla, Laure, Appleton, Philip N., Beaton, Rachael L., Cales, Sabrina L., Crossett, Jacob, Falcón-Barroso, Jesús, Kelson, Daniel D., Kewley, Lisa J., Kriek, Mariska, Medling, Anne M., Mulchaey, John S., Nyland, Kristina, Rich, Jeffrey A., Urry, C. Meg
We investigate the optical and Wide-field Survey Explorer (WISE) colors of "E+A" identified post-starburst galaxies, including a deep analysis of 190 post-starbursts detected in the 2 mu m All Sky Survey Extended Source Catalog. The post-starburst ga
Externí odkaz:
http://hdl.handle.net/10150/624929
http://arizona.openrepository.com/arizona/handle/10150/624929
http://arizona.openrepository.com/arizona/handle/10150/624929
Autor:
Chen(陳建廷), Chien-Ting J., Hickox, Ryan C., Goulding, Andrew D., Stern, Daniel, Assef, Roberto, Kochanek, Christopher S., Brown, Michael J. I., Harrison, Chris M., Hainline, Kevin N., Alberts, Stacey, Alexander, David M., Brodwin, Mark, Moro, Agnese Del, Forman, William R., Gorjian, Varoujan, Jones, Christine, Murray, Stephen S., Pope, Alexandra, Rovilos, Emmanouel
Several recent studies have reported different intrinsic correlations between the active galactic nucleus (AGN) mid-IR luminosity (L-MIR) and the rest-frame 2-10 keV luminosity (L-X) for luminous quasars. To understand the origin of the difference in
Externí odkaz:
http://hdl.handle.net/10150/623867
http://arizona.openrepository.com/arizona/handle/10150/623867
http://arizona.openrepository.com/arizona/handle/10150/623867
Autor:
Pacifici, Camilla, Iyer, Kartheik G., Mobasher, Bahram, da Cunha, Elisabete, Acquaviva, Viviana, Burgarella, Denis, Rivera, Gabriela Calistro, Carnall, Adam C., Chang, Yu-Yen, Chartab, Nima, Cooke, Kevin C., Fairhurst, Ciaran, Kartaltepe, Jeyhan, Leja, Joel, Malek, Katarzyna, Salmon, Brett, Torelli, Marianna, Vidal-Garcia, Alba, Boquien, Mederic, Brammer, Gabriel G., Brown, Michael J. I., Capak, Peter L., Chevallard, Jacopo, Circosta, Chiara, Croton, Darren, Davidzon, Iary, Dickinson, Mark, Duncan, Kenneth J., Faber, Sandra M., Ferguson, Harry C., Fontana, Adriano, Guo, Yicheng, Haeussler, Boris, Hemmati, Shoubaneh, Jafariyazani, Marziye, Kassin, Susan A., Larson, Rebecca L., Lee, Bomee, Mantha, Kameswara Bharadwaj, Marchi, Francesca, Nayyeri, Hooshang, Newman, Jeffrey A., Pandya, Viraj, Pforr, Janine, Reddy, Naveen, Sanders, Ryan, Shah, Ekta, Shahidi, Abtin, Stevans, Matthew L., Triani, Dian Puspita, Tyler, Krystal D., Vanderhoof, Brittany N., de la Vega, Alexander, Wang, Weichen, Weston, Madalyn E.
The study of galaxy evolution hinges on our ability to interpret multi-wavelength galaxy observations in terms of their physical properties. To do this, we rely on spectral energy distribution (SED) models which allow us to infer physical parameters
Externí odkaz:
http://arxiv.org/abs/2212.01915