Zobrazeno 1 - 10
of 55
pro vyhledávání: '"Eisenhardt, Peter R. M."'
Autor:
Trudeau, A., Gonzalez, Anthony H., Thongkham, K., Lee, Kyoung-Soo, Alberts, Stacey, Brodwin, M., Connor, Thomas, Eisenhardt, Peter R. M., Moravec, Emily, Puvvada, Eshwar, Stanford, S. A.
The evolution of galaxies depends on their masses and local environments; understanding when and how environmental quenching starts to operate remains a challenge. Furthermore, studies of the high-redshift regime have been limited to massive cluster
Externí odkaz:
http://arxiv.org/abs/2406.03633
Autor:
Li, Guodong, Assef, Roberto J., Tsai, Chao-Wei, Wu, Jingwen, Eisenhardt, Peter R. M., Stern, Daniel, Díaz-Santos, Tanio, Blain, Andrew W., Jun, Hyunsung D., Arandá, Roman Fernández, Zewdie, Dejene
Hot Dust-Obscured Galaxies (Hot DOGs) are a rare population of hyper-luminous infrared galaxies discovered by the WISE mission. Despite the significant obscuration of the AGN by dust in these systems, pronounced broad and blue-shifted emission lines
Externí odkaz:
http://arxiv.org/abs/2405.20479
Autor:
Marocco, Federico, Kirkpatrick, J. Davy, Schneider, Adam C., Meisner, Aaron M., Popinchalk, Mark, Gelino, Christopher R., Faherty, Jacqueline K., Burgasser, Adam J., Caselden, Dan, Gagné, Jonathan, Aganze, Christian, Bardalez-Gagliuffi, Daniella C., Casewell, Sarah L., Hsu, Chih-Chun, Kiman, Rocio, Eisenhardt, Peter R. M., Kuchner, Marc J., Stern, Daniel, Gramaize, Léopold, Sainio, Arttu, Bickle, Thomas P., Rothermich, Austin, Pendrill, William, Thévenot, Melina, Kabatnik, Martin, Colombo, Giovanni, Higashimura, Hiro, Kiwy, Frank, Marchese, Elijah J., Andersen, Nikolaj Stevnbak, Tanner, Christopher, Walla, Jim, Wedracki, Zbigniew, Collaboration, The Backyard Worlds
We present the discovery of 13 new widely separated T dwarf companions to M dwarf primaries, identified using WISE/NEOWISE data by the CatWISE and Backyard Worlds: Planet 9 projects. This sample represents a $\sim$60% increase in the number of known
Externí odkaz:
http://arxiv.org/abs/2404.14324
Autor:
Aranda, Román Fernández, Santos, Tanio Díaz, Hatziminaoglou, Evanthia, Assef, Roberto J., Aravena, Manuel, Eisenhardt, Peter R. M., Ferkinhoff, Carl, Pensabene, Antonio, Nikola, Thomas, Andreani, Paola, Vishwas, Amit, Stacey, Gordon J., Decarli, Roberto, Blain, Andrew W., Brisbin, Drew, Charmandaris, Vassilis, Jun, Hyunsung D., Li, Guodong, Liao, Mai, Martin, Lee R., Stern, Daniel, Tsai, Chao-Wei, Wu, Jingwen, Zewdie, Dejene
WISE J224607.6-052634.9 (W2246-0526) is a hot dust-obscured galaxy at $z$ = 4.601, and the most luminous obscured quasar known to date. W2246-0526 harbors a heavily obscured supermassive black hole that is most likely accreting above the Eddington li
Externí odkaz:
http://arxiv.org/abs/2401.01871
Autor:
Mainzer, A. K., Masiero, Joseph R., Abell, Paul A., Bauer, J. M., Bottke, William, Buratti, Bonnie J., Carey, Sean J., Cotto-Figueroa, D., Cutri, R. M., Dahlen, D., Eisenhardt, Peter R. M., Fernandez, 6 Y. R., Furfaro, Roberto, Grav, Tommy, Hoffman, T. L., Kelley, Michael S., Kim, Yoonyoung, Kirkpatrick, J. Davy, Lawler, Christopher R., Lilly, Eva, Liu, X., Marocco, Federico, Marsh, K. A., Masci, Frank J., McMurtry, Craig W., Pourrahmani, Milad, Reinhart, Lennon, Ressler, Michael E., Satpathy, Akash, Schambeau, C. A., Sonnett, S., Spahr, Timothy B., Surace, Jason A., Vaquero, Mar, Wright, E. L., Zengilowski, Gregory R., Team, NEO Surveyor Mission
The Near-Earth Object (NEO) Surveyor mission is a NASA observatory designed to discover and characterize near-Earth asteroids and comets. The mission's primary objective is to find the majority of objects large enough to cause severe regional impact
Externí odkaz:
http://arxiv.org/abs/2310.12918
Autor:
Zewdie, Dejene, Assef, Roberto J., Mazzucchelli, Chiara, Aravena, Manuel, Blain, Andrew W., Díaz-Santos, Tanio, Eisenhardt, Peter R. M., Jun, Hyunsung D., Stern, Daniel, Tsai, Chao-Wei, Wu, "and" Jingwen W.
Publikováno v:
A&A 677, A54 (2023)
We report the identification of Lyman Break Galaxy (LBG) candidates around the most luminous Hot Dust-Obscured Galaxy (Hot DOG) known, WISE J224607.56$-$052634.9 (W2246$-$0526) at $z=4.601$, using deep \textit{r}-, \textit{i}-, and \textit{z}-band im
Externí odkaz:
http://arxiv.org/abs/2306.17163
Autor:
Li, Guodong, Tsai, Chao-Wei, Stern, Daniel, Wu, Jingwen, Assef, Roberto J., Blain, Andrew W., Díaz-Santos, Tanio, Eisenhardt, Peter R. M., Griffith, Roger L., Jarrett, Thomas H., Jun, Hyunsung D., Lake, Sean E., Saade, M. Lynne
Publikováno v:
The Astrophysical Journal, Volume 958, Number 2, 2023
We report the discovery of the hyperluminous, highly obscured AGN WISE J190445.04+485308.9 (W1904+4853 hereafter, $L_{bol} = 1.1 \times 10^{13} \ L_{\odot}$) at z=0.415. Its well-sampled spectral energy distribution (SED) is dominated by infrared dus
Externí odkaz:
http://arxiv.org/abs/2305.13739
Autor:
Assef, Roberto J., Bauer, Franz E., Blain, Andrew W., Brightman, Murray, Díaz-Santos, Tanio, Eisenhardt, Peter R. M., Jun, Hyunsung D., Stern, Daniel, Tsai, Chao-Wei, Walton, Dominic J., Wu, Jingwen
We report on VLT/FORS2 imaging polarimetry observations in the $R_{\rm special}$ band of WISE J011601.41-050504.0 (W0116-0505), a heavily obscured hyper-luminous quasar at $z=3.173$ classified as a Hot, Dust-Obscured Galaxy (Hot DOG) based on its mid
Externí odkaz:
http://arxiv.org/abs/2206.04093
Autor:
Alberts, Stacey, Adams, Jéa, Gregg, Benjamin, Pope, Alexandra, Williams, Christina C., Eisenhardt, Peter R. M.
We present the average gas properties derived from ALMA Band 6 dust continuum imaging of 126 massive (log $M_{\star} / M_{\odot} \gtrsim 10.5$), star-forming cluster galaxies across 11 galaxy clusters at $z=1-1.75$. Using stacking analysis on the ALM
Externí odkaz:
http://arxiv.org/abs/2201.01307
Autor:
Decker, Bandon, Brodwin, Mark, Saha, Ripon, Connor, Thomas, Eisenhardt, Peter R. M., Gonzalez, Anthony H., Moravec, Emily, Muhibullah, Mustafa, Stanford, S. Adam, Stern, Daniel, Thongkham, Khunanon, Wylezalek, Dominika, Dicker, Simon R., Mason, Brian, Mroczkowski, Tony, Romero, Charles E., Ruppin, Florian
We present stellar mass fractions and composite luminosity functions (LFs) for a sample of \Ncl\ clusters from the Massive and Distant Clusters of WISE Survey (MaDCoWS) at a redshift range of $0.951 \leq z \leq 1.43$. Using SED fitting of optical and
Externí odkaz:
http://arxiv.org/abs/2112.12239