Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Villafana, Lizvette"'
Autor:
Villafaña, Lizvette, Williams, Peter R., Treu, Tommaso, Brewer, Brendon J., Barth, Aaron J., U, Vivian, Bennert, Vardha N., Guo, Hengxiao, Bentz, Misty C., Canalizo, Gabriela, Filippenko, Alexei V., Gates, Elinor, Joner, Michael D., Malkan, Matthew A., Woo, Jong-Hak, Abolfathi, Bela, Bohn, Thomas, Bostroem, K. Azalee, Brandel, Andrew, Brink, Thomas G., Channa, Sanyum, Cosens, Maren, Donohue, Edward, Halevi, Goni, Hood, Carol E., Horst, J. Chuck, de Kouchkovsky, Maxime, Kuhn, Benjamin, Leonard, Douglas C., Michel, Raul, Olaes, Melanie Kae B., Park, Daeseong, Runco, Jordan N., Sexton, Remington O., Shivvers, Isaac, Spencer, Chance L., Stahl, Benjamin E., Stegman, Samantha, Walsh, Jonelle L., Zheng, WeiKang
We combine our dynamical modeling black hole mass measurements from the Lick AGN Monitoring Project 2016 sample with measured cross-correlation time lags and line widths to recover individual scale factors, f, used in traditional reverberation mappin
Externí odkaz:
http://arxiv.org/abs/2304.06764
Autor:
Shajib, Anowar J., Mozumdar, Pritom, Chen, Geoff C. -F., Treu, Tommaso, Cappellari, Michele, Knabel, Shawn, Suyu, Sherry H., Bennert, Vardha N., Frieman, Joshua A., Sluse, Dominique, Birrer, Simon, Courbin, Frederic, Fassnacht, Christopher D., Villafaña, Lizvette, Williams, Peter R.
Publikováno v:
A&A 673, A9 (2023)
Strong-lensing time delays enable measurement of the Hubble constant ($H_{0}$) independently of other traditional methods. The main limitation to the precision of time-delay cosmography is mass-sheet degeneracy (MSD). Some of the previous TDCOSMO ana
Externí odkaz:
http://arxiv.org/abs/2301.02656
Autor:
Villafaña, Lizvette, Williams, Peter R., Treu, Tommaso, Brewer, Brendon J., Barth, Aaron J., U, Vivian, Bennert, Vardha N., Vogler, H. Alexander, Guo, Hengxiao, Bentz, Misty C., Canalizo, Gabriela, Filippenko, Alexei V., Gates, Elinor, Hamann, Frederick, Joner, Michael D., Malkan, Matthew A., Woo, Jong-Hak, Abolfathi, Bela, Abramson, L. E., Armen, Stephen F., Bae, Hyun-Jin, Bohn, Thomas, Boizelle, Benjamin D., Bostroem, Azalee, Brandel, Andrew, Brink, Thomas G., Channa, Sanyum, Cooper, M. C., Cosens, Maren, Donohue, Edward, Fillingham, Sean P., Gonzalez-Buitrago, Diego, Halevi, Goni, Halle, Andrew, Hood, Carol E., Horne, Keith, Horst, J. Chuck, de Kouchkovsky, Maxime, Kuhn, Benjamin, Kumar, Sahana, Leonard, Douglas C., Loveland, Donald, Manzano-King, Christina, McHardy, Ian, Michel, Raul, Olaes, Melanie Kae B., Park, Daeseong, Park, Songyoun, Pei, Liuyi, Ross, Timothy W., Runco, Jordan N., Samuel, Jenna, Sanchez, Javier, Scott, Bryan, Sexton, Remington O., Shin, Jaejin, Shivvers, Isaac, Spencer, Chance L., Stahl, Benjamin E., Stegman, Samantha, Stomberg, Isak, Valenti, Stefano, Walsh, Jonelle L., Yuk, Heechan, Zheng, WeiKang
We have modeled the velocity-resolved reverberation response of the H\b{eta} broad emission line in nine Seyfert 1 galaxies from the Lick Active Galactic Nucleus (AGN) Monitioring Project 2016 sample, drawing inferences on the geometry and structure
Externí odkaz:
http://arxiv.org/abs/2203.15000
Autor:
Margot, Jean-Luc, Pinchuk, Pavlo, Geil, Robert, Alexander, Stephen, Arora, Sparsh, Biswas, Swagata, Cebreros, Jose, Desai, Sanjana Prabhu, Duclos, Benjamin, Dunne, Riley, Lin, Kristy Kwan, Goel, Shashwat, Gonzales, Julia, Gonzalez, Alexander, Jain, Rishabh, Lam, Adrian, Lewis, Briley, Lewis, Rebecca, Li, Grace, MacDougall, Mason, Makarem, Christopher, Manan, Ivan, Molina, Eden, Nagib, Caroline, Neville, Kyle, O'Toole, Connor, Rockwell, Valerie, Rokushima, Yoichiro, Romanek, Griffin, Schmidgall, Carlyn, Seth, Samar, Shah, Rehan, Shimane, Yuri, Singhal, Myank, Tokadjian, Armen, Villafana, Lizvette, Wang, Zhixian, Yun, In, Zhu, Lujia, Lynch, Ryan S.
We conducted a search for technosignatures in April of 2018 and 2019 with the L-band receiver (1.15-1.73 GHz) of the 100 m diameter Green Bank Telescope. These observations focused on regions surrounding 31 Sun-like stars near the plane of the Galaxy
Externí odkaz:
http://arxiv.org/abs/2011.05265
Akademický článek
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Autor:
Shajib, Anowar J., Mozumdar, Pritom, Chen, Geoff C. -F., Treu, Tommaso, Cappellari, Michele, Knabel, Shawn, Suyu, Sherry H., Bennert, Vardha N., Frieman, Joshua A., Sluse, Dominique, Birrer, Simon, Courbin, Frederic, Fassnacht, Christopher D., Villafana, Lizvette, Williams, Peter R.
Strong-lensing time delays enable the measurement of the Hubble constant (H0) independently of other traditional methods. The main limitation to the precision of time-delay cosmography is mass-sheet degeneracy (MSD). Some of the previous TDCOSMO anal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______185::b04b68a8a039a689dd49b982283fbd80
https://infoscience.epfl.ch/record/303154
https://infoscience.epfl.ch/record/303154