Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Matzko, William"'
Autor:
Reefe, Michael, Satyapal, Shobita, Sexton, Remington O., Secrest, Nathan J., Matzko, William, Schwartzman, Emma, Nyland, Kristina, Canalizo, Gabriela, Rothberg, Barry, Pfeifle, Ryan W., Cann, Jenna M., Aravindan, Archana, Vazquez, Camilo, Clarke, Tracy
Local low metallicity dwarf galaxies are relics of the early universe and hold clues into the origins of supermassive black holes (SMBHs). In recent work, coronal lines have been used to unveil a population of candidate accreting black holes in dwarf
Externí odkaz:
http://arxiv.org/abs/2211.13179
Autor:
Matzko, William, Satyapal, Shobita, Ellison, Sara L., Sexton, Remington O., Secrest, Nathan J., Canalizo, Gabriela, Blecha, Laura, Patton, David R., Scudder, Jillian M.
Powerful outflows are thought to play a critical role in galaxy evolution and black hole growth. We present the first large-scale systematic study of ionised outflows in paired galaxies and post-mergers compared to a robust control sample of isolated
Externí odkaz:
http://arxiv.org/abs/2205.13668
Autor:
Cann, Jenna M., Satyapal, Shobita, Rothberg, Barry, Canalizo, Gabriela, Bohn, Thomas, LaMassa, Stephanie, Matzko, William, Blecha, Laura, Secrest, Nathan J., Seth, Anil, Böker, Torsten, Sexton, Remington O., Kamal, Lara, Schmitt, Henrique
The detection and characterization of supermassive black holes (SMBHs) in local low mass galaxies is crucial to our understanding of the origins of SMBHs. This statement assumes that low mass galaxies have had a relatively quiet cosmic history, so th
Externí odkaz:
http://arxiv.org/abs/2104.05689
Autor:
Sexton, Remington O., Matzko, William, Darden, Nicholas, Canalizo, Gabriela, Gorjian, Varoujan
We present Bayesian AGN Decomposition Analysis for SDSS Spectra (BADASS), an open source spectral analysis code designed for automatic detailed deconvolution of AGN and host galaxy spectra, implemented in Python, and designed for the next generation
Externí odkaz:
http://arxiv.org/abs/2010.09748
Autor:
Plavchan, Peter, Vasisht, Gautam, Beichman, Chas, Cegla, Heather, Dumusque, Xavier, Wang, Sharon, Gao, Peter, Dressing, Courtney, Bastien, Fabienne, Basu, Sarbani, Beatty, Thomas, Bechter, Andrew, Bechter, Eric, Blake, Cullen, Bourrier, Vincent, Cale, Bryson, Ciardi, David, Crass, Jonathan, Crepp, Justin, de Kleer, Katherine, Diddams, Scott, Eastman, Jason, Fischer, Debra, Gagné, Jonathan, Gaudi, Scott, Grier, Catherine, Hall, Richard, Halverson, Sam, Hamze, Bahaa, Casas, Enrique Herrero, Howard, Andrew, Kempton, Eliza, Latouf, Natasha, Leifer, Stephanie, Lightsey, Paul, Lisse, Casey, Martin, Emily, Matzko, William, Mawet, Dimitri, Mayo, Andrew, Newman, Patrick, Papp, Scott, Pope, Benjamin, Purcell, Bill, Quinn, Sam, Ribas, Ignasi, Rosich, Albert, Sanchez-Maes, Sophia, Tanner, Angelle, Thompson, Samantha, Vahala, Kerry, Wang, Ji, Williams, Peter, Wise, Alex, Wright, Jason
EarthFinder is a NASA Astrophysics Probe mission concept selected for study as input to the 2020 Astrophysics National Academies Decadal Survey. The EarthFinder concept is based on a dramatic shift in our understanding of how PRV measurements should
Externí odkaz:
http://arxiv.org/abs/2006.13428
Autor:
Plavchan, Peter, Barclay, Thomas, Gagné, Jonathan, Gao, Peter, Cale, Bryson, Matzko, William, Dragomir, Diana, Quinn, Sam, Feliz, Dax, Stassun, Keivan, Crossfield, Ian J. M., Berardo, David A., Latham, David W., Tieu, Ben, Anglada-Escudé, Guillem, Ricker, George, Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Rinehart, Stephen, Krishnamurthy, Akshata, Dynes, Scott, Doty, John, Adams, Fred, Afanasev, Dennis A., Beichman, Chas, Bottom, Mike, Bowler, Brendan P., Brinkworth, Carolyn, Brown, Carolyn J., Cancino, Andrew, Ciardi, David R., Clampin, Mark, Clark, Jake T., Collins, Karen, Davison, Cassy, Foreman-Mackey, Daniel, Furlan, Elise, Gaidos, Eric J., Geneser, Claire, Giddens, Frank, Gilbert, Emily, Hall, Ryan, Hellier, Coel, Henry, Todd, Horner, Jonathan, Howard, Andrew W., Huang, Chelsea, Huber, Joseph, Kane, Stephen R., Kenworthy, Matthew, Kielkopf, John, Kipping, David, Klenke, Chris, Kruse, Ethan, Latouf, Natasha, Lowrance, Patrick, Mennesson, Bertrand, Mengel, Matthew, Mills, Sean M., Morton, Tim, Narita, Norio, Newton, Elisabeth, Nishimoto, America, Okumura, Jack, Palle, Enric, Pepper, Joshua, Quintana, Elisa V., Roberge, Aki, Roccatagliata, Veronica, Schlieder, Joshua E., Tanner, Angelle, Teske, Johanna, Tinney, C. G., Vanderburg, Andrew, von Braun, Kaspar, Walp, Bernie, Wang, Jason, Wang, Sharon Xuesong, Weigand, Denise, White, Russel, Wittenmyer, Robert A., Wright, Duncan J., Youngblood, Allison, Zhang, Hui, Zilberman, Perri
AU Microscopii (AU Mic) is the second closest pre main sequence star, at a distance of 9.79 parsecs and with an age of 22 million years. AU Mic possesses a relatively rare and spatially resolved3 edge-on debris disk extending from about 35 to 210 ast
Externí odkaz:
http://arxiv.org/abs/2006.13248
Autor:
Colón, Knicole D., Kreidberg, Laura, Welbanks, Luis, Line, Michael R., Madhusudhan, Nikku, Beatty, Thomas, Tamburo, Patrick, Stevenson, Kevin B., Mandell, Avi, Rodriguez, Joseph E., Barclay, Thomas, Lopez, Eric D., Stassun, Keivan G., Angerhausen, Daniel, Fortney, Jonathan J., James, David J., Pepper, Joshua, Ahlers, John P., Plavchan, Peter, Awiphan, Supachai, Kotnik, Cliff, McLeod, Kim K., Murawski, Gabriel, Chotani, Heena, LeBrun, Danny, Matzko, William, Rea, David, Vidaurri, Monica, Webster, Scott, Williams, James K., Cox, Leafia Sheraden, Tan, Nicole, Gilbert, Emily A.
We present an optical-to-infrared transmission spectrum of the inflated sub-Saturn KELT-11b measured with the Transiting Exoplanet Survey Satellite (TESS), the Hubble Space Telescope (HST) Wide Field Camera 3 G141 spectroscopic grism, and the Spitzer
Externí odkaz:
http://arxiv.org/abs/2005.05153
Autor:
Dulz, Shannon D., Plavchan, Peter, Crepp, Justin R., Stark, Christopher, Morgan, Rhonda, Kane, Stephen R., Newman, Patrick, Matzko, William, Mulders, Gijs D.
Planet yield calculations may be used to inform the target selection strategy and science operations of space observatories. Forthcoming and proposed NASA missions, such as the Wide-Field Infrared Survey Telescope (WFIRST), the Habitable Exoplanet Im
Externí odkaz:
http://arxiv.org/abs/2003.01739
Autor:
Gaudi, B. Scott, Seager, Sara, Mennesson, Bertrand, Kiessling, Alina, Warfield, Keith, Cahoy, Kerri, Clarke, John T., Domagal-Goldman, Shawn, Feinberg, Lee, Guyon, Olivier, Kasdin, Jeremy, Mawet, Dimitri, Plavchan, Peter, Robinson, Tyler, Rogers, Leslie, Scowen, Paul, Somerville, Rachel, Stapelfeldt, Karl, Stark, Christopher, Stern, Daniel, Turnbull, Margaret, Amini, Rashied, Kuan, Gary, Martin, Stefan, Morgan, Rhonda, Redding, David, Stahl, H. Philip, Webb, Ryan, Alvarez-Salazar, Oscar, Arnold, William L., Arya, Manan, Balasubramanian, Bala, Baysinger, Mike, Bell, Ray, Below, Chris, Benson, Jonathan, Blais, Lindsey, Booth, Jeff, Bourgeois, Robert, Bradford, Case, Brewer, Alden, Brooks, Thomas, Cady, Eric, Caldwell, Mary, Calvet, Rob, Carr, Steven, Chan, Derek, Cormarkovic, Velibor, Coste, Keith, Cox, Charlie, Danner, Rolf, Davis, Jacqueline, Dewell, Larry, Dorsett, Lisa, Dunn, Daniel, East, Matthew, Effinger, Michael, Eng, Ron, Freebury, Greg, Garcia, Jay, Gaskin, Jonathan, Greene, Suzan, Hennessy, John, Hilgemann, Evan, Hood, Brad, Holota, Wolfgang, Howe, Scott, Huang, Pei, Hull, Tony, Hunt, Ron, Hurd, Kevin, Johnson, Sandra, Kissil, Andrew, Knight, Brent, Kolenz, Daniel, Kraus, Oliver, Krist, John, Li, Mary, Lisman, Doug, Mandic, Milan, Mann, John, Marchen, Luis, Marrese-Reading, Colleen, McCready, Jonathan, McGown, Jim, Missun, Jessica, Miyaguchi, Andrew, Moore, Bradley, Nemati, Bijan, Nikzad, Shouleh, Nissen, Joel, Novicki, Megan, Perrine, Todd, Pineda, Claudia, Polanco, Otto, Putnam, Dustin, Qureshi, Atif, Richards, Michael, Riggs, A. J. Eldorado, Rodgers, Michael, Rud, Mike, Saini, Navtej, Scalisi, Dan, Scharf, Dan, Schulz, Kevin, Serabyn, Gene, Sigrist, Norbert, Sikkia, Glory, Singleton, Andrew, Shaklan, Stuart, Smith, Scott, Southerd, Bart, Stahl, Mark, Steeves, John, Sturges, Brian, Sullivan, Chris, Tang, Hao, Taras, Neil, Tesch, Jonathan, Therrell, Melissa, Tseng, Howard, Valente, Marty, Van Buren, David, Villalvazo, Juan, Warwick, Steve, Webb, David, Westerhoff, Thomas, Wofford, Rush, Wu, Gordon, Woo, Jahning, Wood, Milana, Ziemer, John, Arney, Giada, Anderson, Jay, Maíz-Apellániz, Jesús, Bartlett, James, Belikov, Ruslan, Bendek, Eduardo, Cenko, Brad, Douglas, Ewan, Dulz, Shannon, Evans, Chris, Faramaz, Virginie, Feng, Y. Katherina, Ferguson, Harry, Follette, Kate, Ford, Saavik, García, Miriam, Geha, Marla, Gelino, Dawn, Götberg, Ylva, Hildebrandt, Sergi, Hu, Renyu, Jahnke, Knud, Kennedy, Grant, Kreidberg, Laura, Isella, Andrea, Lopez, Eric, Marchis, Franck, Macri, Lucas, Marley, Mark, Matzko, William, Mazoyer, Johan, McCandliss, Stephan, Meshkat, Tiffany, Mordasini, Christoph, Morris, Patrick, Nielsen, Eric, Newman, Patrick, Petigura, Erik, Postman, Marc, Reines, Amy, Roberge, Aki, Roederer, Ian, Ruane, Garreth, Schwieterman, Edouard, Sirbu, Dan, Spalding, Christopher, Teplitz, Harry, Tumlinson, Jason, Turner, Neal, Werk, Jessica, Wofford, Aida, Wyatt, Mark, Young, Amber, Zellem, Rob
The Habitable Exoplanet Observatory, or HabEx, has been designed to be the Great Observatory of the 2030s. For the first time in human history, technologies have matured sufficiently to enable an affordable space-based telescope mission capable of di
Externí odkaz:
http://arxiv.org/abs/2001.06683
Autor:
Huber, Daniel, Chaplin, William J., Chontos, Ashley, Kjeldsen, Hans, Christensen-Dalsgaard, Joergen, Bedding, Timothy R., Ball, Warrick, Brahm, Rafael, Espinoza, Nestor, Henning, Thomas, Jordan, Andres, Sarkis, Paula, Knudstrup, Emil, Albrecht, Simon, Grundahl, Frank, Andersen, Mads Fredslund, Palle, Pere L., Crossfield, Ian, Fulton, Benjamin, Howard, Andrew W., Isaacson, Howard T., Weiss, Lauren M., Handberg, Rasmus, Lund, Mikkel N., Serenelli, Aldo M., Mosumgaard, Jakob, Stokholm, Amalie, Bierlya, Allyson, Buchhave, Lars A., Latham, David W., Quinn, Samuel N., Gaidos, Eric, Hirano, Teruyuki, Ricker, George R., Vanderspek, Roland K., Seager, Sara, Jenkins, Jon M., Winn, Joshua N., Antia, H. M., Appourchaux, Thierry, Basu, Sarbani, Bell, Keaton J., Benomar, Othman, Bonanno, Alfio, Buzasi, Derek L., Campante, Tiago L., Orhan, Z. Celik, Corsaro, Enrico, Cunha, Margarida S., Davies, Guy R., Deheuvels, Sebastien, Grunblatt, Samuel K., Hasanzadeh, Amir, Di Mauro, Maria Pia, Garcia, Rafael A., Gaulme, Patrick, Girardi, Leo, Guzik, Joyce A., Hon, Marc, Jiang, Chen, Kallinger, Thomas, Kawaler, Steven D., Kuszlewicz, James S., Lebreton, Yveline, Li, Tanda, Lucas, Miles, Lundkvist, Mia S., Mathis, Stephane, Mathur, Savita, Mazumdar, Anwesh, Metcalfe, Travis S., Miglio, Andrea, Monteiro, Mario J., Mosser, Benoit, Noll, Anthony, Nsamba, Benard, Mann, Andrew W., Ong, Jia Mian Joel, Ortel, S., Pereira, Filipe, Ranadive, Pritesh, Regulo, Clara, Rodrigues, Thaise S., Roxburgh, Ian W., Aguirre, Victor Silva, Smalley, Barry, Schofield, Mathew, Sousa, Sergio G., Stassun, Keivan G., Stello, Dennis, Tayar, Jamie, White, Timothy R., Verma, Kuldeep, Vrard, Mathieu, Yildiz, M., Baker, David, Bazot, Michael, Beichmann, Charles, Bergmann, Christoph, Bugnet, Lisa, Cale, Bryson, Carlino, Roberto, Cartwright, Scott M., Christiansen, Jessie L., Ciardi, David R., Creevey, Orlagh, Dittmann, Jason A., Nascimento, Jose Dias Do, van Eylen, Vincent, Furesz, Gabor, Gagne, Jonathan, Gao, Peter, Gazeas, Kosmas, Giddens, Frank, Hall, Oliver, Hekker, Saskia, Ireland, Michael J., Latouf, Natasha, LeBrun, Danny, Levine, Alan M, Matzko, William, Natinsky, Eva, Page, Emma, Plavchan, Peter, Mansouri-Samani, Masoud, McCauliff, Sean, Mullally, Susan E, Orenstein, Brendan, Soto, Aylin, Paegert, Martin, van Saders, Jennifer L., Schnaible, Chloe, Soderblom, David R., Szabo, Robert, Tanner, Angelle, Tinney, C. G., Teske, Johanna, Thomas, Alexandra, Trampedach, Regner, Wright, Duncan, Yuan, Thomas T., Zohrabi, Farzaneh
We present the discovery of TOI-197.01, the first transiting planet identified by the Transiting Exoplanet Survey Satellite (TESS) for which asteroseismology of the host star is possible. TOI-197 (HIP116158) is a bright (V=8.2 mag), spectroscopically
Externí odkaz:
http://arxiv.org/abs/1901.01643