Zobrazeno 1 - 10
of 340
pro vyhledávání: '"Marshall, Jennifer L"'
Autor:
Lim, Dongwook, Koch-Hansen, Andreas J., Hansen, Camilla Juul, Lépine, Sebastien, Marshall, Jennifer L., Wilkinson, Mark I., Peñarrubia, Jorge
Publikováno v:
A&A 655, A26 (2021)
Recently, an increasing number of wide binaries has been discovered. Their chemical and dynamical properties are studied through extensive surveys and pointed observations. However, the formation of these wide binaries is far from clear, although sev
Externí odkaz:
http://arxiv.org/abs/2108.08850
Autor:
Limbach, Mary Anne, Schmidt, Luke M., DePoy, D. L., Mason, Jeffrey C., Scobey, Mike, Brown, Pat, Taylor, Chelsea, Marshall, Jennifer L.
We present the design of a novel instrument tuned to detect transiting exoplanet atmospheres. The instrument, which we call the exoplanet transmission spectroscopy imager (ETSI), makes use of a new technique called common-path multi-band imaging (CMI
Externí odkaz:
http://arxiv.org/abs/2012.00795
Candidate Periodically Variable Quasars from the Dark Energy Survey and the Sloan Digital Sky Survey
Autor:
Chen, Yu-Ching, Liu, Xin, Liao, Wei-Ting, Holgado, A. Miguel, Guo, Hengxiao, Gruendl, Robert A., Morganson, Eric, Shen, Yue, Zhang, Kaiwen, Abbott, Tim M. C., Aguena, Michel, Allam, Sahar, Avila, Santiago, Bertin, Emmanuel, Bhargava, Sunayana, Brooks, David, Burke, David L., Rosell, Aurelio Carnero, Carollo, Daniela, Kind, Matias Carrasco, Carretero, Jorge, Costanzi, Matteo, da Costa, Luiz N., Davis, Tamara M., De Vicente, Juan, Desai, Shantanu, Diehl, H. Thomas, Doel, Peter, Everett, Spencer, Flaugher, Brenna, Friedel, Douglas, Frieman, Joshua, García-Bellido, Juan, Gaztanaga, Enrique, Glazebrook, Karl, Gruen, Daniel, Gutierrez, Gaston, Hinton, Samuel R., Hollowood, Devon L., James, David J., Kim, Alex G., Kuehn, Kyler, Kuropatkin, Nikolay, Lewis, Geraint F., Lidman, Christopher, Lima, Marcos, Maia, Marcio A. G., March, Marisa, Marshall, Jennifer L., Menanteau, Felipe, Miquel, Ramon, Palmese, Antonella, Paz-Chinchón, Francisco, Plazas, Andrés A., Sanchez, Eusebio, Schubnell, Michael, Serrano, Santiago, Sevilla-Noarbe, Ignacio, Smith, Mathew, Suchyta, Eric, Swanson, Molly E. C., Tarle, Gregory, Tucker, Brad E., Varga, Tamas Norbert, Walker, Alistair R.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 499, Issue 2, pp.2245-2264 (2020)
Periodically variable quasars have been suggested as close binary supermassive black holes. We present a systematic search for periodic light curves in 625 spectroscopically confirmed quasars with a median redshift of 1.8 in a 4.6 deg$^2$ overlapping
Externí odkaz:
http://arxiv.org/abs/2008.12329
Autor:
Adhikari, Susmita, Shin, Tae-hyeon, Jain, Bhuvnesh, Hilton, Matt, Baxter, Eric, Chang, Chihway, Wechsler, Risa H., Battaglia, Nick, Bond, J. Richard, Bocquet, Sebastian, DeRose, Joseph, Choi, Steve K., Devlin, Mark, Dunkley, Jo, Evrard, August E., Ferraro, Simone, Hill, J. Colin, Hughes, John P., Gallardo, Patricio A., Lokken, Martine, MacInnis, Amanda, McMahon, Jeffrey, Madhavacheril, Mathew S., Nati, Frederico, Newburgh, Laura B., Niemack, Michael D., Page, Lyman A., Palmese, Antonella, Partridge, Bruce, Rozo, Eduardo, Rykoff, Eli, Salatino, Maria, Schillaci, Alessandro, Sehgal, Neelima, Sifón, Cristóbal, To, Chun-Hao, Wollack, Ed, Wu, Hao-Yi, Xu, Zhilei, Aguena, Michel, Allam, Sahar, Amon, Alexandra, Annis, James, Avila, Santiago, Bacon, David, Bertin, Emmanuel, Bhargava, Sunayana, Brooks, David, Burke, David L., Rosell, Aurelio C., Kind, Matias Carrasco, Carretero, Jorge, Castander, Francisco Javier, Choi, Ami, Costanzi, Matteo, da Costa, Luiz N., De Vicente, Juan, Desai, Shantanu, Diehl, Thomas H., Doel, Peter, Everett, Spencer, Ferrero, Ismael, Ferté, Agnès, Flaugher, Brenna, Fosalba, Pablo, Frieman, Josh, García-Bellido, Juan, Gaztanaga, Enrique, Gruen, Daniel, Gruendl, Robert A., Gschwend, Julia, Gutierrez, Gaston, Hartley, Will G., Hinton, Samuel R., Hollowood, Devon L., Honscheid, Klaus, James, David J., Jeltema, Tesla, Kuehn, Kyler, Kuropatkin, Nikolay, Lahav, Ofer, Lima, Marcos, Maia, Marcio A. G., Marshall, Jennifer L., Martini, Paul, Melchior, Peter, Menanteau, Felipe, Miquel, Ramon, Morgan, Robert, Ogando, Ricardo L. C., Paz-Chinchón, Francisco, Malagón, Andrés Plazas, Sanchez, Eusebio, Santiago, Basilio, Scarpine, Vic, Serrano, Santiago, Sevilla-Noarbe, Ignacio, Smith, Mathew, Soares-Santos, Marcelle, Suchyta, Eric, Swanson, Molly E. C., Varga, Tamas N., Wilkinson, Reese D., Zhang, Yuanyuan, Austermann, Jason E., Beall, James A., Becker, Daniel T., Denison, Edward V., Duff, Shannon M., Hilton, Gene C., Hubmayr, Johannes, Ullom, Joel N., Van Lanen, Jeff, Vale, Leila R., Collaboration, DES, Collaboration, ACT
We measure the projected number density profiles of galaxies and the splashback feature in clusters selected by the Sunyaev--Zeldovich (SZ) effect from the Advanced Atacama Cosmology Telescope (AdvACT) survey using galaxies observed by the Dark Energ
Externí odkaz:
http://arxiv.org/abs/2008.11663
Akademický článek
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Autor:
Martínez, Romy Rodríguez, Gaudi, B. Scott, Rodriguez, Joseph E., Zhou, George, Labadie-Bartz, Jonathan, Quinn, Samuel N., Penev, Kaloyan Minev, Tan, Thiam-Guan, Latham, David W., Paredes, Leonardo A., Kielkopf, John, Addison, Brett C., Wright, Duncan J., Teske, Johanna K., Howell, Steve B., Ciardi, David R., Ziegler, Carl, Stassun, Keivan G., Johnson, Marshall C., Eastman, Jason D., Siverd, Robert J., Beatty, Thomas G., Bouma, Luke G., Pepper, Joshua, Lund, Michael B., Villanueva, Steven, Stevens, Daniel J., Jensen, Eric L. N., Kilby, Coleman, Cohen, David H., Bayliss, Daniel, Bieryla, Allyson, Cargile, Phillip A., Collins, Karen A., Conti, Dennis M., Colon, Knicole D., Curtis, Ivan A., DePoy, Darren L., Evans, Phil A., Feliz, Dax, Gregorio, Joao, Rothenberg, Jason, James, David J., Penny, Matthew T., Reed, Phillip A., Relles, Howard M., Stephens, Denise C., Joner, Michael D., Kuhn, Rudolf B., Stockdale, Chris, Trueblood, Mark, Trueblood, Patricia, Yao, Xinyu, Zambelli, Roberto, Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Henry, Todd J., James, Hodari-Sadiki, Jao, Wei-Chun, Wang, Sharon X., Butler, R. Paul, Crane, Jeffrey D., Thompson, Ian B., Schectman, Stephen, Wittenmyer, Robert A., Bedding, Timothy R., Okumura, Jack, Plavchan, Peter, Bowler, Brendan P., Horner, Jonathan, Kane, Stephen R., Mengel, Matthew W., Morton, Timothy D., Tinney, C. G., Zhang, Hui, Scott, Nicholas J., Matson, Rachel A., Everett, Mark E., Tokovinin, Andrei, Mann, Andrew W., Dragomir, Diana, Guenther, Maximilian N., Ting, Eric B., Fausnaugh, Michael, Glidden, Ana, Quintana, Elisa V., Manner, Mark, Marshall, Jennifer L., McLeod, Kim K., Khakpash, Somayeh
We present the discoveries of KELT-25b (TIC 65412605, TOI-626.01) and KELT-26b (TIC 160708862, TOI-1337.01), two transiting companions orbiting relatively bright, early A-stars. The transit signals were initially detected by the KELT survey, and subs
Externí odkaz:
http://arxiv.org/abs/1912.01017
Autor:
Rodriguez, Joseph E., Eastman, Jason D., Zhou, George, Quinn, Samuel N., Beatty, Thomas G., Penev, Kaloyan, Johnson, Marshall C., Cargile, Phillip A., Latham, David W., Bieryla, Allyson, Collins, Karen A., Dressing, Courtney D., Ciardi, David R., Relles, Howard M., Murawski, Gabriel, Nishiumi, Taku, Yonehara, Atsunori, Ishimaru, Ryo, Yoshida, Fumi, Gregorio, Joao, Lund, Michael B., Stevens, Daniel J., Stassun, Keivan G., Gaudi, B. Scott, Colón, Knicole D., Pepper, Joshua, Narita, Norio, Awiphan, Supachai, Chuanraksasat, Pongpichit, Benni, Paul, Zambelli, Roberto, Garrison, Lehman H., Wilson, Maurice L., Cornachione, Matthew A., Wang, Sharon X., Labadie-Bartz, Jonathan, Rodríguez, Romy, Siverd, Robert J., Yao, Xinyu, Bayliss, Daniel, Berlind, Perry, Calkins, Michael L., Christiansen, Jessie L., Cohen, David H., Conti, Dennis M., Curtis, Ivan A., Depoy, D. L., Esquerdo, Gilbert A., Evans, Phil, Feliz, Dax, Fulton, Benjamin J., Holoien, Thomas W. S., James, David J., Jayasinghe, Tharindu, Jang-Condell, Hannah, Jensen, Eric L. N., Johnson, John A., Joner, Michael D., Khakpash, Somayeh, Kielkopf, John F., Kuhn, Rudolf B., Manner, Mark, Marshall, Jennifer L., McLeod, Kim K., McCrady, Nate, Oberst, Thomas E., Oelkers, Ryan J., Penny, Matthew T., Reed, Phillip A., Sliski, David H., Shappee, B. J., Stephens, Denise C., Stockdale, Chris, Tan, Thiam-Guan, Trueblood, Mark, Trueblood, Pat, Villanueva Jr., Steven, Wittenmyer, Robert A., Wright, Jason T.
We present the discovery of KELT-24 b, a massive hot Jupiter orbiting a bright (V=8.3 mag, K=7.2 mag) young F-star with a period of 5.6 days. The host star, KELT-24 (HD 93148), has a $T_{\rm eff}$ =$6509^{+50}_{-49}$ K, a mass of $M_{*}$ = $1.460^{+0
Externí odkaz:
http://arxiv.org/abs/1906.03276
Autor:
Gilbert, Karoline M., Tollerud, Erik J., Anderson, Jay, Beaton, Rachael L., Bell, Eric F., Brooks, Alyson, Brown, Thomas M., Bullock, James, Carlin, Jeffrey L., Collins, Michelle, Cooper, Andrew, Crnojevic, Denija, Dalcanton, Julianne, del Pino, Andres, D'Souza, Richard, Escala, Ivanna, Fardal, Mark, Font, Andreea, Geha, Marla, Guhathakurta, Puragra, Kirby, Evan, Lewis, Geraint F., Marshall, Jennifer L., Martin, Nicolas F., McQuinn, Kristen, Monachesi, Antonela, Patel, Ekta, Peeples, Molly S., Pillepich, Annalisa, Quirk, Amanda C. N., Rich, R. Michael, Sohn, S. Tony, Ting, Yuan-Sen, van der Marel, Roeland P., Wetzel, Andrew, Williams, Benjamin F., Wojno, Jennifer
The Great Andromeda Galaxy (M31) is the nexus of the near-far galaxy evolution connection and a principal data point for near-field cosmology. Due to its proximity (780 kpc), M31 can be resolved into individual stars like the Milky Way (MW). Unlike t
Externí odkaz:
http://arxiv.org/abs/1904.01074
Autor:
Ferraro, Simone, Wilson, Michael J., Abidi, Muntazir, Alonso, David, Ansarinejad, Behzad, Armstrong, Robert, Asorey, Jacobo, Avelino, Arturo, Baccigalupi, Carlo, Bandura, Kevin, Battaglia, Nicholas, Bavdhankar, Chetan, Bernal, José Luis, Beutler, Florian, Biagetti, Matteo, Blanc, Guillermo A., Blazek, Jonathan, Bolton, Adam S., Borrill, Julian, Frye, Brenda, Buckley-Geer, Elizabeth, Bull, Philip, Burgess, Cliff, Byrnes, Christian T., Cai, Zheng, Castander, Francisco J, Castorina, Emanuele, Chang, Tzu-Ching, Chaves-Montero, Jonás, Chen, Shi-Fan, Chen, Xingang, Balland, Christophe, Yèche, Christophe, Cohn, J. D., Coulton, William, Courtois, Helene, Croft, Rupert A. C., Cyr-Racine, Francis-Yan, D'Amico, Guido, Dawson, Kyle, Delabrouille, Jacques, Dey, Arjun, Doré, Olivier, Douglass, Kelly A., Yutong, Duan, Dvorkin, Cora, Eggemeier, Alexander, Eisenstein, Daniel, Fan, Xiaohui, Ferreira, Pedro G., Font-Ribera, Andreu, Foreman, Simon, García-Bellido, Juan, Gerbino, Martina, Gluscevic, Vera, Gontcho, Satya Gontcho A, Green, Daniel, Guy, Julien, Hahn, ChangHoon, Hanany, Shaul, Handley, Will, Hathi, Nimish, Hawken, Adam J., Hernández-Aguayo, César, Hložek, Renée, Huterer, Dragan, Ishak, Mustapha, Kamionkowski, Marc, Karagiannis, Dionysios, Keeley, Ryan E., Kehoe, Robert, Khatri, Rishi, Kim, Alex, Kneib, Jean-Paul, Kollmeier, Juna A., Kovetz, Ely D., Krause, Elisabeth, Krolewski, Alex, L'Huillier, Benjamin, Landriau, Martin, Levi, Michael, Liguori, Michele, Linder, Eric, Lukić, Zarija, de la Macorra, Axel, Plazas, Andrés A., Marshall, Jennifer L., Martini, Paul, Masui, Kiyoshi, McDonald, Patrick, Meerburg, P. Daniel, Meyers, Joel, Mirbabayi, Mehrdad, Moustakas, John, Myers, Adam D., Palanque-Delabrouille, Nathalie, Newburgh, Laura, Newman, Jeffrey A., Niz, Gustavo, Padmanabhan, Hamsa, Palunas, Povilas, Percival, Will J., Piacentini, Francesco, Pieri, Matthew M., Piro, Anthony L., Prakash, Abhishek, Rhodes, Jason, Ross, Ashley J., Rossi, Graziano, Rudie, Gwen C., Samushia, Lado, Sasaki, Misao, Schaan, Emmanuel, Schlegel, David J., Schmittfull, Marcel, Schubnell, Michael, Sehgal, Neelima, Senatore, Leonardo, Seo, Hee-Jong, Shafieloo, Arman, Shan, Huanyuan, Simon, Joshua D., Simon, Sara, Slepian, Zachary, Slosar, Anže, Sridhar, Srivatsan, Stebbins, Albert, Escoffier, Stephanie, Switzer, Eric R., Tarlé, Gregory, Trodden, Mark, Uhlemann, Cora, Urenña-López, L. Arturo, Di Valentino, Eleonora, Vargas-Magaña, M., Wang, Yi, Watson, Scott, White, Martin, Xu, Weishuang, Yu, Byeonghee, Zhao, Gong-Bo, Zheng, Yi, Zhu, Hong-Ming
The expansion of the Universe is understood to have accelerated during two epochs: in its very first moments during a period of Inflation and much more recently, at $z < 1$, when Dark Energy is hypothesized to drive cosmic acceleration. The undiscove
Externí odkaz:
http://arxiv.org/abs/1903.09208