Zobrazeno 1 - 10
of 42
pro vyhledávání: '"Jelinsky, Sharon"'
Autor:
Hon, Marc, Huber, Daniel, Li, Yaguang, Metcalfe, Travis S., Bedding, Timothy R., Ong, Joel, Chontos, Ashley, Rubenzahl, Ryan, Halverson, Samuel, García, Rafael A., Kjeldsen, Hans, Stello, Dennis, Hey, Daniel R., Campante, Tiago, Howard, Andrew W., Gibson, Steven R., Rider, Kodi, Roy, Arpita, Baker, Ashley D., Edelstein, Jerry, Smith, Chris, Fulton, Benjamin J., Walawender, Josh, Brodheim, Max, Brown, Matt, Chan, Dwight, Dai, Fei, Deich, William, Gottschalk, Colby, Grillo, Jason, Hale, Dave, Hill, Grant M., Holden, Bradford, Householder, Aaron, Isaacson, Howard, Ishikawa, Yuzo, Jelinsky, Sharon R., Kassis, Marc, Kaye, Stephen, Laher, Russ, Lanclos, Kyle, Lee, Chien-Hsiu, Lilley, Scott, McCarney, Ben, Miller, Timothy N., Payne, Joel, Petigura, Erik A., Poppett, Claire, Raffanti, Michael, Rockosi, Constance, Sanford, Dale, Schwab, Christian, Shaum, Abby P., Sirk, Martin M., Smith, Roger, Thorne, Jim, Valliant, John, Vandenberg, Adam, Wang, Shin Ywan, Wishnow, Edward, Wold, Truman, Yeh, Sherry, Baker, Ashley, Basu, Sarbani, Bedell, Megan, Cegla, Heather M., Crossfield, Ian, Dressing, Courtney, Dumusque, Xavier, Knutson, Heather, Mawet, Dimitri, O'Meara, John, Stefánsson, Guðmundur, Teske, Johanna, Vasisht, Gautam, Wang, Sharon Xuesong, Weiss, Lauren M., Winn, Joshua N., Wright, Jason T.
Asteroseismology of dwarf stars cooler than the Sun is very challenging due to the low amplitudes and rapid timescales of oscillations. Here, we present the asteroseismic detection of solar-like oscillations at 4-minute timescales ($\nu_{\mathrm{max}
Externí odkaz:
http://arxiv.org/abs/2407.21234
Autor:
Dai, Fei, Howard, Andrew W., Halverson, Samuel, Orell-Miquel, Jaume, Palle, Enric, Isaacson, Howard, Fulton, Benjamin, Price, Ellen M., Plotnykov, Mykhaylo, Rogers, Leslie A., Valencia, Diana, Paragas, Kimberly, Greklek-McKeon, Michael, Barrientos, Jonathan Gomez, Knutson, Heather A., Petigura, Erik A., Weiss, Lauren M., Lee, Rena, Brinkman, Casey L., Huber, Daniel, Steffansson, Gudmundur, Masuda, Kento, Giacalone, Steven, Lu, Cicero X., Kite, Edwin S., Hu, Renyu, Gaidos, Eric, Zhang, Michael, Rubenzahl, Ryan A., Winn, Joshua N., Han, Te, Beard, Corey, Holcomb, Rae, Householder, Aaron, Gilbert, Gregory J., Lubin, Jack, Ong, J. M. Joel, Polanski, Alex S., Saunders, Nicholas, Van Zandt, Judah, Yee, Samuel W., Zhang, Jingwen, Zink, Jon, Holden, Bradford, Baker, Ashley, Brodheim, Max, Crossfield, Ian J. M., Deich, William, Edelstein, Jerry, Gibson, Steven R., Hill, Grant M., Jelinsky, Sharon R, Kassis, Marc, Laher, Russ R., Lanclos, Kyle, Lilley, Scott, Payne, Joel N., Rider, Kodi, Robertson, Paul, Roy, Arpita, Schwab, Christian, Shaum, Abby P., Sirk, Martin M., Smith, Chris, Vandenberg, Adam, Walawender, Josh, Wang, Sharon X., Shin-Ywan, Wang, Wishnow, Edward, Wright, Jason T., Yeh, Sherry, Caballero, Jos. A., Morales, Juan C., Murgas, Felipe, Nagel, Evangelos, Reiners, Ansgar, Schweitzer, Andreas, Tabernero, Hugo M., Zechmeister, Mathias, Spencer, Alton, Ciardi, David R., Clark, Catherine A., Lund, Michael B., Caldwell, Douglas A., Collins, Karen A., Schwarz, Richard P., Barkaoui, Khalid, Watkins, Cristilyn N., Shporer, Avi, Narita, Norio, Fukui, Akihiko, Srdoc, Gregor, Latham, David W., Jenkins, Jon M., Ricker, George R., Seager, Sara, Vanderspek, Roland
TOI-6255~b (GJ 4256) is an Earth-sized planet (1.079$\pm0.065$ $R_\oplus$) with an orbital period of only 5.7 hours. With the newly commissioned Keck Planet Finder (KPF) and CARMENES spectrographs, we determined the planet's mass to be 1.44$\pm$0.14
Externí odkaz:
http://arxiv.org/abs/2407.21167
Autor:
Silber, Joseph Harry, Fagrelius, Parker, Fanning, Kevin, Schubnell, Michael, Aguilar, Jessica Nicole, Ahlen, Steven, Ameel, Jon, Ballester, Otger, Baltay, Charles, Bebek, Chris, Beard, Dominic Benton, Besuner, Robert, Cardiel-Sas, Laia, Casas, Ricard, Castander, Francisco Javier, Claybaugh, Todd, Dobson, Carl, Duan, Yutong, Dunlop, Patrick, Edelstein, Jerry, Emmet, William T., Elliott, Ann, Evatt, Matthew, Gershkovich, Irena, Guy, Julien, Harris, Stu, Heetderks, Henry, Heetderks, Ian, Honscheid, Klaus, Illa, Jose Maria, Jelinsky, Patrick, Jelinsky, Sharon R., Jimenez, Jorge, Karcher, Armin, Kent, Stephen, Kirkby, David, Kneib, Jean-Paul, Lambert, Andrew, Lampton, Mike, Leitner, Daniela, Levi, Michael, McCauley, Jeremy, Meisner, Aaron, Miller, Timothy N., Miquel, Ramon, Mundet, Juliá, Poppett, Claire, Rabinowitz, David, Reil, Kevin, Roman, David, Schlegel, David, Serrano, Santiago, Van Shourt, William, Sprayberry, David, Tarlé, Gregory, Tie, Suk Sien, Weaverdyck, Curtis, Zhang, Kai, Azzaro, Marco, Bailey, Stephen, Becerril, Santiago, Blackwell, Tami, Bouri, Mohamed, Brooks, David, Buckley-Geer, Elizabeth, Castro, Jose Peñate, Derwent, Mark, Dey, Arjun, Dhungana, Govinda, Doel, Peter, Eisenstein, Daniel J., Fahim, Nasib, Garcia-Bellido, Juan, Gaztañaga, Enrique, Gontcho, Satya Gontcho A, Gutierrez, Gaston, Hörler, Philipp, Kehoe, Robert, Kisner, Theodore, Kremin, Anthony, Kronig, Luzius, Landriau, Martin, Guillou, Laurent Le, Martini, Paul, Moustakas, John, Palanque-Delabrouille, Nathalie, Peng, Xiyan, Percival, Will, Prada, Francisco, Prieto, Carlos Allende, de Rivera, Guillermo Gonzalez, Sanchez, Eusebio, Sanchez, Justo, Sharples, Ray, Soares-Santos, Marcelle, Schlafly, Edward, Weaver, Benjamin Alan, Zhou, Zhimin, Zhu, Yaling, Zou, Hu
A system of 5,020 robotic fiber positioners was installed in 2019 on the Mayall Telescope, at Kitt Peak National Observatory. The robots automatically re-target their optical fibers every 10 - 20 minutes, each to a precision of several microns, with
Externí odkaz:
http://arxiv.org/abs/2205.09014
Autor:
Poppett, Claire, Jelinsky, Patrick, Guy, Julien, Edelstein, Jerry, Jelinsky, Sharon, Aguilar, Jessica, Sharples, Ray, Schmoll, Jurgen, Bramall, David, Tyas, Luke, Martini, Paul, Fanning, Kevin, Levi, Michael, Brooks, David, Doel, Peter, Yutong, Duan, Tarle, Gregory, Gaztanaga, Erique, Prada, Francisco, Collaboration, the DESI
Publikováno v:
SPIE 2020
The recently commissioned Dark Energy Spectroscopic Instrument (DESI) will measure the expansion historyof the universe using the Baryon Acoustic Oscillation technique. The spectra of 35 million galaxies and quasarsover 14000 sq deg will be measured
Externí odkaz:
http://arxiv.org/abs/2101.11564
Autor:
Adams, Bernhard W., Attenkofer, Klaus, Bogdan, Mircea, Byrum, Karen, Elagin, Andrey, Elam, Jeffrey W., Frisch, Henry J., Genat, Jean-Francois, Grabas, Herve, Gregar, Joseph, Hahn, Elaine, Heintz, Mary, Insepov, Zinetula, Ivanov, Valentin, Jelinsky, Sharon, Jokely, Slade, Lee, Sun Wu, Mane, Anil. U., McPhate, Jason, Minot, Michael J., Murat, Pavel, Nishimura, Kurtis, Northrop, Richard, Obaid, Razib, Oberla, Eric, Ramberg, Erik, Ronzhin, Anatoly, Siegmund, Oswald H., Sellberg, Gregory, Sullivan, Neal T., Tremsin, Anton, Varner, Gary, Veryovkin, Igor, Vostrikov, Alexei, Wagner, Robert G., Walters, Dean, Wang, Hsien-Hau, Wetstein, Matthew, Xi, Junqi, Yusov, Zikri, Zinovev, Alexander
The Large Area Picosecond PhotoDetector (LAPPD) Collaboration was formed in 2009 to develop large-area photodetectors capable of time resolutions measured in pico-seconds, with accompanying sub-millimeter spatial resolution. During the next three and
Externí odkaz:
http://arxiv.org/abs/1603.01843
Autor:
Dawson, Kyle, Bebek, Chris, Emes, John, Holland, Steve, Jelinsky, Sharon, Karcher, Armin, Kolbe, William, Palaio, Nick, Roe, Natalie, Saha, Juhi, Takasaki, Koki, Wang, Guobin
Publikováno v:
IEEE Trans.Nucl.Sci.55:1725-1735,2008
Thick, fully depleted p-channel charge-coupled devices (CCDs) have been developed at the Lawrence Berkeley National Laboratory (LBNL). These CCDs have several advantages over conventional thin, n-channel CCDs, including enhanced quantum efficiency an
Externí odkaz:
http://arxiv.org/abs/0711.2105
Autor:
Edelstein, Jerry, Korpela, Eric, Adolfo, Joe, Bowen, Mark, Feuerstein, Michael, Hull, Jeffrey, Jelinsky, Sharon, Nishikida, Kaori, McKee, Ken, Berg, Peter, Chung, Ray, Fischer, Jorg, Min, Kyoung-Wook, Oh, Seung-Han, Rhee, Jin-Guen, Ryu, Kwangsun, Shinn, Jong-Ho, Han, Wonyong, Jin, Ho, Lee, Dae-Hee, Nam, Uk-Won, Park, Jang-Hyun, Seon, Kwang-Il, Yuk, In-Soo
Publikováno v:
Astrophys.J. 644 (2006) L159-L162
The SPEAR (or 'FIMS') instrumentation has been used to conduct the first large-scale spectral mapping of diffuse cosmic far ultraviolet (FUV, 900-1750 AA) emission, including important diagnostics of interstellar hot (10^4 K - 10^6 K) and photoionize
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601588
Akademický článek
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Autor:
Yusof, Zikri, Attenkofer, Klaus, Demarteau, Marcel, Frisch, Henry, Gregar, Joe, Jelinsky, Sharon, Lee, Seon Woo, McPhate, Jason, Northrop, Richard, Paramonov, Alexander, Ronzhin, Anatoly, Sellberg, Greg, Siegmund, Oswald, Wagner, Robert, Walters, Dean, Xie, Junqi
Publikováno v:
In Physics Procedia 2012 37:733-739
Autor:
Evans, Christopher J., Bryant, Julia J., Motohara, Kentaro, Baker, Ashley D., Gibson, Steven R., Grillo, Jason, Ishikawa, Yuzo, Howard, Andrew, Halverson, Samuel, Rider, Kodi, Jelinsky, Sharon, Deich, William, Sirk, Martin M., Isaacson, Howard, Roy, Arpita, Edelstein, Jerry, Smith, Christopher
Publikováno v:
Proceedings of SPIE; August 2022, Vol. 12184 Issue: 1 p121845H-121845H-12, 12062668p