Zobrazeno 1 - 10
of 192
pro vyhledávání: '"P, Kołecki"'
Autor:
Brinkman, Casey L., Weiss, Lauren M., Huber, Daniel, Lee, Rena A., Kolecki, Jared, Tenn, Gwyneth, Zhang, Jingwen, Narayanan, Suchitra, Polanski, Alex S., Dai, Fei, Bean, Jacob L., Beard, Corey, Brady, Madison, Brodheim, Max, Brown, Matt, Deich, William, Edelstein, Jerry, Fulton, Benjamin J., Giacalone, Steven, Gibson, Steven R., Gilbert, Gregory J., Halverson, Samuel, Handley, Luke, Hill, Grant M., Holcomb, Rae, Holden, Bradford, Householder, Aaron, Howard, Andrew W., Isaacson, Howard, Kaye, Stephen, Laher, Russ R., Lanclos, Kyle, Ong, J. M. Joel, Payne, Joel, Petigura, Eric A., Pidhorodetska, Daria, Poppett, Claire, Roy, Arpita, Rubenzahl, Ryan, Saunders, Nicholas, Schwab, Christian, Seifahrt, Andreas, Shaum, Abby P., Sirk, Martin M., Smith, Chris, Smith, Roger, Stefánsson, Guðmundur, Stürmer, Julian, Thorne, Jim, Turtelboom, Emma V., Tyler, Dakotah, Valliant, John, Van Zandt, Judah, Walawender, Josh, Yee, Samuel W., Yeh, Sherry, Zink, Jon
Hundreds of exoplanets between 1-1.8 times the size of the Earth have been discovered on close in orbits. However, these planets show such a diversity in densities that some appear to be made entirely of iron, while others appear to host gaseous enve
Externí odkaz:
http://arxiv.org/abs/2410.00213
Autor:
Martínez, Romy Rodríguez, Gaudi, B. Scott, Schulze, Joseph G., Acuña, Lorena, Kolecki, Jared, Johnson, Jennifer A., Asnodkar, Anusha Pai, Boley, Kiersten M., Deleuil, Magali, Mousis, Olivier, Panero, Wendy R., Wang, Ji
We present a reanalysis of the K2-106 transiting planetary system, with a focus on the composition of K2-106b, an ultra-short period, super-Mercury candidate. We globally model existing photometric and radial velocity data and derive a planetary mass
Externí odkaz:
http://arxiv.org/abs/2208.07883
Autor:
Xuan, Jerry W., Wang, Jason, Ruffio, Jean-Baptiste, Knutson, Heather, Mawet, Dimitri, Mollière, Paul, Kolecki, Jared, Vigan, Arthur, Mukherjee, Sagnick, Wallack, Nicole, Wang, Ji, Baker, Ashley, Bartos, Randall, Blake, Geoffrey A., Bond, Charlotte Z., Bryan, Marta, Calvin, Benjamin, Cetre, Sylvain, Chun, Mark, Delorme, Jacques-Robert, Doppmann, Greg, Echeverri, Daniel, Finnerty, Luke, Fitzgerald, Michael P., Horstman, Katelyn, Inglis, Julie, Jovanovic, Nemanja, López, Ronald, Martin, Emily, Morris, Evan, Pezzato, Jacklyn, Ragland, Sam, Ren, Bin, Ruane, Garreth, Sappey, Ben, Schofield, Tobias, Skemer, Andrew, Venenciano, Taylor, Wallace, J. Kent, Wizinowich, Peter
Direct imaging studies have mainly used low-resolution spectroscopy ($R\sim20-100$) to study the atmospheres of giant exoplanets and brown dwarf companions, but the presence of clouds has often led to degeneracies in the retrieved atmospheric abundan
Externí odkaz:
http://arxiv.org/abs/2208.01657
Autor:
Wang, Ji, Kolecki, Jared R., Ruffio, Jean-Baptiste, Wang, Jason J., Mawet, Dimitri, Baker, Ashley, Bartos, Randall, Blake, Geoffrey A., Bond, Charlotte Z., Calvin, Benjamin, Cetre, Sylvain, Delorme, Jacques-Robert, Doppmann, Greg, Echeverri, Daniel, Finnerty, Luke, Fitzgerald, Michael P., Jovanovic, Nemanja, Liu, Michael C., Lopez, Ronald, Morris, Evan, Asnodkar, Anusha Pai, Pezzato, Jacklyn, Ragland, Sam, Roy, Arpita, Ruane, Garreth, Sappey, Ben, Schofield, Tobias, Skemer, Andrew, Venenciano, Taylor, Wallace, J. Kent, Wallack, Nicole L., Wizinowich, Peter, Xuan, Jerry W.
A benchmark brown dwarf (BD) is a BD whose properties (e.g., mass and chemical composition) are precisely and independently measured. Benchmark BDs are valuable in testing theoretical evolutionary tracks, spectral synthesis, and atmospheric retrieval
Externí odkaz:
http://arxiv.org/abs/2202.02477
Autor:
Kolecki, Jared R., Wang, Ji
With the launch of the JWST, we will obtain more precise data for exoplanets than ever before. However, this data can only inform and revolutionize our understanding of exoplanets when placed in the larger context of planet-star formation. Therefore,
Externí odkaz:
http://arxiv.org/abs/2112.02031
Autor:
Ishikawa, Hiroyuki Tako, Aoki, Wako, Hirano, Teruyuki, Kotani, Takayuki, Kuzuhara, Masayuki, Omiya, Masashi, Hori, Yasunori, Kokubo, Eiichiro, Kudo, Tomoyuki, Kurokawa, Takashi, Kusakabe, Nobuhiko, Narita, Norio, Nishikawa, Jun, Ogihara, Masahiro, Ueda, Akitoshi, Currie, Thayne, Henning, Thomas, Kasagi, Yui, Kolecki, Jared R., Kwon, Jungmi, Machida, Masahiro N., McElwain, Michael W., Nakagawa, Takao, Vievard, Sebastien, Wang, Ji, Tamura, Motohide, Sato, Bun'ei
Detailed chemical analyses of M dwarfs are scarce but necessary to constrain the formation environment and internal structure of planets being found around them. We present elemental abundances of 13 M dwarfs (2900 < Teff < 3500 K) observed in the Su
Externí odkaz:
http://arxiv.org/abs/2112.00173
Autor:
Kolecki, Jared R., Wang, Ji, Johnson, Jennifer A., Zinn, Joel C., Ilyin, Ilya, Strassmeier, Klaus G
By measuring the elemental abundances of a star, we can gain insight into the composition of its initial gas cloud -- the formation site of the star and its planets. Planet formation requires metals, the availability of which is determined by the ele
Externí odkaz:
http://arxiv.org/abs/2106.13251
Autor:
Piotr Sumisławski, Janusz Kołecki, Martyna Piotrowska, Maciej Kotowski, Marcin Szemitko, Jerzy Sieńko
Publikováno v:
Diagnostics, Vol 12, Iss 10, p 2320 (2022)
Fournier gangrene represents a urologic emergency. It is a rapidly progressing necrotizing fasciitis that comprises the perineal, perianal, and genital regions and has a high mortality rate. Diagnosis is usually made clinically, but radiological diag
Externí odkaz:
https://doaj.org/article/e190c2da5a1b45819bd40b1256e2a0f0
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Akademický článek
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