Zobrazeno 1 - 10
of 2 416
pro vyhledávání: '"W, Werner"'
Publikováno v:
The Depositional Record, Vol 9, Iss 4, Pp 1161-1166 (2023)
This is a comment to an article previously published in The Depositional Record.
Externí odkaz:
https://doaj.org/article/328721111a614f41acf9e437123b024b
Publikováno v:
European Journal of Mineralogy, Vol 35, Pp 403-426 (2023)
The Black Forest hosts a wide range of hydrothermal mineralization, including fluorite–barite vein deposits. In a detailed investigation of the Finstergrund and Tannenboden deposits in the Wieden mining district (southern Black Forest), the diversi
Externí odkaz:
https://doaj.org/article/2105a6be9bae4cf58fc926206270ae16
Autor:
Arthur D. Adams, Kimberly Bott, Paul A. Dalba, Tara Fetherolf, Stephen R. Kane, Ian Crossfield, Drake Deming, Diana Dragomir, Varoujan Gorjian, Laura Kreidberg, Farisa Y. Morales, Michael W. Werner
Publikováno v:
The Astronomical Journal, Vol 168, Iss 6, p 248 (2024)
As an inflated hot Jupiter orbiting an early-type primary star in the evolved binary HD 202772 system, HD 202772 A b’s presence invites a study of how such a planet forms and evolves. As a prelude to potential atmospheric characterization with the
Externí odkaz:
https://doaj.org/article/90e0fc10218341b0b09775e7feb0f858
Autor:
Christine H. Chen, Cicero X. Lu, Kadin Worthen, David R. Law, B. A. Sargent, Amaya Moro-Martin, G. C. Sloan, Carey M. Lisse, Dan M. Watson, Julien H. Girard, Yiwei Chai, Dean C. Hines, Jens Kammerer, Alexis Li, Marshall Perrin, Laurent Pueyo, Isabel Rebollido, Karl R. Stapelfeldt, Christopher Stark, Michael W. Werner
Publikováno v:
The Astrophysical Journal, Vol 973, Iss 2, p 139 (2024)
Modeling observations of the archetypal debris disk around β Pic, obtained in 2023 January with the MIRI Medium Resolution Spectrograph on board JWST, reveals significant differences compared with that obtained with the Infrared Spectrograph on boar
Externí odkaz:
https://doaj.org/article/3e0cf6f67f8e4bc78f72ab06374bfc60
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 2, p 162 (2024)
We report our search for infrared excesses in the Spitzer/Infrared Array Camera survey of the Kepler field at 3.6 and 4.5 μ m. The Spitzer Kepler Survey contains ∼190,000 targets, which we reduce to ∼117,000 targets after applying multiple filte
Externí odkaz:
https://doaj.org/article/3519d3e262a1454b87e0770e8e5f9148
Autor:
R. Poyatos, V. Granda, V. Flo, M. A. Adams, B. Adorján, D. Aguadé, M. P. M. Aidar, S. Allen, M. S. Alvarado-Barrientos, K. J. Anderson-Teixeira, L. M. Aparecido, M. A. Arain, I. Aranda, H. Asbjornsen, R. Baxter, E. Beamesderfer, Z. C. Berry, D. Berveiller, B. Blakely, J. Boggs, G. Bohrer, P. V. Bolstad, D. Bonal, R. Bracho, P. Brito, J. Brodeur, F. Casanoves, J. Chave, H. Chen, C. Cisneros, K. Clark, E. Cremonese, H. Dang, J. S. David, T. S. David, N. Delpierre, A. R. Desai, F. C. Do, M. Dohnal, J.-C. Domec, S. Dzikiti, C. Edgar, R. Eichstaedt, T. S. El-Madany, J. Elbers, C. B. Eller, E. S. Euskirchen, B. Ewers, P. Fonti, A. Forner, D. I. Forrester, H. C. Freitas, M. Galvagno, O. Garcia-Tejera, C. P. Ghimire, T. E. Gimeno, J. Grace, A. Granier, A. Griebel, Y. Guangyu, M. B. Gush, P. J. Hanson, N. J. Hasselquist, I. Heinrich, V. Hernandez-Santana, V. Herrmann, T. Hölttä, F. Holwerda, J. Irvine, S. Isarangkool Na Ayutthaya, P. G. Jarvis, H. Jochheim, C. A. Joly, J. Kaplick, H. S. Kim, L. Klemedtsson, H. Kropp, F. Lagergren, P. Lane, P. Lang, A. Lapenas, V. Lechuga, M. Lee, C. Leuschner, J.-M. Limousin, J. C. Linares, M.-L. Linderson, A. Lindroth, P. Llorens, Á. López-Bernal, M. M. Loranty, D. Lüttschwager, C. Macinnis-Ng, I. Maréchaux, T. A. Martin, A. Matheny, N. McDowell, S. McMahon, P. Meir, I. Mészáros, M. Migliavacca, P. Mitchell, M. Mölder, L. Montagnani, G. W. Moore, R. Nakada, F. Niu, R. H. Nolan, R. Norby, K. Novick, W. Oberhuber, N. Obojes, A. C. Oishi, R. S. Oliveira, R. Oren, J.-M. Ourcival, T. Paljakka, O. Perez-Priego, P. L. Peri, R. L. Peters, S. Pfautsch, W. T. Pockman, Y. Preisler, K. Rascher, G. Robinson, H. Rocha, A. Rocheteau, A. Röll, B. H. P. Rosado, L. Rowland, A. V. Rubtsov, S. Sabaté, Y. Salmon, R. L. Salomón, E. Sánchez-Costa, K. V. R. Schäfer, B. Schuldt, A. Shashkin, C. Stahl, M. Stojanović, J. C. Suárez, G. Sun, J. Szatniewska, F. Tatarinov, M. Tesař, F. M. Thomas, P. Tor-ngern, J. Urban, F. Valladares, C. van der Tol, I. van Meerveld, A. Varlagin, H. Voigt, J. Warren, C. Werner, W. Werner, G. Wieser, L. Wingate, S. Wullschleger, K. Yi, R. Zweifel, K. Steppe, M. Mencuccini, J. Martínez-Vilalta
Publikováno v:
Earth System Science Data, Vol 13, Pp 2607-2649 (2021)
Plant transpiration links physiological responses of vegetation to water supply and demand with hydrological, energy, and carbon budgets at the land–atmosphere interface. However, despite being the main land evaporative flux at the global scale, tr
Externí odkaz:
https://doaj.org/article/c24e67cafe694cb3a5179d458e868fd8
Autor:
Matthew L. N. Ashby, Joseph L. Hora, Kiran Lakshmipathaiah, Sarita Vig, Rama Krishna Sai Subrahmanyam Gorthi, Miju Kang, Volker Tolls, Gary J. Melnick, Michael W. Werner, Brendan P. Crill, Daniel C. Masters, Carlos Contreras Peña, Jeong-Eun Lee, Jaeyeong Kim, Ho-Gyu Lee, Sung-Yong Yoon, Soung-Chul Yang, Nicholas Flagey, Bertrand Mennesson
Publikováno v:
The Astrophysical Journal, Vol 949, Iss 2, p 105 (2023)
One of the primary objectives of the SPHEREx mission is to understand the origin of molecules such as H _2 O, CO _2 , and other volatile compounds at the early stages of planetary system formation. Because the vast majority of these compounds—typic
Externí odkaz:
https://doaj.org/article/7181e7dee674455c9e6b79ef904ca035
Autor:
Merrin S. Peterson, Björn Benneke, Karen Collins, Caroline Piaulet, Ian J. M. Crossfield, Mohamad Ali-Dib, Jessie L. Christiansen, Jonathan Gagné, Jackie Faherty, Edwin Kite, Courtney Dressing, David Charbonneau, Felipe Murgas, Marion Cointepas, Jose Manuel Almenara, Xavier Bonfils, Stephen Kane, Michael W. Werner, Varoujan Gorjian, Pierre-Alexis Roy, Avi Shporer, Francisco J. Pozuelos, Quentin Jay Socia, Ryan Cloutier, Jeremy Dietrich, Jonathan Irwin, Lauren Weiss, William Waalkes, Zach Berta-Thomson, Thomas Evans, Daniel Apai, Hannu Parviainen, Enric Pallé, Norio Narita, Andrew W. Howard, Diana Dragomir, Khalid Barkaoui, Michaël Gillon, Emmanuel Jehin, Elsa Ducrot, Zouhair Benkhaldoun, Akihiko Fukui, Mayuko Mori, Taku Nishiumi, Kiyoe Kawauchi, George Ricker, David W. Latham, Joshua N. Winn, Sara Seager, Howard Isaacson, Alex Bixel, Aidan Gibbs, Jon M. Jenkins, Jeffrey C. Smith, Jose Perez Chavez, Benjamin V. Rackham, Thomas Henning, Paul Gabor, Wen-Ping Chen, Nestor Espinoza, Eric L. N. Jensen, Kevin I. Collins, Richard P. Schwarz, Dennis M. Conti, Gavin Wang, John F. Kielkopf, Shude Mao, Keith Horne, Ramotholo Sefako, Samuel N. Quinn, Dan Moldovan, Michael Fausnaugh, Gábor Fűűrész, Thomas Barclay
Publikováno v:
Nature. 617:701-705
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ce9f50ebedcdb204e31886fd240dddca
https://doi.org/10.1038/s41586-023-05934-8
https://doi.org/10.1038/s41586-023-05934-8
Autor:
Maryame El Moutamid, Kevin B Stevenson, Billy Quarles, Nikole K Lewis, Erik Petigura, Daniel Fabrycky, Jacob L Bean, Diana Dragomir, Kristin S Sotzen, Michael W Werner
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 520:4226-4234
While various indirect methods are used to detect exoplanets, one of the most effective and accurate methods is the transit method, which measures the brightness of a given star for periodic dips when an exoplanet is passing in front of the parent st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e249dfcc37db59aaf4ee862061e93e20
https://doi.org/10.1093/mnras/stad238
https://doi.org/10.1093/mnras/stad238