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pro vyhledávání: '"Greco, Jennifer J."'
Autor:
Christie, Duncan A., Lee, Elspeth K. H., Innes, Hamish, Noti, Pascal A., Charnay, Benjamin, Fauchez, Thomas J., Mayne, Nathan J., Deitrick, Russell, Ding, Feng, Greco, Jennifer J., Hammond, Mark, Malsky, Isaac, Mandell, Avi, Rauscher, Emily, Roman, Michael T., Sergeev, Denis E., Sohl, Linda, Steinrueck, Maria E., Turbet, Martin, Wolf, Eric T., Zamyatina, Maria, Carone, Ludmila
With an increased focus on the observing and modelling of mini-Neptunes, there comes a need to better understand the tools we use to model their atmospheres. In this paper, we present the protocol for the CAMEMBERT (Comparing Atmospheric Models of Ex
Externí odkaz:
http://arxiv.org/abs/2211.04048
Autor:
Orton, Glenn S., Antunano, Arrate, Fletcher, Leigh N., Sinclair, James A., Momary, Thomas W., Fujiyoshi, Takuya, Yanamandra-Fisher, Padma, Donnelly, Padraig T., Greco, Jennifer J., Payne, Anna V., Boydstun, Kimberly A., Wakefield, Laura E.
An essential component of planetary climatology is knowledge of the tropospheric temperature field and its variability. Previous studies of Jupiter hinted at periodic behavior that was non-seasonal, as well as dynamical relationships between troposph
Externí odkaz:
http://arxiv.org/abs/2211.04398
Autor:
Greco, Jennifer J.
We present the results of two near-infrared spectroscopic studies of ultracool dwarfs. The first utilizes low-resolution spectroscopy to follow-up discoveries from an all-sky proper motion survey conducted using multi-epoch data from the Wide-field I
Autor:
Schneider, Adam C., Burgasser, Adam J., Gerasimov, Roman, Marocco, Federico, Gagne, Jonathan, Goodman, Sam, Beaulieu, Paul, Pendrill, William, Rothermich, Austin, Sainio, Arttu, Kuchner, Marc J., Caselden, Dan, Meisner, Aaron M., Faherty, Jacqueline K., Mamajek, Eric E., Hsu, Chih-Chun, Greco, Jennifer J., Cushing, Michael C., Kirkpatrick, J. Davy, Gagliuffi, Daniella Bardalez, Logsdon, Sarah E., Allers, Katelyn, Debes, John H., Worlds, The Backyard, Collaboration, Planet 9
We present the discoveries of WISEA J041451.67-585456.7 and WISEA J181006.18-101000.5, two low-temperature (1200$-$1400 K), high proper motion T-type subdwarfs. Both objects were discovered via their high proper motion ($>$0.5 arcsec yr$^{-1}$); WISE
Externí odkaz:
http://arxiv.org/abs/2007.03836
Autor:
Greco, Jennifer J., Schneider, Adam C., Cushing, Michael C., Kirkpatrick, J. Davy, Burgasser, Adam J.
We present low-resolution near-infrared spectra of discoveries from an all-sky proper motion search conducted using multi-epoch data from the Wide-field Infrared Survey Explorer. Using the data from NEOWISE, along with the AllWISE catalog, Schneider
Externí odkaz:
http://arxiv.org/abs/1908.10988
Autor:
Dulaney, Nick, Richardson, Noel D., Gerhartz, Cody J., Bjorkman, J. E., Bjorkman, K. S., Carciofi, Alex C., Klement, Robert, Wang, Luqian, Morrison, Nancy D., Bratcher, Allison D., Greco, Jennifer J., Hardegree-Ullman, Kevin K., Lembryk, Ludwik, Oswald, Wayne L., Trucks, Jesica L.
The late-type Be star $\beta$ CMi is remarkably stable compared to other Be stars that have been studied. This has led to a realistic model of the outflowing Be disk by Klement et al. These results showed that the disk is likely truncated at a finite
Externí odkaz:
http://arxiv.org/abs/1701.05201
Akademický článek
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Ultracool dwarfs, a mix of the lowest mass stars and brown dwarfs (substellar object too low mass to initiate stable hydrogen fusion), are the lowest mass products of star formation. The lack of a stable internal energy source causes brown dwarfs to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::803f41a29653299ec22746d6717db274
Brown dwarfs are substellar objects too low mass to initiate the hydrogen fusion necessary to be considered stars. Ultracool dwarfs, objects with spectral types of M7 or later, are a mix of low mass stars and brown dwarfs. We have obtained the first
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::415d364d8264ccbaced90546e48bd371
Autor:
Orton, Glenn S., Antuñano, Arrate, Fletcher, Leigh N., Sinclair, James A., Momary, Thomas W., Fujiyoshi, Takuya, Yanamandra-Fisher, Padma, Donnelly, Padraig T., Greco, Jennifer J., Payne, Anna V., Boydstun, Kimberly A., Wakefield, Laura E.
Publikováno v:
Nature Astronomy; Apr2023, Vol. 7 Issue 4, p503-503, 1p