Zobrazeno 1 - 10
of 2 905
pro vyhledávání: '"A. Roulston"'
Autor:
K. Gillespie, T. McConnell, A. Roulston, N. Potvin, C. Ghiglieri, I. Gadde, M. Anderson, J. Kirkwood, D. Thomas, L. Roche, M. O.’Sullivan, A. McCullagh, L. Graham-Wisener
Publikováno v:
BMC Palliative Care, Vol 23, Iss 1, Pp 1-68 (2024)
Abstract Background Music therapy interventions with informal carers of individuals with life-threatening illness at pre- and post-bereavement is an increasingly important clinical area. This systematic review is the first to synthesise and criticall
Externí odkaz:
https://doaj.org/article/c69074e8a9db4c5f81d022a54cfc7430
Autor:
El-Badry, Kareem, Shen, Ken J., Chandra, Vedant, Bauer, Evan, Fuller, Jim, Strader, Jay, Chomiuk, Laura, Naidu, Rohan, Caiazzo, Ilaria, Rodriguez, Antonio C., Nagarajan, Pranav, Yamaguchi, Natsuko, Vanderbosch, Zachary P., Roulston, Benjamin R., van Roestel, Jan, Gänsicke, Boris, Han, Jiwon Jesse, Burdge, Kevin B., Filippenko, Alexei V., Brink, Thomas G., Zheng, WeiKang
We report a spectroscopic search for hypervelocity white dwarfs (WDs) that are runaways from Type Ia supernovae (SNe Ia) and related thermonuclear explosions. Candidates are selected from Gaia data with high tangential velocities and blue colors. We
Externí odkaz:
http://arxiv.org/abs/2306.03914
Autor:
Yamaguchi, Natsuko, El-Badry, Kareem, Rodriguez, Antonio C., Gull, Maude, Roulston, Benjamin R., Vanderbosch, Zachary P.
We present follow-up spectroscopy of 21 cataclysmic variables (CVs) with evolved secondaries and ongoing or recently-terminated mass transfer. Evolutionary models predict that the secondaries should have anomalous surface abundances owing to nuclear
Externí odkaz:
http://arxiv.org/abs/2304.13750
Autor:
Nagarajan, Pranav, El-Badry, Kareem, Rodriguez, Antonio C., van Roestel, Jan, Roulston, Benjamin
We present multi-epoch spectroscopic follow-up of a sample of ellipsoidal variables selected from Gaia DR3 as candidates for hosting quiescent black holes (BHs) and neutron stars (NSs). Our targets were identified as BH/NS candidates because their op
Externí odkaz:
http://arxiv.org/abs/2304.07324
Autor:
The Astropy Collaboration, Price-Whelan, Adrian M., Lim, Pey Lian, Earl, Nicholas, Starkman, Nathaniel, Bradley, Larry, Shupe, David L., Patil, Aarya A., Corrales, Lia, Brasseur, C. E., Nöthe, Maximilian, Donath, Axel, Tollerud, Erik, Morris, Brett M., Ginsburg, Adam, Vaher, Eero, Weaver, Benjamin A., Tocknell, James, Jamieson, William, van Kerkwijk, Marten H., Robitaille, Thomas P., Merry, Bruce, Bachetti, Matteo, Günther, H. Moritz, Aldcroft, Thomas L., Alvarado-Montes, Jaime A., Archibald, Anne M., Bódi, Attila, Bapat, Shreyas, Barentsen, Geert, Bazán, Juanjo, Biswas, Manish, Boquien, Médéric, Burke, D. J., Cara, Daria, Cara, Mihai, Conroy, Kyle E, Conseil, Simon, Craig, Matthew W., Cross, Robert M., Cruz, Kelle L., D'Eugenio, Francesco, Dencheva, Nadia, Devillepoix, Hadrien A. R., Dietrich, Jörg P., Eigenbrot, Arthur Davis, Erben, Thomas, Ferreira, Leonardo, Foreman-Mackey, Daniel, Fox, Ryan, Freij, Nabil, Garg, Suyog, Geda, Robel, Glattly, Lauren, Gondhalekar, Yash, Gordon, Karl D., Grant, David, Greenfield, Perry, Groener, Austen M., Guest, Steve, Gurovich, Sebastian, Handberg, Rasmus, Hart, Akeem, Hatfield-Dodds, Zac, Homeier, Derek, Hosseinzadeh, Griffin, Jenness, Tim, Jones, Craig K., Joseph, Prajwel, Kalmbach, J. Bryce, Karamehmetoglu, Emir, Kałuszyński, Mikołaj, Kelley, Michael S. P., Kern, Nicholas, Kerzendorf, Wolfgang E., Koch, Eric W., Kulumani, Shankar, Lee, Antony, Ly, Chun, Ma, Zhiyuan, MacBride, Conor, Maljaars, Jakob M., Muna, Demitri, Murphy, N. A., Norman, Henrik, O'Steen, Richard, Oman, Kyle A., Pacifici, Camilla, Pascual, Sergio, Pascual-Granado, J., Patil, Rohit R., Perren, Gabriel I, Pickering, Timothy E., Rastogi, Tanuj, Roulston, Benjamin R., Ryan, Daniel F, Rykoff, Eli S., Sabater, Jose, Sakurikar, Parikshit, Salgado, Jesús, Sanghi, Aniket, Saunders, Nicholas, Savchenko, Volodymyr, Schwardt, Ludwig, Seifert-Eckert, Michael, Shih, Albert Y., Jain, Anany Shrey, Shukla, Gyanendra, Sick, Jonathan, Simpson, Chris, Singanamalla, Sudheesh, Singer, Leo P., Singhal, Jaladh, Sinha, Manodeep, Sipőcz, Brigitta M., Spitler, Lee R., Stansby, David, Streicher, Ole, Šumak, Jani, Swinbank, John D., Taranu, Dan S., Tewary, Nikita, Tremblay, Grant R., de Val-Borro, Miguel, Van Kooten, Samuel J., Vasović, Zlatan, Verma, Shresth, Cardoso, José Vinícius de Miranda, Williams, Peter K. G., Wilson, Tom J., Winkel, Benjamin, Wood-Vasey, W. M., Xue, Rui, Yoachim, Peter, ZHANG, Chen, Zonca, Andrea
The Astropy Project supports and fosters the development of open-source and openly-developed Python packages that provide commonly needed functionality to the astronomical community. A key element of the Astropy Project is the core package $\texttt{a
Externí odkaz:
http://arxiv.org/abs/2206.14220
Autor:
Estevez, Jose J., Liu, Ebony, Patel, Chirag, Roulston, Tania, Howard, Natasha J., Lake, Stewart, Henderson, Tim, Gleadle, Jonathan, Maple-Brown, Louise J., Brown, Alex, Craig, Jamie E.
Publikováno v:
In Primary Care Diabetes October 2024 18(5):547-554
Autor:
Green, Paul J., Pulgarin-Duque, Lina, Anderson, Scott F., MacLeod, Chelsea L., Eracleous, Michael, Ruan, John J., Runnoe, Jessie, Graham, Matthew, Roulston, Benjamin R., Schneider, Donald P., Ahlf, Austin, Bizyaev, Dmitry, Brownstein, Joel R., del Casal, Sonia Joesephine, Dodd, Sierra A., Hoover, Daniel, Matt, Cayenne, Merloni, Andrea, Pan, Kaike, Ramirez, Arnulfo, Ridder, Margaret
Active galactic nuclei (AGN) can vary significantly in their rest-frame optical/UV continuum emission, and with strong associated changes in broad line emission, on much shorter timescales than predicted by standard models of accretion disks around s
Externí odkaz:
http://arxiv.org/abs/2201.09123
Autor:
Roulston, Mark S.1,2 (AUTHOR), Kaivanto, Kim2,3 (AUTHOR) k.kaivanto@lancaster.ac.uk
Publikováno v:
PLoS ONE. 8/30/2024, Vol. 19 Issue 8, p1-14. 14p.
Autor:
Roulston, Benjamin R., Green, Paul J., Montez, Rodolfo, Filippazzo, Joseph, Drake, Jeremy J., Toonen, Silvia, Anderson, Scott F., Eracleous, Michael, Frank, Adam
As main-sequence stars with C$>$O, dwarf carbon (dC) stars are never born alone but inherit carbon-enriched material from a former asymptotic giant branch (AGB) companion. In contrast to M dwarfs in post-mass transfer binaries, C$_2$ and/or CN molecu
Externí odkaz:
http://arxiv.org/abs/2110.00013
Autor:
Hepner, Mark J., Orcutt, Ellison, Price, Kyle, Goodell, Karen, Roulston, T’ai, Jean, Robert P., Richardson, Rodney T.
Publikováno v:
In Forest Ecology and Management 15 March 2024 556