Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Leslie, Sarah K."'
Autor:
Huang, Rongjun, Battisti, Andrew J., Grasha, Kathryn, da Cunha, Elisabete, Lagos, Claudia del P, Leslie, Sarah K., Wisnioski, Emily
Previous studies have shown that the normalization and scatter of the galaxy 'main sequence' (MS), the relation between star formation rate (SFR) and stellar mass ($M_*$), evolves over cosmic time. However, such studies often rely on photometric reds
Externí odkaz:
http://arxiv.org/abs/2301.01995
Autor:
Cooke, Kevin C., Kartaltepe, Jeyhan S., Rose, Caitlin, Tyler, K. D., Darvish, Behnam, Leslie, Sarah K., Peng, Ying-jie, Häußler, Boris, Koekemoer, Anton M.
We investigate the relationship between environment, morphology, and the star formation rate -- stellar mass relation derived from a sample of star-forming galaxies (commonly referred to as the `star formation main sequence') in the COSMOS field from
Externí odkaz:
http://arxiv.org/abs/2211.16527
Autor:
Algera, Hiddo S. B., Hodge, Jacqueline A., Riechers, Dominik A., Leslie, Sarah K., Smail, Ian, Aravena, Manuel, da Cunha, Elisabete, Daddi, Emanuele, Decarli, Roberto, Dickinson, Mark, Gim, Hansung B., Guaita, Lucia, Magnelli, Benjamin, Murphy, Eric J., Pavesi, Riccardo, Sargent, Mark T., Sharon, Chelsea E., Wagg, Jeff, Walter, Fabian, Yun, Min
Radio free-free emission is considered to be one of the most reliable tracers of star formation in galaxies. However, as it constitutes the faintest part of the radio spectrum -- being roughly an order of magnitude less luminous than radio synchrotro
Externí odkaz:
http://arxiv.org/abs/2111.01153
Autor:
Roy, Namrata, Moravec, Emily, Bundy, Kevin, Hardcastle, Martin J., Gürkan, Gülay, Baldi, Ranieri D., Leslie, Sarah K., Masters, Karen, Gelfand, Joseph, Riffel, Rogerio, Riffel, Rogemar A., Mingo, Beatriz, Drabent, Alexander
We present 150 MHz, 1.4 GHz, and 3 GHz radio imaging (LoTSS, FIRST and VLASS) and spatially resolved ionized gas characteristics (SDSS IV-MaNGA) for 140 local ($z<0.1$) early-type "red geyser" galaxies. These galaxies have low star formation activity
Externí odkaz:
http://arxiv.org/abs/2109.02609
Autor:
Croom, Scott M., Owers, Matt S., Scott, Nicholas, Poetrodjojo, Henry, Groves, Brent, van de Sande, Jesse, Barone, Tania M., Cortese, Luca, D'Eugenio, Francesco, Bland-Hawthorn, Joss, Bryant, Julia, Oh, Sree, Brough, Sarah, Agostino, James, Casura, Sarah, Catinella, Barbara, Colless, Matthew, Cecil, Gerald, Davies, Roger L., Drinkwater, Michael J., Driver, Simon P., Ferreras, Ignacio, Foster, Caroline, Fraser-McKelvie, Amelia, Lawrence, Jon, Leslie, Sarah K., Liske, Jochen, López-Sánchez, Ángel R., Lorente, Nuria P. F., McElroy, Rebecca, Medling, Anne M., Obreschkow, Danail, Richards, Samuel N., Sharp, Rob, Sweet, Sarah M., Taranu, Dan S., Taylor, Edward N., Tescari, Edoardo, Thomas, Adam D., Tocknell, James, Vaughan, Sam P.
We have entered a new era where integral-field spectroscopic surveys of galaxies are sufficiently large to adequately sample large-scale structure over a cosmologically significant volume. This was the primary design goal of the SAMI Galaxy Survey. H
Externí odkaz:
http://arxiv.org/abs/2101.12224
Local galaxies from the Sloan Digital Sky Survey are used to provide additional support for an evolutionary pathway in which AGN activity is associated with star-formation quenching. Composite, Seyfert 2 and LINER galaxies account for $\sim$60\% of a
Externí odkaz:
http://arxiv.org/abs/1810.10021
Autor:
Medling, Anne M., Cortese, Luca, Croom, Scott M., Green, Andrew W., Groves, Brent, Hampton, Elise, Ho, I-Ting, Davies, Luke J. M., Kewley, Lisa J., Moffett, Amanda J., Schaefer, Adam L., Taylor, Edward, Zafar, Tayyaba, Bekki, Kenji, Bland-Hawthorn, Joss, Bloom, Jessica V., Brough, Sarah, Bryant, Julia J., Catinella, Barbara, Cecil, Gerald, Colless, Matthew, Couch, Warrick J., Drinkwater, Michael J., Driver, Simon P., Federrath, Christoph, Foster, Caroline, Goldstein, Gregory, Goodwin, Michael, Hopkins, Andrew, Lawrence, J. S., Leslie, Sarah K., Lewis, Geraint F., Lorente, Nuria P. F., Owers, Matt S., McDermid, Richard, Richards, Samuel N., Sharp, Robert, Scott, Nicholas, Sweet, Sarah M., Taranu, Dan S., Tescari, Edoardo, Tonini, Chiara, van de Sande, Jesse, Walcher, C. Jakob, Wright, Angus
We present the ~800 star formation rate maps for the SAMI Galaxy Survey based on H{\alpha} emission maps, corrected for dust attenuation via the Balmer decrement, that are included in the SAMI Public Data Release 1. We mask out spaxels contaminated b
Externí odkaz:
http://arxiv.org/abs/1801.04283
Autor:
Lee, Nicholas, Sheth, Kartik, Scott, Kimberly S., Toft, Sune, Magdis, Georgios, Damjanov, Ivana, Zahid, H. Jabran, Casey, Caitlin M., Cortzen, Isabella, Guijarro, Carlos Gomez, Karim, Alexander, Leslie, Sarah K., Schinnerer, Eva
Publikováno v:
2017, MNRAS, Volume 471, Issue 2, p.2124-2142
Recent literature suggests that there are two modes through which galaxies grow their stellar mass - a normal mode characterized by quasi-steady star formation, and a highly efficient starburst mode possibly triggered by stochastic events such as gal
Externí odkaz:
http://arxiv.org/abs/1710.02757
Autor:
van de Sande, Jesse, Bland-Hawthorn, Joss, Fogarty, Lisa M. R., Cortese, Luca, d'Eugenio, Francesco, Croom, Scott M., Scott, Nicholas, Allen, James T., Brough, Sarah, Bryant, Julia J., Cecil, Gerald, Colless, Matthew, Couch, Warrick J., Davies, Roger, Elahi, Pascal J., Foster, Caroline, Goldstein, Greg, Goodwin, Michael, Groves, Brent, Ho, I-Ting, Jeong, Hyunjin, Jones, D. Heath, Konstantopoulos, Iraklis S., Lawrence, Jon S., Leslie, Sarah K., Lopez-Sanchez, Angel R., McDermid, Richard M., McElroy, Rebecca, Medling, Anne M., Oh, Sree, Owers, Matt S., Richards, Samuel N., Schaefer, Adam L., Sharp, Rob, Sweet, Sarah M., Taranu, Dan, Tonini, Chiara, Walcher, C. Jakob, Yi, Sukyoung K.
Recent cosmological hydrodynamical simulations suggest that integral field spectroscopy can connect the high-order stellar kinematic moments h3 (~skewness) and h4 (~kurtosis) in galaxies to their cosmological assembly history. Here, we assess these r
Externí odkaz:
http://arxiv.org/abs/1611.07039
Autor:
Ho, I-Ting, Medling, Anne M., Bland-Hawthorn, Joss, Groves, Brent, Kewley, Lisa J., Kobayashi, Chiaki, Dopita, Michael A., Leslie, Sarah K., Sharp, Rob, Allen, James T., Bourne, Nathan, Bryant, Julia J., Cortese, Luca, Croom, Scott M., Dunne, Loretta, Fogarty, L. M. R., Goodwin, Michael, Green, Andy W., Konstantopoulos, Iraklis S., Lawrence, Jon S., Lorente, Nuria P. F., Owers, Matt S., Richards, Samuel, Sweet, Sarah M., Tescari, Edoardo, Valiante, Elisabetta
We investigate a sample of 40 local, main-sequence, edge-on disc galaxies using integral field spectroscopy with the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey to understand the link between properties of the extraplanar
Externí odkaz:
http://arxiv.org/abs/1601.02022