Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Prole, Daniel J."'
The stellar mass - physical effective radius relation for dwarf galaxies in low-density environments
Autor:
Prole, Daniel J.
The scaling relation between stellar mass ($M_{*}$) and physical effective radius ($r_{e}$) has been well-studied using wide spectroscopic surveys. However, these surveys suffer from severe surface brightness incompleteness in the dwarf galaxy regime
Externí odkaz:
http://arxiv.org/abs/2106.14924
Understanding the formation and evolution of low surface brightness galaxies (LSBGs) is critical for explaining their wide-ranging properties. However, studies of LSBGs in deep photometric surveys are often hindered by a lack of distance estimates. I
Externí odkaz:
http://arxiv.org/abs/2010.11210
Autor:
Spitler, Lee R., Longbottom, Fergus D., Alvarado-Montes, Jaime A., Bazkiaei, Amir E., Caddy, Sarah E., Gee, Wilfred T., Horton, Anthony, Lee, Steven, Prole, Daniel J.
The Huntsman Telescope, located at Siding Spring Observatory in Australia, is a system of ten telephoto Canon lenses designed for low surface brightness imaging in the Southern sky. Based upon the Dragonfly Telephoto Array, the refractive lens-based
Externí odkaz:
http://arxiv.org/abs/1911.11579
While much of the focus around Ultra-Diffuse Galaxies (UDGs) has been given to those in galaxy groups and clusters, relatively little is known about them in less-dense environments. These isolated UDGs provide fundamental insights into UDG formation
Externí odkaz:
http://arxiv.org/abs/1910.14057
While we have learned much about Ultra-Diffuse Galaxies (UDGs) in groups and clusters, relatively little is known about them in less-dense environments. More isolated UDGs are important for our understanding of UDG formation scenarios because they fo
Externí odkaz:
http://arxiv.org/abs/1907.01559
Autor:
Prole, Daniel J., Hilker, Michael, van der Burg, Remco F. J., Cantiello, Michele, Venhola, Aku, Iodice, Enrica, van de Ven, Glenn, Wittmann, Carolin, Peletier, Reynier F., Mieske, Steffen, Capaccioli, Massimo, Napolitano, Nicola R., Paolillo, Maurizio, Spavone, Marilena, Valentijn, Edwin
The halo masses $M_{halo}$ of low surface brightness (LSB) galaxies are critical measurements for understanding their formation processes. One promising method to estimate a galaxy's $M_{halo}$ is to exploit the empirical scaling relation between $M_
Externí odkaz:
http://arxiv.org/abs/1901.09648
We report the automatic detection of a new sample of very low surface brightness (LSB) galaxies, likely members of the Virgo cluster. We introduce our new software, {\tt DeepScan}, that has been designed specifically to detect extended LSB features a
Externí odkaz:
http://arxiv.org/abs/1804.08332
The availability of deep, wide area surveys in the optical and near-infrared regime have opened a window of opportunity for the study of the low surface brightness universe over many different scales. One of the key science goals for such research is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f502d02404d92542394245433741c0f