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Extending the evolution of the stellar mass–size relation at z≤2 to low stellar mass galaxies from HFF and CANDELS. / Nedkova, Kalina; Haussler, Boris; Marchesini, Danilo; Dimauro, Paola; Brammer, Gabriel; Eigenthaler, Paul; Feinstein, Adina D.; Ferguson, Henry C.; Huertas-Company, Marc; Johnston, Evelyn J.; Kado-Fong, Erin; Kartaltepe, Jeyhan S.; Labbe, Ivo; Lange-Vagle, Daniel; Martis, Nicholas S.; McGrath, Elizabeth J.; Muzzin, Adam; Oesch, Pascal; Ordenes-Briceno, Yasna; Puzia, Thomas; Shipley, Heath; Simmons, Brooke D.; Skelton, Rosalind E.; Stefanon, Mauro; van der Wel, Arjen; Whitaker, Katherine E.
I:
Monthly Notices of the Royal Astronomical Society, Bind 506, Nr. 1, 01.09.2021, s. 928-956.
Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt
Harvard
Nedkova, K, Haussler, B, Marchesini, D, Dimauro, P
, Brammer, G, Eigenthaler, P, Feinstein, AD, Ferguson, HC, Huertas-Company, M, Johnston, EJ, Kado-Fong, E, Kartaltepe, JS, Labbe, I, Lange-Vagle, D, Martis, NS, McGrath, EJ, Muzzin, A
, Oesch, P, Ordenes-Briceno, Y, Puzia, T, Shipley, H, Simmons, BD, Skelton, RE, Stefanon, M, van der Wel, A & Whitaker, KE 2021, '
Extending the evolution of the stellar mass–size relation at z≤2 to low stellar mass galaxies from HFF and CANDELS',
Monthly Notices of the Royal Astronomical Society, bind 506, nr. 1, s. 928-956.
https://doi.org/10.1093/mnras/stab1744APA
Nedkova, K., Haussler, B., Marchesini, D., Dimauro, P.
, Brammer, G., Eigenthaler, P., Feinstein, A. D., Ferguson, H. C., Huertas-Company, M., Johnston, E. J., Kado-Fong, E., Kartaltepe, J. S., Labbe, I., Lange-Vagle, D., Martis, N. S., McGrath, E. J., Muzzin, A.
, Oesch, P., Ordenes-Briceno, Y., ... Whitaker, K. E. (2021).
Extending the evolution of the stellar mass–size relation at z≤2 to low stellar mass galaxies from HFF and CANDELS.
Monthly Notices of the Royal Astronomical Society,
506(1), 928-956.
https://doi.org/10.1093/mnras/stab1744Vancouver
Nedkova K, Haussler B, Marchesini D, Dimauro P
, Brammer G, Eigenthaler P o.a.
Extending the evolution of the stellar mass–size relation at z≤2 to low stellar mass galaxies from HFF and CANDELS.
Monthly Notices of the Royal Astronomical Society. 2021 sep. 1;506(1):928-956.
https://doi.org/10.1093/mnras/stab1744Author
Nedkova, Kalina ; Haussler, Boris ; Marchesini, Danilo ; Dimauro, Paola ; Brammer, Gabriel ; Eigenthaler, Paul ; Feinstein, Adina D. ; Ferguson, Henry C. ; Huertas-Company, Marc ; Johnston, Evelyn J. ; Kado-Fong, Erin ; Kartaltepe, Jeyhan S. ; Labbe, Ivo ; Lange-Vagle, Daniel ; Martis, Nicholas S. ; McGrath, Elizabeth J. ; Muzzin, Adam ; Oesch, Pascal ; Ordenes-Briceno, Yasna ; Puzia, Thomas ; Shipley, Heath ; Simmons, Brooke D. ; Skelton, Rosalind E. ; Stefanon, Mauro ; van der Wel, Arjen ; Whitaker, Katherine E. / Extending the evolution of the stellar mass–size relation at z≤2 to low stellar mass galaxies from HFF and CANDELS. I: Monthly Notices of the Royal Astronomical Society. 2021 ; Bind 506, Nr. 1. s. 928-956.
Bibtex
@article{82838cd6f7464ba5995f1f87096fda8d,
title = "Extending the evolution of the stellar mass–size relation at z≤2 to low stellar mass galaxies from HFF and CANDELS",
abstract = "We reliably extend the stellar mass-size relation over 0.2 = 10(10.3)M(circle dot) and flattens at lower masses, regardless of whether quiescence is selected based on star-formation activity, rest-frame colours, or structural characteristics. This flattening occurs at sizes of similar to 1 kpc at z = 10(9.5)M(circle dot) and quiescent galaxies with stellar masses >= 10(10.3)M(circle dot) have undergone significant size growth since z similar to 2, as expected; however, low mass galaxies have not. Finally, we supplement our data with predominantly quiescent dwarf galaxies from the core of the Fornax cluster, showing that the stellar mass-size relation is continuous below 10(7)M(circle dot), but a more complicated functional form is necessary to describe the relation.",
keywords = "galaxies: evolution, galaxies: high-redshift, galaxies: structure, DWARF ELLIPTIC GALAXIES, ASSEMBLY GAMA, ENVIRONMENTAL DEPENDENCE, QUIESCENT GALAXIES, PASSIVE GALAXIES, CLUSTER GALAXIES, STAR-FORMATION, COMPACT, REDSHIFT, COLOR",
author = "Kalina Nedkova and Boris Haussler and Danilo Marchesini and Paola Dimauro and Gabriel Brammer and Paul Eigenthaler and Feinstein, {Adina D.} and Ferguson, {Henry C.} and Marc Huertas-Company and Johnston, {Evelyn J.} and Erin Kado-Fong and Kartaltepe, {Jeyhan S.} and Ivo Labbe and Daniel Lange-Vagle and Martis, {Nicholas S.} and McGrath, {Elizabeth J.} and Adam Muzzin and Pascal Oesch and Yasna Ordenes-Briceno and Thomas Puzia and Heath Shipley and Simmons, {Brooke D.} and Skelton, {Rosalind E.} and Mauro Stefanon and {van der Wel}, Arjen and Whitaker, {Katherine E.}",
year = "2021",
month = sep,
day = "1",
doi = "10.1093/mnras/stab1744",
language = "English",
volume = "506",
pages = "928--956",
journal = "Royal Astronomical Society. Monthly Notices",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "1",
}
RIS
TY - JOUR
T1 - Extending the evolution of the stellar mass–size relation at z≤2 to low stellar mass galaxies from HFF and CANDELS
AU - Nedkova, Kalina
AU - Haussler, Boris
AU - Marchesini, Danilo
AU - Dimauro, Paola
AU - Brammer, Gabriel
AU - Eigenthaler, Paul
AU - Feinstein, Adina D.
AU - Ferguson, Henry C.
AU - Huertas-Company, Marc
AU - Johnston, Evelyn J.
AU - Kado-Fong, Erin
AU - Kartaltepe, Jeyhan S.
AU - Labbe, Ivo
AU - Lange-Vagle, Daniel
AU - Martis, Nicholas S.
AU - McGrath, Elizabeth J.
AU - Muzzin, Adam
AU - Oesch, Pascal
AU - Ordenes-Briceno, Yasna
AU - Puzia, Thomas
AU - Shipley, Heath
AU - Simmons, Brooke D.
AU - Skelton, Rosalind E.
AU - Stefanon, Mauro
AU - van der Wel, Arjen
AU - Whitaker, Katherine E.
PY - 2021/9/1
Y1 - 2021/9/1
N2 - We reliably extend the stellar mass-size relation over 0.2 = 10(10.3)M(circle dot) and flattens at lower masses, regardless of whether quiescence is selected based on star-formation activity, rest-frame colours, or structural characteristics. This flattening occurs at sizes of similar to 1 kpc at z = 10(9.5)M(circle dot) and quiescent galaxies with stellar masses >= 10(10.3)M(circle dot) have undergone significant size growth since z similar to 2, as expected; however, low mass galaxies have not. Finally, we supplement our data with predominantly quiescent dwarf galaxies from the core of the Fornax cluster, showing that the stellar mass-size relation is continuous below 10(7)M(circle dot), but a more complicated functional form is necessary to describe the relation.
AB - We reliably extend the stellar mass-size relation over 0.2 = 10(10.3)M(circle dot) and flattens at lower masses, regardless of whether quiescence is selected based on star-formation activity, rest-frame colours, or structural characteristics. This flattening occurs at sizes of similar to 1 kpc at z = 10(9.5)M(circle dot) and quiescent galaxies with stellar masses >= 10(10.3)M(circle dot) have undergone significant size growth since z similar to 2, as expected; however, low mass galaxies have not. Finally, we supplement our data with predominantly quiescent dwarf galaxies from the core of the Fornax cluster, showing that the stellar mass-size relation is continuous below 10(7)M(circle dot), but a more complicated functional form is necessary to describe the relation.
KW - galaxies: evolution
KW - galaxies: high-redshift
KW - galaxies: structure
KW - DWARF ELLIPTIC GALAXIES
KW - ASSEMBLY GAMA
KW - ENVIRONMENTAL DEPENDENCE
KW - QUIESCENT GALAXIES
KW - PASSIVE GALAXIES
KW - CLUSTER GALAXIES
KW - STAR-FORMATION
KW - COMPACT
KW - REDSHIFT
KW - COLOR
U2 - 10.1093/mnras/stab1744
DO - 10.1093/mnras/stab1744
M3 - Journal article
VL - 506
SP - 928
EP - 956
JO - Royal Astronomical Society. Monthly Notices
JF - Royal Astronomical Society. Monthly Notices
SN - 0035-8711
IS - 1
ER -
