activity
20152024
most citedGalaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

249 citations · 776 across the 10 of their papers we have counts for

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Showing astro-ph.GAShow all

18 papers · 1 filter

astro-ph.GA2024

TREASUREHUNT: Transients and Variability Discovered with HST in the JWST North Ecliptic Pole Time Domain Field

Rosalia O'Brien, Rolf A. Jansen, Norman A. Grogin +56

The JWST North Ecliptic Pole (NEP) Time Domain Field (TDF) is a 14 arcmin diameter field optimized for multi-wavelength time-domain science with JWST. It has been observed acros…

astro-ph.GA2022249 cited

Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

Simon P. Driver, Sabine Bellstedt, Aaron S. G. Robotham +67

In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248682 galaxy spectra, and, in combination with earli…

astro-ph.GA202021 cited

Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups

J. A. Vázquez-Mata, J. Loveday, S. D. Riggs +14

How do galaxy properties (such as stellar mass, luminosity, star formation rate, and morphology) and their evolution depend on the mass of their host dark matter halo? Using the Ga…

astro-ph.GA2020

A Strong-Lensing Model for the WMDF JWST/GTO Very Rich Cluster Abell 1489

Adi Zitrin, Ana Acebron, Dan Coe +18

We present a first strong-lensing model for the galaxy cluster RM J121218.5+273255.1 (; hereafter RMJ1212; also known as Abell 1489). This cluster is amongst the top 0.1\%…

astro-ph.GA202011 cited

Galaxy And Mass Assembly (GAMA): Defining Passive Galaxy Samples and Searching for the UV Upturn

S. Phillipps, S. S. Ali, M. N. Bremer +16

We use data from the GAMA and GALEX surveys to demonstrate that the UV upturn, an unexpected excess of ultraviolet flux from a hot stellar component, seen in the spectra of many ea…

astro-ph.GA2019

Connecting SDSS central galaxies to their host halos using total satellite luminosity

Mehmet Alpaslan, Jeremy L. Tinker

The total luminosity of satellite galaxies around a central galaxy, L, is a powerful metric for probing dark matter halos. In this paper we use data from the Sloan Digital…