papers

Publications (22)

astro-ph.GA2024

Increasing AGN sample completeness using long-term near-infrared variability

K. Green, E. Elmer, D. T. Maltby +3

In this work, we use 8 years of deep near-infrared imaging to select and study a new set of 601 active galaxies identified through long-term near-infrared (NIR) variability in the…

astro-ph.GA2023

The role of mass and environment in the build up of the quenched galaxy population since cosmic noon

E. Taylor, O. Almaini, M. Merrifield +4

We conduct the first study of how the relative quenching probability of galaxies depends on environment over the redshift range , using data from the UKIDSS Ultra-Deep…

astro-ph.GA2017

SDSS-IV MaNGA: Uncovering the Angular Momentum Content of Central and Satellite Early-type Galaxies

Jenny E. Greene, Alexie Leauthaud, Eric Emsellem +18

We study 379 central and 159 satellite early-type galaxies with two-dimensional kinematics from the integral-field survey Mapping Nearby Galaxies at APO (MaNGA) to determine how th…

astro-ph.GA2016

SDSS-IV MaNGA: Properties of galaxies with kinematically decoupled stellar and gaseous components

Yifei Jin, Yanmei Chen, Yong Shi +30

We study the properties of 66 galaxies with kinematically misaligned gas and stars from MaNGA survey. The fraction of kinematically misaligned galaxies varies with galaxy physical…

astro-ph2002

The Planetary Nebulae Spectrograph: the green light for Galaxy Kinematics

N. G. Douglas, M. Arnaboldi, K. C. Freeman +10

Planetary nebulae are now well established as probes of galaxy dynamics and as standard candles in distance determinations. Motivated by the need to improve the efficiency of plane…

astro-ph.GA2017

Probing the kinematic morphology-density relation of early-type galaxies with MaNGA

J. E. Greene, A. Leauthaud, E. Emsellem +17

The "kinematic" morphology-density relation for early-type galaxies posits that those galaxies with low angular momentum are preferentially found in the highest-density regions of…

astro-ph2005

Nuclear Properties of Nearby Spiral Galaxies from Hubble Space Telescope NICMOS imaging and STIS Spectroscopy

M. A. Hughes, D. Axon, J. Atkinson +16

We investigate the central regions of 23 spiral galaxies using archival NICMOS imaging and STIS spectroscopy. The sample is taken from our program to determine the masses of centra…

astro-ph.GA2023

Planetary nebulae populations in the haloes of nearby massive early-type galaxies

J. Hartke, M. Arnaboldi, O. Gerhard +8

Planetary nebulae (PNe) are excellent tracers of the metal-poor haloes of nearby early-type galaxies. They are commonly used to trace spatial distribution and kinematics of the hal…

astro-ph.GA2022

The halo of M105 and its group environment as traced by planetary nebula populations: II. Using kinematics of single stars to unveil the presence of intragroup light around the Leo I galaxies NGC 3384 and M105

J. Hartke, M. Arnaboldi, O. Gerhard +11

M105 is an early-type galaxy in the nearby Leo I group, the closest galaxy group to contain all galaxy types and therefore an excellent environment to explore the low-mass end of i…

astro-ph.GA2020

The halo of M105 and its group environment as traced by planetary nebula populations: I. Wide-field photometric survey of planetary nebulae in the Leo I group

J. Hartke, M. Arnaboldi, O. Gerhard +6

M105 (NGC 3379) is an early-type galaxy in the Leo I group. This group is the nearest group that contains all main galaxy types and can thus be used as a benchmark to study the pro…

astro-ph2004

Nuclear properties of a sample of nearby spirals from STIS imaging

C. Scarlata, M. Stiavelli, M. Hughes +17

We present surface photometry for the central regions of a sample of 48 spiral galaxies (mostly unbarred and barred of types Sbc or Sc) observed with the Space Telescope Imaging Sp…

astro-ph.GA2018

Three dynamically distinct stellar populations in the halo of M49

J. Hartke, M. Arnaboldi, O. Gerhard +6

M49 (NGC 4472) is the dominant galaxy in subcluster B of the Virgo Cluster, and a benchmark for studying the build-up of the extended halos of brightest group galaxies in the outsk…

astro-ph.GA2019

SNITCH: Seeking a simple, informative star formation history inference tool

R. J. Smethurst, M. Merrifield, C. J. Lintott +7

Deriving a simple, analytic galaxy star formation history (SFH) using observational data is a complex task without the proper tool to hand. We therefore present SNITCH, an open sou…

astro-ph2000

The black hole mass vs bulge mass relationship in spiral galaxies

A. Marconi, D. Axon, J. Atkinson +15

We describe an on-going HST program aimed at determining the relationship between the nuclear black hole mass and bulge mass in spiral galaxies. We have selected a volume limited s…

astro-ph.GA2021

Long-term NIR Variability in the UKIDSS Ultra Deep Survey: a new probe of AGN activity at high redshift

E. Elmer, O. Almaini, M. Merrifield +5

We present the first attempt to select AGN using long-term NIR variability. By analysing the K-band light curves of all the galaxies in the UKIDSS Ultra Deep Survey, the deepest NI…

astro-ph.GA2018

Resolving the Disc-Halo Degeneracy I: A Look at NGC 628

S. Aniyan, K. C. Freeman, M. Arnaboldi +6

The decomposition of the rotation curve of galaxies into contribution from the disc and dark halo remains uncertain and depends on the adopted mass to light ratio (M/L) of the disc…

astro-ph2005

Integral Field Spectroscopy of 23 Spiral Bulges

D. Batcheldor, D. Axon, D. Merritt +7

We have obtained Integral Field Spectroscopy for 23 spiral bulges using INTEGRAL on the William Herschel Telescope and SPIRAL on the Anglo-Australian Telescope. This is the first 2…

astro-ph.GA2020

Resolving the Disc-Halo Degeneracy II: NGC 6946

S. Aniyan, A. A. Ponomareva, K. C. Freeman +5

The mass-to-light ratio (M/L) is a key parameter in decomposing galactic rotation curves into contributions from the baryonic components and the dark halo of a galaxy. One direct o…

astro-ph.GA2019

SDSS-IV MaNGA: Bar pattern speed estimates with the Tremaine-Weinberg method and their error sources

L. Garma-Oehmichen, M. Cano-Díaz, H. Hernández-Toledo +5

Estimating the bar pattern speed (\Om{}) is one of the main challenges faced in understanding the role of stellar bars in galaxy dynamical evolution. This work aims to characterise…

astro-ph2004

Mapping the Stellar Dynamics of M31

Helen Merrett, M. Merrifield, K. Kuijken +12

Using the Planetary Nebula Spectrograph, we have observed and measured the velocities for some 2764 PNe in the disk and halo of the Andromeda galaxy. Preliminary analysis using a b…

astro-ph.GA2021

Infrared lags in the light curves of AGN measured using a deep survey

E. Elmer, M. Merrifield, O. Almaini +2

Information on the structure around active galactic nuclei (AGN) has long been derived from measuring lags in their varying light output at different wavelengths. In principle, inf…

astro-ph.GA2019

Properties of barred galaxies in the MaNGA galaxy survey

A. Fraser-McKelvie, M. Merrifield, A. Aragón-Salamanca +2

We present the initial results of a census of 684 barred galaxies in the MaNGA galaxy survey. This large sample contains galaxies with a wide range of physical properties, and we a…