SP
S. M. Percival
astro-phastro-ph.GAastro-ph.SRastro-ph.COastro-ph.HE
On Valency
published · living versionsW_v5ejn3vd·v1 · currentpublished
An H-alpha survey of the host environments of 77 type IIn supernovae within z<0.02
with C. L. Ransome, S. M. Habergham Mawson, M. J. Darnley, P. A. James
1 version
Preprints & journals
25 papers in the corpus · 2002–2022An H-alpha survey of the host environments of 77 type IIn supernovae within z<0.022204.09706v2 · C. L. Ransome, S. M. Habergham Mawson, M. J. Darnley et al.2022 · 18 citationsarXivon Valency
Diffuse LINER-type emission from extended disc regions of barred galaxies2005.08985v2 · S.M. Percival, P.A. James2020 · 4 citationsMNRAS 496, 36-48 (2020)
Galaxy and Mass Assembly (GAMA): Variation in Galaxy Structure Across the Green Valley1804.04470v1 · Lee S. Kelvin, Malcolm N. Bremer, Steven Phillipps et al.2018 · 37 citationsarXiv
Galaxy and Mass Assembly (GAMA): Morphological transformation of galaxies across the green valley1801.04277v1 · M.N. Bremer, S. Phillipps, L.S. Kelvin et al.2018 · 88 citationsarXiv
Star formation suppression and bar ages in nearby barred galaxies1711.10537v1 · P. A. James, S. M. Percival2017 · 59 citationsarXiv
SN 2016coi/ASASSN-16fp: An example of residual helium in a type Ic supernova?1709.03593v2 · S. J. Prentice, C. Ashall, P. A. Mazzali et al.2017 · 52 citationsarXiv
Stellar population constraints on the ages of galactic bars1601.04706v1 · Phil A. James, Susan M. Percival2016 · 59 citationsarXiv
Discovery of kpc-scale line emission in barred galaxies, not linked to AGN or star formation1504.04013v1 · Phil A. James, Susan M. Percival2015 · 24 citationsarXiv
Photometric and spectroscopic observations, and abundance tomography modelling of the type Ia supernova SN 2014J located in M821409.7066v3 · C. Ashall, P. Mazzali, D. Bersier et al.2014 · 48 citationsarXiv
Environment-derived constraints on the progenitors of low-luminosity type I supernovae1306.2474v1 · Joseph Lyman, Phil James, Hagai B. Perets et al.2013 · 74 citationsarXiv
Modelling chemical abundance anticorrelations on globular cluster spectra1203.4304v1 · Paula Coelho, Susan Percival, Maurizio Salaris2012 · 1 citationarXiv
The impact of systematic uncertainties in stellar parameters on integrated spectra of stellar populations0908.0951v1 · Susan M. Percival, Maurizio Salaris2009 · 40 citationsarXiv
Optical and near infra-red colours as a discriminant of the age and metallicity of stellar populations0905.0810v1 · David Carter, Daniel J. B. Smith, Susan M. Percival et al.2009 · 27 citationsMon.Not.Roy.Astron.Soc.397:695-708,2009
A large stellar evolution database for population synthesis studies. V. Stellar models and isochrones with CNONa abundance anticorrelations0903.0825v1 · A. Pietrinferni, S. Cassisi, M. Salaris et al.2009 · 145 citationsAstrophys.J.697:275-282,2009
A large stellar evolution database for population synthesis studies. IV. Integrated properties and spectra0809.0265v1 · Susan M. Percival, Maurizio Salaris, Santi Cassisi et al.2008 · 104 citationsAstrophys.J.690:427-439,2009
Constraints on supernova progenitors from spatial correlations with H-alpha emission0704.2387v1 · J.P. Anderson, P.A. James, M. Salaris et al.2007 · 2 citationsAIP Conf.Proc.937:220-224,2007
The H-alpha Galaxy Survey II. Extinction and NII corrections to H-alpha fluxesastro-ph/0410386v1 · P.A. James (JMU), N.S. Shane (JMU), J.H. Knapen et al.2004 · 53 citationsarXiv
The distance to the Pleiades: Main sequence fitting in the near infraredastro-ph/0409362v1 · S.M. Percival, M. Salaris, M.A.T. Groenewegen2004 · 25 citationsAstron.Astrophys. 429 (2005) 887-894
The H alpha Galaxy Survey I. The galaxy sample, H alpha narrow-band observations and star formation parameters for 334 galaxiesastro-ph/0311030v1 · P. A. James, N. S. Shane, J. E. Beckman et al.2003 · 224 citationsAstron.Astrophys. 414 (2004) 23-43
The age of the oldest Open Clustersastro-ph/0310363v1 · Maurizio Salaris, Achim Weiss, Susan M. Percival2003 · 195 citationsAstron.Astrophys. 414 (2004) 163-174
A theoretical analysis of the systematic errors in the Red Clump distance to the LMCastro-ph/0307329v1 · Maurizio Salaris, Susan Percival, Leo Girardi2003 · 20 citationsMon.Not.Roy.Astron.Soc.345:1030,2003
An empirical test of the theoretical population corrections to the Red Clump absolute magnitudeastro-ph/0304140v1 · Susan M. Percival, Maurizio Salaris2003 · 46 citationsMon.Not.Roy.Astron.Soc. 343 (2003) 539
The distance to the LMC cluster NGC 1866 and the surrounding fieldastro-ph/0301532v1 · M. Salaris, S. Percival, E. Brocato et al.2003 · 24 citationsarXiv
The Open Cluster Distance Scale: A New Empirical Approachastro-ph/0301219v1 · Susan M. Percival, Maurizio Salaris, David Kilkenny2003 · 37 citationsAstron.Astrophys.400:541-552,2003
Resolving the 47 Tucanae Distance Problemastro-ph/0203157v1 · Susan M. Percival, Maurizio Salaris, Francois van Wyk et al.2002 · 36 citationsarXiv
Career total: 36 works. 25 are in this corpus.
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