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Table C.3.

References used in the emission line flux compilation for DustPedia galaxies.

Metal sample ID Reference
2dfa Colless et al. (2001)
6dfa Jones et al. (2009)
Anni10 Annibali et al. (2010)
Bres99b Bresolin et al. (1999)
Bres02 Bresolin & Kennicutt (2002)
Bres05 Bresolin et al. (2005)
Bres09 Bresolin et al. (2009)
Bres12 Bresolin et al. (2012)
CALIFAc Sánchez et al. (2012a, 2016)
CHAOS Berg et al. (2015); Croxall et al. (2015, 2016)
Crox09 Croxall et al. (2009)
DGS De Vis et al. (2017b)
Disney77 Disney & Pottasch (1977)
DV17 De Vis et al. (2017b)
GAMA Liske et al. (2015)
Gavazzi04d Gavazzi et al. (2004)
Gavazzi13e Gavazzi et al. (2013)
Gon95 Gonzalez-Delgado et al. (1995)
Gus11 Guseva et al. (2011)
Ho95e Ho et al. (1995)
HRSd Boselli et al. (2013)
Jansen00Id Jansen et al. (2000)
Jansen00Ne Jansen et al. (2000)
Kim95 Kim et al. (1995)
Kniazev2004 Kniazev et al. (2004)
Lee03 Lee et al. (2003)
Lira07 Lira et al. (2007)
MUSEc This work (ESO archival data)
Moust06Id Moustakas & Kennicutt (2006)
Moust06Ne Moustakas & Kennicutt (2006)
Moust10circ Moustakas et al. (2010)
Moust10nuce Moustakas et al. (2010)
Moust10rad Moustakas et al. (2010)
Pilyu14b Pilyugin et al. (2014)
Rodr14c Rodríguez-Baras et al. (2014)
Ros11c Rosales-Ortega et al. (2011)
SAMIc Green et al. (2018)
SDSS Alam et al. (2015)
Sanchez12c Sánchez et al. (2012b)
UZWa Falco et al. (1999)
vanZee97 van Zee et al. (1997)
vanZee98 van Zee et al. (1998)
vanZee06 van Zee & Haynes (2006)

Notes. Every listing in the sample column in Tables C.4 and C.5 here have a corresponding reference. (a) These spectra were not properly flux calibrated. Only calibrations using lines that are very close in wavelength (i.e. N2 and O3N2) can be used reliably. (b)We were not able to make the reddening correction consistent with THEMIS since these references did not provide C(H β). (c) These references provide IFU spectroscopy. (d)These references provide integrated spectroscopy. (e)These references provide nuclear spectroscopy.

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