VizieR Online Data Catalog: Infrared properties of planetary nebulae (Muthumariappan+, 2020)

All the data required for this study were taken from the literature. The near-IR fluxes were calculated from the magnitudes at respective wavelengths which were obtained from the 2MASS archive (Cutri et al. 2003tmc..book.....C, Cat. II/246) archive. IRAS (Neugebauer et al. 1984ApJ...278L...1N) fluxes at 12, 25, 60, and 100μm, and WISE (Wright et al. 2010AJ....140.1868W) fluxes at 3.4, 4.6, 12, and 22μm were used to span the mid- and far-IR emission. In addition, we have used archived fluxes from Akari (Ishihara et al. 2010A&A...514A...1I, Cat. II/297) at its 65-, 90-, 140-, and 160-μm bands to trace the emission from cold dust down to ~30K. The 2MASS and Akari data used for this study are available at the NASA/IPAC Infrared Science Archive.

Our sample of [WR] PNe and wels-PNe are from the catalogue of spectral classification of CSPNe given by Weidmann & Gamen (2011A&A...526A...6W, Cat. J/A+A/526/A6). We have taken the nebular Hβ fluxes and electron densities from Stasinska & Szczerba (1999A&A...352..297S, Cat. J/A+A/352/297). Emission-line fluxes of [OIII] and HeII are obtained from Strasbourg-ESO Catalogue of Galactic PNe (Acker et al. 1992ESOPN...1....1A, Cat. V/84). Distances to PNe in our sample are from Frew, Parker & Bojicic (2016MNRAS.455.1459F).

(3 data files).