1 INTRODUCTION

2 SUPERNOVA REMNANTS IN THE QUĲOTE-MFI SURVEY
2.1 SNRs studied in this paper

3 DATA
3.1 QUĲOTE-MFI wide survey
3.2 Surveys at radio frequencies
3.3 Microwave and infrared surveys: WMAP, Planck and DIRBE
3.4 Colour corrections and additional remarks

4 METHODOLOGY FOR SNR CHARACTERIZATION
4.1 Flux densities and uncertainties
4.2 SED fitting procedure
4.3 Modelling of the polarization angle
4.4 Constraint on the AME intensity

5 RESULTS AND DISCUSSION
5.1 SED of CTB 80
5.2 SED of the Cygnus Loop
5.3 SED of HB 21
5.4 SED of CTA 1
5.5 SED of Tycho
5.6 SED of HB 9
5.7 Overall description of the QUĲOTE SNR sample

6 CONCLUSIONS