Reconstructing the stellar mass distributions of galaxies using S 4G IRAC 3.6 and 4.5 μm images. I. Correcting for contamination by polycyclic aromatic hydrocarbons, hot dust, and intermediate-age stars

  1. Meidt, S.E.
  2. Schinnerer, E.
  3. Knapen, J.H.
  4. Bosma, A.
  5. Athanassoula, E.
  6. Sheth, K.
  7. Buta, R.J.
  8. Zaritsky, D.
  9. Laurikainen, E.
  10. Elmegreen, D.
  11. Elmegreen, B.G.
  12. Gadotti, D.A.
  13. Salo, H.
  14. Regan, M.
  15. Ho, L.C.
  16. Madore, B.F.
  17. Hinz, J.L.
  18. Skibba, R.A.
  19. Gil De Paz, A.
  20. Mũoz-Mateos, J.-C.
  21. Menéndez-Delmestre, K.
  22. Seibert, M.
  23. Kim, T.
  24. Mizusawa, T.
  25. Laine, J.
  26. Comerón, S.
  27. Montrer des auteurs +
Revue:
Astrophysical Journal

ISSN: 1538-4357 0004-637X

Année de publication: 2012

Volumen: 744

Número: 1

Type: Article

DOI: 10.1088/0004-637X/744/1/17 GOOGLE SCHOLAR