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. Show all authors +
Journal:
Astrophysical Journal

ISSN: 1538-4357 0004-637X

Year of publication: 2012

Volume: 744

Issue: 1

Type: Article

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