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. Erakutsi egile guztiak +
Aldizkaria:
Astrophysical Journal

ISSN: 1538-4357 0004-637X

Argitalpen urtea: 2012

Alea: 744

Zenbakia: 1

Mota: Artikulua

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