APA
Amblard A., Cooray A., Serra P., Altieri B., Arumugam V., Aussel H., Blain A., Bock J., Boselli A., Buat V., Castro-Rodríguez N., Cava A., Chanial P., Chapin E., Clements D. L., Conley A., Conversi L., Dowell C. D., Dwek E., Eales S., Elbaz D., Farrah D., Franceschini A., Gear W., Glenn J., Griffin M., Halpern M., Hatziminaoglou E., Ibar E., Isaak K., Ivison R. J., Khostovan A. A., Lagache G., Levenson L., Lu N., Madden S., Maffei B., Mainetti G., Marchetti L., Marsden G., Mitchell-Wynne K., Nguyen H. T., O'Halloran B., Oliver S. J., Omont A., Page M. J., Panuzzo P., Papageorgiou A., Pearson C. P., Pérez-Fournon I., Pohlen M., Rangwala N., Roseboom I. G., Rowan-Robinson M., Portal M. S., Schulz B., Scott D., Seymour N., Shupe D. L., Smith A. J., Stevens J. A., Symeonidis M., Trichas M., Tugwell K., Vaccari M., Valiante E., Valtchanov I., Vieira J. D., Vigroux L., Wang L., Ward R., Wright G., Xu C. K. & Zemcov M. (20110311). Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses. : Nature.
Chicago
Amblard Alexandre, Cooray Asantha, Serra Paolo, Altieri B, Arumugam V, Aussel H, Blain A, Bock J, Boselli A, Buat V, Castro-Rodríguez N, Cava A, Chanial P, Chapin E, Clements D L, Conley A, Conversi L, Dowell C D, Dwek E, Eales S, Elbaz D, Farrah D, Franceschini A, Gear W, Glenn J, Griffin M, Halpern M, Hatziminaoglou E, Ibar E, Isaak K, Ivison R J, Khostovan A A, Lagache G, Levenson L, Lu N, Madden S, Maffei B, Mainetti G, Marchetti L, Marsden G, Mitchell-Wynne K, Nguyen H T, O'Halloran B, Oliver S J, Omont A, Page M J, Panuzzo P, Papageorgiou A, Pearson C P, Pérez-Fournon I, Pohlen M, Rangwala N, Roseboom I G, Rowan-Robinson M, Portal M Sánchez, Schulz B, Scott Douglas, Seymour N, Shupe D L, Smith A J, Stevens J A, Symeonidis M, Trichas M, Tugwell K, Vaccari M, Valiante E, Valtchanov I, Vieira J D, Vigroux L, Wang L, Ward R, Wright G, Xu C K and Zemcov M. 20110311. Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses. : Nature.
Harvard
Amblard A., Cooray A., Serra P., Altieri B., Arumugam V., Aussel H., Blain A., Bock J., Boselli A., Buat V., Castro-Rodríguez N., Cava A., Chanial P., Chapin E., Clements D. L., Conley A., Conversi L., Dowell C. D., Dwek E., Eales S., Elbaz D., Farrah D., Franceschini A., Gear W., Glenn J., Griffin M., Halpern M., Hatziminaoglou E., Ibar E., Isaak K., Ivison R. J., Khostovan A. A., Lagache G., Levenson L., Lu N., Madden S., Maffei B., Mainetti G., Marchetti L., Marsden G., Mitchell-Wynne K., Nguyen H. T., O'Halloran B., Oliver S. J., Omont A., Page M. J., Panuzzo P., Papageorgiou A., Pearson C. P., Pérez-Fournon I., Pohlen M., Rangwala N., Roseboom I. G., Rowan-Robinson M., Portal M. S., Schulz B., Scott D., Seymour N., Shupe D. L., Smith A. J., Stevens J. A., Symeonidis M., Trichas M., Tugwell K., Vaccari M., Valiante E., Valtchanov I., Vieira J. D., Vigroux L., Wang L., Ward R., Wright G., Xu C. K. and Zemcov M. (20110311). Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses. : Nature.
MLA
Amblard Alexandre, Cooray Asantha, Serra Paolo, Altieri B, Arumugam V, Aussel H, Blain A, Bock J, Boselli A, Buat V, Castro-Rodríguez N, Cava A, Chanial P, Chapin E, Clements D L, Conley A, Conversi L, Dowell C D, Dwek E, Eales S, Elbaz D, Farrah D, Franceschini A, Gear W, Glenn J, Griffin M, Halpern M, Hatziminaoglou E, Ibar E, Isaak K, Ivison R J, Khostovan A A, Lagache G, Levenson L, Lu N, Madden S, Maffei B, Mainetti G, Marchetti L, Marsden G, Mitchell-Wynne K, Nguyen H T, O'Halloran B, Oliver S J, Omont A, Page M J, Panuzzo P, Papageorgiou A, Pearson C P, Pérez-Fournon I, Pohlen M, Rangwala N, Roseboom I G, Rowan-Robinson M, Portal M Sánchez, Schulz B, Scott Douglas, Seymour N, Shupe D L, Smith A J, Stevens J A, Symeonidis M, Trichas M, Tugwell K, Vaccari M, Valiante E, Valtchanov I, Vieira J D, Vigroux L, Wang L, Ward R, Wright G, Xu C K and Zemcov M. Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 10(11) solar masses. : Nature. 20110311.