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2011Natur.470..510A - Nature, 470, 510-512 (2011)
Submillimetre galaxies reside in dark matter haloes with masses greater than 3.1011 solar masses.
AMBLARD A., COORAY A., SERRA P., ALTIERI B., ARUMUGAM V., AUSSEL H., BLAIN A., BOCK J., BOSELLI A., BUAT V., CASTRO-RODRIGUEZ 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., PEREZ-FOURNON I., POHLEN M., RANGWALA N., ROSEBOOM I.G., ROWAN-ROBINSON M., SANCHEZ PORTAL M., SCHULZ B., SCOTT D., SEYMOUR N., SHUPE 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.
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