| . | |
| by | MURPHY E. , NAYLOR B.J., NERI R., NGUYEN H.T., OLIVER S.J., OMONT A., PAGE M.J., PAPAGEORGIOU A., PEARSON C.P., PEREZ-FOURNON I., POHLEN M., RANGWALA N., RAWLINGS J.I., RAYMOND G., RIECHERS D., RODIGHIERO G., ROSEBOOM I.G., ROWAN-ROBINSON M., SCHULZ B., SCOTT D., SCOTT K.S., SERRA P., SEYMOUR N., SHUPE D.L., SMITH A.J., SYMEONIDIS M., TUGWELL K.E., VACCARI M., VALIANTE E., VALTCHANOV I., VERMA A., VIEIRA J.D., VIGROUX L., WANG L., WARDLOW J., WIEBE D., WRIGHT G., XU C.K., ZEIMANN G., ZEMCOV M., ZMUIDZINAS J. |
| Astrophys. J., 738, 125 (2011) | |
| Modeling of the HerMES submillimeter source lensed by a dark matter dominated foreground group of galaxies. | |
| o | Fig. 1: <[GCC2011] GN> (Nos G1-G5), <[CCV2011] HLSW-01 Na> (Nos 1a-1b) added. |
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