ubble Treasury program. See also [ACZ2018], [CAZ2018], [CSA2018], [PSC2018]. | |
in source: | RX J0152.7-1357 = ClG J0152-1357 |
Ref: | =2019ApJ...874..132A |
by | ACEBRON A. , ALON M., ZITRIN A., MAHLER G., COE D., SHARON K., CIBIRKA N., BRADAC M., TRENTI M., UMETSU K., ANDRADE-SANTOS F., AVILA R.J., BRADLEY L., CARRASCO D., CERNY C., CZAKON N.G., DAWSON W.A., FRYE B., HOAG A.T., HUANG K.-H., JOHNSON T.L., JONES C., KIKUCHIHARA S., LAM D., LIVERMORE R.C., LOVISARI L., MAINALI R., OESCH P.A., OGAZ S., OUCHI M., PAST M., PATERNO-MAHLER R., PETERSON A., RYAN R.E., SALMON B., SENDRA-SERVER I., STARK D.P., STRAIT V., TOFT S., VULCANI B. |
Astrophys. J., 874, 132-132 (2019) | |
RELICS: high-resolution constraints on the inner mass distribution of the z = 0.83 merging cluster RXJ0152.7-1357 from strong lensing. | |
o | Fig. 1, Table 1: <[AAZ2019] RX J0152.7-1357 N.N> N=24 among (Nos 1.1-1.4 to 8.1-8.3), <[AAZ2019] RX J0152.7-1357 cNN.N> N=7 among (Nos c5.3, c9.1-9.3, c10.1-c10.3). |
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