Dictionary of Nomenclature of Celestial Objects
(Last update: 22-Mar-2024)

Result of query: info cati ZFM2015] RXJHHMM NN.N$
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Details on Acronym:   [ZFM2015]
  
[ZFM2015] (Zitrin+Fabris+Merten+, 2015)
Write:<<[ZFM2015] RXJHHMM NN.N>>
<<[ZFM2015] MS2137 NN.N>>
<<[ZFM2015] MS2137 cN.N>>
<<[ZFM2015] MNNNN NN.N>>
<<[ZFM2015] CL1226 NN.N>>
<<[ZFM2015] ANNNN NN.N>>
<<[ZFM2015] RXJHHMM N.N/N.N>>
<<[ZFM2015] ANNNN aN/N>>
<<[ZFM2015] ANNNN aNN.N>>
<<[ZFM2015] CLNNNN aN.N/N>>
<<[ZFM2015] MNNNN aN.N/aNN.N>>
<<[ZFM2015] MNNNN aN.N>>
N: 579  (SIMBAD class: LensedImage = Gravitationally Lensed Image)
Note:HST WFC3 and ACS observations of N=579 multiple images of N=25 CLASH clusters.
Ref:=2015ApJ...801...44Z
byZITRIN A. , FABRIS A., MERTEN J., MELCHIOR P., MENEGHETTI M., KOEKEMOER A., COE D., MATURI M., BARTELMANN M., POSTMAN M., UMETSU K., SEIDEL G., SENDRA I., BROADHURST T., BALESTRA I., BIVIANO A., GRILLO C., MERCURIO A., NONINO M., ROSATI P., BRADLEY L., CARRASCO M., DONAHUE M., FORD H., FRYE B.L., MOUSTAKAS J.
 Astrophys. J., 801, 44 (2015)
  Hubble Space Telescope combined strong and weak lensing analysis of the CLASH sample: mass and magnification models and systematic uncertainties.
oTable 2: <[ZFM2015] RXJHHMM NN.N>, <[ZFM2015] RXJHHMM N.N/N.N>, <[ZFM2015] ANNNN aN/n>, <[ZFM2015] ANNNN aN.N>, <[ZFM2015] MS2137 N.N>, <[ZFM2015] MS2137 aN.N>, <[ZFM2015] MNNNN aN.N/aNN.N>, <[ZFM2015] MNNNN aNN.N>, <[ZFM2015] CL1226 aN.N/N>, <[ZFM2015] CL1226 NN.NN> N=579.
=E=Catalogue in electronic form as J/ApJ/801/44
Originof the Acronym: S = Created by Simbad, the CDS Database