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Table 2.

New multiple images, in addition to those from Tables 2 and 3 of G16, used in our strong lensing model of MACS 1149.

ID RA Dec zsp QF identification
(J2000) (J2000)
SX (a) 177.40021 22.39681 1.489 3 HST
201.1 177.40562 22.40243 2.950 3 HST
201.2 177.40216 22.39675 2.950 9 HST
201.3 177.39530 22.39182 2.950 9 HST
202.1 177.40014 22.40415 4.384 3 HST
202.2 177.39834 22.40378 4.384 3 HST
203.1 177.40028 22.39641 4.497 9 MUSE
203.2 177.39575 22.40000 4.497 3 MUSE
203.3 177.39457 22.39442 4.497 3 MUSE
204.1 177.40043 22.40389 5.806 9 MUSE
204.2 177.39949 22.40376 5.806 9 MUSE
301.1 177.39504 22.41269 3.447 9 HST
301.2 177.39353 22.41307 3.447 3 HST
301.3 177.39285 22.41287 3.447 3 HST
401.1 177.39591 22.41239 5.983 3 MUSE
401.2 177.39357 22.41142 5.983 3 MUSE
401.3 177.39168 22.41153 5.983 9 MUSE
401.4 177.39319 22.41295 5.983 9 MUSE

Notes. Columns give, from left to right, the identification number ID, right ascension, declination, spectroscopic redshift zsp, the corresponding redshift uncertainty in terms of a quality flag QF, and whether the image position is measured in the HST images or only from the MUSE data cube. Considered quality flags are: 3 very secure (δz < 0.001) and 9 secure (based on a single emission line).

(a)

Published in Kelly et al. (2016).

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