J/A+A/678/A3          ACT-CL J0 102-15 MUSE view                (Caminha+, 2023)

A MUSE view of the massive merging galaxy cluster ACT-CL J0 102-15 (El Gordo) at z = 0.87. Robust strong lensing model and data release. Caminha G., Grillo C., Rosati P., Liu A., Acebron A., Bergamini P., Caputi K.I., Mercurio A., Tozzi P., Vanzella E., Demarco R., Frye B., Rosani G., Sharon K. <Astron. Astrophys. 678, A3 (2023)> =2023A&A...678A...3C 2023A&A...678A...3C (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Gravitational lensing ; Redshifts Keywords: galaxies: clusters: individual: ACT-CL J0102-4915 - gravitational lensing: strong - dark matter Abstract: We present a detailed strong lensing analysis of the massive and distant (z=0.870) galaxy cluster ACT-CL J0102-4915 (ACT0102, also known as El Gordo), taking advantage of new spectroscopic data from the Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope and archival imaging from the Hubble Space Telescope. Thanks to the MUSE data, we were able to measure secure redshifts for 374 single objects, including 23 multiply lensed galaxies, and 167 cluster members of ACT0102. We used the observed positions of 56 multiple images, along with their new spectroscopic redshift measurements, as constraints for our strong lensing model. Remarkably, some multiple images are detected out to a large projected distance of ∼1Mpc from the brightest cluster galaxy, allowing us to estimate a projected total mass value of 1.84-0.04+0.03x1015M within that radius. We find that we need two extended cluster mass components, the mass contributions from the cluster members and the additional lensing effect of a foreground (z=0.633) group of galaxies, to predict the positions of all multiple images with a root mean square offset of 0.75". The main cluster-scale mass component is centred very close to the brightest cluster galaxy, and the other extended mass component is located in the north-west region of the cluster. These two mass components have very similar values of mass projected within 300kpc of their centres, namely 2.29-0.10+0.09x1014M and 2.10-0.09+0.08x1014M, in agreement with the major merging scenario of ACT0102. We make publicly available the lens model, including the magnification maps and posterior distributions of the model parameter values, as well as the full spectroscopic catalogue containing all redshift measurements obtained with MUSE. Description: We make publicly available the lens model of ACT-CL J0102-4915 (aka El Gordo) and the MUSE redshift catalogue presented in the paper. If you use the information in these files please cite the paper, and for any further question contact the author via the e-mail gbcaminha(at)gmail.com Subdirectory files contains the files used by the software lenstool (https://projets.lam.fr/projects/lenstool/wiki) are described below: best_fit.par : input best fit file for the lenstool software to_sample.par : input file for the sampling mode of lenstool bayes.dat : 10000 random points from the full lenstool MCMC sampling output. This file can be used to compute the model parameter confidence levels and the statistical error of lensing related quantities, such as magnification factors (see https://projets.lam.fr/projects/lenstool/wiki for more information). members_all.dat : file containing the list of cluster members, used as input to the lenstool software. The columns follow the format described on https://projets.lam.fr/projects/lenstool/wiki/PotFile. The columns are 1) ID; 2),3) RA and Dec in degrees; 4),5),6) semi major and minor axes and orientation (in our case we adopt circularly symmetric profiles); 7) magnitude measured on the HST/WFC F160W filter. The last columns is not used by lenstool but must be included so that the software can read this file. obsarcsv1newIDs.dat : file containing the list of multiple images, used as input to the lenstool software. The columns are 1) ID; 2),3) RA and Dec in degrees; 4),5) re-scaled positional error on x and y directions in arcseconds; 6) image orientation (not used in this work); 7) spectroscopic redshift; 8) reference magnitude (not used in this work) File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file catalog.dat 65 402 MUSE redshift catalogue (table 1) list.dat 137 9 List of fits maps fits/* . 9 Individual fits maps files/* . 5 Files used by the software lenstool -------------------------------------------------------------------------------- Byte-by-byte Description of file: catalog.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 28 A28 --- Name ID build from the cluster name and object RA and Dec (ACT0102-JHHMMSS.ss+DDMMSS.ss) 30- 39 F10.7 deg RAdeg Observed right ascension (J2000) (1) 41- 51 F11.7 deg DEdeg Observed declination (J2000) (1) 53- 58 F6.4 --- zsp Spectroscopic redshift 61 I1 --- q_zsp [2/9] Redshift quality flag (2) 65 I1 --- Nmult [1/3] Number of entries of the same object in this catalogue used to indicate multiply lensed sources -------------------------------------------------------------------------------- Note (1): The coordinates are with respect to the HST/RELICS public images. See https://archive.stsci.edu/prepds/relics/ Note (2): Redshift quality flag as follows: 2 = likely 3 = secure measurement 9 = single line measurement 4 = field stars -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.5 deg RAdeg Right Ascension of center (J2000) 10- 18 F9.5 deg DEdeg Declination of center (J2000) 20- 23 I4 --- Nx Number of pixels along X-axis 25- 28 I4 --- Ny Number of pixels along Y-axis 30- 33 I4 Kibyte size Size of FITS file 35- 65 A31 --- FileName Name of FITS file, in subdirectory fits 67-137 A71 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Gabriel Caminha, gbcaminha(at)gmail.com
(End) Patricia Vannier [CDS] 08-Aug-2023
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line