J/ApJS/224/33   CLASH-VLT: the FF cluster MACS J0416.1-2403   (Balestra+, 2016)

CLASH-VLT: dissecting the frontier fields galaxy cluster MACS J0416.1-2403 with ∼800 spectra of member galaxies. Balestra I., Mercurio A., Sartoris B., Girardi M., Grillo C., Nonino M., Rosati P., Biviano A., Ettori S., Forman W., Jones C., Koekemoer A., Medezinski E., Merten J., Ogrean G.A., Tozzi P., Umetsu K., Vanzella E., van Weeren R.J., Zitrin A., Annunziatella M., Caminha G.B., Broadhurst T., Coe D., Donahue M., Fritz A., Frye B., Kelson D., Lombardi M., Maier C., Meneghetti M., Monna A., Postman M., Scodeggio M., Seitz S., Ziegler B. <Astrophys. J. Suppl. Ser., 224, 33-33 (2016)> =2016ApJS..224...33B 2016ApJS..224...33B (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy ; Redshifts ; Galaxies, spectra ; Photometry, RI Keywords: galaxies: clusters: general; galaxies: clusters: individual: MACS J0416.1-2403; galaxies: distances and redshifts; galaxies: kinematics and dynamics Abstract: We present VIMOS-Very Large Telescope (VLT) spectroscopy of the Frontier Fields (FF) cluster MACS J0416.1-2403 (z=0.397). Taken as part of the CLASH-VLT survey, the large spectroscopic campaign provided more than 4000 reliable redshifts over ∼600arcmin2, including ∼800 cluster member galaxies. The unprecedented sample of cluster members at this redshift allows us to perform a highly detailed dynamical and structural analysis of the cluster out to ∼2.2r200 (∼4Mpc). Our analysis of substructures reveals a complex system composed of a main massive cluster (M200∼0.9x1015M and σV,r200∼1000km/s) presenting two major features: (i) a bimodal velocity distribution, showing two central peaks separated by ΔVrf∼1100km/s with comparable galaxy content and velocity dispersion, and (ii) a projected elongation of the main substructures along the NE-SW direction, with a prominent sub-clump ∼600kpc SW of the center and an isolated BCG approximately halfway between the center and the SW clump. We also detect a low-mass structure at z∼0.390, ∼10' south of the cluster center, projected at ∼3Mpc, with a relative line-of-sight velocity of ΔVrf~-1700km/s. The cluster mass profile that we obtain through our dynamical analysis deviates significantly from the "universal" NFW, being best fit by a Softened Isothermal Sphere model instead. The mass profile measured from the galaxy dynamics is found to be in relatively good agreement with those obtained from strong and weak lensing, as well as with that from the X-rays, despite the clearly unrelaxed nature of the cluster. Our results reveal an overall complex dynamical state of this massive cluster and support the hypothesis that the two main subclusters are being observed in a pre-collisional phase, in agreement with recent findings from radio and deep X-ray data. In this article, we also release the entire redshift catalog of 4386 sources in the field of this cluster, which includes 60 identified Chandra X-ray sources and 105 JVLA radio sources. Description: The cluster MACS J0416.1-2403 was observed between 2012 December and 2014 November as part of the ESO Large Programme 186.A-0798 "Dark Matter Mass Distributions of Hubble Treasury Clusters and the Foundations of ΛCDM Structure Formation Models" (P.I.: Piero Rosati) using VIMOS at the ESO VLT. A total of 21 masks were observed (15 LR-Blue (low-resolution) masks and 6 MR (medium-resolution) masks). The LR-Blue masks cover the spectral range 3700-6700Å with a resolution of R=180, while the MR masks cover the range 4800-10000Å with a resolution of R=580. The massive cluster has been observed with the Hubble Space Telescope (HST) as part of the Multi-Cycle Treasury program Cluster Lensing And Supernova survey with Hubble (CLASH; P.I.: M. Postman; Postman et al. 2012, J/ApJS/199/25). The HST survey is nicely complemented by Subaru wide-field imaging. Objects: --------------------------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------------------------- 04 16 10.0 -24 03 58 MACS J0416.1-2403 = MCS J0416.1-2403 --------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 68 4386 CLASH-VLT spectroscopic redshift catalog of MACS J0416.1-2403 table8.dat 64 65 Redshifts of X-ray sources in the field of MACS0416 table9.dat 64 105 Redshifts of radio sources in the field of MACS0416 -------------------------------------------------------------------------------- See also: J/A+A/590/A31 : ASTRODEEP Frontier Fields Catalogues (Merlin+, 2016) J/A+A/579/A4 : MCS J1206.2-0847 galaxies spectral classif. (Girardi+, 2015) J/ApJ/801/44 : HST lensing analysis of the CLASH sample (Zitrin+, 2015) J/MNRAS/443/1549 : MACSJ0416.1-2403 strong-lensing analysis (Jauzac+, 2014) J/ApJS/211/21 : Spectroscopic redshifts of galaxies in MACS (Ebeling+, 2014) J/ApJ/776/91 : Spectrosc. redshifts of galaxies in 2 clusters (Lemze+, 2013) J/ApJ/762/L30 : CLASH: MCS J0416.1-2403 strong lensing analysis (Zitrin+, 2013) J/ApJS/199/25 : CLASH sources for MACS1149.6+2223 (Postman+, 2012) J/A+A/517/A65 : Velocities of A2294 galaxies (Girardi+, 2010) J/A+A/512/A12 : VLT/VIMOS spectroscopy in GOODS-South field (Balestra+, 2010) J/A+A/491/379 : Velocities of galaxies in Abell 520 (Girardi+, 2008) J/AJ/132/1275 : CIRS (Cluster Infall Regions in the SDSS). I. (Rines+, 2006) J/ApJ/621/53 : Multiple arc systems in A1689 (Broadhurst+, 2005) J/AJ/126/2152 : Cluster And Infall Region Nearby Survey. I (Rines+, 2003) J/A+A/399/813 : Multiple merging events in Abell 521 (Ferrari, 2003) http://sites.google.com/site/vltclashpublic/ : CLASH-VLT home page http://www.stsci.edu/hst/campaigns/frontier-fields/Lensing-Models : HST Frontier Fields lensing models access Byte-by-byte Description of file: table[289].dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1 I1 --- Type [1/2]? Source type (1=Chandra source; 2=serendipitous AGN; 5 sources) (only for table 8) 3- 10 A8 --- --- [CLASHVLT] 11- 26 A16 --- ID CLASHVLT identifier (JHHMMSS.s+DDMMSS) 28- 36 F9.6 deg RAdeg [63.8/64.3] Right Ascension (J2000) 38- 47 F10.6 deg DEdeg [-24.3/-23.8] Declination (J2000) 49- 54 F6.4 --- z [0/4.2] Spectroscopic redshift 56 I1 --- q_z [2/9] Quality flag on z (1) 58 I1 --- r_z [1/5] Reference code for z (2) 60- 64 F5.2 mag Rmag [15.2/25.7]?=9.99 Subaru/Suprime Cam Kron R-band AB magnitude 66- 68 A3 --- f_ID Flag(s) on ID (3) -------------------------------------------------------------------------------- Note (1): Quality flag as follows: 2 = Likely, VLT-VIMOS (∼80% reliability); 704 sources for table 2. 3 = Secure, VLT-VIMOS (100% reliability); 3363 sources for table 2. 5 = Ebeling et al. (2014, J/ApJS/211/21); 5 sources for table 2. 6 = Literature MAGELLAN (Kelson, private communications); 11 sources for table 2. 9 = Single-line, VLT-VIMOS (>90% reliability); 303 sources for table 2. Note (2): Reference as follows: 1 = CLASH-VLT VIMOS Low Resolution (LR) grism (3582 sources for table 2); 2 = CLASH-VLT VIMOS Medium Resolution (MR) grism (486 sources for table 2); 3 = CLASH-VLT VIMOS Mulitple measures from LR and MR (302 sources for table 2); 4 = Ebeling et al. (2014, J/ApJS/211/21); 5 = Literature MAGELLAN (Kelson, private communications). Note (3): Column added by CDS for table 2. Flag as follows: 1 = Chandra source in the field of MACS0416 (also in table 8) 2 = serendipitous AGN in the field of MACS0416 (also in table 8) R = JVLA radio source in the field of MACS0416 (also in table 9) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Emmanuelle Perret [CDS] 18-Jul-2016
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