Abell 2744 is the first cluster for which both the GLASS spectroscopy and the Hubble Frontier Field (HFF) imaging are complete. InÂ Wang et al. (2015), we perform targeted and blind searches of faint emission lines in the GLASS data and thusÂ compile a sample of 55 galaxies with high-confidence spectroscopic redshift, 5 of which are multiply lensed and 3 of which belong to the same system. We also measure photometric redshifts for this sample fromÂ the HFF 7-filter exposures. A reasonable agreement between these two sorts of redshift estimation is seen, when nebular emission is considered in photometric redshift fitting.
Modeling gravitational potential of galaxy clusters is known as a notorious difficulty, partly because of the inclusion of mis-identified multiple image systems in lens modeling. In this work, we develop a stringent and rigorous procedure to screen off insecure image systems,Â based upon colors derived from HFF, image morphology and spectroscopy from GLASS. This leads to a sample of 25/72 multiple arc systems/images as secure out of a total of 57/179 candidate systems/images. The resulting total mass map is only given by the secure set of arcs.
We also derive a stellar mass map from the Spitzer Frontier Field data and find out thatÂ the stellar to total mass ratio varies substantially across the cluster field, ranging from 0 to 5%, and the light-traces-mass assumption is not valid in this merging cluster.
The broad spectral coverage and high angular resolution of GLASS are idealÂ for detailed studies of galaxies at intermediate redshifts. In Jones et al. 2015Â our teamÂ analyzed the spatially resolved stellar mass and gas-phase metallicity inÂ a system of three strongly lensed galaxies at redshift z=1.855, drawn fromÂ the first complete GLASS data set (MACS0717).
These initial GLASS data reveal strong, spatially extended emission linesÂ in all three galaxies. We find no significant radial variation inÂ metallicity, possibly as a result of gravitational interaction among the galaxies.
These results represent the first constraint of metallicity gradientÂ evolution using HST. Our analysis also extends previous studies of theÂ mass-metallicity relation to an order of magnitude lower stellar mass,Â confirming that GLASS is able to characterize dwarf galaxies atÂ intermediate redshift. The mass-metallicity relation and metallicityÂ gradient evolution are both valuable diagnostics of how gas cycles in andÂ out of galaxies over cosmic time.
For more details go toÂ http://adsabs.harvard.edu/abs/2014arXiv1410.0967J
In GLASS data taken of the MACSJ1149.6+2223 cluster (z=0.54)Â in November, we discovered the first strongly lensed supernova visible in multiple images.Â The supernova occurred in the spiral arm of a galaxy at redshift z=1.49 lensed by a foreground early-type cluster galaxy, whose gravitational potential forms four separate, strongly magnified images of the supernova.Â With the Frontier Fields SN team, we describe the exciting system in Kelly et al. 2014.
Our team is measuring the time delays and relative magnifications between the separate images of the evolving supernova, by comparing the phase and brightness of the multiple light curves. These delays and magnifications will place tight constraints on the cosmic expansion rate, as well as theÂ distribution of luminous and dark matter in the galaxy lens and the cluster.
The MACSJ1149.6+2223 galaxy cluster furthermore lenses the spiral host galaxy of the supernova itself into multiple images, and models of the cluster predict that the supernova will appear in the future at additional locations in the cluster field.
Schmidt et al. (2014), ApJÂ 782:L36Â
The first GLASS dataÂ arrived on 2013 December 24 and 30 and consists of 10029 and 3812 secondsÂ of G102 and G141 spectroscopy on MACS0717, respectively, and comprise only ~1/20th of the final GLASS data product.
For the 9 redshiftÂ 6 galaxy candidates in MACS0717 with GLASS grism spectra clear of contamination we do not detect any emission lines down to aÂ 1Ïƒ noise level of âˆ¼5Ã—10âˆ’18 erg sâˆ’1 cmâˆ’2. This confirms that the targeted high redshift candidates are notÂ strong line emitters at lower redshift.
Furthermore, we spectroscopically confirm four multiply imaged strongly lensed systems by detecting emission lines ([OIII] and [OII]) Â the GLASS grism spectra, confirming the proposedÂ photometric redshifts from the literature.Â
For more details follow the link to ADSÂ .