arXiv · astro-ph/0312511
ACS Observations of a Strongly Lensed Arc in a Field Elliptical
Abstract
We report the discovery of a strongly lensed arc system around a field elliptical galaxy in Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS) images of a parallel field observed during NICMOS observations of the HST Ultra-Deep Field. The ACS parallel data comprise deep imaging in the F435W, F606W, F775W, and F850LP bandpasses. The main arc is at a radius of 1.6 arcsec from the galaxy center and subtends about 120 deg. Spectroscopic follow-up at Magellan Observatory yields a redshift z=0.6174 for the lensing galaxy, and we photometrically estimate z_phot = 2.4\pm0.3 for the arc. We also identify a likely counter-arc at a radius of 0.6 arcsec, which shows structure similar to that seen in the main arc. We model this system and find a good fit to an elliptical isothermal potential of velocity dispersion $σ\approx 300$ \kms, the value expected from the fundamental plane, and some external shear. Several other galaxies in the field have colors similar to the lensing galaxy and likely make up a small group.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
J. P. Blakeslee, K. C. Zekser, N. Benitez, M. Franx, R. L. White, H. C. Ford, R. J. Bouwens, L. Infante, N. J. Cross, G. Hertling, B. P. Holden, G. D. Illingworth, V. Motta, F. Menanteau, G. R. Meurer, M. Postman, P. Rosati, W. Zheng. 2003-12-19. ACS Observations of a Strongly Lensed Arc in a Field Elliptical. https://doi.org/10.1086/382505
Cite the original work for its findings. Save a collection to share your selection of sources.