Optical SBFs of shell galaxies Export

@article{citeulike:3789047, abstract = {We measure F814W Surface Brightness Fluctuations (SBFs) for a sample of distant shell galaxies observed with the Advanced Camera for Survey (ACS) on board of HST. To evaluate the distance at galaxies, theoretical SBF magnitudes for the ACS@HST filters are computed for single burst stellar populations covering a wide range of ages (t=1.5-14 Gyr) and metallicities (Z=0.008-0.04). Using these stellar population models we provide the first M\_SBF,F814W versus (F475W-F814W)0 calibration. The results suggest that optical SBFs can be measured at d\>100 Mpc using high resolution spatial optical data.}, archivePrefix = {arXiv}, author = {Biscardi, I. and Raimondo, G. and Cantiello, M. and Brocato, E.}, citeulike-article-id = {3789047}, citeulike-linkout-0 = {http://arxiv.org/abs/0812.2346}, citeulike-linkout-1 = {http://arxiv.org/pdf/0812.2346}, day = {12}, eprint = {0812.2346}, keywords = {brightness, distances, fluctuations, surface}, month = {Dec}, posted-at = {2008-12-15 08:48:04}, priority = {2}, title = {Optical SBFs of shell galaxies}, url = {http://arxiv.org/abs/0812.2346}, year = {2008} }

TY - JOUR ID - citeulike:3789047 L3 - citeulike-article-id:3789047 N2 - We measure F814W Surface Brightness Fluctuations (SBFs) for a sample of distant shell galaxies observed with the Advanced Camera for Survey (ACS) on board of HST. To evaluate the distance at galaxies, theoretical SBF magnitudes for the ACS@HST filters are computed for single burst stellar populations covering a wide range of ages (t=1.5-14 Gyr) and metallicities (Z=0.008-0.04). Using these stellar population models we provide the first M_SBF,F814W versus (F475W-F814W)0 calibration. The results suggest that optical SBFs can be measured at d>100 Mpc using high resolution spatial optical data. TI - Optical SBFs of shell galaxies KW - brightness KW - distances KW - fluctuations KW - surface AU - Biscardi, I AU - Raimondo, G AU - Cantiello, M AU - Brocato, E PY - 2008/Dec/12/ UR - http://arxiv.org/abs/0812.2346 ER -