S. E. Persson — Page 6

arXiv1999

Near Infrared Observations of the Extremely Red Object CL0939+4713B: An Old Galaxy at z~1.58?

Near infrared imaging and spectroscopic observations of the extremely red object (R-K~ 7 mag) CL 0939+4713 B have been obtained with the Near Infrared Camera on the Keck I Telescope of the W. M. Keck Observatory. The imaging shows a slightly elongated structure, while the spectroscopy shows a continuum break that allows us to determine the redshift of z = 1.58 + 0.01/-0.03 for this system. The fits of a range of models to the infrared spectrum suggests that it is predominantly an old (> 10^9 yrs) stellar system that suffers little extinction, while the measurerd R and I magnitudes suggests an age of ~ 3 x 10^8 years. The limit on the equivalent width of any emission line in the infrared spectrum argues that CL 0939+4713 B is not an actively star forming galaxy. This system, though similar in R-K color to HR 10 [also known as J1645+46] (Dey et al. 1999), is much different in morphology and emission line strengths, demonstrating the heterogeneity of extremely red extragalactic objects (EROs) selected on the basis of large values of R-K.

astro-ph↗

arXiv1994

Field Galaxy Evolution Since Z~1 from a Sample of QSO Absorption-Selected Galaxies

We present some of the results of a large survey aimed at establishing the properties of galaxies selected by their having produced detectable Mg~II $λλ2796$, 2803 absorption in the spectra of background QSOs. The present sample covers the redshift range $0.2 \le z \le 1.0 $, with $\langle z \rangle = 0.65$. From an extensive program of optical and near-IR imaging and optical spectroscopy, we find that the galaxies appear to be similar to normal galaxies at the present epoch, ranging from late--type spiral galaxies to those whose spectra and colors resemble present--day ellipticals. Contrary to some faint field galaxy samples selected using different criteria, over the redshift range observed we find no evidence for significant evolution in rest--frame $B-K$ color, space density, or (rest--frame $B$ or $K$) luminosity. The ``average'' Mg~II absorbing galaxy appears to be consistent with a normal 0.7$L_B^{\ast}$ Sb galaxy having a roughly constant star formation rate since $z \sim 1$, although galaxies spanning a range of a factor of $\sim 70$ in luminosity are found in the absorber sample. The diffuse gas cross-section selection imposed by studies of this kind appears to be biased {\it against} the relatively underluminous, blue galaxies which apparently dominate the number counts at faint magnitudes. However, essentially all ``normal'' field galaxies, independent of spectroscopic type, appear to be potential QSO absorbers.

astro-ph↗