RESUMEN
Galaxy clusters are the most massive virialized structures in the Universe and are formed through the gravitational accretion of matter over cosmic time1. The discovery2 of an evolved galaxy cluster at redshift z = 2, corresponding to a look-back time of 10.4 billion years, provides an opportunity to study its properties. The galaxy cluster XLSSC 122 was originally detected as a faint, extended X-ray source in the XMM Large Scale Structure survey and was revealed to be coincident with a compact over-density of galaxies2 with photometric redshifts of 1.9 ± 0.2. Subsequent observations3 at millimetre wavelengths detected a Sunyaev-Zel'dovich decrement along the line of sight to XLSSC 122, thus confirming the existence of hot intracluster gas, while deep imaging spectroscopy from the European Space Agency's X-ray Multi-Mirror Mission (XMM-Newton) revealed4 an extended, X-ray-bright gaseous atmosphere with a virial temperature of 60 million Kelvin, enriched with metals to the same extent as are local clusters. Here we report optical spectroscopic observations of XLSSC 122 and identify 37 member galaxies at a mean redshift of 1.98, corresponding to a look-back time of 10.4 billion years. We use photometry to determine a mean, dust-free stellar age of 2.98 billion years, indicating that star formation commenced in these galaxies at a mean redshift of 12, when the Universe was only 370 million years old. The full range of inferred formation redshifts, including the effects of dust, covers the interval from 7 to 13. These observations confirm that XLSSC 122 is a remarkably mature galaxy cluster with both evolved stellar populations in the member galaxies and a hot, metal-rich gas composing the intracluster medium.
RESUMEN
The identification of galaxies at extreme distances provides the most direct information about the earliest phases of galaxy formation. But at redshifts z > 5 even the most luminous galaxies appear faint; the interpretation of low signal-to-noise ratio data is difficult and misidentifications do occur. Here we report optical and near-infrared observations of the source STIS123627+621755, which was previously suggested to be at a redshift of 6.68 (ref. 1). At that redshift, and with the reported spectral energy distribution, the galaxy should be essentially invisible at wavelengths less than 9,300 A, because the intervening intergalactic medium absorbs almost all light energetic enough to ionize neutral hydrogen--that is, with wavelengths less than the redshifted Lyman limit of lambda = (1 + z) x 912A. At near-infrared wavelengths, however, the galaxy should be relatively bright. Here we report a detection of the galaxy at 6,700 A and a non-detection at a wavelength of 1.2 microm, contrary to expectations for z approximately 6.68. The data conservatively require that STIS123627+621755 has a redshift z < 6.
RESUMEN
A functional role of class II antigen in the binding of Epstein-Barr virus (EBV) was deduced from the study of membrane proteins on Jijoye, an EBV receptor (EBVR)-positive B cell line, and its mutant, EBVR-negative daughter cell line, P3HR-1. From gel electrophoresis of radiolabeled microsomal membrane proteins and immunoprecipitates, we identified class II antigen on Jijoye but not on P3HR-1 cells and the presence of Ii on both cell lines. The role of these molecules in EBVR function was tested by antibody blocking of virus adsorption. Anti-p23,30 serum (to class II antigen) was found to block binding of EBV to B lymphoblasts under conditions in which normal rabbit serum, rabbit antiserum to butyrate-treated P3HR-1 cells (with ample anti-Ii antibodies), and rabbit anti-p44,12 (to class I antigen and beta 2-microglobulin) serum did not block virus binding. Only one of four commercial monoclonal antibodies (MoAb) to framework epitopes on class II antigens blocked binding of EBV, whereas all four MoAb demonstrated immunofluorescent reactivity with the EBVR+ Raji cells. In previous studies of binding of EBV to hairy leukemic cells, a substantial subpopulation of HLA-DR+, EBVR- cells was identified, in addition to HLA-DR+, EBVR+ cells. These findings were consistent with the view that the HLA-DR complex has a role in the binding of EBV but that other components are also needed for the expression of EBVR function.