Chandra Observations of a Cluster and Two Quasars at High Redshift

Abstract

We observed MS 1054-0321, the highest redshift cluster of galaxies in the Einstein Medium Sensitivity Survey (EMSS), with the Chandra ACIS-S detector. We find the X-ray temperature of the cluster to be 10.4^{+1.7}_{-1.5} keV, slightly lower than that inferred previously and in agreement with the observed velocity dispersion and that found from weak lensing. We confirm significant substructure in the form of two distinct clumps in the X-ray distribution. We find the virial mass of the cluster to be at least 4.5 x 10^{14} h^{-1} M_{\odot} and the existence of this cluster constrains Omega_m to be less than one. If Omega_m = 1 and assuming Gaussian initial perturbations, we find the probability of observing MS 1054 in the EMSS is ~ 7 x 10^{-4}. We also present the first high-resolution X-ray spectra of two high-redshift quasars, S5 0836+710 and PKS 2149-306, obtained with the Chandra HETGS. The primary goal of this observation is to use the high spectral resolving power of the HETGS to detect X-ray absorption produced by a hot intergalactic medium. No significant emission or absorption feature is detected in either source at +/-3sigma level. Based on the detection limits we constrain the properties of possible emitters and absorbers. We propose a method to constrain the cosmological parameters via the X-ray forest theory, but current data do not give significant constraints. We also find that combined with the constraints from the distortion of the CMB spectrum, the X-ray Gunn-Peterson test can marginally constrain a uniform, enriched IGM.