ﻻ يوجد ملخص باللغة العربية
We present redshift space two-point ($xi$), three-point ($zeta$) and reduced three-point (Q) correlation of Ly$alpha$ absorbers (i.e Voigt profile components having HI column density $N_{HI}>10^{13.5}$cm$^{-2}$) over three redshift bins spanning $1.7<z<3.5$ using high resolution spectra of 292 quasars. We detect positive $xi$ up to 8$h^{-1}$cMpc in all three redshift bins. The strongest detection of $zeta$ is seen in $z=1.7-2.3$ redshift bin at $1-2h^{-1}$cMpc with an amplitude of $1.81pm0.59$ ($sim3.1sigma$ level). The corresponding Q is found to be $0.68pm0.23$. The measured $xi$ and $zeta$ values show an increasing trend with $N_{HI}$, while Q remains relatively independent of $N_{HI}$. We find $xi$ and $zeta$ to evolve strongly with $z$ over the redshift range studied. Using hydrodynamical simulations, we find that the $xi$ and especially $zeta$ seen in real space may be strongly amplified by peculiar velocities in redshift space. Simulations also suggest that while feedback, thermal and pressure smoothing effects affect the clustering of Ly$alpha$ absorbers at small scales, i.e $<0.5h^{-1}$cMpc, the HI photo-ionization rates ($Gamma_{HI}$) strongly influence the correlation amplitudes at all scales. We find that the strong redshift evolution shown by $xi$ and $zeta$ is primarily sourced by the redshift evolution of the relationship between $N_{HI}$ and baryon overdensity ($Delta$). Our simulations that uses available best fitted $Gamma_{HI}(z)$ measurements produce consistent clustering signals with observations at $zsim2$ but under-predict the clustering at higher redshifts. One possible remedy is to have higher values of $Gamma_{HI}$ at higher redshifts compared to the existing measurements. Alternatively the discrepancy could be related to non-equilibrium and inhomogeneous conditions prevailing during HeII reionization not captured by our simulations.
We report observations of four sub-damped Lyman-alpha (sub-DLA) quasar absorbers at z<0.5 obtained with the Hubble Space Telescope Cosmic Origins Spectrograph. We measure the available neutrals or ions of C, N, O, Si, P, S, Ar, Mn, Fe, and/or Ni. Our
The Ly-alpha luminosity function (LF) of high-redshift Ly-alpha emitters (LAEs) is one of the few observables of the re-ionization epoch accessible to date with 8-10 m class telescopes. The evolution with redshift allows one to constrain the evolutio
We characterise the thermal state of the intergalactic medium (IGM) in ten redshift bins in the redshift range $2 leq z leq 4$ with a sample of 103 high resolution, high S/N Ly$alpha$ forest spectra using four different flux distribution statistics.
We report on the detection of two O VI absorbers separated in velocity by 710 km/s at z ~ 0.4 towards the background quasar SBS0957+599. Both absorbers are multiphase systems tracing substantial reservoirs of warm baryons. The low and intermediate io
Ultraviolet spectrographs aboard the Hubble Space Telescope (HST) and the Far Ultraviolet Spectroscopic Explorer (FUSE) have proved their value as sensitive probes of the low-density intergalactic medium (IGM) at low redshifts (z < 0.1). Recent obser