Legacy HST Spectroscopy of the Low Redshift Intergalactic Medium

Computer Science

Scientific paper

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Hst Proposal Id #10665 Quasar Absorption Lines And Igm

Scientific paper

We propose a homogeneous analysis of all HST spectra of quasars and AGN that probe the low redshift intergalactic medium {z < 0.4}. Data taken at moderate resolution with each of the three spectroscopic instruments - FOS, GHRS, and STIS - will be included. The analysis will involve 316 targets, span a total redshift path of 110 and yield an estimated 1500 Lyman-alpha absorbers. In this redshift range, it will incease the number of absorbers by a factor of 15 over the HST Absorption Line Key Project. Data products include co-added and calibrated spectra, continuum fits, absorption line lists, and line identifications, all on a web site that includes hyperlinked information from NED and ADS. About 90% of the sightlines are in regions covered by the SDSS, 2dF and 6dF surveys. This Archive Legacy database will facilitate a range of scientific investigations, including {a} studies of the relationship between luminous baryons in galaxies and diffuse baryons in the IGM, {b} comparisons between the observations and simulations that incorporate gas dynamics, {c} measures of cosmic variance in structure on the largest scales, {d} new tests of the gravitational instability paradigm, {e} accurate determination of the proximity effect at low redshift, and {f} measurements of the chemical enrichment of the IGM. With no prospect of sensitive UV spectroscopy in the forseeable future, this dataset will form part of HST's unique and enduring legacy.

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