The Magellan Uniform Survey of Damped Lyman alpha Systems II: Paucity of Strong Molecular Hydrogen Absorption
Regina A. Jorgenson, Michael T. Murphy, Rodger Thompson, Robert F., Carswell

TL;DR
This large survey of damped Lyman alpha systems reveals a surprisingly low occurrence of strong molecular hydrogen absorption, challenging previous expectations about H_2 prevalence in these systems.
Contribution
First large, blind, uniformly selected survey for H_2 in DLAs, providing new constraints on the covering factor and detection rate of molecular hydrogen.
Findings
Detection rate of strong H_2 absorbers is about 1%, lower than previous estimates.
The covering factor for N(H_2) >= 10^17.5 cm^-2 is approximately 1%.
Most upper limits are consistent with previous surveys, but detection rate remains unexpectedly low.
Abstract
We present the first large, blind and uniformly selected survey for molecular hydrogen (H_2) in damped Lyman alpha systems (DLAs) with moderate-to-high resolution spectra. 86 DLAs were searched for absorption in the many Lyman and Werner H_2 transitions, with approximately 79% completeness for H_2 column densities above N(H_2)=10^17.5 cm^-2 for an assumed Doppler broadening parameter b=2 km s^-1. Only a single strong H_2 absorber was found -- a system detected previously in VLT/UVES spectra. Given our distribution of N(H_2) upper limits, this ~1% detection rate is smaller than expected from previous surveys at 99.8% confidence. Assuming the N(H_2) distribution shape from previous surveys, our detection rate implies a covering factor of ~1% for N(H_2) >= 10^17.5 cm^-2 gas in DLAs (<6% at 95% confidence). We obtained new Magellan/MagE spectra for 53 DLAs; 8 km s^-1 -resolution spectra…
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