  As of October 2021 (Period 108), the European Southern Observatory (ESO)
offers a new mode of the ESPRESSO spectrograph designed to use the High
Resolution grating with 4x2 binning (spatial by spectral; HR42 mode) with the
specific objective of observing faint targets with a single Unit Telescope at
Paranal. We validated the new HR42 mode using four hours of on-target
observations of the quasar J0003-2603, known to host an intervening metal-poor
absorber along the line of sight. The capabilities of the ESPRESSO HR42 mode
(resolving power R~137 000) were evaluated by comparing to a UVES spectrum of
the same target with a similar integration time but lower resolving power (R~48
000). For both data sets we tested the ability to decompose the velocity
profile of the intervening absorber using Voigt profile fitting and extracted
the total column densities of CIV, NI, SiII, AlII, FeII, and NiII. With ~3x the
resolving power and ~2x lower S/N for a nearly equivalent exposure time, the
ESPRESSO data is able to just as accurately characterize the individual
components of the absorption lines as the comparison UVES data, but has the
added bonus of identifying narrower components not detected by UVES. For UVES
to provide similar spectral resolution (R>100 000; 0.3'' slit) and the broad
wavelength coverage of ESPRESSO, the Exposure Time Calculator (ETC) supplied by
ESO estimates 8 hrs of exposure time spread over two settings; requiring double
the time investment than that of ESPRESSO's HR42 mode whilst not properly
sampling the UVES spectral resolution element. Thus ESPRESSO's HR42 mode offers
nearly triple the resolving power of UVES (0.8'' slit to match typical ambient
conditions at Paranal) and provides more accurate characterization of quasar
absorption features for an equivalent exposure time.
