  The presence of blueshifted absorption lines in the X-ray spectra of Black
Hole Low Mass X-ray Binaries is the telltale of massive outflows called winds.
These signatures are found almost exclusively in soft states of high-inclined
systems, hinting at equatorial ejections originating from the accretion disk
and deeply intertwined with the evolution of the outburst patterns displayed by
these systems. In the wake of the launch of the new generation of X-ray
spectrometers, studies of wind signatures remain mostly restricted to single
sources and outbursts, with some of the recent detections departing from the
commonly expected behaviors. We thus give an update to the current state of
iron band absorption lines detections, through the analysis of all publicly
available XMM-$Newton$-PN and $Chandra$-HETG exposures of known Black Hole
Low-Mass X-ray Binary candidates. Our results agree with previous studies, with
wind detections exclusively found in dipping, high-inclined sources, and almost
exclusively in bright ($L_{X}>0.01L_{Edd}$) soft ($HR<0.8$) states, with
blueshift values generally restricted to few 100 km s$^{-1}$. The line
parameters indicate similar properties between objects and outbursts of single
sources, and despite more than 20 years of data, very few sources have the HID
sampling necessary to properly study the evolution of the wind during single
outbursts. We provide an online tool with details of the wind signatures and
outburst evolution data for all sources in the sample.
