  The open problems related to cosmological tensions in current times have
opened new paths to study new probes to constrain cosmological parameters in
standard and extended cosmologies, in particular, to determine at a local level
the value of the Hubble constant $H_0$, through independent techniques.
However, while standard Cosmological Constant Cold Dark Matter ($\Lambda$CDM)
model has been well constrained and parts of extended cosmology have been
intensively studied, the physics behind them aspects restrains our
possibilities of selecting the best cosmological model that can show a
significant difference from the first model. Therefore, to explore a possible
deviation from a such model that can explain the current discrepancy on the
$H_0$ value, in this work we consider adding the current local observables,
e.g. Supernovae Type Ia (SNIa), $H(z)$ measurements, and Baryon Acoustic
Observations (BAO) combined with two new calibrated Quasars (QSO) datasets
using ultraviolet, x-ray and optical plane techniques. While these can be
identified as part of the high-redshift standard candle objects, the main
characteristics of these are based on fluxes distributions calibrated up to $z
\sim 7 $. We consider five $H_0$ prior scenarios to develop these calibrations.
Furthermore, we found that our estimations provide the possibility to relax the
$H_0$ tension at 2$\sigma$ using a QSO ultraviolet sample in combination with
late measurements showing higher values of $H_0$. Our results can be an initial
start for more serious treatments in the quasars physics from ultraviolet,
x-ray, and optical plane techniques behind the local observations as
cosmological probes to relax the cosmological tensions problems.
