  The relation between the observed UV continuum slope ($\beta$) and the
infrared excess (IRX) is used as a powerful probe to understand the nature of
dust attenuation law in high-redshift galaxies. We present a study of 83
UV-selected galaxies between redshift 0.5 and 0.7 from the AstroSat UV Deep
Field north (AUDFn) that encloses the GOODS-north field. Using empirical
relation, we estimate the observed IRX of 52 galaxies that are detected in
either one or both of the Herschel PACS 100$\mu$m and 160$\mu$m bands. We
further utilize the multi-band photometric data in 14 - 18 filters from the
UVIT, KPNO, HST, Spitzer, and Herschel telescopes to perform spectral energy
distribution (SED) modeling. Both the observed and model-derived IRX - $\beta$
values show a large scatter within the span of previously known relations,
signifying diversity in dust attenuation. We found a distinct relation between
the best-fit power law slope of the modified Calzetti relation ($\delta$) in
the IRX - $\beta$ plane: where the steeper SMC-like attenuation law prefers
lower $\delta$ values. Our SED model based IRX - $\beta$ relation shows a
preference for steeper SMC-like attenuation which we further confirm from the
agreement between extinction-corrected star formation rates derived using
H$\alpha$ emission line and the observed FUV plus reprocessed far-IR fluxes.
The current study reveals a strong positive correlation between IRX and the
galaxy stellar mass between $10^{9.5}$ and $10^{11.0}$ M$_{\odot}$, signifying
increased dust production in more massive star-forming galaxies.
