We present our discovery of a new hybrid pulsating subdwarf B star , J08069+1527 .
The effective temperature and surface gravity of 28,500 \pm 400 K and 5.37 \pm 0.04 dex , respectively , place this object inside the instability strip and also among other pulsating hot subdwarfs of a hybrid nature , right next to another fascinating star : Balloon 090100001 .
From this proximity , we anticipated this star could pulsate in both high and low frequency modes .
Indeed , our analysis of photometric data confirmed our prediction .
We detected two peaks in the high frequency region and two other peaks at low frequencies .
In addition , the amplitude of the dominant mode is very high and comparable to the dominant peaks in other hybrid subdwarf B stars .
Since this star is bright , we performed time-series low resolution spectroscopy .
Despite a low signal-to-noise ( S/N ) ratio , we were able to detect the main peak from these data .
All our results strongly indicate that J08069+1527 is a high amplitude pulsating hot subdwarf B star of hybrid nature .
By analogy to the other pulsating sdB star , we judge that the dominant mode we detected here has radial nature .
Future stellar modeling should provide us with quite good constrains as p- and g-modes presented in this star are driven in different parts of its interior .