  We report the detection of seven new galaxy candidates with redshift $z$ $>$
11 within the JWST Advanced Deep Extragalactic Survey (JADES) GOODS-S and
GOODS-N fields. These new candidates are detected through meticulous analysis
of NIRCam photometry in eight filters spanning a wavelength range of 0.8-5.0
$\mu$m. Photometric redshifts of these galaxy candidates are independently
measured utilizing spectral energy distribution (SED) fitting techniques using
\texttt{EAZY} and \texttt{BAGPIPES} codes, followed by visual scrutiny. Two of
these galaxy candidates are located in GOODS-S field, while the remaining five
galaxies are located in GOODS-N field. Our analysis reveals that the stellar
masses of these galaxies typically range from log $M_{\ast}$/$M_{\odot}$ =
7.75--8.75. Futhermore, these galaxies are typically young with their
mass-weighted ages spanning from 80 to 240 Myr. Their specific star formation
rates (sSFR), quantified as $\log (\text{sSFR}/\text{Gyr}$), are measured to
vary between $\sim 0.95$ to 1.46. These new galaxy candidates offer a robust
sample for probing the physical properties of galaxies within the first few
hundred Myr of the history of the Universe. We also analyze the relationship
between star formation rate (SFR) and stellar mass ($M_\ast$) within our
sample. Using linear regression, our analysis yields a slope of $0.71 \pm
0.12$, which we then compare with results from previous studies. Continued
investigation through spectroscopic analysis using JWST/NIRSpec is needed to
spectroscopically confirm these high-redshift galaxy candidates and investigate
further into their physical properties. We plan to follow up on these
candidates with future NIRSpec observations.
