  We present the most complete emission spectrum for inflated hot Jupiter
HAT-P-41b combining new HST WFC/G141 spectrum from the Hubble Panchromatic
Comparative Exoplanet Treasury (PanCET) program with archival Spitzer eclipse
observations. We found a near blackbody-like emission spectrum which is best
fitted with an isothermal temperature-pressure (TP) profile that agrees well
with the dayside heat redistribution scenario assuming zero Bond albedo. The
non-inverted TP profile is consistent with the non-detection of NUV/optical
absorbers in the transit spectra. We do not find any evidence for significant
H$^-$ opacity nor a metal-rich atmosphere. HAT-P-41b is an ideal target that
sits in the transitioning parameter space between hot and ultra-hot Jupiters,
and future JWST observations will help us to better constrain the thermal
structure and chemical composition.
