  Coronal jets are always produced by magnetic reconnection between emerging
flux and pre-existing overlying magnetic fields. When the overlying field is
vertical/obilique or horizontal, the coronal jet will appear as anemone type or
two-sided-loop type. Most of observational jets are of the anemone type, and
only a few of two-sided-loop jets have been reported. Using the high-quality
data from New Vacuum Solar Telescope, Interface Region Imaging Spectrograph,
and Solar Dynamics Observatory, we present an example of two-sided-loop jets
simultaneously observed in the chromosphere, transition region, and corona. The
continuous emergence of magnetic flux brought in successively emerging of
coronal loops and the slowly rising of an overlying horizontal filament
threads. Sequentially, there appeared the deformation of the loops, the
plasmoids ejection from the loop top, and pairs of loop brightenings and jet
moving along the untwisting filament threads. All the observational results
indicate there exist magnetic reconnection between the emerging loops and
overlying horizontal filament threads, and it is the first example of
two-sided-loop jets associated with ejected plasmoids and twisted overlying
fields.
