  The unique morphology of head-tail (HT) radio galaxies suggests that radio
jets and their intra-cluster medium interact strongly. We conducted a
systematic search for HT radio galaxies using the LOFAR Two-metre Sky Survey
first data release (LoTSS DR1) at 144 MHz. In this paper, a catalogue of
fifty-five new HT radio galaxies is presented, ten of which are narrow-angle
tailed sources (NATs) and forty-five of which are wide-angle tailed sources
(WATs). NATs are characterised by tails that are bent like a narrow `V' shape
with a less than 90 degree opening angle. The opening angle between jets in WAT
radio galaxies is greater than ninety degrees, exhibiting wide `C'-like
morphologies. We found that thirty out of fifty-five HT radio galaxies reported
in this article are associated with known galaxy clusters. Most of the sources
presented in the current paper have redshifts $<$ 0.5. The various physical
properties and statistical studies of these HT radio galaxies are presented.
