Deformed configuration mixing shell model calculations for the energy spectra and electromagnetic properties of low-lying collective states of $^{51}\mathrm{Cr}$, $^{53}\mathrm{Fe}$, $^{50}\mathrm{Ti}$, $^{52}\mathrm{Cr}$, $^{54}\mathrm{Fe}$, $^{53}\mathrm{Cr}$, and $^{55}\mathrm{Fe}$ have been performed. For each of these nuclei these calculations give rise to a highly deformed band when a neutron is promoted from the predominantly ${({f}_{\frac{7}{2}})}^{n}$ spherical ground intrinsic configuration to the unoccupied ($\mathrm{pf}$) orbits. The ${K}^{\ensuremath{\pi}}$ values of these excited bands are $\frac{1}{{2}^{\ensuremath{-}}}$, ${4}^{+}$, and $\frac{7}{{2}^{\ensuremath{-}}}$ for the nuclei having $N=27, 28, \mathrm{and} 29$, respectively. The energy spectra and electromagnetic properties of these calculated excited bands are compared with those experimentally observed. Following high-spin members of the collective bands have been predicted by the calculations: $J=\frac{11}{2}, \frac{13}{2}, \frac{15}{2}, \frac{17}{2}, \mathrm{and} \frac{19}{2}$ levels at 2.7, 3.8, 4.36, 5.94, and 6.47 MeV, respectively, in $^{51}\mathrm{Cr}$, $J=\frac{9}{2}, \frac{11}{2}, \frac{13}{2}, \frac{15}{2}, \mathrm{and} \frac{17}{2}$ levels at 2.94, 3.67, 4.95, 6.01, and 7.47 MeV, respectively, in $^{53}\mathrm{Fe}$, $J=\frac{15}{2}, \frac{17}{2}, \frac{19}{2}, \mathrm{and} \frac{21}{2}$ levels at 4.65, 5.77, 7.04, and 8.41 MeV, respectively, in $^{53}\mathrm{Cr}$, and $J=\frac{15}{2}, \frac{17}{2}, \mathrm{and} \frac{19}{2}$ levels at 5.53, 6.92, and 8.33 MeV, respectively, in $^{55}\mathrm{Fe}$. In $^{50}\mathrm{Ti}$, $^{52}\mathrm{Cr}$, and $^{54}\mathrm{Fe}$ the present model suggests an interesting possibility of $K={3}^{+}$ collective band lying close in energy to the recently observed $K={4}^{+}$ collective bands.NUCLEAR STRUCTURE $^{50}\mathrm{Ti}$, $^{51,52,53}\mathrm{Cr}$, and $^{53,54,55}\mathrm{Fe}$. Calculated spectra, $B(E2)$ and $B(M1)$ transition strengths, $\frac{E2}{M1}$ mixing ratios, branching ratios and lifetimes in deformed configuration mixing shell model formalism in ${(\mathrm{fp})}^{n}$ model space. Modified Kuo-Brown interaction. Comparison with experiment and shell model and Nilsson model calculations.
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