Searching for Radio Transients with Inverted Spectra in Epoch 1 of VLASS and VCSS, and Identification of a Sample of Candidate Relativistic Nuclear Transients

For radio transients, an inverted spectrum (defined as \(\alpha > 0\) for a power law spectrum \(S_{\nu}\propto \nu^{\alpha}\)) constrains physical properties, which in principle can be a useful criterion for selecting specific targets of interest in a transient search. To test and develop this concept, we have searched epoch 1 of the Very Large Array Sky Survey (VLASS; 3.0 GHz) and the VLITE Commensal Sky Survey (VCSS; 340 MHz) for radio transients with inverted spectra. We discover a sample of 22 inverted-spectra transient candidates that are not associated with cataloged active galactic nuclei (AGNs). To the best of our knowledge, none of our candidates have transient counterparts at other wavelengths, and only one has previously been reported as a radio transient. We find that our candidates evolve slowly over years and show either highly inverted spectra or peaked spectra over \(\sim\)1--3 GHz. Within our sample, nine candidates are matched to optical centers of galaxies and have estimated radio spectral luminosities of \(L_{3.0\mathrm{GHz}}\sim10^{30}-10^{33}\,\mathrm{erg}\,\mathrm{s}^{-1}\,\mathrm{Hz}^{-1}\). Based on the observed properties, we find the most plausible transient classification for our candidates to be relativistic tidal disruption events. However, we are unable to fully rule out variable or transient AGNs with highly inverted spectra. Upon examining physical constraints, we confirm that mainly relativistic transients (on-axis or off-axis) with equipartition energy \(E_{\mathrm{eq}}\gtrsim10^{49}-10^{53}\,\mathrm{erg}\) are expected from searching VLASS and VCSS based on inverted spectra. The obtainable physical constraints, however, can be weak due to degeneracy introduced by viewing angle.