Searching for Spider-Like Pulsars from TESS Ellipsoidal Lightcurves with X-ray counterparts

TL;DR

This study identifies four new spider pulsar candidates by cross-matching multi-wavelength data, analyzing optical modulations from TESS, and assessing their properties to suggest they are likely redback-type binaries.

Contribution

The paper introduces a novel multi-wavelength approach combining TESS, X-ray, and gamma-ray data to discover new spider pulsar candidates, expanding the known population.

Findings

Four promising spider pulsar candidates identified.

Optical variability periods range from 5 to 13 hours.

Candidates are likely redback-type binaries based on their properties.

Abstract

We present a search for new spider pulsar candidates through multi-wavelength cross-matching, including $\gamma$-ray, X-ray, and optical data. A search for sinusoidal-like optical modulations in TESS data of 183 eROSITA X-ray sources coincident with unassociated Fermi-LAT gamma-ray sources led to the identification of four promising spider pulsar candidates. We found optical variability periods ranging from 5 to 13 hours. All candidates display smooth sinusoidal-like phase light curves, similar to what can be expected from ellipsoidal variation; one shows double-peaked profiles indicative of harmonics. The absence of sharp minima, which are often found in black widow systems due to irradiation, together with their optical magnitudes of about G~14, suggests these sources are more likely redback-type binaries. One of the Fermi-LAT counterparts is included in a machine-learning catalog of unassociated gamma-ray sources, with relatively high pulsar probabilities. We also identify potential Gaia counterparts for several sources and estimate their distances and luminosities where parallax measurements are available. Future observations, including further spectroscopic and multi-wavelength studies, are needed to fully characterize these systems.