HI Galaxy Signatures in the SARAO MeerKAT Galactic Plane Survey \(-\) I. Probing the richness of the Great Attractor Wall across the inner Zone of Avoidance

Abstract

This paper presents the first HI results extracted from the SARAO MeerKAT Galactic Plane Survey (SMGPS) \(-\) a narrow strip (\(b \sim 3^\circ\)) along the southern Milky Way. The primary goal consisted in tracing the Great Attractor (GA) Wall across the innermost Zone of Avoidance. We reduced a segment spanning the longitude range \(302^\circ \leq \ell \leq 332^\circ\) for the redshift range \(z \leq 0.08\). The superb SMGPS sensitivity (rms = 0.3-0.5 mJy beam\(^{-1}\) per 44 kms\(^{-1}\) channel) and angular resolution (\(\sim\) 31" \(\times\) 26") lead to a detection limit of log\((M_{\rm HI}/\)M\(_\odot) \geq\) 8.5 at the GA distance (\(V_{\rm hel} \sim 3500 - 6500\) kms\(^{-1}\)). A total of 477 galaxy candidates were identified over the full redshift range. A comparison of the few HI detections with counterparts in the literature (mostly HIZOA) found the HI fluxes and other HI parameters to be highly consistent. The continuation of the GA Wall is confirmed through a prominent overdensity of \(N = 214\) detections in the GA distance range. At higher latitudes, the wall moves to higher redshifts, supportive of a possible link with the Ophiuchus cluster located behind the Galactic Bulge. This deep interferometric HI survey demonstrates the power of the SMGPS in improving our insight of large-scale structures at these extremely low latitudes, despite the high obscuration and continuum background.