# A Correlated Search for Local Dwarf Galaxies in GALFA-HI and Pan-STARRS

## TL;DR

This study searches for gas-rich, optically obscured ultrafaint dwarf galaxies in the GALFA-HI survey, identifying 690 candidates but finding no Leo T-like galaxies within 500 kpc of the Milky Way, thus constraining their abundance.

## Contribution

It introduces a novel radio survey-based method to identify nearby gas-rich dwarf galaxies, expanding the search beyond optical surveys and probing lower Galactic latitudes.

## Key findings

- 690 dwarf galaxy candidates identified
- No Leo T-like galaxies found within 500 kpc
- One promising candidate near the Galactic plane

## Abstract

In recent years, ultrafaint dwarf (UFD) galaxies have been found through systematic searches of large optical surveys. However, the existence of Leo T, a nearby gas-rich dwarf, suggests that there could be other nearby UFDs that are optically obscured but have gas detectable at nonoptical wavelengths. With this in mind, we perform a search of the full Galactic Arecibo $L-$band Feed Array HI (GALFA-HI) survey, a radio survey which covers one-third of the sky at velocities $-650 < V_{\rm{LSR}} < +650 \; \rm{km} \; \rm{s^{-1}}$, for neutral hydrogen sources. We are able to probe regions of the sky at lower Galactic latitudes and smaller $|V_{LSR}|$ compared to previous explorations. We use the Source Finding Application (SoFiA) on GALFA-HI and select all sources with similar properties to Leo T and other local dwarf galaxies. We find 690 dwarf galaxy candidates, one of which is particularly promising and likely a new galaxy near the Galactic plane ($b=-8^{\circ}$) that is comparable in velocity width and HI-flux to other recently discovered local volume galaxies. We find we are sensitive to Leo T-like objects out to $1 \; \rm{Mpc}$ at velocities clear from background HI emission. We check each candidate's corresponding optical fields from Pan-STARRS and fit stars drawn from isochrones, but find no evidence of stellar populations. We thus find no other Leo T-like dwarfs within $500 \; \rm{kpc}$ of the Milky Way in the one-third of the sky covered by the GALFA-HI footprint and discuss our nondetection in a cosmological context.