1 INTRODUCTION

2 THE EXTENDED ALMAQUEST SAMPLE

3 DATA

3.1 MaNGA data

3.2 ALMA data

4 STAR FORMATION SCALING RELATIONS

4.1 The Resolved Schmidt-Kennicutt Relation

4.2 The Resolved Molecular Gas Main Sequence

4.3 The Resolved Star Forming Main Sequence

4.4 The Resolved Dynamical Equilibrium Pressure Relation

5 DISCUSSION

5.1 Is the rPDE relation universal?

5.2 Is the rPDE relation the most fundamental star formation scaling relation?

5.3 Uncertainties in the measurement of $P_{DE}$

5.4 What causes the discrepancy between the PRFM model and the ALMaQUEST data?

6 CONCLUSIONS