1 INTRODUCTION
2 OBSERVATIONS AND DATA REDUCTION
2.1 WISP Survey - HST WFC3/IR Grism Spectroscopy and Imaging
2.2 HST WFC3/UVIS Imaging
2.3 Ground-based Imaging
2.4 Spitzer IRAC Imaging
3 WISP PHOTOMETRIC PIPELINE
3.1 Photometric Zeropoints
3.2 HST PSF- and Aperture-matched Isophotal Photometry (high spatial resolution)
3.3 Ground-based and Spitzer Forced Photometry (low spatial resolution)
4 WISP PHOTOMETRIC CATALOGUE
4.1 Photometric Catalogue Description
4.2 Summary of Imaging Depth and Completeness
4.3 Comparison of Ground-based Catalogue Photometry to SDSS
5 WISP SPECTROSCOPIC PIPELINE
5.1 Emission Line Candidate Identification
5.2 Emission Line Candidate Inspection
5.3 Emission Line Measurements
5.4 Completeness Corrections
6 WISP EMISSION LINE CATALOGUE
6.1 Emission Line Catalogue Description
6.2 Grism Redshift Accuracy and Precision
7 RESULTS
7.1 Sample Selection Criteria
7.2 SED Modelling for Stellar Masses
7.3 Spectral Stacking and Emission Line Fitting of Stacked Spectra
7.4 Stellar Mass Stack Results
8 CONCLUSION