Thesis Data Summary

Nebular Component	Type of Observation	Instrument	Wavelength Coverage	Field Size	Angular Resolution	Velocity Sampling
Dust Grains	Scattered Light Surface Photometry	WISP^a	1400-1900 & 1900-2500 Å	5.0 x 1.7 degrees	30'' pixels, 2.5' PSF	N/A
	Scattered Light Surface Photometry	Burrell Schmidt	3600-5200 Å	WISP field mosaic (40 1.1 degree fields)	4'' pixels (binned)
	Thermal Radiation Surface Photometry	IRAS^b	60 & 100 µm	All-Sky Survey data base	5' PSF
	Thermal Radiation Surface Photometry	DIRBE^c	60, 100, 140 & 240 µm	All-Sky Survey data base	0.7 degree field of view
Neutral Atomic Gas	Single Dish Mapping Emission Spectroscopy	Green Bank 140-ft.	H I 21cm line	171 square degree mosaic (6151 pointings)	21' beam	0.52 km/s channels
	Array Mapping Emission Spectroscopy	Very Large Array D-configuration	H I 21cm line	2 x 2 degree mosaic (64 fields)	1' beam	1.3 km/s channels
	Optical Absorption Point Spectroscopy	Coudé Feed Echelle	Na I D 5890 & 5896 Å lines	48 sightlines over an 8 x 7 degree area	< 0.002'' (stellar disk)	1.3 km/s channels

a: Wide-field Imaging Survey Polarimeter (Nordsieck et al. 1994)

b: Infrared Astronomical Satellite (Beichman et al. 1988)

c: Diffuse Infrared Background Explorer (Hauser et al. 1995)

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a:	Wide-field Imaging Survey Polarimeter (Nordsieck et al. 1994)
b:	Infrared Astronomical Satellite (Beichman et al. 1988)
c:	Diffuse Infrared Background Explorer (Hauser et al. 1995)