Schedule of Events GBT Science Workshop Sunday, July 26 1900-2200: Reception in residence hall lounge Monday, July 27 0830-0835: Welcome .............................................. Lockman 0835-0845: Workshop overview ............................ Condon/McKinnon 0845-0900: Bus to GBT 0900-1030: Tour of GBT a. Antenna ............................................. Smith b. Servo ...................................... Lacasse/Weadon c. Laser metrology .................................... Parker 1030-1045: Return to Jansky Lab 1045-1100: Break 1100-1120: Capabilities & status of GBT receivers ............... Stennes 1120-1140: GBT IF & optical fiber transmission .................... White 1140-1200: GBT backends ............................... McKinnon/Langston 1200-1220: Capabilities/status of monitor/control software ... Hunt/Clark 1220-1330: Lunch 1330-1430: Tour of equipment & control rooms a. Equipment room ..................................... Weadon b. Control room ..................................... Lawrence c. Integrated testing of electronics & software ....... Norrod 1430-1500: Observer's software interface ......................... Fisher 1500-1520: Break 1520-1540: Operator's software interface ...................... Maddalena 1540-1600: Operations plans & policies .......................... Bignell 1600-1640: Data reduction in AIPS++ a. Single dish, spectral line data ................... Garwood b. Continuum data ................................... McMullin 1640-1700: GBT schedule & claim .................................... Hogg 1700-1720: Optical controls & mapping techniques .................. Wells 1730-1830: Dinner 1900-2200: Reception in residence hall lounge Tuesday, July 28 0830-0850: Pulsars studies with the GBT........................... Backer 0850-0910: Pulsar searches and pulsar astrometry.................. Cordes 0910-0930: Pulsar scintillation observations with the GBT..... Stinebring 0930-0950: Supernova-remnant studies with the GBT............... Reynolds 0950-1010: X-ray and radio comparisons of supernova remnants........ Dyer 1010-1030: Settling basic questions on how galaxies form from hi-Z HI........................................... Briggs 1030-1050: Break 1050-1110: Detecting galaxies via their HI.......................... Kerr 1110-1130: A high-quality standardized 21cm survey of local galaxies.......................................... Tifft 1130-1150: Spectral baselines and 3He.............................. Bania 1150-1210: Radio recombination lines from extragalactic nuclei...... Zhao 1210-1230: Radio quasar absorption line systems.................. Carilli 1230-1330: Lunch 1330-1400: Spectropolarimetry..................................... Heiles 1400-1420: Continuum imaging...................................... Condon 1420-1440: Microwave background and VLA zero-spacing observations... Uson 1440-1500: VLBI............................................... Kellermann 1500-1520: The GBT and planetary radar studies.................. Campbell 1520-1540: Break 1540-1600: Rationale for a GBT focal-plane receiver array at 1.3 cm.............................................. Barnes 1600-1620: In which frequency range is the GBT most likely to have its greatest scientific impact?........... Vanden Bout 1620-1640: Millimeter studies with the GBT of the ISM, SF, and other acronyms................................... McMullin 1640-1700: Molecular spectroscopy at 3mm and the molecular Zeeman effect............................ Turner 1700-1720: The CO Tully-Fisher relation: Can the GBT beat Arecibo?.............................. Dickey 1720-1740: Organize working groups 1740-1840: Dinner 1900-????: Science working groups Wednesday, July 29 0830-1100: Reports from Science Working Groups 1100-1115: Break 1115-1230: Open discussion 1230-1330: Lunch 1330-1350: Preliminary plan for GBT commissioning............... McKinnon 1350-1410: Holography issues................................... Maddalena 1410-1430: Position and flux-density calibration.................. Condon 1430-1450: Initial observations of standard galaxies at 21 cm...... Tifft 1450-1510: Break 1510-1530: Commissioning of the Arecibo Upgrade ................... Davis 1530-????: Open discussion 1730-1830: Dinner 1930-2030: Garth Newell Concert ................... Oberon String Quartet