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Featured researches published by J. A. Moran.


arXiv: Astrophysics | 2005

PROMPT: Panchromatic robotic optical monitoring and polarimetry telescopes

Daniel E. Reichart; Melissa C. Nysewander; J. A. Moran; J. W. Bartelme; Matthew B. Bayliss; A. Foster; J. C. Clemens; P. Price; C. R. Evans; J. D. Salmonson; Susan R. Trammell; Bruce W. Carney; Jonathan Wilmore Keohane; R. Gotwals

Funded by


The Astrophysical Journal | 2006

Early-Time Chromatic Variations in the Wind-Swept Medium of GRB 021211 and the Faintness of its Afterglow

Melissa C. Nysewander; Daniel E. Reichart; H.-S. Park; George Grant Williams; K. Kinugasa; D. Q. Lamb; Arne A. Henden; Sylvio Klose; Taichi Kato; A. Harper; Hitoshi Yamaoka; Chris Laws; K. Torii; D. G. York; J. C. Barentine; Jack Dembicky; Russet Jennifer McMillan; J. A. Moran; Dieter H. Hartmann; B. Ketzeback; Matthew B. Bayliss; J. W. Bartelme; J. A. Crain; A. Foster; M. Schwartz; P. Holvorcem; Paul A. Price; Ronald W. Canterna; Geoffrey Crew; George R. Ricker

1.2M in grants and donations, we are now building PROMPT at CTIO. When completed in late 2005, PROMPT will consist of six 0.41-meter diameter Ritchey-Chretien telescopes on rapidly slewing mounts that respond to GRB alerts within seconds, when the afterglow is potentially extremely bright. Each mirror and camera coating is being optimized for a different wavelength range and function, including a NIR imager, two red-optimized imagers, a blue-optimized imager, an UV-optimized imager, and an optical polarimeter. PROMPT will be able to identify high-redshift events by dropout and distinguish these events from the similar signatures of extinction. In this way, PROMPT will act as a distance-finder scope for spectroscopic follow up on the larger 4.1-meter diameter SOAR telescope, which is also located at CTIO. When not chasing GRBs, PROMPT serves broader educational objectives across the state of North Carolina. Enclosure construction and the first two telescopes are now complete and functioning: PROMPT observed Swifts first GRB in December 2004. We upgrade from two to four telescope in February 2005 and from four to six telescopes in mid-2005.


Archive | 2004

GRB 041217: PROMPT observations.

Matthew B. Bayliss; Melissa C. Nysewander; A. Foster; Daniel E. Reichart; J. A. Moran


Archive | 2003

GRB 030824: candidate follow-up.

Melissa C. Nysewander; J. Christopher Clemens; J. A. Moran; Daniel E. Reichart


Archive | 2003

GRB 031026: further Ic observations.

Melissa C. Nysewander; J. A. Moran; Christian Michel Zdanowicz; Daniel E. Reichart; M. Schwartz


Archive | 2003

GRB 030416: optical observations.

Arne A. Henden; J. Silvay; J. A. Moran; R. Soule; Daniel E. Reichart; Gerald Schaefer; Ronald W. Canterna; B. Scoggins


Archive | 2003

GRB 030324: optical and NIR observations.

J. A. Moran; Arne A. Henden; Donald Q. Lamb; Donald G. York; Melissa C. Nysewander; John C. Barentine; Jack Dembicky; Carlo Alberto Graziani; E. Sheldon; R. Soule; Matthew B. Bayliss; H.-J. Cheng; Curtis R. Cook; Mercedes Lopez-Morales; Daniel E. Reichart; Russet Jennifer McMillan; B. Ketsebeck; C. V. Blacker; A. Reese


Archive | 2003

GRB 030329: correction to GCN 2254.

H.-J. Cheng; Matthew B. Bayliss; Daniel E. Reichart; J. A. Moran; Melissa C. Nysewander; M. Schwartz; P. R. Holvorcem


Archive | 2003

GRB 030824: candidate afterglow (or Variable/Flare star?).

J. A. Moran; Melissa C. Nysewander; Daniel E. Reichart; Peter B. Yim; Christian Michel Zdanowicz; Johan Ormel Reichart


Archive | 2003

GRB 030226: ic observations.

Melissa C. Nysewander; J. A. Moran; Daniel E. Reichart; Arne A. Henden; M. Schwartz

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Daniel E. Reichart

University of North Carolina at Chapel Hill

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Melissa C. Nysewander

University of North Carolina at Chapel Hill

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Arne A. Henden

American Association of Variable Star Observers

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Matthew B. Bayliss

University of North Carolina at Chapel Hill

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A. Foster

University of North Carolina at Chapel Hill

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J. W. Bartelme

University of North Carolina at Chapel Hill

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A. Harper

University of Chicago

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