A survey for fast transients in the Fornax Cluster of galaxies (2008)
Rau, A., Ofek, E. O., Kulkarni, S. R., Madore, B. F., Pevunova, O., Ajello, M.
The luminosity gap between novae (M_R ≤ − 10) and supernovae (M_R ≥ − 14) has been well known since the pioneering research of Zwicky and Hubble. Nearby galaxy clusters and concentrations...
A Survey for Fast Transients in the Fornax Cluster of Galaxies (2008)
Rau, A., Ofek, E. O., Kulkarni, S. R., Madore, B. F., Pevunova, O., Ajello, M.
The luminosity gap between novae (M_R < -10) and supernovae (M_R > -14) is well known since the pioneering research of Zwicky and Hubble. Nearby galaxy clusters and concentrations offer an excellent...
A survey for fast transients in the Fornax cluster of galaxies (2008)
Rau, A., Ofek, E. O., Kulkarni, S. R., Madore, B. F., Pevunova, O., Ajello, M.
The Curious Case of NGC6908 (2007)
Madore, B. F., De Paz, A. Gil, Pevunova, O., Thompson, I.
The object NGC6908 was once thought to be simply a surface-brightness enhancement in the eastern spiral arm of the nearby spiral galaxy NGC6907. Based on an examination of near-infrared imaging, the...
IC 1257: A New Globular Cluster in the Galactic Halo (2004)
Harris, W. E., Phelps, R. L., Madore, B. F., Pevunova, O., Skiff, B. A., Crute, C., ...
New CCD photometry of the faint, compact star cluster IC 1257 (L = 17? = ± 15?obtained with the Palomar 5m telescope, reveals that it is a highly reddened globular cluster well beyond the...
A new complete sample of submillijansky radio sources: An optical and near-infrared study (2004)
Masci, F., Condon, J., Barlow, T., Lonsdale, C., Xu, C., Shupe, D., ...
The Very Large Array has been used in C configuration to map an area similar or equal to 0.3 deg(2) at 1.4 GHz with 5 sigma sensitivities of 0.305, 0.325, 0.380, and 0.450 mJy beam(-1)over four equal...
De Paz, A. Gil, Madore, B. F., Pevunova, O.
We present B, R, and Halpha images for a total of 114 nearby galaxies (v_helio-21mag), peak surface brightness (mu_B,peak
Multi-Color Observations of the GRB000926 Afterglow (2000)
Price, P. A., Harrison, F. A., Galama, T. J., Reichart, D. E., Axelrod, T. S., Berger, E. J., ...
We present multi-color light-curves of the optical afterglow of GRB 000926. Beginning ~1.5 days after the burst, the light-curves of this GRB steepen measurably. The existence of such achromatic...
A New Complete Sample of Sub-millijansky Radio Sources: An Optical and Near-Infrared Study (2000)
Masci, Frank J., Condon, J. J., Barlow, T. A., Lonsdale, C. J., Shupe, D. L., Pevunova, O., ...
The Very Large Array (VLA) has been used in C-configuration to map an area \~0.3 square degrees at 1.4 GHz with 5sigma sensitivities of 0.305, 0.325, 0.380 and 0.450 mJy/beam over four equal...