Mochejska, B. J., Stanek, K. Z., Sasselov, D. D., Szentgyorgyi, A. H., Cooper, R. L., Hickox, R. C., ...
We have undertaken a long-term project, Planets in Stellar Clusters Extensive Search (PISCES), to search for transiting planets in open clusters. In this paper we present the results for NGC 188, an...
Mroczkowski, T., Bonamente, M., Carlstrom, J. E., Culverhouse, T. L., Greer, C., Hawkins, D., ...
We investigate the utility of a new, self-similar pressure profile for fitting Sunyaev-Zel'dovich (SZ) effect observations of galaxy clusters. Current SZ imaging instruments - such as the...
An X-ray, IR, and Submillimeter Flare of Sagittarius A* (2007)
Marrone, D. P., Baganoff, F. K., Morris, M. R., Moran, J. M., Ghez, A. M., Hornstein, S. D., ...
Energetic flares are observed in the Galactic supermassive black hole Sagittarius A* from radio to X-ray wavelengths. On a few occasions, simultaneous flares have been detected in IR and X-ray...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
Archeops In-flight Performance, Data Processing and Map Making (2007)
Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...
Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...
Archeops In-flight Performance, Data Processing and Map Making (2007)
Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...
Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...
Archeops In-flight Performance, Data Processing and Map Making (2007)
Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...
Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...
Cosmological constraints from Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...
Cosmological constraints from Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...
Cosmological constraints from Archeops (2007)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
An Unambiguous Detection of Faraday Rotation in Sagittarius A* (2006)
Marrone, D. P., Moran, J. M., Rao, R.
The millimeter/submillimeter wavelength polarization of Sgr A* is known to be variable in both magnitude and position angle on time scales down to a few hours. The unstable polarization has prevented...
Radio Sources Toward Galaxy Clusters at 30 GHz (2006)
Coble, K., Bonamente, M., Carlstrom, J. E., Dawson, K., Hasler, N., Holzapfel, W., ...
Extra-galactic radio sources are a significant contaminant in cosmic microwave background and Sunyaev-Zel'dovich effect experiments. Deep interferometric observations with the BIMA and OVRO arrays...
Archeops In-flight Performance, Data Processing and Map Making (2006)
Macias-Perez, J. F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...
Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...
Archeops In-flight Performance, Data Processing and Map Making (2006)
Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...
Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...
Archeops In-flight Performance, Data Processing and Map Making (2006)
Macias-Perez, J.F., Lagache, G., Maffei, B., Ade, P., Amblard, A., Ansari, R., ...
Archeops is a balloon--borne experiment widely inspired by the Planck satellite and by its High Frequency Instrument (HFI). It is mainly dedicated to measure the Cosmic Microwave Background (CMB)...
Interferometric Measurements of Variable 340 GHz Linear Polarization in Sagittarius A* (2005)
Marrone, D. P., Moran, J. M., Rao, R.
Using the Submillimeter Array, we have made the first high angular resolution measurements of the linear polarization of Sagittarius A* at submillimeter wavelengths, and the first detection of...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
Observations in the 1.3 and 1.5 THz Atmospheric Windows with the Receiver Lab Telescope (2005)
Marrone, D. P., Blundell, R., Tong, E., Paine, S. N., Loudkov, D., Kawamura, J. H., ...
The Receiver Lab Telescope (RLT) is a ground-based terahertz telescope; it is currently the only instrument producing astronomical data between 1 and 2 THz. The capabilities of the RLT have been...
Mochejska, B. J., Stanek, K. Z., Sasselov, D. D., Szentgyorgyi, A. H., Bakos, G. A., Devor, J., ...
We have undertaken a long-term project, Planets in Stellar Clusters Extensive Search (PISCES), to search for transiting planets in open clusters. In this paper we present the results for NGC 6791 --...
Characterization and Status of a Terahertz Telescope (2004)
Marrone, D. P., Blundell, R., Gibson, H., Paine, S., Papa, D. C., Tong, E.
The Receiver Lab Telescope (RLT) is a ground-based terahertz observatory, located at an altitude of 5525 m on Cerro Sairecabur, Chile. The RLT has been in operation since late 2002, producing the...
A map of OMC-1 in CO 9-8 (2004)
Marrone, D. P., Battat, J., Bensch, F., Blundell, R., Diaz, M., Gibson, H., ...
The distribution of 12C16O J=9-8 (1.037 THz) emission has been mapped in OMC-1 at 35 points with 84" resolution. This is the first map of this source in this transition and only the second...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
Cosmological constraints from Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
The cosmic microwave background anisotropy power spectrum measured by Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R, Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
The cosmic microwave background anisotropy power spectrum measured by Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R, Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present the first determination of the Galactic polarized emission at 353 GHz by Archeops. The data were taken during the Arctic night of February 7, 2002 after the balloon--borne instrument was...
Cosmological constraints from Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2003)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops (2002)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We present a determination by the Archeops experiment of the angular power spectrum of the cosmic microwave background anisotropy in 16 bins over the multipole range l=15-350. Archeops was conceived...
Cosmological constraints from Archeops (2002)
Benoit, A., Ade, P., Amblard, A., Ansari, R., Aubourg, E., Bargot, S., ...
We analyze the cosmological constraints that Archeops places on adiabatic cold dark matter models with passive power-law initial fluctuations. Because its angular power spectrum has small bins in l...
Philhour, B. J., Keating, B. G., Ade, P. A. R., Bhatia, R. S., Bock, J. J., Church, S. E., ...
We describe the development of a bolometric receiver designed to measure the arcminute-scale polarization of the cosmic microwave background (CMB). The Polatron will be mounted at the Cassegrain...