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Start Over Author "Rabii B" Publisher american astronomical society
11 results on '"Rabii B"'

1. MAXIPOL: Data Analysis and Results

Author

Wu, J. H. P., primary, Zuntz, J., additional, Abroe, M. E., additional, Ade, P. A. R., additional, Bock, J., additional, Borrill, J., additional, Collins, J., additional, Hanany, S., additional, Jaffe, A. H., additional, Johnson, B. R., additional, Jones, T., additional, Lee, A. T., additional, Matsumura, T., additional, Rabii, B., additional, Renbarger, T., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Tran, H. T., additional, and Winant, C. D., additional

Published
2007
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2. MAXIPOL: Cosmic Microwave Background Polarimetry Using a Rotating Half‐Wave Plate

Author

Johnson, B. R., primary, Collins, J., additional, Abroe, M. E., additional, Ade, P. A. R., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, de Bernardis, P., additional, Hanany, S., additional, Jaffe, A. H., additional, Jones, T., additional, Lee, A. T., additional, Levinson, L., additional, Matsumura, T., additional, Rabii, B., additional, Renbarger, T., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Tran, H. T., additional, Winant, C. D., additional, Wu, J. H. P., additional, and Zuntz, J., additional

Published
2007
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3. Determining Foreground Contamination in Cosmic Microwave Background Observations: Diffuse Galactic Emission in the MAXIMA‐I Field

Author

Jaffe, A. H., primary, Balbi, A., additional, Bond, J. R., additional, Borrill, J., additional, Ferreira, P. G., additional, Finkbeiner, D., additional, Hanany, S., additional, Lee, A. T., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Winant, C. D., additional, and Wu, J. H. P., additional

Published
2004
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5. A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data

Author

Lee, A. T., primary, Ade, P., additional, Balbi, A., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, de Bernardis, P., additional, Ferreira, P. G., additional, Hanany, S., additional, Hristov, V. V., additional, Jaffe, A. H., additional, Mauskopf, P. D., additional, Netterfield, C. B., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Winant, C. D., additional, and Wu, J. H. P., additional

Published
2001
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6. Cosmological Implications of the MAXIMA-1 High-Resolution Cosmic Microwave Background Anisotropy Measurement

Author

Stompor, R., primary, Abroe, M., additional, Ade, P., additional, Balbi, A., additional, Barbosa, D., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, de Bernardis, P., additional, Ferreira, P. G., additional, Hanany, S., additional, Hristov, V., additional, Jaffe, A. H., additional, Lee, A. T., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Winant, C. D., additional, and Wu, J. H. P., additional

Published
2001
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7. Asymmetric Beams in Cosmic Microwave Background Anisotropy Experiments

Author

Wu, J. H. P., primary, Balbi, A., additional, Borrill, J., additional, Ferreira, P. G., additional, Hanany, S., additional, Jaffe, A. H., additional, Lee, A. T., additional, Oh, S., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, and Winant, C. D., additional

Published
2001
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8. Constraints on Cosmological Parameters from MAXIMA-1

Author

Balbi, A., primary, Ade, P., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, De Bernardis, P., additional, Ferreira, P. G., additional, Hanany, S., additional, Hristov, V., additional, Jaffe, A. H., additional, Lee, A. T., additional, Oh, S., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Winant, C. D., additional, and Wu, J. H. P., additional

Published
2000
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9. MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10[arcmin]–5°

Author

Hanany, S., primary, Ade, P., additional, Balbi, A., additional, Bock, J., additional, Borrill, J., additional, Boscaleri, A., additional, de Bernardis, P., additional, Ferreira, P. G., additional, Hristov, V. V., additional, Jaffe, A. H., additional, Lange, A. E., additional, Lee, A. T., additional, Mauskopf, P. D., additional, Netterfield, C. B., additional, Oh, S., additional, Pascale, E., additional, Rabii, B., additional, Richards, P. L., additional, Smoot, G. F., additional, Stompor, R., additional, Winant, C. D., additional, and Wu, J. H. P., additional

Published
2000
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10. Preliminary cosmic microwave background anisotropy results from the MAXIMA balloon borne experiment

Author

Johnson, B. R., Hanany, S., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., DeBernardis, P., Ferreira, P., Hristov, V., Lange, A. E., Pascale, Enzo, Jaffe, A. H., Lee, A. T., Oh, S., Rabii, B., Richards, P. L., Winant, C. D., Mauskopf, Philip Daniel, Netterfield, C. B., Johnson, B. R., Hanany, S., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., DeBernardis, P., Ferreira, P., Hristov, V., Lange, A. E., Pascale, Enzo, Jaffe, A. H., Lee, A. T., Oh, S., Rabii, B., Richards, P. L., Winant, C. D., Mauskopf, Philip Daniel, and Netterfield, C. B.

Abstract

We present preliminary cosmic microwave background anisotropy results from the first flight of the MAXIMA balloon borne experiment. The flight (MAXIMA-1) took place in August of 1998 from the National Scientific Ballooning Facility in Palestine, Texas. During the four hour flight we mapped a 124 deg2 section of the sky which has extremely low galactic dust contamination. The combination of the beam size and scan strategy make MAXIMA sensitive to CMB fluctuations on a range of angular scales from 10 arcmin to 5 degrees. The instrument consists of a Gregorian telescope with a 1.3m primary mirror and a receiver housing a 16 element bolometer array cooled to 100mK. Observations were made at 3 frequency bands centered on 150, 240, and 410 GHz. The results presented will include a map of the CMB anisotropy at 150 GHz. We will also briefly describe the second MAXIMA flight that took place in June of 1999. During this flight we observed 230 deg2 of sky with very low galactic dust contamination. About 20% of this region overlaps the MAXIMA-1 map. The MAXIMA experiment is supported by NASA through grant Nos. NAG5-4454, and NAG5-3941, and by the Center for Particle Astrophysics, a National Science Foundation Science and Technology Center operated by the University of California, Berkeley, under Cooperative Agreement No. AST-9120005.

11. MAXIMA: Observations of the Cosmic Microwave Background Anisotropy on Angular Scales of 10' to 5 Degrees

Author

Winant, C. D., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., De Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Johnson, B., Lange, A. E., Lee, A. T., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, Enzo, Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., Wu, J. H. P., Winant, C. D., Ade, Peter A. R., Balbi, A., Bock, J., Borrill, J., Boscaleri, A., De Bernardis, P., Ferreira, P., Hanany, S., Hristov, V., Jaffe, A. H., Johnson, B., Lange, A. E., Lee, A. T., Mauskopf, Philip Daniel, Netterfield, C. B., Oh, S., Pascale, Enzo, Rabii, B., Richards, P. L., Smoot, G. F., Stompor, R., and Wu, J. H. P.

Abstract

We discuss the status of our analysis of the data obtained from the first flight of the MAXIMA balloon borne experiment. The flight (MAXIMA-1) took place in August of 1998 from the National Scientific Ballooning Facility in Palestine, Texas. During the four hour flight we mapped a 124 deg2 section of the sky which has extremely low galactic dust contamination. The combination of the beam size and scan strategy make MAXIMA sensitive to CMB fluctuations on a range of angular scales from 10 arcmin to 5 degrees. The instrument consists of a Gregorian telescope with a 1.3 m primary mirror and a receiver housing a 16 element bolometer array cooled to 100 mK. Observations were made at 3 frequency bands centered on 150, 240, and 410 GHz. The results presented will include maps of the CMB anisotropy at 150 GHz. We will also briefly describe the second MAXIMA flight that took place in June of 1999 and our plans for the future. During the second flight we observed 230 deg2 of sky with very low galactic dust contamination. About 20% of this region overlaps the MAXIMA-1 map. The MAXIMA experiment is supported by NASA through grants NAG5-4454, and NAG5-3941, and by the Center for Particle Astrophysics, a National Science Foundation Science and Technology Center operated by the University of California, Berkeley, under Cooperative Agreement No. AST-9120005.

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