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Interferometric mapping of magnetic fields: The massive star-forming region G34.4+0.23 MM
(UNIV CHICAGO PRESS, 2008-03-20)
the Berkeley-Illinois-Maryland Association (BIMA) array. Our results show a remarkably uniform polarization pattern in both dust and in CO J = 1 -> 0 emission. In addition, the line emission presents a consistent uniform polarization pattern over most...
Extended mosaic observations with the Cosmic Background Imager
(IOP PUBLISHING, 2004-07-10)
. Under the assumption that any signal in excess of the primary anisotropy is due to a secondary Sunyaev-Zeldovich anisotropy in distant galaxy clusters, we use CBI, Arcminute Cosmology Bolometer Array Receiver, and Berkeley-Illinois-Maryland Association...
Ultra-pure digital sideband separation at sub-millimeter wavelengths
(EDP Sciences, 2015)
by the ADCs SFDR.
4. FPGA firmware
The ROACH-I FPGA open platform (CASPER-Berkeley 2015)
was used to implement the sideband-separating spectrometer.
The FPGA firmware used here, and presented schematically in
Fig. 4, was similar in function to the one...
FPGA, Tech. Rep., Pontificia Universidad Católica de Valparaíso, memoria para optar al Título de Ingeniero Civil Eléctrico Bout, J., Baryshev, A., Barkhof, J., et al. 2008, in 19th Int. Symp. on Space Terahertz Technology, Groningen, 28–30 April CASPER-Berkeley...
FPGA, Tech. Rep., Pontificia Universidad Católica de Valparaíso, memoria para optar al Título de Ingeniero Civil Eléctrico Bout, J., Baryshev, A., Barkhof, J., et al. 2008, in 19th Int. Symp. on Space Terahertz Technology, Groningen, 28–30 April CASPER-Berkeley...
A FPGA-based fast converging digital adaptive filter for real time RFI mitigation on ground based radio telescopes
(IOP Publishing Ltd, 2018)
and
Electronics Research) led by Berkeley University. The most
important components of the board are the Xilinx Virtex-66
XC6VSX475T FPGA, and a couple of 5GSPS ADC boards
(Jiang et al. 2014) manufactured by ASIAA (Academia Sinica
Institute of Astronomy...
America Center for Astronomy (CASSACA). D.L. and D.R. also acknowledge the support from the International Partnership 5 https://casper.berkeley.edu/wiki/ROACH2 6 https://www.xilinx.com/support/documentation/data_sheets/ds150.pdf 7 https://www.e2v...
America Center for Astronomy (CASSACA). D.L. and D.R. also acknowledge the support from the International Partnership 5 https://casper.berkeley.edu/wiki/ROACH2 6 https://www.xilinx.com/support/documentation/data_sheets/ds150.pdf 7 https://www.e2v...
Spiral structure in the outer galactic disk. I. The third galactic quadrant
(UNIV CHICAGO PRESS, 2008-01-10)
,
Haffner 11, Haffner 4, Haffner 15, Haffner 7, Berkeley 76, or
Auner 1. In some cases (Ruprecht 150 and the field centered in
the Canis Major overdensity) we do not find any star cluster but
only a diffuse young population. Photometric diagrams of all...
................ Berkeley 76 225.099 �1.998 16.50 � 0.40 0.40 � 0.15 11.30 � 1.50 2000 � 250 �7.645 7.619 �0.377 BP Berkeley 76 225.099 �1.998 15.80 � 0.50 0.50 � 0.02 7.30 � 1.60 �100 �5.168 5.150 �0.255 4................ Haffner 4 227.900 �3.586 14.75 � 0.20 0.53 � 0.07 4...
................ Berkeley 76 225.099 �1.998 16.50 � 0.40 0.40 � 0.15 11.30 � 1.50 2000 � 250 �7.645 7.619 �0.377 BP Berkeley 76 225.099 �1.998 15.80 � 0.50 0.50 � 0.02 7.30 � 1.60 �100 �5.168 5.150 �0.255 4................ Haffner 4 227.900 �3.586 14.75 � 0.20 0.53 � 0.07 4...
The Q/U Imaging ExperimenT: Polarization Measurements of the Galactic Plane at 43 and 95 GHz
(IOP Publishing, 2015)
, USA
7 High Energy Accelerator Research Organization (KEK), 1–1 Oho, Tsukuba, Ibaraki 305–0801, Japan
8 Department of Physics, University of California, Berkeley, CA 94720, USA
9 Cahill Center for Astronomy and Astrophysics, California Institute...
of Technology, 1200 E. California Boulevard M/C 249–17, Pasadena, CA 91125, USA 10 Physics Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA 11 Joseph Henry Laboratories of Physics, Jadwin Hall, Princeton University...
of Technology, 1200 E. California Boulevard M/C 249–17, Pasadena, CA 91125, USA 10 Physics Division, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720, USA 11 Joseph Henry Laboratories of Physics, Jadwin Hall, Princeton University...
First intrinsic anisotropy observations with the cosmic background imager
(UNIV CHICAGO PRESS, 2001-03-01)
Conte Hall, Berkeley, CA 94720-7300
S. T. Myers
National Radio Astronomy Observatory, P.O. Box O, Socorro, NM 87801
J. E. Carlstrom and E. M. Leitch
University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637
M. Joy
Department of Space Science, SD50...
Where is OH and Does It Trace the Dark Molecular Gas (DMG)?
(Institute of Physics Publishing, 2018)
of Astronomy, University of California, Berkeley, 601 Campbell Hall 3411, Berkeley, CA 94720-3411, USA
7 Department of Astronomy, The University of Texas at Austin, Austin, TX 78712, USA
8 Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak...
The anisotropy of the microwave background to l = 3500: Mosaic observations with the cosmic background imager
(Institute of Physics Publishing, 2003)
. Carlstrom, J. Kovac, E. M. Leitch, and C. Pryke
Department of Astronomy andAstrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637
N.W. Halverson and W. L. Holzapfel
Department of Physics, University of California, Berkeley, 366 Le...
Conte Hall, Berkeley, CA 94720-7300 P. Altamirano, L. Bronfman, S. Casassus, and J. May Departamento de Astronomı´a, Universidad de Chile, Casilla 36-D, Santiago, Chile and M. Joy Department of Space Science, SD50, NASAMarshall Space Flight Center, Huntsville...
Conte Hall, Berkeley, CA 94720-7300 P. Altamirano, L. Bronfman, S. Casassus, and J. May Departamento de Astronomı´a, Universidad de Chile, Casilla 36-D, Santiago, Chile and M. Joy Department of Space Science, SD50, NASAMarshall Space Flight Center, Huntsville...
The anisotropy of the microwave background to l = 3500: Deep field observations with the cosmic background imager
(Institute of Physics Publishing, 2003)
. M. Leitch, and C. Pryke
Department of Astronomy andAstrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637
N.W. Halverson and W. L. Holzapfel
Department of Physics, University of California, Berkeley, 366 Le Conte Hall...
, Berkeley, CA 94720-7300 P. Altamirano, L. Bronfman, S. Casassus, and J. May Departamento de Astronomı´a, Universidad de Chile, Casilla 36-D, Santiago, Chile and M. Joy Department of Space Science, SD50, NASAMarshall Space Flight Center, Huntsville, AL 35812...
, Berkeley, CA 94720-7300 P. Altamirano, L. Bronfman, S. Casassus, and J. May Departamento de Astronomı´a, Universidad de Chile, Casilla 36-D, Santiago, Chile and M. Joy Department of Space Science, SD50, NASAMarshall Space Flight Center, Huntsville, AL 35812...