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Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise...

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Low Frequency Radio Astronomy

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Page 1: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Low Frequency Radio Astronomy

Page 2: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 3: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 4: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 5: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 6: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 7: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 8: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 9: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 10: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

SKA-low site

Page 11: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 12: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 13: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

MeerKAT and SKA-mid array

Page 14: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 15: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 16: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 17: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 18: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 19: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 20: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 21: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 22: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 23: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 24: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 25: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

Page 26: Low Frequency Radio Astronomy - uwyo.eduphysics.uwyo.edu/~chip/JC/LowFreq.pdf · and the noise bias, we detect a non-zero A12 = (56 ± 13 mK)2 (I-CT) excess variance and a best 2-0-

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