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This special page shows all uploaded files.
| Date | Name | Thumbnail | Size | User | Description | Versions |
|---|---|---|---|---|---|---|
| 04:00, 15 December 2016 | XSP20151005173526.png (file) |  |
97 KB | Nkuroda | 1 | |
| 03:58, 15 December 2016 | FLM20151005.png (file) |  |
35 KB | Nkuroda | 1 | |
| 02:27, 15 December 2016 | 2016-04-15 hpol.png (file) |  |
171 KB | Nkuroda | 1 | |
| 02:27, 15 December 2016 | 2016-04-13 hpol.png (file) |  |
136 KB | Nkuroda | 1 | |
| 16:23, 12 December 2016 | Rot ctr search4.png (file) |  |
83 KB | Dgary | Result of search for best rotation axis center position. | 1 |
| 12:40, 20 November 2016 | Pha vs ha 2253+161 20161009 one fit.png (file) |  |
116 KB | Bchen | Phase vs. hour angle for Antennas 9, 10, 11, 13 w.r.t. Antenna 14 at both XX and YY polarizations. This is based on an hour observation of 2136+006 (9.9 Jy at C band) and 2253+161 (10 Jy at C band) on 2016 Sep 7 under the fast frequency-sweeping mode o... | 1 |
| 12:37, 20 November 2016 | Pha vs ha 2253+161 20161009 independent fits.png (file) |  |
125 KB | Bchen | Phase vs. hour angle for Antennas 9, 10, 11, 13 w.r.t. Antenna 14 at both XX and YY polarizations. This is based on an hour observation of 2136+006 (9.9 Jy at C band) and 2253+161 (10 Jy at C band) on 2016 Sep 7 under the fast frequency-sweeping mode o... | 1 |
| 12:02, 20 November 2016 | Pha vs ha 0319+415 20160907 corrected.png (file) |  |
71 KB | Bchen | Corrected phase vs. hour angle for Antennas 9, 10, 11, 13 w.r.t. Antenna 14 at both XX and YY polarizations. This is based on a ~5.5 hour observation of 3C84 on 2016 Sep 7. Different colors represent measurements/fits at different frequency channels. | 1 |
| 20:55, 19 November 2016 | Pha vs ha 0319+415 20160907.png (file) |  |
145 KB | Bchen | Phase vs. hour angle for Antennas 9, 10, 11, 13 w.r.t. Antenna 14 at both XX and YY polarizations. This is based on a ~5.5 hour observation of 3C84 on 2016 Sep 7. Circular symbols are measured phases and curves are the corresponding sinusoidal curves.... | 1 |
| 19:54, 16 November 2016 | Cal src vis.png (file) |  |
484 KB | Nkuroda | Produced by dg_src_visibility for 2016-10-14, minflux = 4.0 and for 24 hours. | 1 |
| 14:21, 15 November 2016 | 3C84 cos-el-correction.png (file) |  |
323 KB | Dgary | 3C84 data without, and with Cos Elevation phase rotation. | 1 |
| 15:36, 13 November 2016 | 3C273 PA test.png (file) |  |
141 KB | Dgary | Effect of rotating ant 14 feed position angle (PA) on AzEl antennas 1-5 and 12, vs. Equatorial antennas 8-11 and 13. | 1 |
| 07:29, 13 November 2016 | 3C84 Hi Rcvr.png (file) |  |
211 KB | Dgary | 3C84 phases on high-frequency receiver (first fringes on this receiver!) | 1 |
| 04:48, 8 November 2016 | 3C273 cos-el-rotation.png (file) |  |
64 KB | Dgary | Observations and simulation on 3C273, with cos E term applied. | 1 |
| 04:47, 8 November 2016 | 3C84 cos-el-rotation.png (file) |  |
149 KB | Dgary | Observations and simulation on 3C84 with cos E term applied | 1 |
| 21:39, 2 November 2016 | Interferometer3 Antenna position wiki fig2.gif (file) |  |
5 KB | Nkuroda | 1 | |
| 19:49, 2 November 2016 | Coords Antenna position wiki fig1.gif (file) |  |
3 KB | Nkuroda | 1 | |
| 16:59, 27 October 2016 | Notch filter case.png (file) |  |
141 KB | Dgary | 1 | |
| 16:58, 27 October 2016 | Notch filter curve.png (file) |  |
306 KB | Dgary | 1 | |
| 16:21, 27 October 2016 | RFI2.png (file) |  |
70 KB | Dgary | Data taken prior to EOVSA construction, showing RFI in the 1-2 GHz band. | 2 |
| 16:19, 27 October 2016 | RFI1.png (file) |  |
68 KB | Dgary | Data taken prior to EOVSA construction, showing RFI in the 1-2 GHz band. | 1 |
| 04:26, 22 October 2016 | 3C84 multi-freq.png (file) |  |
216 KB | Dgary | 3C84 Phase difference on multiple frequencies for Ant 1-14 | 1 |
| 04:21, 22 October 2016 | 3C84 multi-ant.png (file) |  |
184 KB | Dgary | 3C84 Phase on AzEl antennas 1-6 | 1 |
| 17:47, 21 October 2016 | 3C84 no-rotation.png (file) |  |
146 KB | Dgary | Observation and simulation of 3C84 without phase rotation | 1 |
| 15:24, 21 October 2016 | 1996A+AS 117 137H.pdf (file) |  |
286 KB | Dgary | Hamaker, Bregman and Sault (1996) | 1 |
| 10:27, 21 October 2016 | Feed diagram.PNG (file) |  |
154 KB | Dgary | Added 27-m feed illustration | 2 |
| 16:57, 20 October 2016 | Parallactic.png (file) |  |
42 KB | Dgary | Parallactic Angle at OVRO for range of hour angle and declination | 1 |
| 13:55, 20 October 2016 | 3C273 chi-rotation.png (file) |  |
67 KB | Dgary | Observation and simulation of 3C273, applying 2*chi rotation | 1 |
| 13:54, 20 October 2016 | 3C273 abs-chi-rotation.png (file) |  |
66 KB | Dgary | Observation and simulation of 3C273, applying 2*abs(chi) rotation | 1 |
| 13:54, 20 October 2016 | 3C84 abs-chi-rotation.png (file) |  |
148 KB | Dgary | Observation and simulation of 3C84, applying 2*abs(chi) rotation | 1 |
| 13:53, 20 October 2016 | 3C84 chi-rotation.png (file) |  |
148 KB | Dgary | Observation and simulation of 3C84 feed-rotation effect, applying 2*chi | 1 |
| 02:48, 16 October 2016 | DownConversionDiagram 1120MHz.png (file) |  |
41 KB | Dgary | Bandpass if we use an 1120 MHz ADC clock speed | 1 |
| 01:19, 28 September 2016 | New telescope mount.png (file) |  |
4.24 MB | Sjyu | Figure 1: The new mount for the optical telescope, to be put in place of the radio front-end receiver. This should greatly reduce vibrations that lead to non-circular stars. | 1 |
| 15:24, 27 September 2016 | 7.png (file) |  |
15 KB | Schhabra | 1 | |
| 15:23, 27 September 2016 | 6.png (file) |  |
20 KB | Schhabra | 1 | |
| 15:23, 27 September 2016 | 5.png (file) |  |
19 KB | Schhabra | 1 | |
| 14:57, 27 September 2016 | 4.png (file) |  |
32 KB | Schhabra | 1 | |
| 14:56, 27 September 2016 | 3.png (file) |  |
72 KB | Schhabra | 1 | |
| 14:56, 27 September 2016 | 2.png (file) |  |
15 KB | Schhabra | 1 | |
| 04:20, 27 September 2016 | Spectrogram.png (file) |  |
164 KB | Sshaik | 1 | |
| 04:01, 27 September 2016 | Figure 2.png (file) |  |
57 KB | Yjluo | 1 | |
| 03:45, 27 September 2016 | Figure 1.png (file) |  |
127 KB | Yjluo | 4 | |
| 01:00, 26 September 2016 | 1.png (file) |  |
277 KB | Schhabra | 1 | |
| 00:50, 26 September 2016 | 4.pdf (file) | |
149 KB | Schhabra | 1 | |
| 18:53, 25 September 2016 | Image4.png (file) |  |
34 KB | Ychai | 1 | |
| 18:52, 25 September 2016 | Image3.png (file) |  |
41 KB | Ychai | 1 | |
| 18:52, 25 September 2016 | Image2.png (file) |  |
46 KB | Ychai | 1 | |
| 18:50, 25 September 2016 | Image6.png (file) |  |
569 KB | Ychai | 1 | |
| 18:43, 25 September 2016 | Image5.png (file) |  |
694 KB | Ychai | 1 | |
| 18:40, 25 September 2016 | Image8.png (file) |  |
297 KB | Ychai | Figure 7: Direct (not normalized) spectrum for roughly the same region as in Figure 6, but now with the optical link supposedly centered on its linear range. The second-harmonic distortion is now much reduced, but certainly not eliminated. We can do... | 1 |
