Interferometría... Magia o Ciencia? Rubén Herrero-Illana
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1 Interferometría... Magia o Ciencia? Rubén Herrero-Illana
2 Introduction
3 Introduction Hubble resolution: 0.05 (2.4m mirror).
4 Introduction Hubble resolution: 0.05 (2.4m mirror). Radio (1cm) 50 Km mirror!
5 Introduction Hubble resolution: 0.05 (2.4m mirror). Radio (1cm) 50 Km mirror!
6 Introduction Hubble resolution: 0.05 (2.4m mirror). Radio (1cm) 50 Km mirror!
7 Basics Rubén Herrero-Illana Charla CCD - 16/03/2011
8 Double slit experiment Rubén Herrero-Illana Charla CCD - 16/03/2011
9 Double slit experiment D
10 Double slit experiment D
11 Double slit experiment D
12 Double slit experiment D
13 Double slit experiment D
14 Double slit experiment Rubén Herrero-Illana Charla CCD - 16/03/2011
15 Double slit experiment Rubén Herrero-Illana Charla CCD - 16/03/2011
16 Double slit experiment Rubén Herrero-Illana Charla CCD - 16/03/2011
17 Double slit experiment FT!!
18 Double slit experiment Rendijas Foco Pantalla
19 Double slit experiment Rendijas Fuente Pantalla
20 Double slit experiment Antenas Fuente Pantalla
21 Double slit experiment Antenas Fuente Ordenador
22 Double slit experiment Antenas D Fuente Ordenador
23 u-v plane B
24 u-v plane B
25 u-v plane v v u u B
26 u-v plane v v u u B
27 u-v plane v v u u B
28 u-v plane v v u u B
29 u-v plane v v u u B
30 u-v coverage: Dirty beam 2 antennas Antenas
31 u-v coverage: Dirty beam 3 antennas Antenas
32 u-v coverage: Dirty beam 4 antennas Antenas
33 u-v coverage: Dirty beam 5 antennas Antenas
34 u-v coverage: Dirty beam 6 antennas Antenas
35 u-v coverage: Dirty beam 7 antennas Antenas
36 u-v coverage: Dirty beam 8 antennas Antenas
37 u-v coverage: Dirty beam 8 antennas x 2 samples Antenas
38 u-v coverage: Dirty beam 8 antennas x 6 samples Antenas
39 u-v coverage: Dirty beam 8 antennas x 30 samples Antenas
40 u-v coverage: Dirty beam 8 antennas x 107 samples Antenas
41 Observations Rubén Herrero-Illana Charla CCD - 16/03/2011
42 Main ideas Flux calibrator. Phase calibrators. Best u-v coverage. Real time VS Tapes.
43 Interferometers Rubén Herrero-Illana Charla CCD - 16/03/2011
44 Interferometers EVLA
45 Interferometers EVLA emerlin
46 Interferometers EVLA emerlin Plateau de Bure
47 ALMA Interferometers
48 Interferometers ALMA LOFAR
49 Interferometers SKA ALMA LOFAR
50 VLBI Rubén Herrero-Illana Charla CCD - 16/03/2011
51 Space - VLBI Rubén Herrero-Illana Charla CCD - 16/03/2011
52 IR and beyond... Rubén Herrero-Illana Charla CCD - 16/03/2011
53 Cygnus A Jennison & Das Gupta (1953)
54 Cygnus A Jennison & Das Gupta (1953)
55 Cygnus A Jennison & Das Gupta (1953)
56 Cygnus A Jennison & Das Gupta (1953)
57 Cygnus A Jennison & Das Gupta (1953) Krichbaum et al. (1998)
58 Data reduction Rubén Herrero-Illana Charla CCD - 16/03/2011
59 AIPS Software Most powerful software. IRAF like. Created in 1970s (ancient FORTRAN).
60 AIPS Software Most powerful software. IRAF like. Created in 1970s (ancient FORTRAN). CASA Developed for ALMA. C/C++ kernel / Python interface. Nearly completed.
61 Step by step Data examination. Amplitude calibration. Phase calibration. Imaging.
62 Step by step Data examination. Amplitude calibration. Phase calibration. Imaging.
63 Imaging (J. Pety) Source
64 Imaging (J. Pety) Source Dirty beam (PSF) Rubén Herrero-Illana Charla CCD - 16/03/2011
65 Imaging (J. Pety) Source Dirty beam (PSF) Dirty image Rubén Herrero-Illana Charla CCD - 16/03/2011
66 Imaging (J. Pety) Source Dirty beam (PSF) Dirty image Clean image Rubén Herrero-Illana Charla CCD - 16/03/2011
67 Some examples (LIRG biased!)
68 rp 299: Hunting SNe & AGN Pérez-Torres et al. 2009
69 rp 299: Hunting SNe & AGN Pérez-Torres et al Pérez-Torres et al. 2010
70 IC cm 814nm 435nm Rubén Herrero-Illana Charla CCD - 16/03/2011
71 Muchas gracias!
72
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