Interferometría ¿Magia o Ciencia?Rubén Herrero-Illana Charla CCD - 16/03/2011 Pérez-Torres et...

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Rubén Herrero-Illana Interferometría... ¿Magia o Ciencia?

Transcript of Interferometría ¿Magia o Ciencia?Rubén Herrero-Illana Charla CCD - 16/03/2011 Pérez-Torres et...

  • Rubén Herrero-Illana

    Interferometría...¿Magia o Ciencia?

  • Introduction

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Introduction

    • • Hubble resolution: 0.05” (2.4m mirror).

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Introduction

    • • Hubble resolution: 0.05” (2.4m mirror).• Radio (1cm) 50 Km mirror!

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Introduction

    • • Hubble resolution: 0.05” (2.4m mirror).• Radio (1cm) 50 Km mirror!

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Introduction

    • • Hubble resolution: 0.05” (2.4m mirror).• Radio (1cm) 50 Km mirror!

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Basics

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    D

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    DD

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    DD

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    DD

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    DD

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    FT!!

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    Rendijas

    Pantalla

    Foco

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    Rendijas

    Pantalla

    Fuente

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    Pantalla

    Fuente

    Antenas

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    Fuente

    Antenas

    Ordenador

  • Double slit experiment

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    Fuente

    Antenas

    Ordenador

    D

  • u-v plane

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    B

  • u-v plane

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    B

  • u-v plane

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    B

    u

    v

    u

    v

  • u-v plane

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    B

    u

    v

    u

    v

  • u-v plane

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    B

    u

    v

    u

    v

  • u-v plane

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    B

    u

    v

    u

    v

  • u-v plane

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    B

    u

    v

    u

    v

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    2 antennas

    u-v coverage: Dirty beam

  • u-v coverage: Dirty beam

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    3 antennas

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    4 antennas

    u-v coverage: Dirty beam

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    5 antennas

    u-v coverage: Dirty beam

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    6 antennas

    u-v coverage: Dirty beam

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    7 antennas

    u-v coverage: Dirty beam

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    8 antennas

    u-v coverage: Dirty beam

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    8 antennas x 2 samples

    u-v coverage: Dirty beam

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    8 antennas x 6 samples

    u-v coverage: Dirty beam

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    8 antennas x 30 samples

    u-v coverage: Dirty beam

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Antenas

    8 antennas x 107 samples

    u-v coverage: Dirty beam

  • Observations

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Main ideas

    • Flux calibrator.• Phase calibrators.• Best u-v coverage.• Real time VS Tapes.

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Interferometers

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Interferometers

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    EVLA

  • Interferometers

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    EVLAeMERLIN

  • Interferometers

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    EVLAeMERLIN

    Plateau de Bure

  • Interferometers

    ALMA

  • Interferometers

    ALMA

    LOFAR

  • Interferometers

    ALMASKA

    LOFAR

  • VLBI

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Space - VLBI

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    IR and beyond...

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Cygnus A

    Jennison & Das Gupta (1953)

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Cygnus A

    Jennison & Das Gupta (1953)

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Cygnus A

    Jennison & Das Gupta (1953)

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Cygnus A

    Jennison & Das Gupta (1953)

  • Rubén Herrero-Illana Charla CCD - 16/03/2011

    Jennison & Das Gupta (1953)

    Krichbaum et al. (1998)

    Cygnus A

  • Data reduction

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Software

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    AIPSMost powerful software.

    Created in 1970s (ancient FORTRAN).

    IRAF ‘like’.

  • Software

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    AIPS

    CASA

    Most powerful software.

    Created in 1970s (ancient FORTRAN).

    IRAF ‘like’.

    Developed for ALMA.

    C/C++ kernel / Python interface.

    Nearly completed.

  • Step by step

    • Data examination.• Amplitude calibration.• Phase calibration.• Imaging.

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Step by step

    • Data examination.• Amplitude calibration.• Phase calibration.• Imaging.

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Imaging

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    (J. Pety)

    Source

  • Imaging

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    (J. Pety)

    Source Dirty beam(PSF)

  • Imaging

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    (J. Pety)

    Source Dirty beam(PSF)

    Dirtyimage

  • Imaging

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    (J. Pety)

    Source Dirty beam(PSF)

    Dirtyimage

    Cleanimage

  • Some examples(LIRG biased!)

    Rubén Herrero-Illana Charla CCD - 16/03/2011

  • Arp 299: Hunting SNe & AGN

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    Pérez-Torres et al. 2009

  • Arp 299: Hunting SNe & AGN

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    Pérez-Torres et al. 2009 Pérez-Torres et al. 2010

  • IC 1623

    Rubén Herrero-Illana Charla CCD - 16/03/2011

    3.6cm 814nm 435nm

  • ¡Muchas gracias!