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Мulti-frequency VLA observations of M87

М ulti-frequency VLA observations of M87

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М ulti-frequency VLA observations of M87. Observations’ parameters. Test VLA observations (configuration D) of M87 ( RA=12:28, Dec=12:40 ) took place on November 16 th , 2005. There were 22 antennas enabled. - PowerPoint PPT Presentation

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Page 1: М ulti-frequency VLA observations of M87

Мulti-frequency VLA observations of M87

Page 2: М ulti-frequency VLA observations of M87

Observations’ parameters

Test VLA observations (configuration D) of M87 (RA=12:28, Dec=12:40) took place on November 16th, 2005.

• There were 22 antennas enabled.

• Frequency bands: K (K1=21300, K2=22200, K3=23000 , K4=23400 MHz) и U (U1=14700, U1=15200 MHz) Total observation time were 3 hours.

• Official participants: N. Kardashev, L. Kogan, S. Likhachev, V. Vasilkov, E. Fomalont, F. Owen, E. Greisen, K. Kellermann.

Page 3: М ulti-frequency VLA observations of M87

Goals of the experiment

• Multi-frequency synthesis (MFS) of a M87 map on the reference frequency (19 GHz) with bandwidth of 7 GHz by means of a new class of the multi-frequency imaging (MFI) algorithms developed at the ASC.

• Multi-frequency analysis (MFA) of M87. Estimation of a spectral index maps of the source on the same reference frequency.

• Comparison of the obtained results with the existing MFI-technologies at NRAO.

• Investigations of the improvement of image fidelity by means of MFS.

Page 4: М ulti-frequency VLA observations of M87

Tools

• NRAO has used AIPS software (one can find the results of the data processing obtained by L. Kogan on the web site http://www.aoc.nrao.edu/~lkogan/m87plots.ps

• ASC has used ASL for Windows software (see below)

Page 5: М ulti-frequency VLA observations of M87

Part 1

Multi-frequency synthesis and analysis

Page 6: М ulti-frequency VLA observations of M87

(u,v)-coverageU-band K-band

Page 7: М ulti-frequency VLA observations of M87

Sequence of MFI of M87 (ASL for Windows)

• Maps synthesis be means of generalized self-calibration procedure for all six frequencies (14665, 15135, 21535, 21965, 22935, 23364 MHz).

• Synthesis of the image of M87 on the reference frequency (19014 MHz) by means of generalized linear multi-frequency deconvolution algorithm.

• Spectral analysis of the image (spectral indexes map, spectrum of different parts of the image of M87).

Page 8: М ulti-frequency VLA observations of M87

Generalized linear deconvolution algorithm

,

00

, , , ,x y

I x y I x y

,2

21 1 1 1

001 1 1 11 1

ˆ minx y

K N N K N Nk

ijkij kij kiji j i jk k

V V V I

F

U-band K -band

U+K band

Page 9: М ulti-frequency VLA observations of M87

Map Parameters

• Angular resolution: 0.6 “

• Map size: 256 by 256

• Weighting: uniform

• Tapering: uniform (no tapering)

• Gridding: by averaging

Page 10: М ulti-frequency VLA observations of M87

M87. Integral synthesis(two-frequencies data processing: 14.6 и 23.3 GHz)

IF1 =14.6 GHz

IF1 =23.3 GHz

IF1 =19.01 GHz (MFS)

Page 11: М ulti-frequency VLA observations of M87

remnantpeak flux

Dynamic range 5000:1

M87. Integral analysis(two-frequencies data processing: 14.6 и 23.3 GHz)

Page 12: М ulti-frequency VLA observations of M87

M87. Component analysis(two-frequencies data processing: 14.6 и 23.3 GHz)

Page 13: М ulti-frequency VLA observations of M87

AIPS ASL(two-frequency

analysis)

ASL(six-frequency

analysis)

Integral -0.73 -1.04 -1.17

Core -0.4 -0.35 -0.43

Right jet center -0.6 -0.84 -0.82

Left bulb -0.8 -1.09 -1.05

M87. Comparison of the Spectral Indexes(two-frequencies data processing: 14.6 и 23.3 GHz)

Page 14: М ulti-frequency VLA observations of M87

Spectral analysis of the right jet of М87(six-frequency analysis)

Page 15: М ulti-frequency VLA observations of M87

Dynamic range

where is rms of a remnant map.

Dynamic range remnant ,peak brightness

remnant

Peak brightness

[Jy/beam] rms

2 frequency 2.67 4700

6 frequencies 2.67 5600

Δ

-45.7×10

-44.8×10

Page 16: М ulti-frequency VLA observations of M87

Part 2

Improvement of Image Fidelity

Page 17: М ulti-frequency VLA observations of M87

Data Editing

The idea: to make worse fidelity of the images on each frequency and then to improve the fidelity by means of MFS

To decrease the quality of the observational data editing for all frequency bands and for all the sources (two calibration sources and a target source) was done:

1. given visibilities were edited by time;

2. edited visibilities were edited once again on the (u,v) –plane.

Page 18: М ulti-frequency VLA observations of M87

Time Editing

• The observation time was decreased from 3 hour to 5 minutes

Page 19: М ulti-frequency VLA observations of M87

Spatial EditingAfter time editing the number of the baselines were decreased from 231 to 75 with a gap between center of the (u,v)-plane and its longest baselines (similar to the high-apogee Radioastron orbit)

Page 20: М ulti-frequency VLA observations of M87

U-band (color maps)

IF1 =14.6 GHz

IF2 =15.1 GHz

Page 21: М ulti-frequency VLA observations of M87

U-band (contour maps)

IF1 =14.6 GHz

IF2 =15.1 GHz

Page 22: М ulti-frequency VLA observations of M87

K-band (FreqID1, color maps)

IF1 =21.5 GHz

IF1 =21.9 GHz

Page 23: М ulti-frequency VLA observations of M87

K-band (FreqID1, contour maps)

IF1 =21.5 GHz

IF1 =21.9 GHz

Page 24: М ulti-frequency VLA observations of M87

K-band (FreqID2, color maps)IF1 =22.9 GHz

IF1 =23.3 GHz

Page 25: М ulti-frequency VLA observations of M87

K-band (FreqID2, contour maps)IF1 =22.9 GHz

IF1 =23.3 GHz

Page 26: М ulti-frequency VLA observations of M87

Multi-frequency synthesis(six-frequency analysis)

Dynamic range: 4000

Reference frequency: 19014.9 MHz

Total flux: 19.3 Jy

Page 27: М ulti-frequency VLA observations of M87

Multi-frequency analysis(six-frequency analysis)

Spectral index map

M87 core spectra