Spectralindex
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This page documents the spectralindex function of Python module analysisUtils.
This function is designed to fit a power-law spectral index to the results output from casa's fluxscale task (using scipy.optimize.leastsq). Currently, it also requires the output from the listobs task to determine the center frequencies of each spectral window. (To simplify the usage in the future, we have submitted an improvement request for fluxscale to also print these frequencies.) It runs a brief Monte-Carlo series of fits to determine the uncertainty on the fitted slope on the basis of the error bars on each flux density. Finally, it produces a plot. Note: spectralIndex is a synonym for spectralindex.
Usage:
spectralindex(filename, yfilename, source=, verbose=False, maxpoints=0, trials=2000, spw=, help=False)
filename: contains a listobs output file yfilename: contains a fluxscale output file source: sourcename to choose from the (possibly) multi-source fluxscale file maxpoints: the maximum number of spws to select for the fit (0=no max) trials: number of Monte-Carlo fits to run to estimate the fit uncertainties spw: the spws to use, e.g. ' '=all, '1~3,5,6~8'=[1,2,3,5,6,7,8]
Examples
# In CASA
au.linfit().spectralIndex('listobs.txt','fluxscale_d2_new.txt','J19')
Read 16 x values for J1924-2914 (avg=44125.000)
Read 16 y values for J1924-2914 (avg=13.359)
Completed 2000 Monte-Carlo error trials to estimate the standard deviation of the fitted parameters.
Error-weighted fit: Slope: -0.503+-0.088 Flux D. @ 42802.00MHz: 13.563+-2.569
Un-weighted fit: Slope: -0.498 Flux D. @ 42802.00MHz: 13.561
Plot saved in fluxscale_d2_new.txt.J1924-2914.png
File formats
The listobs file should look like this. It is keying off the string "TOPO", so there can be any number of leading comment characters on each line, and any number of unrelated lines of text at the top.
SpwID #Chans Frame Ch1(MHz) ChanWid(kHz) TotBW(kHz) Corrs 0 128 TOPO 42738 1000 128000 RR LL 1 128 TOPO 42866 1000 128000 RR LL 2 128 TOPO 42994 1000 128000 RR LL 3 128 TOPO 43122 1000 128000 RR LL 4 128 TOPO 43250 1000 128000 RR LL 5 128 TOPO 43378 1000 128000 RR LL 6 128 TOPO 43506 1000 128000 RR LL 7 128 TOPO 43634 1000 128000 RR LL 8 128 TOPO 44488 1000 128000 RR LL 9 128 TOPO 44616 1000 128000 RR LL 10 128 TOPO 44744 1000 128000 RR LL 11 128 TOPO 44872 1000 128000 RR LL 12 128 TOPO 45000 1000 128000 RR LL 13 128 TOPO 45128 1000 128000 RR LL 14 128 TOPO 45256 1000 128000 RR LL 15 128 TOPO 45384 1000 128000 RR LL
Similarly, the fluxscale file should look like this. It can contain the results for multiple sources. It is keying off of the string 'SpW', so there can be any number of leading comment characters on each line, and any number of unrelated lines of text at the top.
# Opening MS: 10C186_B_Q_d1_3s.ms for calibration. # Found reference field(s): J1331+3030 # Found transfer field(s): J1717-3342 J1924-2914 # Flux density for J1717 3342 in SpW=0 is: 2.33891 ± 0.0620232 (SNR = 37.7102, N= 44) # Flux density for J1717-3342 in SpW=1 is: 2.33168 ± 0.0608224 (SNR = 38.3358, N= 44) # Flux density for J1717-3342 in SpW=2 is: 2.33139 ± 0.0642111 (SNR = 36.3082, N= 44) # Flux density for J1717-3342 in SpW=3 is: 2.33639 ± 0.0697579 (SNR = 33.4929, N= 44) # Flux density for J1717-3342 in SpW=4 is: 2.31025 ± 0.0631668 (SNR = 36.5738, N= 44) # Flux density for J1717-3342 in SpW=5 is: 2.32929 ± 0.0667446 (SNR = 34.8986, N= 44) # Flux density for J1717-3342 in SpW=6 is: 2.35698 ± 0.0698231 (SNR = 33.7564, N= 44) # Flux density for J1717-3342 in SpW=7 is: 2.32728 ± 0.0668059 (SNR = 34.8364, N= 44) # Flux density for J1717-3342 in SpW=8 is: 2.23395 ± 0.0394774 (SNR = 56.588, N= 46) # Flux density for J1717-3342 in SpW=9 is: 2.23898 ± 0.0404523 (SNR = 55.3487, N= 46) # Flux density for J1717-3342 in SpW=10 is: 2.20212 ± 0.0408321 (SNR = 53.9311, N= 46) # Flux density for J1717-3342 in SpW=11 is: 2.18275 ± 0.0392774 (SNR = 55.5727, N= 46) # Flux density for J1717-3342 in SpW=12 is: 2.17859 ± 0.0388576 (SNR = 56.0659, N= 46) # Flux density for J1717-3342 in SpW=13 is: 2.16182 ± 0.0405544 (SNR = 53.3066, N= 46) # Flux density for J1717-3342 in SpW=14 is: 2.16303 ± 0.0413542 (SNR = 52.305, N= 46) # Flux density for J1717-3342 in SpW=15 is: 2.19681 ± 0.0400311 (SNR = 54.8777, N= 46) # Flux density for J1924-2914 in SpW=0 is: 14.6731 ± 0.138529 (SNR = 105.921, N= 44) # Flux density for J1924-2914 in SpW=1 is: 14.5996 ± 0.136761 (SNR = 106.753, N= 44) # Flux density for J1924-2914 in SpW=2 is: 14.6242 ± 0.146673 (SNR = 99.7061, N= 44) # Flux density for J1924-2914 in SpW=3 is: 14.6802 ± 0.158394 (SNR = 92.6816, N= 44) # Flux density for J1924-2914 in SpW=4 is: 14.5259 ± 0.141069 (SNR = 102.97, N= 44) # Flux density for J1924-2914 in SpW=5 is: 14.6075 ± 0.151812 (SNR = 96.2206, N= 44) # Flux density for J1924-2914 in SpW=6 is: 14.7261 ± 0.157892 (SNR = 93.2666, N= 44) # Flux density for J1924-2914 in SpW=7 is: 14.5783 ± 0.14938 (SNR = 97.5919, N= 44) # Flux density for J1924-2914 in SpW=8 is: 13.9264 ± 0.0748849 (SNR = 185.971, N= 46) # Flux density for J1924-2914 in SpW=9 is: 13.9368 ± 0.0751502 (SNR = 185.452, N= 46) # Flux density for J1924-2914 in SpW=10 is: 13.7826 ± 0.0785357 (SNR = 175.494, N= 46) # Flux density for J1924-2914 in SpW=11 is: 13.7178 ± 0.0778214 (SNR = 176.273, N= 46) # Flux density for J1924-2914 in SpW=12 is: 13.6833 ± 0.0748109 (SNR = 182.905, N= 46) # Flux density for J1924-2914 in SpW=13 is: 13.6308 ± 0.0772038 (SNR = 176.555, N= 46) # Flux density for J1924-2914 in SpW=14 is: 13.6372 ± 0.0792322 (SNR = 172.117, N= 46) # Flux density for J1924-2914 in SpW=15 is: 13.7463 ± 0.0735882 (SNR = 186.8, N= 46)
