0345+7252 Scan 4290

Contents

Observing log information

  Object:           0345+7252
  On scan num:      4290 4292 4294 4296 4298 4300
  Off scan num:     4291 4293 4295 4297 4299 4301
  R.A.:             3.843480 hrs
  Dec.:             73.030909 deg
  On azimuth:       357.435652 deg
  On zenith dist.:  34.603926 deg
  Off azimuth:      357.463500 deg
  Off zenith dist.: 34.601670 deg
  MJD:              52533
  UTC:              0.407581
  Center freq.:     1400.351045 MHz
  Doppler:          0.00006117
  Num. correlators: 2
  Spectrom. atten.: 35 42 dB
  Bandwidth:        10.0 MHz
  Num. channels:    1024
  Eff. integration: 1800 seconds

Raw spectrum

This spectrum is the integration of all data for the scan with spectra from both polarizations added together. The spectral intensities are Ssys * (on - off) / off, where Ssys is the system temperature in Jy. The system noise flux density equivalent is calibrated for each scan with a calibration noise source firing during each scan. The cal value, in Jy, is calibrated by comparison with a number of continuum sources as described in the summary web page

Figure 1. Unedited spectrum

Measured spectrum

This is the section of spectrum measured to obtain the parameters listed below. The three horizontal dotted lines are the baseline, the peak level selected, and 20% of the peak level. The two vertical dotted lines mark the selected 20% line width edges. The solid horizontal line marks the velocity range chosen for the the line profile flux density integral. This spectrum has a second-order least squares fit baseline removed using most of the baseline shown in Figure 1.

Figure 2. Measured spectrum

Measured parameters

  Peak intensity:      0.012 Jy
  Lower 20% velocity: 4129.5 km/s
  Upper 20% velocity: 4570.1 km/s
   Systemic velocity: 4349.8 km/s
   Line width (20%):   440.6 km/s
  Profile integral:    4.89 Jy * km/s
                 A:    3.84
                 B:    4.72
         Ratio B/A:   1.228
  Flux integral
     velocity range:  4085.0 - 4591.9 km/s

Comments