VLA Observational Status Summary 2014B

VLA capabilities September 2014 - January 2015

APIwind_October.png

APIwind_September.png

Lband_sweep.png

Lband_sweep_small.png

Figure 3

RcvrAvailDec12.png

RcvrAvailDec12_small.png

Figure 1

S-bandRFI.png

S-bandRFI_small.png

Figure 4

Pulsar Observing

While the WIDAR correlator will eventually allow flexible pulsar phase-binning and real-time correction for dispersion, those aspects of the correlator have not yet been commissioned.  Similarly the use of the phased array for high time-resolution observations is not yet possible for general use.

corr-cfg-fig:3bit_4x16x128MHz

Correlator configuration figure: 3bit_4x16x128MHz.png

corr-cfg-fig:8bit_1x16x128MHz

Correlator configuration figure: 8bit_1x16x128MHz.png

corr-cfg-fig:8bit_2x1x128MHz

Correlator configuration figure: 8bit_2x1x128MHz.png

corr-cfg-fig:8bit_2x8x128MHz

VLA OSS correlator configuration figure: 8bit_2x8x128MHz.png

corr-cfg-fig:8bit_2x8x128MHz

Correlator configuration figure: 8bit_2x8x128MHz.png

corr-cfg-fig:8bit_ac1+12_bd16

Correlator configuration figure: 8bit_ac1+12_bd16.png

corr-cfg-fig:8bit_ac1+12_bd16a

Correlator configuration figure: 8bit_ac1+12_bd16a.png

corr-cfg-fig:8bit_ac1+14_bd14

Correlator configuration figure: 8bit_ac1+14_bd14.png

corr-cfg-fig:8bit_ac1+14_bd16

Correlator configuration figure: 8bit_ac1+14_bd16.png

corr-cfg-fig:8bit_ac1+15_bd15

Correlator configuration figure: 8bit_ac1+15_bd15.png

Connect with NRAO

The NSF National Radio Astronomy Observatory and NSF Green Bank Observatory are facilities of the U.S. National Science Foundation operated under cooperative agreement by Associated Universities, Inc.