VLA Observational Status Summary 2014A

VLA capabilities February 2014 - September 2014

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

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:sro1_8bit_ac40+3+17_bd1+3

Correlator configuration figure: sro1_8bit_ac40+3+17_bd1+3.png

corr-cfg-fig:sro2_8bit_ac17+9_bd3+35

Correlator configuration figure: sro2_8bit_ac17+9_bd3+35.png

corr-cfg-tab:sbBWspecRes

Correlator configuration table: table_sbBWspecRes.png

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+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

Connect with NRAO

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Founded in 1956, the NSF NRAO provides state-of-the-art radio telescope facilities for use by the international scientific community. NSF NRAO telescopes are open to all astronomers regardless of institutional or national affiliation. Observing time on NSF NRAO telescopes is available on a competitive basis to qualified scientists after evaluation of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time. NSF NRAO also provides both formal and informal programs in education and public outreach for teachers, students, the general public, and the media.

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