test collection

New SEFD LSCX

New SEFDs

VLA Observational Status Summary 2020A

VLA capabilities February 2020 - October 2020

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3bit_4x16x128MHz.png

VLA OSS correlator configuration figure: 3bit_4x16x128MHz.png

APIwind_April.png

APIwind_August.png

APIwind_December.png

APIwind_February.png

APIwind_January.png

APIwind_June.png

APIwind_March.png

APIwind_May.png

APIwind_November.png

APIwind_October.png

APIwind_September.png

Lband_sweep.png

Lband_sweep_small.png

Figure 3

P-band SEFD Small

RcvrAvailDec12.png

RcvrAvailDec12_small.png

Figure 1

S-bandRFI.png

S-bandRFI_small.png

Figure 4

SEFD_small.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

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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