test collection

2025.jpg

casa_cont_imaging_pipescript_666.py

text/x-python casa_cont_imaging_pipescript_666.py — 1 KB

File contents

# This CASA pipescript is meant for use with CASA 6.6.6 and pipeline 2025.1.0.32
context = h_init()
context.set_state('ProjectSummary', 'observatory', 'Karl G. Jansky Very Large Array')
context.set_state('ProjectSummary', 'telescope', 'EVLA')
try:
    hifv_importdata(vis=['myCaldMS.ms'], datacolumns={'data': 'raw','corrected': 'regcal_contline_all'})
    hifv_flagtargetsdata()
    hifv_mstransform()
    hif_checkproductsize(maximsize=16384)
    hif_makeimlist(specmode='cont', datatype='regcal')
    hif_makeimages(hm_cyclefactor=3.0)
    hif_selfcal()
    hif_makeimlist(specmode='cont', datatype='selfcal')
    hif_makeimages(hm_cyclefactor=3.0)    
    hifv_exportdata(imaging_products_only=True)
finally:
    h_save()

VLA Observational Status Summary 2016A

VLA capabilities February 2016 - October 2016

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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

RcvrAvailDec12.png

RcvrAvailDec12_small.png

Figure 1

S-bandRFI.png

S-bandRFI_small.png

Figure 4

SEFD_small.png

Performance of the VLA during the Next Semester

There are currently no items in this folder.

Complex Gain Calibration

There are currently no items in this folder.

The WIDAR Correlator

There are currently no items in this folder.

VLA Observational Status Summary 2016B

VLA capabilities September 2016 - January 2017

There are currently no items in this folder.

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.

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.

The U.S. National Science Foundation (U.S. NSF) is an independent federal agency created by Congress in 1950 "to promote the progress of science; to advance the national health, prosperity, and welfare; to secure the national defense..."

AUI collaborates with the scientific community and research sponsors to plan, build, and operate cutting-edge facilities. We cultivate excellence, deliver value, enhance education, and engage the public.