Introduction

Check the survey web page: https://greenbankobservatory.org/science/gbt-surveys/drift-scan-survey-for-pulsars-frbs-radio-transients-and-gas-in-galaxies/

Observations

  • Configure.
  • Balance.
  • Track with no noise diode for an hour.
  • Track with noise diode for 20 seconds.
  • Repeat the above.

AGBT22B_234

  • Spectral windows 187.5 MHz wide.
  • 32768 channels.
  • Bank B: 1500 MHz
  • Bank C: 1665 MHz
  • Bank D: 1160 MHz
  • Bank E: 1370 MHz
  • Data in the topocentric velocity frame.
  • Used VEGAS.
  • There are 12 sessions for this project code (01 to 12).

AGBT21B_332

  • There are 14 sessions for this project code in the archive (01 to 14).

AGBT21A_352

  • There are 7 sessions for this project code in the archive (01 to 07).

AGBT19A_374

AGBT19A_474

  • There are 33 sessions for this project code in the archive (01 to 33).

AGBT18A_478

  • There are 33 sessions for this project code in the archive (01 to 33).

Data reduction

References

HI surveys

Python tutorials

Calibrated Data

* VEGAS Bank E, AGBT22B_234: Polarization 0 (YY) - Sessions 02 (25 scans), 03 (25 scans), 04 (25 scans), 05 (25 scans), 06 (45 scans), ; Polarization 1 (XX) - Sessions 02 (25 scans), 03 (25 scans), 04 (25 scans), 05 (25 scans). ; Merged (both pol) - 02,

-- PedroSalas - 2023-06-01
Topic revision: r14 - 2023-07-25, PedroSalas
This site is powered by FoswikiCopyright © by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding NRAO Public Wiki? Send feedback