Information on resource 'Apertif DR-2'
Services defined within this resource descriptor
- Apertif DR-2
This datalink service gives all data products related to the selected
continuum image.
- Apertif DR-2
This datalink service gives all data products related to the selected
polarization cube.
- Apertif DR-2
This datalink service gives all data products related to the selected
spectral cube.
- Apertif DR2 - Continuum images
Apertif is a phased-array feed system for the Westerbork Synthesis
Radio Telescope (WSRT), providing forty instantaneous beams over 300
MHz of bandwidth. A description of the second data release is to be
included here. This service queries the continuum images from the
second data release of Apertif. Multi-frequency synthesis (mfs) Stokes
I images are produced over the full frequency range (1292.5– 1430 MHz)
and saved as fits files for each beam. The size of the continuum
images is 3.4 deg × 3.4 deg (3073 × 3073 pixels, with 4''/pixel). The
median noise in the continuum images is 41.4 uJy/beam and the median
angular resolution is 11.6''/sin(declination). A companion VO table
provides a continuum source catalog based on all continuum images
contained in this data release and is described in Kutkin et al.
(2022) (see
https://vo.astron.nl/apertif_dr2/q/apertif_dr2_catalogue/form).
- Apertif DR2 - Field calibrated visibilities
Apertif is a phased-array feed system for the Westerbork Synthesis
Radio Telescope (WSRT), providing forty instantaneous beams over 300
MHz of bandwidth. A description of the second data release is to be
included here. This service queries the calibrated visibility
measurement sets. The calibrated visibility data, with
cross-calibration and self-calibration solutions applied, are
currently stored as an intermediate data product at full time and
spectral resolution. These are stored on tape with the raw data and
are not immediately available for download. The data release
documentation should be consulted for up-to-date information on how to
access the data.
- Apertif DR2 - Field raw visibilities
Apertif is a phased-array feed system for the Westerbork Synthesis
Radio Telescope (WSRT), providing forty instantaneous beams over 300
MHz of bandwidth. A description of the second data release is to be
included here. The raw visibility data are provided as separate
collections for the survey fields, flux calibrator and polarization
calibrator observations. The tables can be joined to identify the
associated calibrators for a target observation. This service queries
the raw visibilities for the survey fields. These are stored on tape
and are not immediately available for download. The data release
documentation should be consulted for up-to-date information on how to
access the data.
- Apertif DR2 - Flux calibrator raw visibilities
Apertif is a phased-array feed system for the Westerbork Synthesis
Radio Telescope (WSRT), providing forty instantaneous beams over 300
MHz of bandwidth. A description of the second data release is to be
included here. The raw visibility data are provided as separate
collections for the survey fields, flux calibrator and polarization
calibrator observations. The tables can be joined to identify the
associated calibrators for a target observation. This service queries
the raw visibilities for the flux calibrator. These are stored on tape
and are not immediately available for download. The data release
documentation should be consulted for up-to-date information on how to
access the data.
- Apertif DR2 - HI spectral cubes
Apertif is a phased-array feed system for the Westerbork Synthesis
Radio Telescope (WSRT), providing forty instantaneous beams over 300
MHz of bandwidth. A description of the second data release is to be
included here. This service queries the spectral line cubes from the
second data release of Apertif. Four line cubes are produced over a
set of different frequency ranges as follows. Cube 0: 1292.5–1337.1
MHz, Cube 1: 1333.1–1377.7 MHz, Cube 2: 1373.8–1418.4 MHz, Cube 3:
1414.5–1429.3 MHz. Cube 3 is produced at full spectral resolution of
12.2 kHz while other cubes are produced with a 3-channel averaging at
36.6 kHz resolution. The cubes have a spatial extent of 1.1 deg × 1.1
deg (661 × 661 pixels, with 6''/pixel). The median noise for all line
cubes, with a spectral resolution of 36.6 kHz, is 1.6 mJy/beam,
corresponding to a 3-σ H I column density sensitivity of 1.8 × 10^20
atoms cm^−2 over 20 km s^−1 (for a median angular resolution of 24″ ×
15″). The corresponding dirty beam cubes are also released to allow
offline cleaning of source emission.
- Apertif DR2 - Polarization calibrator raw visibilities
Apertif is a phased-array feed system for the Westerbork Synthesis
Radio Telescope (WSRT), providing forty instantaneous beams over 300
MHz of bandwidth. A description of the second data release is to be
included here. The raw visibility data are provided as separate
collections for the survey fields, flux calibrator and polarization
calibrator observations. The tables can be joined to identify the
associated calibrators for a target observation. This service queries
the raw visibilities for the polarization calibrator. These are stored
on tape and are not immediately available for download. The data
release documentation should be consulted for up-to-date information
on how to access the data.
- Apertif DR2 - Polarization cubes
Apertif is a phased-array feed system for the Westerbork Synthesis
Radio Telescope (WSRT), providing forty instantaneous beams over 300
MHz of bandwidth. A description of the second data release is to be
included here. This service queries the polarization cubes from the
second data release of Apertif. In order to prevent bandwidth
depolarization and enable rotation measure synthesis studies, Stokes Q
and U cubes with a frequency resolution of 6.25 MHz are produced. The
cubes have a smaller spatial extent of 2.7 deg × 2.7 deg (2049 × 2049
pixels, with 4''/pixel ) than the continuum or Stokes V images but
still extend well beyond the primary beam.
- Visibilitiy access link
Tables defined within this resource descriptor
Copyright, License, Acknowledgements
If you use this data, cite Adams et al. 2022 (2022A&A...667A..38A). Additionally, you can cite the service reference. The Apertif data release 2 is licensed under the Creative Commons Attribution 3.0 License
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