Data

Spectra and Polarisation In Cutouts of Extragalactic sources from RACS First Data Release (SPICE-RACS-DR1)

Commonwealth Scientific and Industrial Research Organisation
Thomson, Alec ; McConnell, David ; Lenc, Emil ; Galvin, Tim ; Rudnick, Lawrence ; Heald, George ; Hale, Catherine Laura ; Duchesne, Stefan ; Anderson, Craig ; Carretti, Ettore ; Federrath, Christoph ; Gaensler, Bryan ; Harvey-Smith, Lisa ; Haverkorn, Marijke ; Hotan, Aidan ; Ma, Jackie ; Murphy, Tara ; Mcclure-Griffiths, Naomi ; Moss, Vanessa ; O'Sullivan, Shane ; Raja, Wasim ; Seta, Amit ; Van Eck, Cameron ; West, Jennifer ; Whiting, Matthew ; Wieringa, Mark ; Huynh, Minh
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ctx_ver=Z39.88-2004&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Adc&rfr_id=info%3Asid%2FANDS&rft_id=info:doi10.25919/w37t-nw98&rft.title=Spectra and Polarisation In Cutouts of Extragalactic sources from RACS First Data Release (SPICE-RACS-DR1)&rft.identifier=https://doi.org/10.25919/w37t-nw98&rft.publisher=Commonwealth Scientific and Industrial Research Organisation&rft.description=*NOTICE* July 2024: We have discovered an error in the flux density of Stokes Q and U in this data release. Full details are provided in a corrigendum in PASA (see link below). If you are reading this notice the catalogue, spectra and images in this collection have been corrected. The data in the linked 'full' DAP collection are also corrected. Users of the old data can apply their own correction by multiplying Stokes Q and U by 2 for correct results. However, we recommend using the updated products provided here. Users can confirm they are using updated files by inspecting the HISTORY card in the FITS headers.\n\nSpectra and Polarisation In Cutouts of Extragalactic sources from RACS (SPICE-RACS) is a project to derive an all-Southern-sky, linear polarisation map from the Rapid ASKAP Continuum Survey (RACS). Through this project, we will derive the following products: \n- Cutout image cubes in Stokes I, Q, and U around every source detected in total intensity as a function of frequency\n- Polarisation spectra as a function of frequency and Faraday depth for every component detected in total intensity\n- A catalogue summarising the polarisation properties, including rotation measure (RM), for every component.\n\nThis collection represents a subset of the data presented in SPICE-RACS-DR1 (Thomson et al. 2023). This subset refers to the 24680 components ('cut') (out of the 'full' 105912) for which a reliable polynomial fit could be derived for the Stokes I spectra that were extracted. This collection contains the 'cut' subset, please see the linked collections for the 'full' data.\n\nOur final data products are as follows:\n\nspice-racs.dr1.corrected.{cut,full}.xml:\n\n- Our component catalogue in VOTable format for the first (cut) and second (full) sets of components described above. The former is included with this deposit.\n\n{source_id}.cutout.{image,weights}.*.fits:\n\n- Image and weights cube cutout in Stokes I, Q, and U cutout around a RACS-low source identified by ‘source_id’. The data dimensions are J2000 right ascension and declination, Stokes parameter, and frequency.\n\n{cat_id}_polspec.fits:\n\n- Polarisation spectra extracted on the position of the RACS-low component identified by ‘cat_id’ in POLSPECTRA format. Each table contains a single row, corresponding to the component.\n\nspice_racs_dr1_polspec_{cut,full}.tar:\n- A tarball containing all of the POLSPECTRA for the 'cut' and second 'full' sets of components described above. These are available in the linked collections.\n\nRecommended catalogue subsets:\nOur 'full' catalogue contains extracted polarisation data for all 105912 Stokes I components detected in our DR1 region. It is important to note that the majority of these do not have reliably detected polarised emission. When using this catalogue please use the provided flags, and uncertainty/quality metrics to derive a subset suitable for your science goals. If you're unsure where to start, these are our recommended basic subsets:\n\n- 'goodI' : Where our Stokes I model is reliable -- channel_flag and stokesI_fit_flag are False (this produces the 'cut' catalogue from the 'full').\n- 'goodL': Where we have a reliable detection of polarised signal, but not necessarily a reliable RM -- goodI plus leakage_flag is False and snr_polint >= 5.\n- 'goodRM': Where the RM is reliable -- goodL plus snr_flag is False.\nLineage: 8576,8577,8584,8585,8589,8590,8593,8594,8674,8675,12422,12423,12426,12428,12429,12455,12494,12496,12497,12500,12509,13591,13595,13615,13671,13672,13673,13678,13708,13746,13747,13749&rft.creator=Thomson, Alec &rft.creator=McConnell, David &rft.creator=Lenc, Emil &rft.creator=Galvin, Tim &rft.creator=Rudnick, Lawrence &rft.creator=Heald, George &rft.creator=Hale, Catherine Laura &rft.creator=Duchesne, Stefan &rft.creator=Anderson, Craig &rft.creator=Carretti, Ettore &rft.creator=Federrath, Christoph &rft.creator=Gaensler, Bryan &rft.creator=Harvey-Smith, Lisa &rft.creator=Haverkorn, Marijke &rft.creator=Hotan, Aidan &rft.creator=Ma, Jackie &rft.creator=Murphy, Tara &rft.creator=Mcclure-Griffiths, Naomi &rft.creator=Moss, Vanessa &rft.creator=O'Sullivan, Shane &rft.creator=Raja, Wasim &rft.creator=Seta, Amit &rft.creator=Van Eck, Cameron &rft.creator=West, Jennifer &rft.creator=Whiting, Matthew &rft.creator=Wieringa, Mark &rft.creator=Huynh, Minh &rft.date=2024&rft.edition=v6&rft.relation=https://doi.org/10.1017/pasa.2023.38&rft.relation=https://doi.org/10.1017/pasa.2024.34&rft.relation=https://doi.org/10.1017/pasa.2020.41&rft.relation=https://doi.org/10.1017/pasa.2021.47&rft_rights=Creative Commons Attribution 4.0 International Licence https://creativecommons.org/licenses/by/4.0/&rft_rights=Data is accessible online and may be reused in accordance with licence conditions&rft_rights=All Rights (including copyright) CSIRO 2023.&rft_subject=racs&rft_subject=racs-low&rft_subject=spice-racs&rft_subject=askap&rft_subject=polarisation&rft_subject=radio&rft_subject=Cosmology and extragalactic astronomy&rft_subject=Astronomical sciences&rft_subject=PHYSICAL SCIENCES&rft_subject=Astronomical sciences not elsewhere classified&rft.type=dataset&rft.language=English Access the data

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Creative Commons Attribution 4.0 International Licence
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Data is accessible online and may be reused in accordance with licence conditions

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Brief description

*NOTICE* July 2024: We have discovered an error in the flux density of Stokes Q and U in this data release. Full details are provided in a corrigendum in PASA (see link below). If you are reading this notice the catalogue, spectra and images in this collection have been corrected. The data in the linked 'full' DAP collection are also corrected. Users of the old data can apply their own correction by multiplying Stokes Q and U by 2 for correct results. However, we recommend using the updated products provided here. Users can confirm they are using updated files by inspecting the HISTORY card in the FITS headers.

Spectra and Polarisation In Cutouts of Extragalactic sources from RACS (SPICE-RACS) is a project to derive an all-Southern-sky, linear polarisation map from the Rapid ASKAP Continuum Survey (RACS). Through this project, we will derive the following products:
- Cutout image cubes in Stokes I, Q, and U around every source detected in total intensity as a function of frequency
- Polarisation spectra as a function of frequency and Faraday depth for every component detected in total intensity
- A catalogue summarising the polarisation properties, including rotation measure (RM), for every component.

This collection represents a subset of the data presented in SPICE-RACS-DR1 (Thomson et al. 2023). This subset refers to the 24680 components ('cut') (out of the 'full' 105912) for which a reliable polynomial fit could be derived for the Stokes I spectra that were extracted. This collection contains the 'cut' subset, please see the linked collections for the 'full' data.

Our final data products are as follows:

spice-racs.dr1.corrected.{cut,full}.xml:

- Our component catalogue in VOTable format for the first (cut) and second (full) sets of components described above. The former is included with this deposit.

{source_id}.cutout.{image,weights}.*.fits:

- Image and weights cube cutout in Stokes I, Q, and U cutout around a RACS-low source identified by ‘source_id’. The data dimensions are J2000 right ascension and declination, Stokes parameter, and frequency.

{cat_id}_polspec.fits:

- Polarisation spectra extracted on the position of the RACS-low component identified by ‘cat_id’ in POLSPECTRA format. Each table contains a single row, corresponding to the component.

spice_racs_dr1_polspec_{cut,full}.tar:
- A tarball containing all of the POLSPECTRA for the 'cut' and second 'full' sets of components described above. These are available in the linked collections.

Recommended catalogue subsets:
Our 'full' catalogue contains extracted polarisation data for all 105912 Stokes I components detected in our DR1 region. It is important to note that the majority of these do not have reliably detected polarised emission. When using this catalogue please use the provided flags, and uncertainty/quality metrics to derive a subset suitable for your science goals. If you're unsure where to start, these are our recommended basic subsets:

- 'goodI' : Where our Stokes I model is reliable -- channel_flag and stokesI_fit_flag are False (this produces the 'cut' catalogue from the 'full').
- 'goodL': Where we have a reliable detection of polarised signal, but not necessarily a reliable RM -- goodI plus leakage_flag is False and snr_polint >= 5.
- 'goodRM': Where the RM is reliable -- goodL plus snr_flag is False.
Lineage: 8576,8577,8584,8585,8589,8590,8593,8594,8674,8675,12422,12423,12426,12428,12429,12455,12494,12496,12497,12500,12509,13591,13595,13615,13671,13672,13673,13678,13708,13746,13747,13749

Available: 2024-07-12

Data time period: 2019-04-25 to 2020-05-02

This dataset is part of a larger collection

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