Second Public Data Release (DR2)

Release date: April 30, 2025 

Description and Executive Summary

This is the second Public Data Release (DR2), including all GOGREEN and GCLASS data.  It includes new photometric data and catalogues for one cluster, SpARCS1033. In addition some minor errors in DR1 have been fixed. A description of the changes from DR1 can be found in this document. The data structure and content is largely the same as DR1. Any use of these data should cite the published DR1 paper Balogh et al. (2021) MNRAS 500, 358.

This release includes photometry (imaging, catalogues and derived products) and spectroscopy for all systems in GOGREEN and GCLASS. We include the available, reduced HST images for all GOGREEN clusters.  The Ultravista photometric catalogues (Muzzin et al. 2013) are also included, as these are the source of photometry for the COSMOS- systems in the sample.  The SXDF catalogue of Mehta et al. (2018) must be downloaded separately, from http://homepages.spa.umn.edu/~mehta074/splash/

Finally we provide four python3 Jupyter notebooks for reading, manipulating and plotting the data.

Errata and updates

Please report problems and questions to mbalogh@uwaterloo.ca. 

Data Access

The whole data release is ~26Gb in size.  This is dominated by the images in the PHOTOMETRY/IMAGES directory.   If you don’t need access to those you can save a lot of download time.

  1. CADC (https://www.canfar.net/storage/list/GOGREEN/DR2)
  2. NSF’s NOIRLab Data Labs (link pending). At Data Lab the catalogs are also accessible through a TAP service (via SQL queries), while all survey data products (identical to what is available at CADC) are accessible through a file service (aka a “public VOSpace”). Data Lab also provides access to the survey image files through a Simple Image Access (SIA) protocol. The biggest benefit of the Data Lab platform is that you don’t have to download any data or install any software on your local computer. All data and necessary code are installed remotely on their science platform, and all you need to start working with the data is a web browser.

Acknowledgements and Citations

If you make use of these data in your research, please cite the Data Release paper,  Balogh et al. (2021).  In addition, depending on your usage:

  • The GOGREEN survey description paper, Balogh et al. (2017) , where the survey strategy, sample selection and parts of the data reduction are described in more detail.
  • The data reduction and analysis of SpARCS1033 is presented in Hewitt et al. (2025). Users that make use of data from this cluster should cite that paper as well.
  • Muzzin et al. (2012),  for more details about the GCLASS survey and data reduction
  • Research that makes significant use of the GOGREEN photometric catalogues should cite van der Burg et al. (2020) for details of data reduction and measurements. 
  • Any research that makes use of the reduced HST/WFC3 F160W imaging of the GOGREEN clusters should cite Chan et al. (2021). Research that uses the HST/WFC3 F140W imaging of the GCLASS clusters should cite Matharu et al. (2019).
  • Spectroscopy in the SXDF and COSMOS fields is coupled with photometry from the SPLASH and Ultravista surveys, respectively.  Please cite Mehta et al. (2018) and/or Muzzin et al. (2013) if you make use of these data.

Cluster Sample

This data release includes data on all GOGREEN and GCLASS clusters. From Table 1 in the Data Release Paper:

Table 1 from the DR2 paper, describing the 26 clusters in GCLASS and GOGREEN, their positions, redshifts, and information about the number of spectra and members.

Catalogues

For many applications, this is all you will need.

In directory CATS/

  • Clusters.fits : is a FITS table with information about each group or cluster in the sample.  Described in Table 4 of the DR2 paper.
  • Redshift_catalogue.fits :  This is a catalogue of all unique objects (mostly galaxies) with either GCLASS or GOGREEN spectroscopy. Includes redshifts, line indices and other information as described in Table 6 of the DR2 paper.
  • Photo.fits : Contains all sources with good photometry in all available filters, and a subset of relevant columns extracted from the photometric catalogues. Matches with the spectroscopic sample are identified. It is described in Table 5 of the Data Release paper. It is conservative in the sense that objects are excluded if they are missing data in even one filter (totmask=0 in original catalogues).

Scripts

We provide four Jupyter python3 notebooks with the data release.

  1. DR2_Notebook:  An updated version of the notebook provided with DR1. It provides examples for reading the data, displaying spectra and images, and reproducing many of the plots in the DR1 paper..
  2. build_Table3:    The notebook used to construct Photo.fits from the raw photometric and spectroscopic catalogues. This is also an updated version of the notebook provided in DR1.
  3. DR2 stats and checks: some scripts for comparing the catalogues of DR2 with those of DR1, to illustrate the additional features and corrected errors. It also includes code to compute the number of redshifts and members reported in Table 1, and the velocity dispersions in column 2 of Table 2 of the DR2 paper.
  4. Checkphotozp: Used to compare our photometry to that of PanStarrs (see DR2 paper)

Spectroscopy

If you want the 1D and 2D spectra, you will need this directory as well. This is unchanged from DR1

For each cluster there is a file called SPECTROSCOPY/OneD/CLUSTER_final.fits.  This is a multiextension FITS (MEF) file containing 1D spectra for all unique objects in CLUSTER, from GOGREEN and GCLASS. 

FITS Extension
Description
[SCI,i] for i=1,N
science data.  Absolute flux calibrated 1D spectra for each target i of N.
[VAR,i] for i=1,NCorresponding variance array.
[DQ,i] for i=1,Ndata quality array (GOGREEN spectra only).  Here this corresponds to the number of pixels extracted in each column.  So DQ=0 means no data and in general DQ<5 or so means a badly contaminated column for one reason or another.  Shouldn’t usually need to worry about this as the VAR array contains what you need
[MDF]A FITS table with information about the target.

The corresponding 2D spectra are in  SPECTROSCOPY/TwoD/CLUSTER_twod.fits.  Important notes about these:

  • These only include GOGREEN spectra.  So the dimension of the MEF does not always match that of the 1D file.  In the latter, the GCLASS spectra are appended to the GOGREEN spectra, so the entries in the 2D file should align with the first entries in the 1D.
  • No relative or absolute flux calibration has been applied to these spectra
  • The spatial dimension is in pixels, with a pixel scale of 0.16″  

Photometry

Warning: the photometry directory is large (>20Gb), mostly due to the IMAGES subdirectory.  Unless you want access to the images and the input photometric catalogues (information not contained in CATS/Photo.fits), you may not need this.

The photometry is arranged in different subdirectories.  Note there are some differences between the data formats and availability for the five GCLASS clusters that are not part of GOGREEN.  Please read the README and README.gclass documentation carefully.

The Photo.fits file provided in the CATS/ directory provides the most commonly used photometric information, for all systems, in a homogeneous way.  This is the safest way to access the data.  We provide the python script that generates this file, which would be a good starting point if you want to access other information.

IMAGES

This is the largest subdirectory.  We provide reduced images in all available filters for all SpARCS and SPT systems.

  • The GOGREEN images are resampled to 3000×3000 pixels with pixel scale 0.200″/pix in the center (~ 10′ on a side). All filters are aligned in x and y.
  • The two northern GCLASS-only images are resampled to 5000×5000 pixels with pixel scale 0.185″/pix in the center (approx 15′ on a side)
  • The three southern GCLASS-only images are resampled to 3000×3000 pixels with pixel scale 0.185″/pix in the center (approx 10′ on a side)

Note the zeropoints of the images vary, and are described in an associated file MAGZPs_cal.list. 
 

HST images

These are treated differently and are available in a separate subdirectory (12Gb).  Reduced images only are provided.  See the data release paper and Chan et al. (2021) for a description.

PHOTOM_CATS

Ks-band selected catalogs, where each detected object is required to have 5 adjacent pixels with at least 1.5 sigma in the original (unconvolved) Ks-band image. All flux values have an AB magnitude zeropoint of 25 (equivalent to a flux scale of 0.3631 uJy per count). Therefore m_filter = -2.5*log10(flux_filter) + 25.

The column totmask is a conservative mask, equal to zero only if good photometric data is available in all filters. Otherwise it is set to 1, and not include in the compilation catalogue Photo.fits. Many of these data will still be useful, to those who don’t require access to all filters.

The five GCLASS-only clusters have a slightly different structure to the catalogue.  See the README.gclass file provided with the data for details.

PHOTOZ_CATS

ID-matched to the main photometric catalogue.
photoz-cats using EAZY code. (extension .zout)
id – same identifier as PHOTOM_CAT
z_peak – probably best estimate for photo-z

A quadratic function is fit to z_peak(z_spec) for the GOGREEN clusters. This correction has been applied to the redshifts in *_zphot.dat files.

RESTFRAME_COLOURS

For the GOGREEN clusters we provide SDSS, FUV, NUV, U, B, V, J rest-frame colours estimated with EAZY.  For each source, two different set of rest-frame colours are estimated:

  • The first set assumes the cluster mean redshift for each source.
  • The second set is based on the individually-measured spectroscopic redshifts, or, if there is no spec-z measured, the peak of the posterior P(z).
  • Offsets to U-V and V-J colours have been applied to make the quiescent loci match those of UltraVISTA.  Corrections are in UVJcorrections.dat

The five GCLASS-only clusters have only U-V and V-J colours provided, in a differently formatted file.

SPECZ_MATCHED

ID-matched to the main photometric catalogue. Simple shifts are applied to bring the spectroscopic catalogue to the same astrometric reference as photometric catalogue prior to matching. Matching was done within 1.0”, with priority:

  1. GOGREEN
  2. GCLASS
  3. SPT
  4. FORS2 (SpARCS-0335)
  5. VIPERS
  6. PRIMUS
  7. SDSS
  8. NED general search for spectroscopic redshifts

When there are two (or more) matches to spectroscopic catalogues, the second match is also reported (following the same priority list). To help cross-matching with GOGREEN spectra, the spectroscopic GOGREEN ID is reported in the last column.

STELMASS_CATS

ID-matched to the main photometric catalogue.
Stellar masses and other SED-fitting parameters from FAST. There are two versions:

*Ks.fout takes the z_peak from the photo-z catalogue, or the spectroscopic redshift when available.
*Ks_fixz.fout fixes the redshift of all objects to the cluster mean redshift. This may come in handy when performing a statistical background subtraction.

All relevant parameters for the grid of template models are listed in the header of the files.
 

BESTFIT_SEDs

Best-fitting SED models to the photometry based on the BC03 library and the best spectroscopic redshift for each source.  Includes the aperture correction to MAG_AUTO. These are not available for SpARCS1033.

COLORIMS

RGB colour images of the clusters (except SpARCS1033), constructed from B, I and Ks images.   
Spectroscopic targets are indicated, using a very simple division between green (within 0.01 of mean cluster redshift) and red (rest).
 

COSMOS

We provide the DR1 Ultravista catalogue v4.1  here, for convenience.  We use this as the source of photometry for the relevant GOGREEN systems.

The catalogue was obtained from https://www.strw.leidenuniv.nl/galaxyevolution/ULTRAVISTA/Ultravista/UltraVISTA_Catalog_Home.html

If you use this catalog in your research directly, or if you use the photometric information associated with the COSMOS groups or field sample in GOGREEN, please acknowledge it by citing the catalog paper, Muzzin et al. (2013), ApJS, 206, 8.

SXDF

We use the SPLASH v1.6 catalogue as the source of photometry for the GOGREEN systems in the SXDF field.  The catalogue can be obtained from http://splash.caltech.edu/public/catalogs.html#sxds

If you use this catalog in your research directly, or if you use the photometric information associated with the SXDF groups or field sample in GOGREEN, please acknowledge it by citing the catalog paper, Mehta et al. (2018).

In this directory we provide a .csv file with a subset of columns and restframe UVJ colours computed consistently with the rest of our sample.