Published August 31, 2026 | Version 31 August 2026

The Spitzer Spectroscopic Data Fusion - Merged Spectroscopic Redshift Catalogs in Spitzer Fields

Authors/Creators

  • 1. University of Cape Town

Description

The Spitzer Spectroscopic Data Fusion merges miscellaneous spectroscopic information available within "popular" extragalactic survey fields.

Last Updated on 31 August 2026 - https://doi.org/10.5281/zenodo.6368347 - https://www.mattiavaccari.net/df/specz

Vaccari 2026 - https://scixplorer.org/abs/2026RNAAS..10..118V/abstract

Based on the Spitzer Data Fusion Project - https://doi.org/10.5281/zenodo.6120913 - https://www.mattiavaccari.net/df

Vaccari 2026 - https://scixplorer.org/abs/2026RNAAS..10..276V/abstract

Vaccari 2015 - https://scixplorer.org/abs/2015fers.confE..27V/abstract

Merged Spec-Z ("specz-merged") catalogs merge miscellaneous spec-z information available
within a given field. Different spec-z catalogs available within a given field are merged
(using a search radius of 1.0 arcsec), and for sources with multiple spec-z measurements
the most reliable one is chosen following the assumed order of decreasing reliability
indicated below for each field.  Since the 31 August 2026 release this order is no longer
arbitrary: large, homogeneous, high-resolution surveys come first, heterogeneous compilations
last, and NED is always the LAST catalogue in every field so that it contributes its unique
redshifts without ever overriding a dedicated survey. If CAT1,...,CATN spec-z catalogs are
available in a given field, Z_1 from CAT1 is adopted as "best" redshift (i.e. ZBEST),
if available, otherwise Z_2 from CAT_2 is adopted if available, and so on up to Z_N and CAT_N.
In using ZBEST it's thus important to bear in mind that this is not necessarily / actually
THE "best" redshift for science purposes. However, Z_1,...,Z_N are included to allow user
to define the "best" redshift based on their science needs when multiple redshift estimates
are available for a given source.

ZFLAG specifies which catalog is providing the ZBEST value according to the CATN number below.

ZCLASS is meant to provide further info about the class/quality of the spectroscopic redshift
measurement, but for the time being is not populated and is simply a copy of ZFLAG.

ZWHERE is an additional binary/bit flag indicating in which of the N catalogs each source
was given a spec-z estimate in. ZWHERE will e.g. be 2^0=1 if a redshift if available *only*
from CAT_1, whereas it will be 2^0+2^1=3 if a redshift is available *only* from CAT1 and CAT2,
so that a source with a redshift available from all N catalogues will have ZWHERE=2^0+...+2^(N-1).

Notes

MV acknowledges support from the European Commission Research Executive Agency (FP7-SPACE-2013-1 GA 607254) and the South African Department of Science and Technology (DST/CON 0134/2014) as part of the Herschel Extragalactic Legacy Project - HELP. MV acknowledges financial support from the Inter-University Institute for Data Intensive Astronomy (IDIA), a partnership of the University of Cape Town, the University of Pretoria and the University of the Western Cape, and from the South African Department of Science and Innovation's National Research Foundation under the ISARP RADIOMAP Joint Research Scheme (DSI-NRF Grant Number 150551) and the CPRR HIPPO Project (DSI-NRF Grant Number SRUG22031677).

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Additional details

Funding

European Commission
HELP - Herschel Extragalactic Legacy Project 607254

Dates

Updated
2026-08-31
31 August 2026