DEBASS - The ultimate low redshift supernova sample for cosmology

Unlocking the mystery of dark energy is one of the key goals of observational cosmology. The LambdaCDM model, in which the dark energy equation-of-state parameter is exactly -1, has so far survived the enormous improvement in constraints achieved since the original discovery of the accelerating universe using type Ia supernovae (SNe Ia) as standard candles. However, recent results from the Dark Energy Survey (DES) and the Dark Energy Spectroscopic Instrument (DESI) are putting the LambdaCDM model under pressure [1,2]. Both experiments provide hints that dark energy varies with time.  If verified, this would rule out Einstein's cosmological constant as the reason for the accelerating universe

While this is a tantalising development, the slight disagreement with Einstein's cosmological constant seen in recent results may be driven by the low-redshift SN sample that anchors the Hubble diagram. The SNe Ia come from a variety of historical external surveys.  The uncertain calibration of these surveys may be driving the result. To reduce the systematic uncertainty related to the low-redshift sample, we need to replace it with a larger, modern, and more precisely calibrated sample of low-redshift SNe Ia.  We are currently assembling this sample. It is called DEBASS.

To place SNe Ia on the Hubble diagram, we need a redshift of the SN or its host galaxy. The DEBASS sample consists of 525 SNe Ia.  We lack redshifts for 70 of them.

The project consists of the following elements

- searching online databases for redshifts

- updating the DEBASS redshift catalogue

Refs:

[1] DES Collaboration et al. 2024,ApJ, 973, 14:

[2] DESI Collaboration et al. 2025, arXiV 2503.14738