v1.1: fixes a bug that was affecting the distance moduli of a single data point (thanks to Zac Lane). Code used in the analysis of Dam et al., 2017, Mon. Not. Roy. Astron. Soc., 472, 835 [arxiv:1706.07236]. Includes covariance matrices as used in Nielsen et al., 2016, Sci. Rep., 6, 35596
We describe catalogue-level simulations of Type Ia supernova (SN Ia) light curves in the Dark Energy...
We present a systematic analysis of the cosmological constraints from the "Pantheon Sample" of 1048 ...
Aims. The nearby, bright, almost completely unreddened Type Ia supernova 2011fe in M101 provides a u...
Code used in the analysis of Dam et al. (2017), arxiv:1706.07236. Includes covariance matrices as u...
Distance measurements using Type Ia Supernovae have enabled the startling discovery that the expansi...
Aims. The nearby, bright, almost completely unreddened Type Ia supernova 2011fe in M101 provide...
We present a recalibration of the photometric systems in the Pantheon+ sample of Type Ia supernovae ...
We present here a re-calibration of the photometric systems used in the Pantheon+ sample of Type Ia ...
International audienceWe show how spectra of Type Ia supernovae (SNe Ia) at maximum light can be use...
Many researchers have performed cosmological-model-independent tests for the distance-duality (DD) r...
This research explores the correlation between the absolute magnitude and the redshift of Type Ia su...
This is a bug-fixing replacement for the previous release. Two bugs are fixed. Firstly, there was a ...
We describe catalogue-level simulations of Type Ia supernova (SN Ia) light curves in the Dark Energy...
We introduce a method for identifying "twin" Type Ia supernovae (SNe Ia) and using them to improve d...
International audienceWe describe catalog-level simulations of Type Ia supernova (SN~Ia) light curve...
We describe catalogue-level simulations of Type Ia supernova (SN Ia) light curves in the Dark Energy...
We present a systematic analysis of the cosmological constraints from the "Pantheon Sample" of 1048 ...
Aims. The nearby, bright, almost completely unreddened Type Ia supernova 2011fe in M101 provides a u...
Code used in the analysis of Dam et al. (2017), arxiv:1706.07236. Includes covariance matrices as u...
Distance measurements using Type Ia Supernovae have enabled the startling discovery that the expansi...
Aims. The nearby, bright, almost completely unreddened Type Ia supernova 2011fe in M101 provide...
We present a recalibration of the photometric systems in the Pantheon+ sample of Type Ia supernovae ...
We present here a re-calibration of the photometric systems used in the Pantheon+ sample of Type Ia ...
International audienceWe show how spectra of Type Ia supernovae (SNe Ia) at maximum light can be use...
Many researchers have performed cosmological-model-independent tests for the distance-duality (DD) r...
This research explores the correlation between the absolute magnitude and the redshift of Type Ia su...
This is a bug-fixing replacement for the previous release. Two bugs are fixed. Firstly, there was a ...
We describe catalogue-level simulations of Type Ia supernova (SN Ia) light curves in the Dark Energy...
We introduce a method for identifying "twin" Type Ia supernovae (SNe Ia) and using them to improve d...
International audienceWe describe catalog-level simulations of Type Ia supernova (SN~Ia) light curve...
We describe catalogue-level simulations of Type Ia supernova (SN Ia) light curves in the Dark Energy...
We present a systematic analysis of the cosmological constraints from the "Pantheon Sample" of 1048 ...
Aims. The nearby, bright, almost completely unreddened Type Ia supernova 2011fe in M101 provides a u...
DOI
Add to ORKG