Observations of SN 1997ff at z ~ 1.7 favor the accelerating Universe interpretation of the high-redshift type Ia supernova data over simple models of intergalactic dust or SN luminosity evolution. Taken at face-value, they provide direct lines of evidence that the Universe was decelerating in the past, an expected but untested feature of the current cosmological model. We show that the strength of this conclusion depends upon the nature of the dark energy causing the present acceleration. Only for a cosmological constant is the SNe evidence definitive. Using a new test which is independent of the contents of the Universe, we show that the SN data favor recent acceleration (z 0.5)
We present spectral and photometric observations of 10 Type Ia supernovae (SNe Ia) in the redshift r...
We explore the possible role of evolution in the analysis of data on SNe Ia at cosmological distance...
The energy conditions give upper bounds on the luminosity distance. We apply these upper bounds to t...
The unexpected faintness of high-redshift Type Ia supernovae (SNe Ia), as measured by two teams, has...
We discuss recent evidence for an accelerating Universe from measurements of type Ia supernovae at h...
We have discovered 21 new Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have...
We present photometric observations of an apparent Type Iasupernova (SN Ia) at a redshift of approxi...
In this paper, three kinds of simple parameterized deceleration parameters are reconstructed from th...
I review the use of Type Ia supernovae (SNe Ia) for cosmological distance determinations. Low-redshi...
The High-z Supernova Search Team has discovered and observed 8 new supernovae in the redshift interv...
International audienceIn the late 1990’s, observations of two directionally-skewed samples of, in to...
We review the use of Type Ia supernovae for cosmological distance determinations. Low-redshift SNe I...
The comparison of redshift-distance relationship for high and low-redshift supernovae revealed the s...
Type Ia supernovae (SNe Ia) are powerful standardizable candles for constraining cosmological models...
International audienceContext. The cosmological concordance model (ΛCDM) matches the cosmological ob...
We present spectral and photometric observations of 10 Type Ia supernovae (SNe Ia) in the redshift r...
We explore the possible role of evolution in the analysis of data on SNe Ia at cosmological distance...
The energy conditions give upper bounds on the luminosity distance. We apply these upper bounds to t...
The unexpected faintness of high-redshift Type Ia supernovae (SNe Ia), as measured by two teams, has...
We discuss recent evidence for an accelerating Universe from measurements of type Ia supernovae at h...
We have discovered 21 new Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have...
We present photometric observations of an apparent Type Iasupernova (SN Ia) at a redshift of approxi...
In this paper, three kinds of simple parameterized deceleration parameters are reconstructed from th...
I review the use of Type Ia supernovae (SNe Ia) for cosmological distance determinations. Low-redshi...
The High-z Supernova Search Team has discovered and observed 8 new supernovae in the redshift interv...
International audienceIn the late 1990’s, observations of two directionally-skewed samples of, in to...
We review the use of Type Ia supernovae for cosmological distance determinations. Low-redshift SNe I...
The comparison of redshift-distance relationship for high and low-redshift supernovae revealed the s...
Type Ia supernovae (SNe Ia) are powerful standardizable candles for constraining cosmological models...
International audienceContext. The cosmological concordance model (ΛCDM) matches the cosmological ob...
We present spectral and photometric observations of 10 Type Ia supernovae (SNe Ia) in the redshift r...
We explore the possible role of evolution in the analysis of data on SNe Ia at cosmological distance...
The energy conditions give upper bounds on the luminosity distance. We apply these upper bounds to t...