Holographic dark energy
We review the paradigm of holographic dark energy (HDE), which arises from a theoretical
attempt of applying the holographic principle (HP) to the dark energy (DE) problem. Making�…
attempt of applying the holographic principle (HP) to the dark energy (DE) problem. Making�…
Large Magellanic Cloud Cepheid standards provide a 1% foundation for the determination of the Hubble constant and stronger evidence for physics beyond ΛCDM
We present an improved determination of the Hubble constant from Hubble Space
Telescope (HST) observations of 70 long-period Cepheids in the Large Magellanic Cloud�…
Telescope (HST) observations of 70 long-period Cepheids in the Large Magellanic Cloud�…
The complete light-curve sample of spectroscopically confirmed SNe Ia from Pan-STARRS1 and cosmological constraints from the combined pantheon sample
We present optical light curves, redshifts, and classifications for 365 spectroscopically
confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium�…
confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium�…
A 2.4% determination of the local value of the Hubble constant
AG Riess, LM Macri, SL Hoffmann…�- The Astrophysical�…, 2016 - iopscience.iop.org
ABSTRACT We use the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope
(HST) to reduce the uncertainty in the local value of the Hubble constant from 3.3% to 2.4�…
(HST) to reduce the uncertainty in the local value of the Hubble constant from 3.3% to 2.4�…
[HTML][HTML] Planck 2015 results-xiii. cosmological parameters
PAR Ade, N Aghanim, M Arnaud, M Ashdown…�- Astronomy &�…, 2016 - aanda.org
This paper presents cosmological results based on full-mission Planck observations of
temperature and polarization anisotropies of the cosmic microwave background (CMB)�…
temperature and polarization anisotropies of the cosmic microwave background (CMB)�…
The pan-starrs1 surveys
KC Chambers, EA Magnier, N Metcalfe…�- arXiv preprint arXiv�…, 2016 - arxiv.org
Pan-STARRS1 has carried out a set of distinct synoptic imaging sky surveys including the
$3\pi $ Steradian Survey and the Medium Deep Survey in 5 bands ($ grizy_ {P1} $). The�…
$3\pi $ Steradian Survey and the Medium Deep Survey in 5 bands ($ grizy_ {P1} $). The�…
Planck 2015 results-III. LFI systematic uncertainties
PAR Ade, J Aumont, C Baccigalupi, AJ Banday…�- Astronomy &�…, 2016 - aanda.org
We present the current accounting of systematic effect uncertainties for the Low Frequency
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results�…
Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results�…
Type Ia supernova distances at redshift> 1.5 from the Hubble space telescope multi-cycle treasury programs: the early expansion rate
AG Riess, SA Rodney, DM Scolnic…�- The Astrophysical�…, 2018 - iopscience.iop.org
Type Ia Supernova Distances at Redshift >1.5 from the Hubble Space Telescope Multi-cycle
Treasury Programs: The Early Expansion Rate - IOPscience This site uses cookies. By�…
Treasury Programs: The Early Expansion Rate - IOPscience This site uses cookies. By�…
Hints of FLRW breakdown from supernovae
A 10% difference in the scale for the Hubble parameter constitutes a clear problem for
cosmology. Here, considering angular distribution of type Ia supernovae (SN) within the�…
cosmology. Here, considering angular distribution of type Ia supernovae (SN) within the�…
It's dust: solving the mysteries of the intrinsic scatter and host-galaxy dependence of standardized type Ia supernova brightnesses
Abstract The use of Type Ia supernovae (SNe Ia) as cosmological tools has motivated
significant effort to understand what drives the intrinsic scatter of SN Ia distance modulus�…
significant effort to understand what drives the intrinsic scatter of SN Ia distance modulus�…