activity
20222024
most citedA galaxy-driven model of type Ia supernova luminosity variations

41 citations · 152 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.CO202418 cited

The Dark Energy Survey Supernova Program: Cosmological Analysis and Systematic Uncertainties

M. Vincenzi, D. Brout, P. Armstrong +93

We present the full Hubble diagram of photometrically-classified Type Ia supernovae (SNe Ia) from the Dark Energy Survey supernova program (DES-SN). DES-SN discovered more than 20,…

astro-ph.CO20233 cited

Amalgame: Cosmological Constraints from the First Combined Photometric Supernova Sample

Brodie Popovic, Daniel Scolnic, Maria Vincenzi +11

Future constraints of cosmological parameters from Type Ia supernovae (SNe Ia) will depend on the use of photometric samples, those samples without spectroscopic measurements of th…

astro-ph.CO202312 cited

Binning is Sinning: Redemption for Hubble Diagram using Photometrically Classified Type Ia Supernovae

Richard Kessler, Maria Vincenzi, Patrick Armstrong

Bayesian Estimation Applied to Multiple Species (BEAMS) is implemented in the BEAMS with Bias Corrections (BBC) framework to produce a redshift-binned Hubble diagram (HD) for Type…

astro-ph.CO202312 cited

The Dark Energy Survey Supernova Program: Corrections on photometry due to wavelength-dependent atmospheric effects

J. Lee, M. Acevedo, M. Sako +64

Wavelength-dependent atmospheric effects impact photometric supernova flux measurements for ground-based observations. We present corrections on supernova flux measurements from th…

astro-ph.CO202335 cited

SALT2 Versus SALT3: Updated Model Surfaces and Their Impacts on Type Ia Supernova Cosmology

G. Taylor, D. O. Jones, B. Popovic +6

For the past decade, SALT2 has been the most common model used to fit Type Ia supernova (SN Ia) light curves for dark energy analyses. Recently, the SALT3 model was released, which…

astro-ph.SR202218 cited

The He I 10830 line as a probe of winds and accretion in young stars in Lupus and Upper Scorpius

J. Erkal, C. F. Manara, P. C. Schneider +6

The He I 1 micron line is a high excitation line which allows us to probe the innermost regions of protostellar disks, and to trace both accreting and outflowing material. We use X…