activity
20032023
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 17.6k across the 78 of their papers we have counts for

collaborators

80 papers

astro-ph.CO2023★ 7 cited

Detecting strongly-lensed type Ia supernovae with LSST

Nikki Arendse, Suhail Dhawan, Ana Sagués Carracedo +8

Strongly-lensed supernovae are rare and valuable probes of cosmology and astrophysics. Upcoming wide-field time-domain surveys, such as the Vera C. Rubin Observatory's Legacy Surve…

astro-ph.IM2022★ 8 cited

SNGuess: A method for the selection of young extragalactic transients

N. Miranda, J. C. Freytag, J. Nordin +7

With a rapidly rising number of transients detected in astronomy, classification methods based on machine learning are increasingly being employed. Their goals are typically to obt…

astro-ph.HE2021★ 16 cited

Supernova Siblings and their Parent Galaxies in the Zwicky Transient Facility Bright Transient Surve

M. L. Graham, C. Fremling, D. A. Perley +19

Supernova (SN) siblings -- two or more SNe in the same parent galaxy -- are useful tools for exploring progenitor stellar populations as well as properties of the host galaxies suc…

astro-ph.CO2021★ 37 cited

SNIa-Cosmology Analysis Results from Simulated LSST Images: from Difference Imaging to Constraints on Dark Energy

B. Sánchez, R. Kessler, D. Scolnic +19

The Vera Rubin Observatory Legacy Survey of Space and Time (LSST) is expected to process transient detections per night. For precision measurements of cosmological par…

astro-ph.CO2021★ 46 cited

The Zwicky Transient Facility Type Ia supernova survey: first data release and results

S. Dhawan, A. Goobar, M. Smith +17

Type Ia supernovae (SNe~Ia) in the nearby Hubble flow are excellent distance indicators in cosmology. The Zwicky Transient Facility (ZTF) has observed a large sample of supernovae…

astro-ph.IM2021★ 2 cited

Considerations for optimizing photometric classification of supernovae from the Rubin Observatory

Catarina S. Alves, Hiranya V. Peiris, Michelle Lochner +3

The Vera C. Rubin Observatory will increase the number of observed supernovae (SNe) by an order of magnitude; however, it is impossible to spectroscopically confirm the class for a…