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Ragnhild Lunnan

Researcher at Stockholm University

Publications -  169
Citations -  13348

Ragnhild Lunnan is an academic researcher from Stockholm University. The author has contributed to research in topics: Supernova & Galaxy. The author has an hindex of 57, co-authored 159 publications receiving 10627 citations. Previous affiliations of Ragnhild Lunnan include Swinburne University of Technology & CFA Institute.

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The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample

TL;DR: Scolnic et al. as discussed by the authors presented optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Survey.
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The zwicky transient facility: System overview, performance, and first results

Eric C. Bellm, +121 more
TL;DR: The Zwicky Transient Facility (ZTF) as mentioned in this paper is a new optical time-domain survey that uses the Palomar 48 inch Schmidt telescope, which provides a 47 deg^2 field of view and 8 s readout time, yielding more than an order of magnitude improvement in survey speed relative to its predecessor survey.
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The Zwicky Transient Facility: Science Objectives

Matthew J. Graham, +116 more
TL;DR: The Zwicky Transient Facility (ZTF) as discussed by the authors is a new time domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 deg$^2$ field of view and 8 second readout time.
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Cosmological Constraints from Measurements of Type Ia Supernovae Discovered During the First 1.5 Yr of the Pan-STARRS1 Survey

TL;DR: In this article, the authors present griz P1 light curves of 146 spectroscopically confirmed Type Ia supernovae (SNe Ia; 0.03 < z < 0.65) discovered during the first 1.5 yr of the Pan-STARRS1 Medium Deep Survey.
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Slowly fading super-luminous supernovae that are not pair-instability explosions

TL;DR: Observations of two slow-to-fade super-luminous supernovae that show relatively fast rise times and blue colours, which are incompatible with pair-instability models are reported.