| Title: | iPTF Discoveries of Recent Type Ia Supernovae |
|---|
| Authors: | ID Papadogiannakis, S., Oskar Klein Centre, Department of Physics, Stockholm University, SE 106 91 Stockholm, Sweden (Author)
ID Petrushevska, Tanja, Oskar Klein Centre, Department of Physics, Stockholm University, SE 106 91 Stockholm, Sweden (Author), et al. |
|---|
| Files: |
This document has no files that are freely available to the public. This document may have a physical copy in the library of the organization, check the status via COBISS.  |
|---|
| Language: | English |
|---|
| Work type: | Not categorized |
|---|
| Typology: | 1.25 - Other Component Parts |
|---|
| Organization: | UNG - University of Nova Gorica
|
|---|
| Abstract: | Abstract
The intermediate Palomar Transient Factory (ATel #4807) reports the discovery and classification of the following Type Ia SNe. Our automated candidate vetting to distinguish a real astrophysical source (1.0) from bogus artifacts (0.0) is powered by three generations of machine learning algorithms: RB2 (Brink et al. 2013MNRAS.435.1047B), RB4 (Rebbapragada et al. 2015AAS...22543402R) and RB5 (Wozniak et al. 2013AAS...22143105W). |
|---|
| Keywords: | Supernovae, Transients |
|---|
| Publication status: | Published |
|---|
| Place of publishing: | Montreal |
|---|
| Publisher: | McGill University |
|---|
| Year of publishing: | 2016 |
|---|
| PID: | 20.500.12556/RUNG-3598-387a99e8-ac92-921a-9d31-f5239cc894e9 |
|---|
| COBISS.SI-ID: | 5003259 |
|---|
| NUK URN: | URN:SI:UNG:REP:YMHNX9NB |
|---|
| Publication date in RUNG: | 23.01.2018 |
|---|
| Views: | 4168 |
|---|
| Downloads: | 0 |
|---|
| Metadata: |    |
|---|
|
:
|
Copy citation |
|---|
| | | | Average score: | (0 votes) |
|---|
| Your score: | Voting is allowed only for logged in users. |
|---|
| Share: |  |
|---|
Hover the mouse pointer over a document title to show the abstract or click
on the title to get all document metadata. |
