Large sky surveys are increasingly relying on image subtraction pipelines for real-time (and archival) transient detection. In this process one has to contend with varying point-spread function (PSF) and small brightness variations in many sources, as well as artefacts resulting from saturated stars and, in general, matching errors. Very often the differencing is done with a reference image that is deeper than individual images and the attendant difference in noise characteristics can also lead to artefacts. We present here a deep-learning approach to transient detection that encapsulates all the steps of a traditional image-subtraction pipeline – image registration, background subtraction, noise removal, PSF matching and subtraction – in a...
Efficient identification and follow-up of astronomical transients is hindered by the need for humans...
International audienceThe observation of the transient sky through a multitude of astrophysical mess...
Searches for counterparts to multimessenger events with optical imagers use difference imaging to de...
Large sky surveys are increasingly relying on image subtraction pipelines for real-time (and archiva...
Current synoptic sky surveys monitor large areas of the sky to find variable and transient astronomi...
We present a technique for optical transient detection using artificial neural networks, particularl...
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons A...
We present a technique to detect optical transients based on an artificial neural networks method. W...
We present a study of the potential for convolutional neural networks (CNNs) to enable separation of...
International audienceContext. Scientific interest in studying high-energy transient phenomena in th...
A fast-turnaround pipeline for realtime data reduction plays an essential role in discovering and pe...
The ability to discover new transients via image differencing without direct human intervention is a...
Efficient automated detection of flux-transient, re-occurring flux-variable, and moving objects is i...
The ability to discover new transient candidates via image differencing without direct human interve...
Efficient identification and follow-up of astronomical transients is hindered by the need for humans...
International audienceThe observation of the transient sky through a multitude of astrophysical mess...
Searches for counterparts to multimessenger events with optical imagers use difference imaging to de...
Large sky surveys are increasingly relying on image subtraction pipelines for real-time (and archiva...
Current synoptic sky surveys monitor large areas of the sky to find variable and transient astronomi...
We present a technique for optical transient detection using artificial neural networks, particularl...
This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons A...
We present a technique to detect optical transients based on an artificial neural networks method. W...
We present a study of the potential for convolutional neural networks (CNNs) to enable separation of...
International audienceContext. Scientific interest in studying high-energy transient phenomena in th...
A fast-turnaround pipeline for realtime data reduction plays an essential role in discovering and pe...
The ability to discover new transients via image differencing without direct human intervention is a...
Efficient automated detection of flux-transient, re-occurring flux-variable, and moving objects is i...
The ability to discover new transient candidates via image differencing without direct human interve...
Efficient identification and follow-up of astronomical transients is hindered by the need for humans...
International audienceThe observation of the transient sky through a multitude of astrophysical mess...
Searches for counterparts to multimessenger events with optical imagers use difference imaging to de...