We present RAPID (Real-time Automated Photometric IDentification), a novel timeseries classification tool capable of automatically identifying transients from within a day of the initial alert to the full lifetime of a light curve. Using a deep recurrent neural network with Gated Recurrent Units (GRUs), we present the first method specifically designed to provide early classifications of astronomical timeseries data, typing 12 different transient classes (including supernovae, kilonovae, and rare transients). Our classifier can process light curves with any phase coverage, and it does not rely on deriving computationally expensive features from the data, making RAPID well‐suited for processing the millions of alerts that ongoing and upcomin...
International audienceThe large sky localization regions offered by the gravitational-wave interfero...
Substantial effort has been devoted to the characterization of transient phenomena from photometric ...
International audienceOne of the brightest objects in the universe, supernovae (SNe) are powerful ex...
We present RAPID (Real-time Automated Photometric IDentification), a novel time-series classificatio...
We apply deep recurrent neural networks, which are capable of learning complex sequential informatio...
Upcoming fast radio burst (FRB) surveys will search ~103 beams on the sky with a very high duty cycl...
We identify minimal observing cadence requirements that enable photometric astronomical surveys to d...
Time-domain astronomy has reached an incredible new era where unprecedented amounts of data are beco...
International audienceWe describe the fast transient classification algorithm in the center of the k...
Context. With a rapidly rising number of transients detected in astronomy, classification methods ba...
International audienceWe describe an algorithm for identifying point-source transients and moving ob...
Astronomy light curves are sparse, gappy, and heteroscedastic. As a result standard time series meth...
We describe an algorithm for identifying point-source transients and moving objects on reference-sub...
Context. Modern-day time-domain photometric surveys collect a lot of observations of various astrono...
International audienceThe large sky localization regions offered by the gravitational-wave interfero...
Substantial effort has been devoted to the characterization of transient phenomena from photometric ...
International audienceOne of the brightest objects in the universe, supernovae (SNe) are powerful ex...
We present RAPID (Real-time Automated Photometric IDentification), a novel time-series classificatio...
We apply deep recurrent neural networks, which are capable of learning complex sequential informatio...
Upcoming fast radio burst (FRB) surveys will search ~103 beams on the sky with a very high duty cycl...
We identify minimal observing cadence requirements that enable photometric astronomical surveys to d...
Time-domain astronomy has reached an incredible new era where unprecedented amounts of data are beco...
International audienceWe describe the fast transient classification algorithm in the center of the k...
Context. With a rapidly rising number of transients detected in astronomy, classification methods ba...
International audienceWe describe an algorithm for identifying point-source transients and moving ob...
Astronomy light curves are sparse, gappy, and heteroscedastic. As a result standard time series meth...
We describe an algorithm for identifying point-source transients and moving objects on reference-sub...
Context. Modern-day time-domain photometric surveys collect a lot of observations of various astrono...
International audienceThe large sky localization regions offered by the gravitational-wave interfero...
Substantial effort has been devoted to the characterization of transient phenomena from photometric ...
International audienceOne of the brightest objects in the universe, supernovae (SNe) are powerful ex...