Replicar los datos para: The high cadence transient survey (Hits): Source, light-curve and classification catalogs (doi:10.34691/FK2/9SGXZG)

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Part 2: Study Description
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Document Description

Citation

Title:

Replicar los datos para: The high cadence transient survey (Hits): Source, light-curve and classification catalogs

Identification Number:

doi:10.34691/FK2/9SGXZG

Distributor:

Repositorio de datos de investigación de la Universidad de Chile

Date of Distribution:

2019-06-20

Version:

1

Bibliographic Citation:

Martínez Palomera, Jorge; Förster, Francisco, 2019, "Replicar los datos para: The high cadence transient survey (Hits): Source, light-curve and classification catalogs", https://doi.org/10.34691/FK2/9SGXZG, Repositorio de datos de investigación de la Universidad de Chile, V1

Study Description

Citation

Title:

Replicar los datos para: The high cadence transient survey (Hits): Source, light-curve and classification catalogs

Identification Number:

doi:10.34691/FK2/9SGXZG

Authoring Entity:

Martínez Palomera, Jorge (Universidad de Chile)

Förster, Francisco (Universidad de Chile)

Distributor:

Repositorio de datos de investigación de la Universidad de Chile

Access Authority:

Martínez Palomera, Jorge

Depositor:

Calabrano, Cristián

Date of Deposit:

2019-06-19

Holdings Information:

https://doi.org/10.34691/FK2/9SGXZG

Study Scope

Keywords:

Astronomy and Astrophysics, Light-curve catalog, Variable stars

Abstract:

The High Cadence Transient Survey (HiTS) aims to discover and study transient objects with characteristic timescales between hours and days, such as pulsating, eclipsing and exploding stars. This survey represents a unique laboratory to explore large etendue observations from cadences of about 0.1 days and to test new computational tools for the analysis of large data. This work follows a fully Data Science approach: from the raw data to the analysis and classification of variable sources. We compile a catalog of ~15 million object detections and a catalog of ~2.5 million light-curves classified by variability. The typical depth of the survey is 24.2, 24.3, 24.1 and 23.8 in u, g, r, and i bands, respectively. We classified all point-like non-moving sources by first extracting features from their light--curves and then applying a Random Forest classifier. For the classification, we used a training set constructed using a combination of cross-matched catalogs, visual inspection, transfer/active learning, and data augmentation. The classification model consists of several Random Forest classifiers organized in a hierarchical scheme. The classifier accuracy estimated on a test set is approximately 97%. In the unlabeled data, 3,485 sources were classified as variables, of which 1,321 were classified as periodic. Among the periodic classes we discovered with high confidence, 1 δ scuti, 39 eclipsing binaries, 48 rotational variables, and 90 RR-Lyrae. For the non-periodic classes we discovered 1 cataclysmic variables, 630 QSO, and 1 supernova candidate.

Methodology and Processing

Sources Statement

Data Access

Other Study Description Materials

Related Publications

Citation

Bibliographic Citation:

Martínez-Palomera, Jorge, & Förster, Francisco. (2018). THE HIGH CADENCE TRANSIENT SURVEY (HITS): Source, light-curve and classification catalogs.

Other Study-Related Materials

Label:

HiTS_labeled_set.fits

Text:

FITS file, 2 HDUs total: The primary HDU; 1 Table HDU(s) The following recognized metadata keys have been found in the FITS file: NAXIS; NAXIS1; NAXIS0;

Notes:

application/fits