The S-PLUS Transient Extension Program: imaging pipeline, transient identification, and survey optimization for multimessenger astronomy

Author:

Santos A1,Kilpatrick C D2ORCID,Bom C R13ORCID,Darc P1,Herpich F R4ORCID,Lacerda E A D5,Sartori M J5,Alvarez-Candal A67ORCID,Mendes de Oliveira C5,Kanaan A8,Ribeiro T9,Schoenell W10

Affiliation:

1. Centro Brasileiro de Pesquisas Físicas , Rua Dr Xavier Sigaud 150, CEP 22290-180, Rio de Janeiro, RJ , Brazil

2. Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy, Northwestern University , Evanston, IL 60208 , USA

3. Centro Federal de Educação Tecnológica Celso Suckow da Fonseca, Rodovia Mário Covas , lote J2, quadra J, CEP 23810-000, Itaguaí, RJ , Brazil

4. Cambridge Survey Astronomical Unit (CASU), Institute of Astronomy , Madingley Road, Cambridge CB3 0HA , UK

5. Universidade de São Paulo , IAG, Rua do Mato 1225, Sao Paulo, SP , Brazil

6. Instituto de Astrofísica de Andalucía , CSIC, Apt 3004, E-18080 Granada , Spain

7. Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante, San Vicent del Raspeig , E-03080 Alicante , Spain

8. Departamento de Física, Universidade Federal de Santa Catarina , Florianópolis, SC 88040-900 , Brazil

9. Departamento de Astronomia, Instituto de Física, Universidade Federal do Rio Grande do Sul (UFRGS) , Av. Bento Goncalves 9500, Porto Alegre, RS , Brazil

10. NOAO , PO Box 26732, Tucson, AZ 85726 , USA

Abstract

ABSTRACT We present the S-PLUS Transient Extension Program (STEP): a supernova and fast transient survey conducted in the southern hemisphere using data from the Southern Photometric Local Universe Survey (S-PLUS) Main Survey and the T80-South telescope. Transient astrophysical phenomena have a range of interest that goes through different fields of astrophysics and cosmology. With the detection of an electromagnetic counterpart to the gravitational wave (GW) event GW170817 from a binary neutron stars merger, new techniques and resources to study fast astrophysical transients in the multimessenger context have increased. In this paper, we present the STEP overview, the SN follow-up data obtained, data reduction, analysis of new transients and deep learning algorithms to optimize transient candidate selection. Additionally, we present prospects and optimized strategy for the search of gravitational wave counterparts in the current LIGO/Virgo/Kagra observational run (O4) in the context of T80-South telescope.

Funder

FAPESP

CNPq

CAPES

FAPERJ

FINEP

Publisher

Oxford University Press (OUP)

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