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Exploiting data from SAM-FP and T80-South

Abstract

This Projeto Regular is the continuation of three previous grants, which supported the construction and maintenance of SAM-FP and T80-South. SAM-FP installed inside the SOAR Adaptive Module (SAM), at the SOAR telescope, is functional and can be used to obtain data cubes with spectral resolution of 11200 and spatial resolution of 0.5 arcsec (with ground-layer adaptive optics correction). We want to complete studies that are underway using data already obtained in previous runs. SAM-FP will allow the study of the internal kinematics of galaxies and interstellar medium among other studies. T80-south, a robotic 80cm telescope, located at Cerro Tololo Interamerican Observatory, in Chile, has an optical camera with a wide field of view of 2 square degrees that is performing a survey of 9300 sq degrees of the sky: the Southern Local Universe Survey, S-PLUS. We want to maximize the use of the data collected by this survey by promoting a rich scientific environment at IAG and organizing events every semester. S-PLUS will enable, among other studies, photo-z, galaxy morphology and stellar population studies, detection of globular clusters and dwarf galaxies around the most nearby galaxies and search for groups and clusters, for galaxy evolution studies. (AU)

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VEICULO: TITULO (DATA)
VEICULO: TITULO (DATA)

Scientific publications (4)
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
BOM, C. R.; CORTESI, A.; LUCATELLI, G.; DIAS, L. O.; SCHUBERT, P.; OLIVEIRA SCHWARZ, G. B.; CARDOSO, N. M.; LIMA, E. V. R.; DE OLIVEIRA, C. MENDES; SODRE, L.; SMITH CASTELLI, V, A.; FERRARI, F.; DAMKE, G.; OVERZIER, R.; KANAAN, A.; RIBEIRO, T.; SCHOENELL, W. Deep Learning assessment of galaxy morphology in S-PLUS Data Release 1. Monthly Notices of the Royal Astronomical Society, v. 507, n. 2, p. 1937-1955, OCT 2021. Web of Science Citations: 0.
WHITTEN, DEVIN D.; PLACCO, VINICIUS M.; BEERS, TIMOTHY C.; AN, DEOKKEUN; LEE, YOUNG SUN; ALMEIDA-FERNANDES, FELIPE; HERPICH, FABIO R.; DAFLON, SIMONE; BARBOSA, CARLOS E.; PEROTTONI, HELIO D.; ROSSI, SILVIA; TISSERA, PATRICIA B.; YOON, JINMI; YOUAKIM, KRIS; SCHOENELL, WILLIAM; RIBEIRO, TIAGO; KANAAN, ANTONIO. The Photometric Metallicity and Carbon Distributions of the Milky Way's Halo and Solar Neighborhood from S-PLUS Observations of SDSS Stripe 82. ASTROPHYSICAL JOURNAL, v. 912, n. 2 MAY 2021. Web of Science Citations: 1.
MOLINO, A.; COSTA-DUARTE, V, M.; SAMPEDRO, L.; HERPICH, F. R.; SODRE JR, L.; MENDES DE OLIVEIRA, C.; SCHOENELL, W.; BARBOSA, C. E.; QUEIROZ, C.; LIMA, E. V. R.; AZANHA, L.; MUNOZ-ELGUETA, N.; RIBEIRO, T.; KANAAN, A.; HERNANDEZ-JIMENEZ, J. A.; CORTESI, A.; AKRAS, S.; LOPES DE OLIVEIRA, R.; TORRES-FLORES, S.; LIMA-DIAS, C.; NILO CASTELLON, J. L.; DAMKE, G.; ALVAREZ-CANDAL, A.; JIMENEZ-TEJA, Y.; COELHO, P.; PEREIRA, E.; MONTERO-DORTA, A. D.; BENITEZ, N.; GONCALVES, T. S.; SANTANA-SILVA, L.; WERNER, V, S.; ALMEIDA, L. A.; LOPES, P. A. A.; CHIES-SANTOS, A. L.; TELLES, E.; THOM DE SOUZA, R. C.; GONCALVES, D. R.; DE SOUZA, R. S.; MAKLER, M.; BUZZO, M. L.; PLACCO, V. M.; NAKAZONO, I, L. M.; SAITO, R. K.; OVERZIER, R. A.; ABRAMO, L. R. Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case. Monthly Notices of the Royal Astronomical Society, v. 499, n. 3, p. 3884-3908, DEC 2020. Web of Science Citations: 0.
BARBOSA, C. E.; ZARITSKY, D.; DONNERSTEIN, R.; ZHANG, H.; DEY, A.; DE OLIVEIRA, C. MENDES; SAMPEDRO, L.; MOLINO, A.; COSTA-DUARTE, M. V.; COELHO, P.; CORTESI, A.; HERPICH, F. R.; HERNANDEZ-JIMENEZ, J. A.; SANTOS-SILVA, T.; PEREIRA, E.; WERLE, A.; OVERZIER, R. A.; FERNANDES, R.; CASTELLI, A. V. SMITH; RIBEIRO, T.; SCHOENELL, W.; KANAAN, A. One Hundred SMUDGes in S-PLUS: Ultra-diffuse Galaxies Flourish in the Field. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, v. 247, n. 2 APR 2020. Web of Science Citations: 0.

Please report errors in scientific publications list by writing to: cdi@fapesp.br.