Programa de Pós Graduação em Física (PPGF)

Iara Tosta e Melo

Possui doutorado pela Universidade La Sapienza de Roma, atuando na área de Astrofísica Extragalactica. Atualmente é professor assistente na universidade de Catania e professor do programa de pos-graduaçao da Unifal. Atua principalmente na área de astrofísica multimessenger envolvendo GW, neutrinos e outros fenômenos de alta energia. Foi professor visitante na Unifei em 2022 e na Unifal nos anos de 2023 e 2024. Participou de mais de 20 congressos internacionais (desde 2010) e organizou 7 conferencias internacionais. Participou de bancas de mestrado e doutorado de alunos do INPE, UNESP e Unifal. Atualmente orienta 3 alunos de doutorado e 3 de mestrado de universidade brasileiras. Participou da banca de comissao examinadora para seleçao de um pesquisador do INPE (PQ29 - Multimessenger Astronomy) e para um professor de ingles cientifico na Universidade de Catania. É leader do grupo VirgoBR e um dos leaders de analises multimensageira dentro a colaboração LVK. É coordenadora das analises GWHEN dentro de LVK representando o telescópio de neutrino KM3Net. Faz parte de uma colaboraçao que venceu o premio Nobel e é co-autora de um paper na Nature sobre a observação do neutrino de maior energia observado até então. Ganhou 1 prêmio internacional para internazionaliação, ERAMUS +, e 2 prêmios nacionais de internazionalização. É PI dos telescópios brasileiros na colaboração GRANDMA. Busca consolidar a pesquisa multimessenger no Brasil. (Texto informado pelo autor)

http://lattes.cnpq.br/7286059807128292 (11/04/2025)

Rótulo/Grupo:

Bolsa CNPq:

Período de análise:

Endereço: Università degli Studi di Catania, UniCT. via santa sofia 62 cittadella Catania, - Itália Telefone: (35) 999602359

Grande área: Ciências Exatas e da Terra

Área: Astronomia

Citações: Google Acadêmico

Produção bibliográfica

Artigos completos publicados em periódicos (70)
1. RAMAN, GAYATHRI ; RONCHINI, SAMUELE ; DELAUNAY, JAMES ; TOHUVAVOHU, AARON ; KENNEA, JAMIE A. ; PARSOTAN, TYLER ; AMBROSI, ELENA ; BERNARDINI, MARIA GRAZIA ; CAMPANA, SERGIO ; CUSUMANO, GIANCARLO ; D?AÌ, ANTONINO ; D?AVANZO, PAOLO ; D?ELIA, VALERIO ; DE PASQUALE, MASSIMILIANO ; DICHIARA, SIMONE ; EVANS, PHIL ; HARTMANN, DIETER ; KUIN, PAUL ; MELANDRI, ANDREA ; TOSTA E MELO, I. ; et.al. Swift-BAT GUANO Follow-up of Gravitational-wave Triggers in the Third LIGO-Virgo-KAGRA Observing Run. The Astrophysical Journal. v. 980, p. 207, issn: 0004-637X, 2025. Qualis: A1
2. AIELLO, S. ; ALBERT, A. ; ALHEBSI, A. R. ; ALSHAMSI, M. ; ALVES GARRE, S. ; AMBROSONE, A. ; AMELI, F. ; ANDRE, M. ; ANGHINOLFI, M. ; APHECETCHE, L. ; ARDID, M. ; ARDID, S. ; ARGÜELLES, C. ; ATMANI, H. ; AUBLIN, J. ; BADARACCO, F. ; BAILLY-SALINS, L. ; BARDAč ; BARET, B. ; TOSTA E MELO, I. ; et.al. Observation of an ultra-high-energy cosmic neutrino with KM3NeT. NATURE. v. 638, p. 376-382, issn: 0028-0836, 2025. Qualis: A1
3. AIELLO, S. ; ALBERT, A. ; ALHEBSI, A.R. ; ALSHAMSI, M. ; ALVES GARRE, S. ; AMBROSONE, A. ; AMELI, F. ; ANDRE, M. ; APHECETCHE, L. ; ARDID, M. ; ARDID, S. ; AUBLIN, J. ; BADARACCO, F. ; BAILLY-SALINS, L. ; BARDAč ; BARET, B. ; BARIEGO-QUINTANA, A. ; BECHERINI, Y. ; BENDAHMAN, M. ; TOSTA E MELO, I. ; et.al. Search for non-standard neutrino interactions with the first six detection units of KM3NeT/ORCA. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. v. 2025, p. 073, issn: 1475-7516, 2025. Qualis: A1
4. DAVARI, N. ; TOSTA E MELO, I. ; Rozza, D. ; DELL?AQUILA, D. ; D?URSO, D. ; ANZUINELLI, S. ; PESENTI, L. ; Sipala, V.. Analytical study of the merging rate of low-mass intermediate-mass black holes in preparation for the future Telescope. ASTRONOMY & ASTROPHYSICS. v. 692, p. A85, issn: 0004-6361, 2024. Qualis: A1
5. TOSTA E MELO, I.; DUCOIN, J.-G. ; VIDADI, Z. ; ANDRADE, C. ; RUPCHANDANI, V. ; AGAYEVA, S. ; ABDELHADI, J. ; ABE, L. ; AGUERRE-CHARIOL, O. ; AIVAZYAN, V. ; ALISHOV, S. ; ANTIER, S. ; BAI, J.-M. ; BARANSKY, A. ; BEDNARZ, S. ; BENDJOYA, PH. ; BENKHALDOUN, Z. ; BERADZE, S. ; BIZOUARD, M. A. ; BHARDWAJ, U. ; et.al. Ready for O4 II: GRANDMA observations of Swift GRBs over eight weeks in spring 2022. ASTRONOMY & ASTROPHYSICS. v. 682, p. A141, issn: 0004-6361, 2024. Qualis: A1
6. MARTINS, JULIO CÉSAR ; HENG, IK SIONG ; MELO, IARA TOSTA E ; AGUIAR, ODYLIO DENYS. Search for gravitational-wave bursts in LIGO data at the Schenberg antenna sensitivity range. PHYSICAL REVIEW D. v. 109, p. -, issn: 2470-0010, 2024. Qualis: A1
7. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADKINS, V. K. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. Search for Gravitational-wave Transients Associated with Magnetar Bursts in Advanced LIGO and Advanced Virgo Data from the Third Observing Run. The Astrophysical Journal. v. 966, p. 137, issn: 0004-637X, 2024. Qualis: A1
8. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHICARY, S. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADKINS, V. K. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; ALFAIDI, R. A. ; TOSTA E MELO, I. ; et.al. Search for Gravitational-lensing Signatures in the Full Third Observing Run of the LIGO-Virgo Network. The Astrophysical Journal. v. 970, p. 191, issn: 0004-637X, 2024. Qualis: A1
9. ABAC, A. G. ; ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADAMCEWICZ, C. ; ADHICARY, S. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADKINS, V. K. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGUIAR, O. D. ; AGUILAR, I. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; TOSTA E MELO, I. ; et.al. Search for Eccentric Black Hole Coalescences during the Third Observing Run of LIGO and Virgo. The Astrophysical Journal. v. 973, p. 132, issn: 0004-637X, 2024. Qualis: A1
10. FLETCHER, C. ; WOOD, J. ; HAMBURG, R. ; VERES, P. ; HUI, C. M. ; BISSALDI, E. ; BRIGGS, M. S. ; BURNS, E. ; CLEVELAND, W. H. ; GILES, M. M. ; GOLDSTEIN, A. ; HRISTOV, B. A. ; KOCEVSKI, D. ; LESAGE, S. ; MAILYAN, B. ; MALACARIA, C. ; POOLAKKIL, S. ; VON KIENLIN, A. ; WILSON-HODGE, C. A. ; TOSTA E MELO, I. ; et.al. A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run. The Astrophysical Journal. v. 964, p. 149, issn: 0004-637X, 2024. Qualis: A1
11. HUSSENOT-DESENONGES, T ; WOUTERS, T ; GUESSOUM, N ; ABDI, I ; ABULWFA, A ; ADAMI, C ; AGÜÍ FERNÁNDEZ, J F ; AHUMADA, T ; AIVAZYAN, V ; AKL, D ; ANAND, S ; ANDRADE, C M ; ANTIER, S ; ATA, S A ; D?AVANZO, P ; AZZAM, Y A ; BARANSKY, A ; BASA, S ; BLAZEK, M ; TOSTA E MELO, I. ; et.al. Multiband analyses of the bright GRB 230812B and the associated SN2023pel. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. v. 530, p. 1-19, issn: 0035-8711, 2024. Qualis: A1
12. ABAC, A.'G. ; ABBOTT, R. ; ABE, H. ; ABOUELFETTOUH, I. ; ACERNESE, F. ; ACKLEY, K. ; ADAMCEWICZ, C. ; ADHICARY, S. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADKINS, V.'K. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGUIAR, O.'D. ; AGUILAR, I. ; AIELLO, L. ; AIN, A. ; TOSTA E MELO, I. ; et.al. Ultralight vector dark matter search using data from the KAGRA O3GK run. PHYSICAL REVIEW D. v. 110, p. ., issn: 2470-0010, 2024. Qualis: A1
13. AIELLO, S. ; ALBERT, A. ; ALSHAMSI, M. ; ALVES GARRE, S. ; AMBROSONE, A. ; AMELI, F. ; ANDRE, M. ; ANDROUTSOU, E. ; ANGUITA, M. ; APHECETCHE, L. ; ARDID, M. ; ARDID, S. ; ATMANI, H. ; AUBLIN, J. ; BADARACCO, F. ; BAILLY-SALINS, L. ; BARDAč ; BARET, B. ; BARIEGO-QUINTANA, A. ; TOSTA E MELO, I. ; et.al. Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. v. 2024, p. 006, issn: 1475-7516, 2024. Qualis: A1
14. AIELLO, S. ; ALBERT, A. ; ALSHAMSI, M. ; ALVES GARRE, S. ; ALY, Z. ; AMBROSONE, A. ; AMELI, F. ; ANDRE, M. ; ANDROUTSOU, E. ; ANGUITA, M. ; APHECETCHE, L. ; ARDID, M. ; ARDID, S. ; ATMANI, H. ; AUBLIN, J. ; BADARACCO, F. ; BAILLY-SALINS, L. ; BARDAč ; BARET, B. ; TOSTA E MELO, I. ; et.al. Astronomy potential of KM3NeT/ARCA. EUROPEAN PHYSICAL JOURNAL C. PARTICLES AND FIELDS. v. 84, p. 885, issn: 1434-6052, 2024. Qualis: A2
15. AIELLO, SEBASTIANO ; ALBERT, ARNAULD ; GARRE, SERGIO ; ALY, ZINEB ; AMBROSONE, ANTONIO ; AMELI, FABRIZIO ; ANDRE, MICHEL ; ANDROUTSOU, ELENI ; ANGUITA, MANCIA ; APHECETCHE, LAURENT ; ARDID, MIGUEL ; ARDID, SALVA ; ATMANI, HICHAM ; AUBLIN, JULIEN ; BADARACCO, FRANCESCA ; BAILLY-SALINS, LOUIS ; BARDACOVA, ZUZANA ; BARET, BRUNY ; BARIEGO, ADRIANA ; TOSTA E MELO, I. ; et.al. The Power Board of the KM3NeT Digital Optical Module: Design, Upgrade, and Production. ELECTRONICS. v. 13, p. 2044, issn: 2079-9292, 2024. Qualis: Não identificado (ELECTRONICS)
16. AIELLO, S. ; ALBERT, A. ; ALVES GARRE, S. ; ALY, Z. ; AMBROSONE, A. ; AMELI, F. ; ANDRE, M. ; ANDROUTSOU, E. ; ANGUITA, M. ; APHECETCHE, L. ; ARDID, M. ; ARDID, S. ; ATMANI, H. ; AUBLIN, J. ; BAILLY-SALINS, L. ; BARDAč ; BARET, B. ; BARIEGO-QUINTANA, A. ; BASEGMEZ DU PREE, S. ; TOSTA E MELO, I. ; et.al. Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. v. 2024, p. 026, issn: 1475-7516, 2024. Qualis: A1
17. UNBEHAUN, T. ; MOHRMANN, L. ; FUNK, S. ; AIELLO, S. ; ALBERT, A. ; GARRE, S. ALVES ; ALY, Z. ; AMBROSONE, A. ; AMELI, F. ; ANDRE, M. ; ANDROUTSOU, E. ; ANGHINOLFI, M. ; ANGUITA, M. ; APHECETCHE, L. ; ARDID, M. ; ARDID, S. ; ATMANI, H. ; AUBLIN, J. ; BAGATELAS, C. ; TOSTA E MELO, I. ; et.al. Prospects for combined analyses of hadronic emission from $$gamma $$-ray sources in the Milky Way with CTA and KM3NeT. EUROPEAN PHYSICAL JOURNAL C. PARTICLES AND FIELDS. v. 84, p. 112, issn: 1434-6052, 2024. Qualis: A2
18. AIELLO, S. ; ALBERT, A. ; ALVES GARRE, S. ; ALY, Z. ; AMBROSONE, A. ; AMELI, F. ; ANDRE, M. ; ANDROUTSOU, E. ; ANGHINOLFI, M. ; ANGUITA, M. ; APHECETCHE, L. ; ARDID, M. ; ARDID, S. ; ATMANI, H. ; AUBLIN, J. ; BAGATELAS, C. ; BAILLY-SALINS, L. ; BARDAč ; BARET, B. ; TOSTA E MELO, I. ; et.al. Embedded software of the KM3NeT central logic board. COMPUTER PHYSICS COMMUNICATIONS. v. 296, p. 109036, issn: 0010-4655, 2024. Qualis: A2
19. ABBOTT, R. ; ABBOTT, T. D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO-Virgo Observing Run O3a. The Astrophysical Journal. v. 955, p. 155, issn: 0004-637X, 2023. Qualis: A1
20. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADKINS, V. K. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. Constraints on the Cosmic Expansion History from GWTC-3. The Astrophysical Journal. v. 949, p. 76, issn: 0004-637X, 2023. Qualis: A1
21. ABBOTT, R. ; ABBOTT, T.'D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKCAY, S. ; AKUTSU, T. ; TOSTA E MELO, I. ; et.al. GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run. Physical Review X. v. 13, p. ., issn: 2160-3308, 2023. Qualis: A1
22. ABBOTT, R. ; ABBOTT, T.'D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; DE ALARCÓN, P.'F. ; TOSTA E MELO, I. ; et.al. Population of Merging Compact Binaries Inferred Using Gravitational Waves through GWTC-3. Physical Review X. v. 13, p. ,, issn: 2160-3308, 2023. Qualis: A1
23. ACERNESE, F ; AGATHOS, M ; AIN, A ; ALBANESI, S ; ALLOCCA, A ; AMATO, A ; ANDRADE, T ; ANDRES, N ; ANDRÉS-CARCASONA, M ; ANDRI', T ; ANSOLDI, S ; ANTIER, S ; APOSTOLATOS, T ; APPAVURAVTHER, E Z ; ARÈNE, M ; ARNAUD, N ; ASSIDUO, M ; ASSIS DE SOUZA MELO, S ; ASTONE, P ; TOSTA E MELO, I. ; et.al. Virgo detector characterization and data quality: results from the O3 run. CLASSICAL AND QUANTUM GRAVITY. v. 40, p. 185006, issn: 0264-9381, 2023. Qualis: A1
24. F ACERNESE ; AGATHOS, M ; AIN, A ; ALBANESI, S ; ALLOCCA, A ; AMATO, A ; ANDRADE, T ; ANDRES, N ; ANDRÉS-CARCASONA, M ; ANDRI', T ; ANSOLDI, S ; ANTIER, S ; APOSTOLATOS, T ; APPAVURAVTHER, E Z ; ARÈNE, M ; ARNAUD, N ; ASSIDUO, M ; ASSIS DE SOUZA MELO, S ; ASTONE, P ; TOSTA E MELO, I. ; et.al. Virgo detector characterization and data quality: tools. CLASSICAL AND QUANTUM GRAVITY. v. 40, p. 185005, issn: 0264-9381, 2023. Qualis: A1
25. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHICARY, S. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADKINS, V. K. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; ALFAIDI, R. A. ; TOSTA E MELO, I. ; et.al. Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. v. 267, p. 29, issn: 0067-0049, 2023. Qualis: A1
26. ABBOTT, R. ; ABBOTT, T. D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b. The Astrophysical Journal. v. 928, p. 186, issn: 0004-637X, 2022. Qualis: A1
27. AIVAZYAN, V ; ALMUALLA, M ; ANTIER, S ; BARANSKY, A ; BARYNOVA, K ; BASA, S ; BAYARD, F ; BERADZE, S ; BEREZIN, D ; BLAZEK, M ; BOUTIGNY, D ; BOUST, D ; BROENS, E ; BURKHONOV, O ; CAILLEAU, A ; CHRISTENSEN, N ; CEJUDO, D ; COLEIRO, A ; COUGHLIN, M W ; TOSTA E MELO, I. ; et.al. GRANDMA observations of ZTF/Finktransients during summer 2021. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. v. 515, p. 6007-6022, issn: 0035-8711, 2022. Qualis: A1
28. ALLOCCA, ANNALISA ; AVINO, SAVERIO ; BALESTRIERI, SERGIO ; CALLONI, ENRICO ; CAPRARA, SERGIO ; CARPINELLI, MASSIMO ; D?ONOFRIO, LUCA ; D?URSO, DOMENICO ; DE ROSA, ROSARIO ; ERRICO, LUCIANO ; GAGLIARDI, GIANLUCA ; GRILLI, MARCO ; MANGANO, VALENTINA ; MARSELLA, MARIA ; NATICCHIONI, LUCA ; PASQUALETTI, ANTONIO ; PEPE, GIOVANNI PIERO ; PERCIBALLI, MAURIZIO ; PESENTI, LUCA ; TOSTA E MELO, I. ; et.al. Casimir energy for N superconducting cavities: a model for the YBCO (GdBCO) sample to be used in the Archimedes experiment. European Physical Journal Plus. v. 137, p. 826, issn: 2190-5444, 2022. Qualis: A2
29. ABBOTT, R. ; ABBOTT, T.'D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. Constraints on dark photon dark matter using data from LIGO?s and Virgo?s third observing run. PHYSICAL REVIEW D. v. 105, p. -, issn: 2470-0010, 2022. Qualis: A1
30. ACERNESE, F ; AGATHOS, M ; AIN, A ; ALBANESI, S ; ALLOCCA, A ; AMATO, A ; ANDRADE, T ; ANDRES, N ; ANDRI', T ; ANSOLDI, S ; ANTIER, S ; ARÈNE, M ; ARNAUD, N ; ASSIDUO, M ; ASTONE, P ; AUBIN, F ; BABAK, S ; BADARACCO, F ; BADER, M K M ; TOSTA E MELO, I. ; et.al. Calibration of advanced Virgo and reconstruction of the detector strain h(t) during the observing run O3. CLASSICAL AND QUANTUM GRAVITY. v. 39, p. 045006, issn: 0264-9381, 2022. Qualis: A1
31. ABBOTT, R. ; ABBOTT, T.'D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AKUTSU, T. ; ALBANESI, S. ; ALLOCCA, A. ; TOSTA E MELO, I. ; et.al. Search for continuous gravitational waves from 20 accreting millisecond x-ray pulsars in O3 LIGO data. PHYSICAL REVIEW D. v. 105, p. ., issn: 2470-0010, 2022. Qualis: A1
32. ABBOTT, R. ; ABBOTT, T.'D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; ALBANESI, S. ; ALLOCCA, A. ; TOSTA E MELO, I. ; et.al. Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO?s and Advanced Virgo?s Third Observing Run. PHYSICAL REVIEW LETTERS. v. 129, p. ., issn: 0031-9007, 2022. Qualis: A1
33. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADKINS, V. K. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs. The Astrophysical Journal. v. 935, p. 1, issn: 0004-637X, 2022. Qualis: A1
34. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADKINS, V.'K. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. All-sky search for gravitational wave emission from scalar boson clouds around spinning black holes in LIGO O3 data. PHYSICAL REVIEW D. v. 105, p. ., issn: 2470-0010, 2022. Qualis: A1
35. ABBOTT, R. ; ABBOTT, T. D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run. The Astrophysical Journal. v. 932, p. 133, issn: 0004-637X, 2022. Qualis: A1
36. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADKINS, V.'K. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data. PHYSICAL REVIEW D. v. 106, p. ., issn: 2470-0010, 2022. Qualis: A1
37. ABBOTT, R ; ABE, H ; ACERNESE, F ; ACKLEY, K ; ADHIKARI, N ; ADHIKARI, R X ; ADKINS, V K ; ADYA, V B ; AFFELDT, C ; AGARWAL, D ; AGATHOS, M ; AGATSUMA, K ; AGGARWAL, N ; AGUIAR, O D ; AIELLO, L ; AIN, A ; AJITH, P ; AKUTSU, T ; ALBANESI, S ; TOSTA E MELO, I. ; et.al. First joint observation by the underground gravitational-wave detector KAGRA with GEO 600. Progress of Theoretical and Experimental Physics. v. 2022, p. ., issn: 2050-3911, 2022. Qualis: A2
38. ACERNESE, F ; AGATHOS, M ; AIN, A ; ALBANESI, S ; ALLOCCA, A ; AMATO, A ; ANDRADE, T ; ANDRES, N ; ANDRÉS-CARCASONA, M ; ANDRI', T ; ANSOLDI, S ; ANTIER, S ; APOSTOLATOS, T ; APPAVURAVTHER, E Z ; ARÈNE, M ; ARNAUD, N ; ASSIDUO, M ; ASSIS DE SOUZA MELO, S ; ASTONE, P ; TOSTA E MELO, I. ; et.al. The Virgo O3 run and the impact of the environment. CLASSICAL AND QUANTUM GRAVITY. v. 39, p. 235009, issn: 0264-9381, 2022. Qualis: A1
39. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADKINS, V.'K. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO-Virgo data. PHYSICAL REVIEW D. v. 106, p. ., issn: 2470-0010, 2022. Qualis: A1
40. ABBOTT, R. ; ABE, H. ; ACERNESE, F. ; ACKLEY, K. ; ADHICARY, S. ; ADHIKARI, N. ; ADHIKARI, R. X. ; ADKINS, V. K. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; ALFAIDI, R. A. ; TOSTA E MELO, I. ; et.al. Model-based Cross-correlation Search for Gravitational Waves from the Low-mass X-Ray Binary Scorpius X-1 in LIGO O3 Data. Astrophysical Journal Letters. v. 941, p. L30, issn: 2041-8205, 2022. Qualis: A1
41. DI PACE, SIBILLA ; MANGANO, VALENTINA ; PIERINI, LORENZO ; REZAEI, AMIRSAJJAD ; HENNIG, JAN-SIMON ; HENNIG, MARGOT ; PASCUCCI, DANIELA ; ALLOCCA, ANNALISA ; TOSTA E MELO, IARA ; NAIR, VISHNU G. ; ORBAN, PHILIPPE ; SIDER, AMEER ; SHANI-KADMIEL, SHAHAR ; VAN HEIJNINGEN, JORIS. Research Facilities for Europe?s Next Generation Gravitational-Wave Detector Einstein Telescope. GALAXIES ? OPEN ACCESS COSMOLOGY, ASTRONOMY & ASTROPHYSICS JOURNAL. v. 10, p. 65, issn: 2075-4434, 2022. Qualis: B1
42. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKCAY, S. ; ALLEN, G. ; TOSTA E MELO, I. ; et.al. GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo during the First Half of the Third Observing Run. Physical Review X. v. 11, p. 2010.14527, issn: 2160-3308, 2021. Qualis: A1
43. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKCAY, S. ; ALLEN, G. ; TOSTA E MELO, I. ; et.al. Tests of general relativity with binary black holes from the second LIGO-Virgo gravitational-wave transient catalog. PHYSICAL REVIEW D. v. 103, p. 122002 (2021), issn: 2470-0010, 2021. Qualis: A1
44. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; ALLEN, G. ; ALLOCCA, A. ; TOSTA E MELO, I. ; et.al. Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog. Astrophysical Journal Letters. v. 913, p. L7, issn: 2041-8205, 2021. Qualis: A1
45. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AICH, A. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; ALLEN, G. ; ALLOCCA, A. ; TOSTA E MELO, I. ; et.al. Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3a. The Astrophysical Journal. v. 915, p. 86, issn: 0004-637X, 2021. Qualis: A1
46. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; ALEMAN, K.'M. ; TOSTA E MELO, I. ; et.al. All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems. PHYSICAL REVIEW D. v. 103, p. 064017 (2021), issn: 2470-0010, 2021. Qualis: A1
47. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; TOSTA E MELO, I. ; et.al. Diving below the Spin-down Limit: Constraints on Gravitational Waves from the Energetic Young Pulsar PSR J0537-6910. Astrophysical Journal Letters. v. 913, p. L27, issn: 2041-8205, 2021. Qualis: A1
48. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AKUTSU, T. ; ALEMAN, K.'M. ; TOSTA E MELO, I. ; et.al. Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo?s third observing run. PHYSICAL REVIEW D. v. 104, p. 022004 (2021), issn: 2470-0010, 2021. Qualis: A1
49. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; TOSTA E MELO, I. ; et.al. Constraints on Cosmic Strings Using Data from the Third Advanced LIGO-Virgo Observing Run. PHYSICAL REVIEW LETTERS. v. 126, p. 241102 (2021), issn: 0031-9007, 2021. Qualis: A1
50. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; TOSTA E MELO, I. ; et.al. Observation of Gravitational Waves from Two Neutron Star-Black Hole Coalescences. Astrophysical Journal Letters. v. 915, p. L5, issn: 2041-8205, 2021. Qualis: A1
51. ALLOCCA, A. ; BERBELLINI, A. ; BOSCHI, L. ; CALLONI, E. ; CARDELLO, G. L. ; CARDINI, A. ; CARPINELLI, M. ; CONTU, A. ; D?ONOFRIO, L. ; D?URSO, D. ; DELL?AQUILA, D. ; ROSA, R. DE ; FIORE, L. DI ; GIOVANNI, M. DI ; PACE, S. DI ; ERRICO, L. ; FIORI, I. ; GIUNCHI, C. ; GRADO, A. ; TOSTA E MELO, I. ; et.al. Seismic glitchness at Sos Enattos site: impact on intermediate black hole binaries detection efficiency. European Physical Journal Plus. v. 136, p. 511, issn: 2190-5444, 2021. Qualis: A2
52. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; TOSTA E MELO, I. ; et.al. Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo?s first three observing runs. PHYSICAL REVIEW D. v. 104, p. -, issn: 2470-0010, 2021. Qualis: A1
53. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; TOSTA E MELO, I. ; et.al. Constraints from LIGO O3 Data on Gravitational-wave Emission Due to R-modes in the Glitching Pulsar PSR J0537-6910. The Astrophysical Journal. v. 922, p. 71, issn: 0004-637X, 2021. Qualis: A1
54. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; ALEMAN, K. M. ; TOSTA E MELO, I. ; et.al. Search for Lensing Signatures in the Gravitational-Wave Observations from the First Half of LIGO-Virgo?s Third Observing Run. The Astrophysical Journal. v. 923, p. 14, issn: 0004-637X, 2021. Qualis: A1
55. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; TOSTA E MELO, I. ; et.al. Searches for Continuous Gravitational Waves from Young Supernova Remnants in the Early Third Observing Run of Advanced LIGO and Virgo. The Astrophysical Journal. v. 921, p. 80, issn: 0004-637X, 2021. Qualis: A1
56. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; TOSTA E MELO, I. ; et.al. All-sky search for continuous gravitational waves from isolated neutron stars in the early O3 LIGO data. PHYSICAL REVIEW D. v. 104, p. ., issn: 2470-0010, 2021. Qualis: A1
57. ABBOTT, R. ; ABBOTT, T.'D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. All-sky search for short gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run. PHYSICAL REVIEW D. v. 104, p. ., issn: 2470-0010, 2021. Qualis: A1
58. ABBOTT, R. ; ABBOTT, T.'D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run. PHYSICAL REVIEW D. v. 104, p. ., issn: 2470-0010, 2021. Qualis: A1
59. ABBOTT, R. ; ABBOTT, T.'D. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, N. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGARWAL, D. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKUTSU, T. ; ALBANESI, S. ; TOSTA E MELO, I. ; et.al. All-sky search for long-duration gravitational-wave bursts in the third Advanced LIGO and Advanced Virgo run. PHYSICAL REVIEW D. v. 104, p. ., issn: 2470-0010, 2021. Qualis: A1
60. HAMBURG, R. ; FLETCHER, C. ; BURNS, E. ; GOLDSTEIN, A. ; BISSALDI, E. ; BRIGGS, M. S. ; CLEVELAND, W. H. ; GILES, M. M. ; HUI, C. M. ; KOCEVSKI, D. ; LESAGE, S. ; MAILYAN, B. ; MALACARIA, C. ; POOLAKKIL, S. ; PREECE, R. ; ROBERTS, O. J. ; VERES, P. ; VON KIENLIN, A. ; WILSON-HODGE, C. A. ; TOSTA E MELO, I. ; et.al. A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers from the First and Second Gravitational-wave Observing Runs. The Astrophysical Journal. v. 893, p. 100, issn: 1538-4357, 2020. Qualis: A1
61. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AICH, A. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKCAY, S. ; ALLEN, G. ; TOSTA E MELO, I. ; et.al. GW190412: Observation of a binary-black-hole coalescence with asymmetric masses. PHYSICAL REVIEW D. v. 102, p. LIGO-P190412, issn: 2470-0010, 2020. Qualis: A1
62. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AICH, A. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKCAY, S. ; ALLEN, G. ; TOSTA E MELO, I. ; et.al. GW190814: Gravitational Waves from the Coalescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object. The Astrophysical Journal. v. 896, p. L44, issn: 2041-8213, 2020. Qualis: A1
63. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, A. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; ALLEN, G. ; ALLOCCA, A. ; TOSTA E MELO, I. ; et.al. Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars. The Astrophysical Journal. v. 902, p. L21, issn: 2041-8213, 2020. Qualis: A1
64. ABBOTT, R. ; ABBOTT, T.'D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, R.'X. ; ADYA, V.'B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O.'D. ; AICH, A. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKCAY, S. ; ALLEN, G. ; TOSTA E MELO, I. ; et.al. GW190521: A Binary Black Hole Merger with a Total Mass of 150 - - M -. PHYSICAL REVIEW LETTERS. v. 125, p. 2009.01075, issn: 0031-9007, 2020. Qualis: A1
65. ABBOTT, R. ; ABBOTT, T. D. ; ABRAHAM, S. ; ACERNESE, F. ; ACKLEY, K. ; ADAMS, C. ; ADHIKARI, R. X. ; ADYA, V. B. ; AFFELDT, C. ; AGATHOS, M. ; AGATSUMA, K. ; AGGARWAL, N. ; AGUIAR, O. D. ; AICH, A. ; AIELLO, L. ; AIN, A. ; AJITH, P. ; AKCAY, S. ; ALLEN, G. ; TOSTA E MELO, I. ; et.al. Properties and Astrophysical Implications of the 150 M - Binary Black Hole Merger GW190521. The Astrophysical Journal. v. 900, p. L13, issn: 2041-8213, 2020. Qualis: A1
66. RASTELLO, S ; AMARO-SEOANE, P ; ARCA-SEDDA, M ; CAPUZZO-DOLCETTA, R ; FRAGIONE, G ; TOSTA E MELO, I. Stellar black hole binary mergers in open clusters. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. v. 483, p. 1233-1246, issn: 0035-8711, 2019. Qualis: A1
67. CAPUZZO-DOLCETTA, R. ; TOSTA E MELO, I.. On the relation between the mass of Compact Massive Objects and their host galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. v. 472, p. 4013-4023, issn: 0035-8711, 2017. Qualis: A1
68. TOSTA E MELO, I; CAPUZZO-DOLCETTA, R. Scaling Correlations Amoung Central Massive Objects and Their Host Galaxies. JOURNAL OF PHYSICS. CONFERENCE SERIES (PRINT). v. 689, p. 012008, issn: 1742-6588, 2016. Qualis: Não identificado (JOURNAL OF PHYSICS. CONFERENCE SERIES)
69. TOSTA E MELO, I; CAPUZZO-DOLCETTA, R. Compact Massive Objects in galaxies. MEMORIE DELLA SOCIETA ASTRONOMICA ITALIANA (ONLINE). v. 87, p. 703, issn: 1824-016X, 2016.Qualis: B3
70. CAPRONI, A. ; MELO, I. T. E. ; ABRAHAM, Z. ; MONTEIRO, H. ; ROLAND, J.. Kinematic study of the parsec-scale jet of the quasar PKS 1741-03. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. v. 441, p. 187-202, issn: 0035-8711, 2014. Qualis: A1
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1. AGAYEVA, S. ; AIVAZYAN, V. ; ALISHOV, S. ; ALMUALLA, M. ; ANDRADE, 'C. ; ANTIER, SARAH ; BAI, J.-M. ; BARANSKY, A. ; BASA, S. ; BENDJOYA, P. ; BENKHALDOUN, Z. ; BERADZE, S. ; BEREZIN, D. ; BHARDWAJ, U. ; BLAZEK, M. ; BURKHONOV, O. ; BURNS, E. ; CAUDILL, S. ; CHRISTENSEN, N. ; TOSTA E MELO, I. ; et.al. The GRANDMA network in preparation for the fourth gravitational-wave observing run. Em: Observatory Operations: Strategies, p. 52, 2022.
2. TOSTA E MELO, IARA. Search for multi-messenger events during LIGO/Virgo era. Em: The European Physical Society Conference on High Energy Physics, p. 111, 2021.
3. TOSTA E MELO, I; CAPUZZO-DOLCETTA, R. Compact Massive Object in Galaxies. Em: Mem. S.A.It, v. 75, 2016.
Resumos expandidos publicados em anais de congressos (0)
Resumos publicados em anais de congressos (0)
Artigos aceitos para publicação (0)
Apresentações de trabalho (16)
1. TOSTA E MELO, I. Gravitational Waves data analysis. 2024. Apresentação de Trabalho/Conferência ou palestra
2. TOSTA E MELO, I. Prespectives on MM astronomy in the new era of Telescopes. 2023. Apresentação de Trabalho/Conferência ou palestra
3. TOSTA E MELO, I. Search for GW in coincidence with burst sources during 03. 2022. Apresentação de Trabalho/Conferência ou palestra
4. TOSTA E MELO, I. Search for GW and multimessenger events during LIGO/Virgo era. 2022. Apresentação de Trabalho/Conferência ou palestra
5. TOSTA E MELO, I. GRANDMA GRB campaign. Work package - C (Photometry & Spectroscopy Tools). 2022. Apresentação de Trabalho/Conferência ou palestra
6. I. TOSTA E MELO. Search for multi-messenger events during LIGO/Virgo era. 2021. Apresentação de Trabalho/Seminário
7. I. TOSTA E MELO. Sar-Grav Laboratory and the third generation of gravitational waves detectors. 2021. Apresentação de Trabalho/Seminário
8. TOSTA E MELO, I. Massive objects in their multiple environments. 2017. Apresentação de Trabalho/Conferência ou palestra
9. TOSTA E MELO, I.; CAPUZZO-DOLCETTA, R.. Compact Massive Objects in Galaxies. 2016. Apresentação de Trabalho/Congresso
10. TOSTA E MELO, I. CMO in Galaxies. 2016. Apresentação de Trabalho/Seminário
11. TOSTA E MELO, I.; CAPUZZO-DOLCETTA, R.. Compact Massive Objects and the Scaling Correlations with their Host Galaxies. 2016. Apresentação de Trabalho/Congresso
12. RASTELLO, S. ; TOSTA E MELO, I. ; ARCA-SEDDA, M. ; CAPUZZO-DOLCETTA, R. ; FRAGIONE, G.. Stellar Black Hole Binary Merging in Open Clusters. 2016. Apresentação de Trabalho/Congresso
13. TOSTA E MELO, I.; CAPUZZO-DOLCETTA, R.. Scaling Correlations Among Central Massive Objects and Their Host Galaxies. 2015. Apresentação de Trabalho/Congresso
14. TOSTA E MELO, I.; Caproni. A. Estudando a cinemática do Jato do Quasar PKS 1741-03 em escalas de Parsec. 2012. Apresentação de Trabalho/Congresso
15. TOSTA E MELO, I.; Caproni. A. Kinematic analysis of 15 GHz interferometric images of the quasar PSK-1741-038. 2012. Apresentação de Trabalho/Conferência ou palestra
16. TOSTA E MELO, I.; GIANNINI, H. ; BOTTI, L. C. L.. Morofologia de rádio fontes que apresentam jatos. 2010. Apresentação de Trabalho/Simpósio
Demais tipos de produção bibliográfica (4)
1. TOSTA E MELO, I. Astronomy through the ages: an overview!. 2018. Outreach Publications and Contributions
2. TOSTA E MELO, I. From optical to extragalactic astronomy. 2018. Outreach Publications and Contributions
3. TOSTA E MELO, I. Extragalactic astronomy. 2018. Outreach Publications and Contributions
4. TOSTA E MELO, I. A galaxy and its structures. 2018. Outreach Publications and Contributions

Produção técnica

Programas de computador com registro (0)
Programas de computador sem registro (0)
Produtos tecnológicos (0)
Processos ou técnicas (0)
Trabalhos técnicos (0)
Demais tipos de produção técnica (0)

Produção artística

Total de produção artística (0)

Orientações em andamento

Supervisão de pós-doutorado (0)
Tese de doutorado (0)
Dissertação de mestrado (0)
Monografia de conclusão de curso de aperfeiçoamento/especialização (0)
Trabalho de conclusão de curso de graduação (0)
Iniciação científica (0)
Orientações de outra natureza (0)

Supervisões e orientações concluídas

Supervisão de pós-doutorado (0)
Tese de doutorado (0)
Dissertação de mestrado (0)
Monografia de conclusão de curso de aperfeiçoamento/especialização (0)
Trabalho de conclusão de curso de graduação (0)
Iniciação científica (0)
Orientações de outra natureza (0)

Projetos de pesquisa

Total de projetos de pesquisa (15)
1. 2024-Atual. VirgoBR
  Descrição: Since I joined the LVK collaboration, I established contacts in my home country to form a group focused on experimental GWs astronomy. Through different collaborations, I was able to put together a group whose members are from 5 different Universities in Brazil (UNESP, ITA, UNIFEI, UNIFAL, and UFRN) and myself. The group was approved by the Virgo Scientific Committee August this year with me as its leader: the first non-European group to join Virgo collaboration. The group brings together my experience in GW multi-messenger astronomy and other members' backgrounds in theoretical astrophysics (from formalisms to probe gravity to alternative theories of gravity).. Situação: Em andamento; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Coordenador / cassius de melo - Integrante / Marcio Alves - Integrante / eduardo bittencourt - Integrante / Leo Medeiros - Integrante / Pedro Pompeia - Integrante / Rodrigo Cuzinatto - Integrante.
  Membro: Iara Tosta e Melo.
2. 2023-Atual. KM3Net - multimessenger studies
  Descrição: Searches for neutrinos associated with GW signals from compact binary mergers have already been performed with neutrino telescopes such as ANTARES (Adrian-Martinez et al. 2016), and its successor, the KM3Net telescope is currently under construction. Recently, an exceptionally high-energy event was observed by KM3NeT, which is associated with cosmic neutrino detection: muon with an estimated energy of about 12 petaelectronvolts (PeV) (Nature 2025, here figure 4), the first one of its kind. KM3Net infrastructures are composed of two detectors: ARCA detector is located offshore Portopalo di Capo Passero, Sicily, Italy, at a depth of about 3,450#8201;m and its geometry is optimized for the study of high-energy cosmic neutrinos. The ORCA detector is located at a depth of about 2,450#8201;m, offshore Toulon, France, and is optimized for the study of neutrino oscillations. Both detectors are under construction but already operational, and once completed, they will comprise 345 (230 for ARCA and 115 for ORCA) vertical detection lines, each holding 18 optical modules. Both detectors can identify all flavours of neutrino interactions: long-lived muons, denominated tracks, and those denominated showers.. Situação: Em andamento; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Coordenador / cassius de melo - Integrante / Marcio Alves - Integrante.
  Membro: Iara Tosta e Melo.
3. 2023-Atual. FAPEMIG Grant, Edital No 009/2023
  Descrição: Awarded with fundings for international collaboration/mobility. The "Fundação de Amparo àPesquisa do Estado de Minas Gerais" (FAPEMIG Agency) funds programs for the dissemination of scientific research results between researches.. Situação: Em andamento; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Coordenador / cassius de melo - Integrante.
  Membro: Iara Tosta e Melo.
4. 2023-Atual. FAPEMIG Grant, Edital No 009/2023
  Descrição: Awarded with fundings for international collaboration/mobility. The "Fundação de Amparo àPesquisa do Estado de Minas Gerais" (FAPEMIG Agency) funds programs for the dissemination of scientific research results between researches.. Situação: Em andamento; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Coordenador / cassius de melo - Integrante.
  Membro: Iara Tosta e Melo.
5. 2023-Atual. FAPEMIG Grant, Edital No 009/2023
  Descrição: Awarded with fundings for international collaboration/mobility. The "Fundação de Amparo àPesquisa do Estado de Minas Gerais" (FAPEMIG Agency) funds programs for the dissemination of scientific research results between researches.. Situação: Em andamento; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Coordenador / cassius de melo - Integrante.
  Membro: Iara Tosta e Melo.
6. 2023-Atual. FAPEMIG Grant, Edital No 009/2023
  Descrição: Awarded with fundings for international collaboration/mobility. The "Fundação de Amparo àPesquisa do Estado de Minas Gerais" (FAPEMIG Agency) funds programs for the dissemination of scientific research results between researches.. Situação: Em andamento; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Coordenador / cassius de melo - Integrante.
  Membro: Iara Tosta e Melo.
7. 2022-2025. Erasmus+ International Credit Mobility Action (KA171)
  Descrição: Funding awarded for international mobility between UNISS and UNIFEI (Brazil). The projecthas a duration of 3 year. Situação: Concluído; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Coordenador / eduardo bittencourt - Integrante.
  Membro: Iara Tosta e Melo.
8. 2021-Atual. GRANDMA
  Descrição: Since the first detection of gravitational waves (GWs) in 2015, physics and astronomy have entered a new era in which diverse messengers ? photons, neutrinos, cosmic rays and gravitational waves ? provide a new picture of the Universe. On 17 August 2017, multi-messenger observations of the coalescence of two neutron stars demonstrated the potential to test different astrophys- ical scenarios, collect information on the dynamics of the astrophysical system with GWs, provide a new way to measure the expansion rate of the Universe and study the properties of matter under extreme conditions1. Multi-messenger astronomy is a rapidly growing field thanks to the increasing sensitivity of GW detectors, the emergence of the next generation of neutrino detec- tors and the new electromagnetic surveys boosting the number of alerts and discovery opportunities. However, the complexity of these instruments (in particular that of GW interferometers and neutrino detectors) brings observational challenges, leading to a time race to use telescopes and requiring simulation and data analysis tools from distinct fields of physics and astron- omy in order to enable scientific discovery. Based on experience from the second observing run of LIGO and Virgo, there are three main issues that require immediate attention: the coordination of rapid obser- vations of large sky localizations from GWs and γ-ray observatories, the computational resources for online data analysis of telescope signals and images, and a community effort to share reports and data releases on longer timescales. GRANDMA aims to overcome these observational, operational and data analysis challenges by harnessing resources from professional and amateur telescope networks and bringing together experts from different fields.. Situação: Em andamento; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Coordenador / Sarah Antier - Integrante.
  Membro: Iara Tosta e Melo.
9. 2021-Atual. Virgo, ET, SarGrav
  Descrição: Virgo and EGO is scientific forum - the VESF - for astrophysicists and theorists, dedicated specifically to the furthering of scientific knowledge related to Virgo. Virgo is an interferometric gravitational-wave antenna. It consists of two 3-kilometre-long arms, which house the various machinery required to form a laser interferometer. The Einstein Telescope (ET), on the other hand, project is dedicated to the development of a critical research infrastructure for a third-generation gravitational-wave interferometer. The surroundings of Sos Enattos mine in Sardinia is being considered as a possible location for ET due to its very low seismic and anthropogenic noise. Such local characteristics allowed the construction of the Sar-Grav laboratory which aims to host underground experiments including low seismic noise experiments, cryogenic payloads, low frequency, and cryogenic sensor development. Nonetheless, a fundamental physics experiment, Archimedes, is the first experiment already under installation in the surface area.. Situação: Em andamento; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Integrante / Domenico D'Urso - Coordenador / Annalisa alloca - Integrante / Enrico Calloni - Integrante / Davide Rozza - Integrante.
  Membro: Iara Tosta e Melo.
10. 2020-Atual. High energy multi-messenger astrophysics
  Descrição: Today we are in a historically exciting period for the study of the Universe as we can observe the whole spectrum of cosmic messengers and explore the Universe with cosmic rays, neutrinos, and GWs. The first observations from the inspiral and merger of a BBH system by the advanced LIGO interferometers marked the onset of GW astronomy (GW150914, Abbott et al. 2016). On 17 August 2017, multi-messenger (MM) astronomy related to GWs had its breakthrough: the LIGO-Virgo network observed a GW signal of two low-mass neutron stars (NS) associated with a gamma-ray burst detected by Fermi-GBM (GW170817, GRB170817A, Abbott et al. 2017a,b). This was a phenomena of rare violence (Figure 1): the matter was expelled in all directions and at velocities close to the speed of light. New heavy atomic nuclei were synthesized by the rapid capture of neutrons and their disintegration heated the ejecta. Its cooling producing radiation, lead to the emission of a kilonova (KN-AT2017gfo, (Andreoni et al. 2017)), observable in detail for the first time. Almost simultaneously, an accretion disk, resulting from the debris of the neutron stars, was formed around the new compact object. In a still unknown mechanism, a jet of matter pointing towards the Earth was emitted and detected by space-based gamma-ray detectors in the form of a gamma-ray burst (GRB170817A). The slowing down of the jet by the interstellar medium produced photons at all wavelengths.. Situação: Em andamento; Natureza: Pesquisa. Alunos envolvidos: Mestrado acadêmico: (3) Doutorado: (4) . Integrantes: Iara Tosta e Melo - Coordenador / cassius de melo - Integrante.
  Membro: Iara Tosta e Melo.
11. 2019-2021. Virgo and EGO/ET.
  Descrição: Virgo and EGO is scientific forum - the VESF - for astrophysicists and theorists, dedicated specifically to the furthering of scientific knowledge related to Virgo.Virgo is an interferometric gravitational-wave antenna. It consists of two 3-kilometre-long arms, which house the various machinery required to form a laser interferometer.The Einstein Telescope (ET), on the other hand, project is dedicated to the development of a critical research infrastructure for a third-generation gravitational-wave interferometer. Situação: Concluído; Natureza: Pesquisa. Integrantes: Iara Tosta e Melo - Integrante / Domenico D'Urso - Coordenador.
  Membro: Iara Tosta e Melo.
12. 2015-2019. Stellar Black Hole Binary Mergers in Open Clusters
  Descrição: A study of the evolution of a primordial black hole binary (BHB) in a sample of over 1500 direct-summation N-body simulations of small-and intermediate-size isolated star clusters as proxies of galactic open clusters. The BHBs have masses in the range of the first LIGO/Virgo detections. Some of our models show a significant hardening of the BHB in a relatively short time. Some of them merge within the cluster, while ejected binaries, typically, have exceedingly long merger timescales. The perturbation of stars around BHB systems is key to induce their coalescence. The BHBs which merge in the cluster could be detected with a delay of a few years between space detectors, as future LISA, and ground-based ones, due to their relatively high eccentricity. We estimate a BHB merger rate of about 2 yr^-1 Gpc^-3. We also noticed that in many cases the BHB triggers tidal disruption events which, however, are not linked to the GW emission. Open cluster-like systems are, hence, a promising environment for GWs from BHBs and tidal disruptions.. Situação: Concluído; Natureza: Pesquisa. Alunos envolvidos: Doutorado: (5) . Integrantes: Iara Tosta e Melo - Integrante / Sara Rastello - Integrante / Manuel Arca-Sedda - Integrante / GIACOMO FRAGIONE - Integrante / CAPUZZO-DOLCETTA, R - Coordenador / Pau Amaro-Seoane - Integrante.
  Membro: Iara Tosta e Melo.
13. 2014-2018. CMOs and their host galaxies
  Descrição: Galaxies belonging to the entire Hubble sequence show the presence of MBH and/or very dense stellar clusters, commonly referred as NSC, in their centers. NSC and MBH have a long study history, and significant progress has been made regarding their understanding. Many fundamental problems, however, are still open and new physical studies are needed for this matter. Both objects seem to follow similar host-galaxy correlations, suggesting that they are 'faces of the same coin': the family of compact massive objects (CMOs). In this context, I dedicated our attention to the investigation of scaling relations behind the largest set of data published so far with an astrophysical context involving CMOs and their host galaxy properties. Such correlations may indicate a direct link between large galactic spatial scales and the much smaller scales of the nuclear environment. Such study was possible due to the growing quantity of high-resolution data, in the last few years, focused on the central region of galaxies. Thanks to the images provided by the Hubble Space Telescope and Advanced Camera Survey, it is clear now that the nuclei of the majority of both elliptical and spiral galaxies (M > 10^10 solar masses) harbour a massive or a supermassive black hole (SMBH), with mass between M > 10^6 - 10^10 solar masses. NSCs on the other hand, are most common in fainter galaxies than in brighter ones in a wide galaxy mass range. It is also well known that both types can be found in the intermediate mass galaxies range where the central MBH is surrounded by the NSC. In an attempt to shed light on this astrophysical open question, I have collected here the most extensive data set containing NSCs and MBHs, with a total amount of more than 700 objects. In particular, the attention was directed to some differences between the correlations of NSC and MBH as subsets of CMOs with hosting galaxies making an analytical discussion between them on various different relations: M_CMO-M_B, M_CMO-M_g and M_CMO-sigma. Also, a thorough comparison of NSC and MBH relations was made and there was found a significant difference between the 2 sets. In this context, the slopes found for the M_NSC vs. M_B relation are very similar to those already obtained in previous similar studies, but with a much greater number of objects. Also, the slopes of the relation CMO mass vs. host galaxy B magnitude of the two types of CMOs are indistinguishable within the errors. On the other hand, the relation NSC mass-host galaxy mass relation is significantly smaller than for MBHs, the first stop being b_NSC = 0.66 against a slope of b_{MBH} = 1.04, suggesting that they do not share the same evolutionary path. It appears that the NSC formation in early-type galaxies is consistent with the GC dry-merger scenario, despite the fact that the GC accretion model still fails to explain why the nucleation fraction goes down at the faint end where dynamical friction should be more efficient. The mass-velocity dispersion relation plays a relevant role because it seems to be the one that better shows a clearer difference between the MBHs and NSCs. The M_MBH vs. sigma has a slope of 5.19 while M_NSC vs. sigma has the much smaller slope, 1.84. A small slope for the NSC - sigma relation in the regime of dynamical friction dominated infall process is expected than that one presented by the MBH} - sigma relation. In fact, the small slope found in my studies of over the various sets of data gave strong support to the GC infall-merger scenario of NSC formation.. Situação: Concluído; Natureza: Pesquisa. Alunos envolvidos: Graduação: (0) / Especialização: (0) / Mestrado acadêmico: (0) / Mestrado profissional: (0) / Doutorado: (1) . Integrantes: Iara Tosta e Melo - Integrante / CAPUZZO-DOLCETTA, R - Coordenador.
  Membro: Iara Tosta e Melo.
14. 2011-2013. Kinematic study of the parsec-scale jet of the quasar PKS 1741-03
  Descrição: the quasar PKS 1741-03 (OT 068) exhibits strong flux density fluctuations at radio wavelengths, and those that occur at shorter time-scales have been attributed to refractive interstellar scintillation phenomena. Located at redshift z ∼ 1.054, PKS 1741-03 shows a core-like radio morphology at kiloparsec scales, meaning that its brightness distribution is compatible with an unresolved source. An inconspicuous jet, in which a few discrete components, have been identified on PKS 1741-03 as well. In this matter, I analysed the jet of 1741-03 using a statistical technique known as cross-entropy. Such approach indicated the presence of a central component, identified as the core region (the most strong component in terms of flux density in all the 21 epochs and respon- sible for 56?95 percent of the total flux density of PKS 1741-03), and two to five (usually two) jet components per image.. Situação: Concluído; Natureza: Pesquisa. Alunos envolvidos: Mestrado acadêmico: (1) . Integrantes: Iara Tosta e Melo - Integrante / CAPRONI, A. - Coordenador.
  Membro: Iara Tosta e Melo.
15. 2009-2011. O centro galáctico
  Descrição: O Centro da Nossa Galáxia possui um comportamento semelhante ao dos quasares, que são objetos que estão à distâncias colossais da Terra. Acredita-se que tanto nos quasares distantes como no Centro de Nossa Galáxia (que se encontra muito mais próxima), exista um buraco-negro super-massivo. No caso dos quasares, o buraco- negro deve ter bilhões de massas solares, enquanto que a Nossa Galáxia, possui cerca de milhões de massas solares. Foi realizado um estudo comparativo desses dois objetos para entender melhor os Núcleos Galácticos Ativos (AGN).. Situação: Concluído; Natureza: Pesquisa. Alunos envolvidos: Graduação: (2) . Integrantes: Iara Tosta e Melo - Integrante / Henrique Giannini - Integrante / Luiz Claudio Lima Botti - Coordenador.
  Membro: Iara Tosta e Melo.

Prêmios e títulos

Total de prêmios e títulos (0)

Participação em eventos

Total de participação em eventos (19)

XVI Seminar on Software for Nuclear, Subnuclear and Applied Physics. 2019. (Outra).
12th Astro-GR event. Stellar Black Hole Binary Mergers in Open Clusters. 2017. (Congresso).
Gravitational Waves Workshop. 2017. (Oficina).
New Frontiers in Gravitation-Waves Astrophysics. 2017. (Congresso).
The 2017 edition of the Workshop of the Ph.D. students in Astronomy, Astrophysics, and Space Science.Massive objects in their multiple environments. 2017. (Simpósio).
631. Wilhelm und Else Heraeus-Seminar: Stellar aggregates over mass and spatial scales..Stellar Black Hole Binary Merging in Open Clusters. 2016. (Seminário).
631. Wilhelm und Else Heraeus-Seminar: Stellar aggregates over mass and spatial scales..Compact Massive Objects and the Scaling Correlations with their Host Galaxies. 2016. (Seminário).
Perspectives of GPU Computing in Science. 2016. (Seminário).
PhD program in Astronomy, astrophysics and space science workshop..CMO in Galaxies. 2016. (Seminário).
Star Cluster as Cosmic Laboratories for Astrophysics, Dynamics and Fundamental Physics ? MODEST 16. Compact Massive Objects in Galaxies. 2016. (Congresso).
Marcel Grossmann Meeting MG14. 2015. (Seminário).
YRM ? Young Researcher Meeting. Scaling Correlations Among Central Massive Objects and Their Host Galaxies. 2015. (Congresso).
International Workshop. 2014. (Congresso).
The Alajar Meeting. 2014. (Encontro).
Conferência e workshop em homenagem a Professora Dra. Miriani G. Patoriza, Galactic Nuclei and their connection with stars and the environment..Kinematic analysis of 15 GHz interferometric images of the quasar PSK-1741-038. 2012. (Outra).
I NAT Lectures on Astrophysics Collapsing or Colliding Systems: Solving the Galactic Puzzle.. 2012. (Congresso).
SAB 2012 - Sociedade Astronômica Brasileira -. Estudando a cinemática do Jato do Quasar PKS 1741-03 em escalas de Parsec. 2012. (Congresso).
XVI Advanced School on Astrophysic. 2012. (Congresso).
SICINPE 2010.Morofologia de rádio fontes que apresentam jatos. 2010. (Simpósio).

Organização de eventos

Total de organização de eventos (7)

TOSTA E MELO, I. MAYORANA (Multi-Aspect Young ORiented Advanced Neutrino Academy) School&Workshops II edition - in preparation. 2025. (Congresso).. . 0.
TOSTA E MELO, I. South American Gravitational Waves Conference: 10 Years 1st Since GW Detection - in preparation. 2025. (Congresso).. . 0.
TOSTA E MELO, I. PPGF UNIFAL-MG/UFSJ International Conference on Multimessenger Astrophysics. 2024. (Congresso).. . 0.
TOSTA E MELO, I. 1st Astrophysics in the New Era of Multi Messenger Astronomy International Conference. 2023. (Congresso).. . 0.
TOSTA E MELO, I. ET - Site Studies and Characterization workshop. 2021. (Congresso).. . 0.
TOSTA E MELO, I.; DURSO, D. ; Sipala, V.. 10th Einstein Telescope Symposium. 2019. Congresso
DURSO, D. ; TOSTA E MELO, I. ; Sipala, V.. Vacuum Fluctuations at Nanoscale and Gravitation: theory and experiments. 2019. Congresso

Lista de colaborações

Colaborações endôgenas (0)

(*) Relatório criado com produções desde 1914 até 2114
Data de processamento: 16/05/2025 09:40:42

Relatório gerado por scriptLattes V9. Os resultados podem ser afetados por possíveis falhas decorrentes de inconsistências no preenchimento dos Currículos Lattes. E-mail de contato: icamps@unifal-mg.edu.br