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Results 1 - 6 of 6
On the Use of Field RR Lyrae as Galactic Probes. II. A new $Delta$S calibration to estimate their metallicity. (arXiv:2012.02284v1 [astro-ph.SR])
Volume 15, Issue 50 - article #6
J. Crestani
(1,2,3),
M. Fabrizio
(3,4),
V.F. Braga
(3,4),
C. Sneden
(5),
G.W. Preston
(6),
I. Ferraro
(3),
G. Iannicola
(3),
G. Bono
(2,3),
A. Alves-Brito
(1),
M. Nonino
(7),
V. D'Orazi
(8,9),
L. Inno
(10),
M. Monelli
(11),
J. Storm
(12),
G. Altavilla
(3,4),
B. Chaboyer
(13),
M. Dall'Ora
(14),
G. Fiorentino
(3),
C.K. Gilligan
(13),
E. Grebel
(15),
H. Lala
(16),
B. Lemasle
(16),
M. Marengo
(17),
S. Marinoni
(3,4),
P.M. Marrese
(3,4),
C.E. Martínez-Vázquez
(18),
N. Matsunaga
(19),
J.P. Mullen
(17),
J. Neeley
(20),
Z. Prudil
(15),
R. da Silva
(3,4),
P.B. Stetson
(21),
F. Thévenin
(15),
E. Valenti
(22),
A.R. Walker
(18),
M. Zoccali
(23,24)
((1) Departamento de Astronomia, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil,
(2) Dipartimento di Fisica, Università di Roma Tor Vergata, Roma, Italy,
(3) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(4) Space Science Data Center, Roma, Italy,
(5) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(6) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(7) INAF-Osservatorio Astronoico di Trieste, Trieste, Italy,
(8) INAF-Osservatorio Astronomico di Padova, Padova, Italy,
(9) School of Physics, Astronomy, Monash University, Clayton, Melbourne, Australia,
(10) Università degli Studi di Napoli "Parthenope'', Napoli, Italy,
(11) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(12) Leibniz-Institut für Astrophysik Potsdam, Potsdam, Germany,
(13) Department of Physics, Astronomy, Dartmouth College, Hanover, USA,
(14) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(15) Université de Nice Sophia-antipolis, CNRS, Observatoire de la Côte d'Azur, Laboratoire Lagrange, Nice, France,
(16) Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Heidelberg, Germany,
(17) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(18) Cerro Tololo Inter-American Observatory, NSF's National Optical-Infrared Astronomy Research Laboratory, La Serena, Chile,
(19) Department of Astronomy, The University of Tokyo, Tokyo, Japan,
(20) Department of Physics, Florida Atlantic University, Boca Raton, FL, USA,
(21) Herzberg Astronomy, Astrophysics, National Research Council, Victoria, BC, Canada,
(22) European Southern Observatory, Garching bei Munchen, Germany,
(23) Instituto Milenio de Astrofísica, Santiago, Chile,
(24) Pontificia Universidad Catolica de Chile, Instituto de Astrofisica, Santiago, Chile)
http://arxiv.org/abs/2012.02284
On a new method to estimate distance, reddening and metallicity of RR Lyrae stars using optical/near-infrared ($B$,$V$,$I$,$J$,$H$,$K$) mean magnitudes: $omega$ Centauri as a first test case. (arXiv:1811.07069v1 [astro-ph.SR])
Volume 13, Issue 47 - article #2
G. Bono
(1, 2),
G. Iannicola
(2),
V.F. Braga
(3, 4),
I. Ferraro
(2),
P.B. Stetson
(5),
D. Magurno
(1),
N. Matsunaga
(6),
R.L. Beaton
(7),
R. Buonanno
(8),
B. Chaboyer
(9),
M. Dall'Ora
(10),
M. Fabrizio
(2, 11),
G. Fiorentino
(12),
W.L. Freedman
(13,7),
C.K. Gilligan
(9),
B.F. Madore
(7),
M. Marconi
(10),
M. Marengo
(14),
S. Marinoni
(2, 11),
P. Marrese
(2, 11),
C.E. Martinez-Vazquez
(15),
M. Mateo
(16),
M. Monelli
(17, 18),
J.R. Neeley
(19),
M. Nonino
(20),
C. Sneden
(21),
F. Thevenin
(22),
E. Valenti
(23),
A.R. Walker
(15)
((1) Department of Physics, Università di Roma Tor Vergata, Roma, Italy,
(2) INAF-Osservatorio Astronomico di Roma, Monte Porzio Catone, Italy,
(3) Instituto Milenio de Astrofisica, Santiago, Chile,
(4) Departamento de Fisica, Facultad de Ciencias Exactas, Universidad Andres Bello, Santiago, Chile,
(5) NRC-Herzberg, Dominion Astrophysical Observatory, Victoria BC, Canada,
(6) Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Nagano Japan,
(7) The Observatories of the Carnegie Institution for Science, Pasadena, CA, USA,
(8) INAF-Osservatorio Astronomico d'Abruzzo, Teramo, Italy,
(9) Department of Physics, Astronomy, Dartmouth College, Hanover, NH, USA,
(10) INAF-Osservatorio Astronomico di Capodimonte, Napoli, Italy,
(11) SSDC, Roma, Italy,
(12) INAF-Osservatorio di Astrofisica e Scienza dello Spazio di Bologna, Bologna, Italy,
(13) Department of Astronomy, Astrophysics, University of Chicago, Chicago, IL, USA,
(14) Department of Physics, Astronomy, Iowa State University, Ames, IA, USA,
(15) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, La Serena, Chile,
(16) Department of Astronomy, University of Michigan, Ann Arbor, MI, USA,
(17) Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain,
(18) Departamento de Astrofisica, Universidad de La Laguna, Tenerife, Spain,
(19) Department of Physics, Florida Atlantic University, Boca Raton, FL 33431, USA,
(20) INAF-Osservatorio Astronomico di Trieste, Trieste, Italy,
(21) Department of Astronomy, McDonald Observatory, The University of Texas, Austin, TX, USA,
(22) Universite de Nice Sophia-antipolis, CNRS, Observatoire de la Cote d'Azur, Laboratoire Lagrange, Nice, France,
(23) European Southern Observatory, Garching bei Munchen, Germany)
http://arxiv.org/abs/1811.07069
A Photometric Study of the Outer Halo Globular Cluster NGC 5824. (arXiv:1705.05280v1 [astro-ph.GA])
Volume 12, Issue 20 - article #2
A.R. Walker
,
G. Andreuzzi
,
C.E. Martínez-Vázquez
,
A.M. Kunder
,
P.B. Stetson
,
S. Cassisi
,
M. Monelli
,
G. Bono
,
M. Dall'Ora
,
A.K. Vivas
http://arxiv.org/abs/1705.05280
On a new Near-Infrared method to estimate the absolute ages of star clusters: NGC3201 as a first test case
Volume 4, Issue 50 - article #9
G. Bono
(2,3),
P.B. Stetson
(4),
D.A. VandenBerg
(5),
A. Calamida
(6),
M. Dall'Ora
(7),
G. Iannicola
(3),
P. Amico
(6),
A. Di Cecco
(2),
E. Marchetti
(6),
M. Monelli
(7),
N. Sanna
(2),
A.R. Walker
(9),
M. Zoccali
(10),
R. Buonanno
(2),
F. Caputo
(3),
S. Degl'Innocenti
(11,12),
S. D'Odorico
(6),
I. Ferraro
(3),
R. Gilmozzi
(6),
J. Melnick
(6),
M. Nonino
(13),
S. Ortolani
(14),
A.M. Piersimoni
(15),
P.G. Prada Moroni
(11,12),
L. Pulone
(3),
M. Romaniello
(6),
J. Storm
(16)
((2) UniToV
(3) INAF/OAR
(4) HIA-NRC
(5) UVIC
(6) ESO
(7) INAF/OACN
(8) IAC
(9) CTIO
(10) PUC
(11) Univ. Pisa
(12) INFN Pisa
(13) INAF/OAT
(14) Univ. of Padova
(15) INAF-OACTe
(16) AIP
(8) Aarhus Univ.
(9) IAC
(10) Univ. Concepcion
(11) Astrophys. In. Potsdam
(12) CTIO)
arXiv.org - Astrophysics - Volume: 2009, Issue: 11 Dec
arXiv:0912.0824
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,
other
]
Stromgren photometry of Galactic Globular Clusters. II Metallicity distribution of red giants in Omega Centauri
Volume 4, Issue 40 - article #14
A. Calamida
(1),
G. Bono
(2),
P.B. Stetson
(3),
L.M. Freyhammer
(4),
A.M. Piersimoni
(5),
R. Buonanno
(2),
F. Caputo
(6),
S. Cassisi
(5),
M. Castellani
(6),
C.E. Corsi
(6),
M. Dall'Ora
(7),
S. Degl'Innocenti
(8),
I. Ferraro
(6),
F. Grundahl
(9),
M. Hilker
(1),
M. Monelli
(10),
M. Nonino
(11),
N. Patat
(1),
A. Pietrinferni
(5),
P.G. Prada Moroni
(8),
F. Primas
(1),
L. Pulone
(6),
T. Richtler
(12),
M. Romaniello
(1),
J. Storm
(13),
A.R. Walker
(14)
((1) ESO
(2) Univ. Roma Tor Vergata
(3) HIA-NRC
(4) Univ. Lancashire
(5) INAF/OATe
(6) INAF/OAR
(7) INAF/OAC
(8) Univ. Pisa
(9) Aarhus Univ.
(10) IAC
(11) OAT
(12) Univ. Concepcion
(13) Astrophys. In. Potsdam
(14) CTIO)
arXiv.org - Astrophysics - Volume: 2009, Issue: 2 Oct
arXiv:0909.4661
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On the radial distribution of horizontal branch stars in ngc2808
Volume 4, Issue 13 - article #25
G. Iannicola
,
M. Monelli
,
G. Bono
,
P.B. Stetson R. Buonanno
,
A. Calamida
,
M. Zoccali
,
F. Caputo
,
M. Castellani
,
C.E. Corsi
,
M. Dall'Ora
,
A. Di Cecco
,
S. Degl'Innocenti
,
I. Ferraro
,
M. Nonino
,
A. Pietrinferni
,
L. Pulone
,
P.G. Prada Moroni
,
M. Romaniello
,
N. Sanna
,
A.R. Walker
arXiv.org - Astrophysics - Volume: 2009, Issue: 27 Mar
arXiv:0903.4531
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Results 1 - 6 of 6
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