activity
20022024
most citedM22: A [Fe/H] Abundance Range Revealed

143 citations · 485 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.IM2024★ 1 cited

Walking with SOXS towards the transient sky

P. Schipani, S. Campana, R. Claudi +59

SOXS (Son Of X-Shooter) is the new ESO instrument that is going to be installed on the 3.58-m New Technology Telescope at the La Silla Observatory. SOXS is a single object spectrog…

astro-ph.GA2023

Shock Excitation in Narrow Line Regions Powered by AGN Outflows

Misaki Mizumoto, Hiroaki Sameshima, Naoto Kobayashi +10

Outflows in the Active Galactic Nucleus (AGN) are considered to play a key role in the host galaxy evolution through transfer of a large amount of energy. A Narrow Line Region (NLR…

astro-ph.IM2020★ 40 cited

Sky Quality Meter and satellite correlation for the night cloud cover analysis at astronomical sites

S. Cavazzani, S. Ortolani, A. Bertolo +5

The analysis of the night cloud cover is very important for astronomical observation in real time, considering a typical observation time of about 15 minutes, and to have a statist…

astro-ph.SR2019★ 27 cited

The vertical Na-O relation in the bulge globular cluster NGC 6553

C. Muñoz, S. Villanova, D. Geisler +7

In this article, we present a detailed chemical analysis of seven red giant members of NGC 6553 using high-resolution spectroscopy from VLT FLAMES. We obtained the stellar paramete…

astro-ph.GA2019★ 19 cited

Another relic bulge globular cluster: ESO 456-SC38 (Djorgovski~2)

S. Ortolani, E. V. Held, D. Nardiello +7

The object ESO456-SC38 (Djorgovski 2) is one of the globular clusters that is closest to the Galactic center. It is on the blue horizontal branch and has a moderate metallicity of…

astro-ph.GA2018★ 10 cited

Variable broad lines and outflow in the weak blazar PBC J2333.9-2343

L. Hernández-García, G. Vietri, F. Panessa +12

PBC J2333.9-2343 is a peculiar active nucleus with two giant radio lobes and a weak blazar-like nucleus at their center. In the present work we show new optical, UV, and X-ray data…

astro-ph.SR2017★ 18 cited

The chemical composition of the stellar cluster Gaia1: no surprise behind Sirius

A. Mucciarelli, L. Monaco, P. Bonifacio +1

We observed 6 He-clump stars of the intermediate-age stellar cluster Gaia1 with the MIKE/MAGELLAN spectrograph. A possible extra-galactic origin of this cluster, recently discovere…

astro-ph.SR2017★ 41 cited

The peculiar Na-O anticorrelation of the bulge globular cluster NGC 6440

C. Muñoz, S. Villanova, D. Geisler +4

Context. Galactic Globular Clusters (GCs) are essential tools to understand the earliest epoch of the Milky Way, since they are among the oldest objects in the Universe and can be…

astro-ph.EP2016★ 1 cited

An extensive radial velocity survey toward NGC 6253

M. Montalto, C. H. F. Melo, N. C. Santos +6

The old and metal rich open cluster NGC 6253 was observed with the FLAMES multi-object spectrograph during an extensive radial velocity campaign monitoring 317 stars with a median…

astro-ph.SR2013★ 44 cited

NGC 5824: a luminous outer halo globular cluster with an intrinsic abundance spread

G. S. Da Costa, E. V. Held, I. Saviane

We present a detailed study of the strengths of the calcium triplet absorption lines in the spectra of a large sample of red giant members of the luminous outer Galactic halo globu…

astro-ph.GA2010★ 11 cited

High Resolution HDS/SUBARU chemical abundances of the young stellar cluster Palomar 1

L. Monaco, I. Saviane, M. Correnti +2

Context. Palomar\,1 is a peculiar globular cluster (GC). It is the youngest Galactic GC and it has been tentatively associated to several of the substructures recently discovered i…

astro-ph.SR2010★ 7 cited

A multiwavelength view of the protostellar binary IRAS04325+2402: a case for turbulent fragmentation

A. Scholz, K. Wood, D. Wilner +6

IRAS04325+2402 (herafter IRAS04325) is a complex protostellar system hosting two young stellar objects (AB and C in the following) at a separation of 1250AU. Here we present new de…

astro-ph.CO2010★ 11 cited

A near-infrared study of AGB and red giant stars in the Leo I dSph galaxy

E. V. Held, M. Gullieuszik, L. Rizzi +3

A near-infrared imaging study of the evolved stellar populations in the dwarf spheroidal galaxy Leo I is presented. Based on JHK observations obtained with the WFCAM wide-field arr…

astro-ph.GA2009★ 143 cited

M22: A [Fe/H] Abundance Range Revealed

G. S. Da Costa, E. V. Held, I. Saviane +1

Intermediate resolution spectra at the Ca II triplet have been obtained for 55 candidate red giants in the field of the globular cluster M22 with the VLT/FORS instrument. Spectra w…

astro-ph.CO2009★ 40 cited

New constraints on the chemical evolution of the dwarf spheroidal galaxy LeoI from VLT spectroscopy

M. Gullieuszik, E. V. Held, I. Saviane +1

(Abridged) We present the spectroscopy of red giant stars in the dwarf spheroidal galaxy LeoI, aimed at further constraining its chemical enrichment history. Intermediate-resolutio…

astro-ph2006★ 1 cited

The emission line galaxy TV Reticuli: Evidence for an ultraluminous supernova

L. Schmidtobreick, C. Tappert, H. Horst +2

TV Ret was classified as a cataclysmic variable due to an outburst observed in 1977. We intended to confirm this classification and derive some basic properties of the system. Low…

astro-ph2006★ 36 cited

Early spectral evolution of Nova Sgr 2004 (V5114 Sgr)

A. Ederoclite, E. Mason, M. Della Valle +15

We present optical and near-infrared spectral evolution of the Galactic nova V5114 Sgr (2004) during few months after the outburst. We use multi-band photometry and line intensitie…

astro-ph2002★ 35 cited

New abundance measurements in UKS 1927-177, a very metal-poor galaxy in the Local Group

I. Saviane, L. Rizzi, E. V. Held +2

We present new results from optical spectroscopy of the brightest Hii region in the dwarf irregular galaxy UKS 1927-177 in Sagittarius (SagDIG). From high signal-to-noise spectra,…