activity
19962017
most citedThe Ital-FLAMES survey of the Sagittarius dwarf Spheroidal galaxy. I. Chemical abundances of bright RGB stars

157 citations · 711 across the 19 of their papers we have counts for

collaborators
Showing astro-phShow all

9 papers · 1 filter

astro-ph2007★ 1 cited

VIMOS total transmission profiles for broad-band filters

S. Mieske, M. Rejkuba, S. Bagnulo +2

VIMOS is a wide-field imager and spectrograph mounted on UT3 at the VLT, whose FOV consists of four 7'x8' quadrants. Here we present the measurements of total transmission profiles…

astro-ph2005★ 157 cited

The Ital-FLAMES survey of the Sagittarius dwarf Spheroidal galaxy. I. Chemical abundances of bright RGB stars

L. Monaco, M. Bellazzini, P. Bonifacio +5

We present iron and element (Mg, Ca, Ti) abundances for a sample of 15 Red Giant Branch stars belonging to the main body of the Sagittarius dwarf Spheroidal galaxy. Abundances…

astro-ph2004★ 43 cited

Accurate X-ray position of the Anomalous X-ray Pulsar XTE J1810-197 and identification of its likely IR counterpart

G. L. Israel, N. Rea, V. Mangano +13

We report the accurate sub-arcsec X-ray position of the new Anomalous X-ray Pulsar (AXP) XTE J1810-197, derived with a Chndra-HRC Target of Opportunity observation carried out in N…

astro-ph2003★ 60 cited

The IR counterpart to the Anomalouos X-ray Pulsar 1RXS J1708-4009

G. L. Israel, S. Covino, R. Perna +10

We report the discovery of the likely IR counterpart to the Anomalous X-ray Pulsar (AXP) 1RXS J1708-4009, based on the combination of Chandra HRC-I X-ray position, and deep optical…

astro-ph2002★ 64 cited

The detection of variability from the candidate IR counterpart to the Anomalous X-ray Pulsar 1E1048.1-5937

G. L. Israel, S. Covino, L. Stella +9

We report on the detection of variability from the proposed IR counterpart to the Anomalous X-ray Pulsar (AXP) 1E1048.1-5937 based on Chandra and ESO optical/IR deep observations c…

astro-ph2001★ 11 cited

Mass segregation of different populations inside the cluster NGC6101

G. Marconi, G. Andreuzzi, L. Pulone +3

We have used ESO telescopes at La Silla and the Hubble Space Telescope (HST) in order to obtain accurate B,V,I CCD photometry for the stars located within 200" (~= 2 half-mass radi…