activity
20122022
most citedThe Gaia spectrophotometric standard stars survey. I. Preliminary results

61 citations · 238 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2022★ 1 cited

XGAPS: a sub-arcsecond cross-match of Galactic Plane Surveys

S. Scaringi, M. Monguio, C. Knigge +5

We present a sub-arcsecond cross-match of Gaia Data Release 3 (DR3) against the INT Galactic Plane Surveys (IGAPS) and the United Kingdom Infrared Deep Sky Survey (UKIDSS). The res…

astro-ph.GA2021★ 17 cited

Proper motions of OB stars in the far Carina Arm

J. E. Drew, M. Monguió, N. J. Wright

In large scale maps of the Galactic disc, the Carina Arm stands out as a clear spiral feature, hosting prominent star clusters and associations rich in massive stars. We study the…

astro-ph.GA2021★ 9 cited

Population-based identification of Hα-excess sources in the Gaia DR2 and IPHAS catalogues

M. Fratta, S. Scaringi, J. E. Drew +8

We present a catalogue of point-like Hα-excess sources in the Northern Galactic Plane. Our catalogue is created using a new technique that leverages astrometric and photomeric info…

astro-ph.SR2018★ 10 cited

The Gaia/IPHAS and Gaia/KIS Value-Added Catalogues

S. Scaringi, C. Knigge, J. E. Drew +7

We present a sub-arcsecond cross-match of Gaia DR2 against the INT Photometric H-alpha Survey of the Northern Galactic Plane Data Release 2 (IPHAS DR2) and the Kepler-INT Survey (K…

astro-ph.SR2018★ 35 cited

Massive stars in the hinterland of the young cluster, Westerlund 2

J. E. Drew, A. Herrero, M. Mohr-Smith +4

An unsettled question concerning the formation and distribution of massive stars is whether they must be born in massive clusters and, if found in less dense environments, whether…

astro-ph.EP2017★ 14 cited

280 one-opposition near-Earth asteroids recovered by the EURONEAR with the Isaac Newton Telescope

O. Vaduvescu, L. Hudin, T. Mocnik +80

One-opposition near-Earth asteroids (NEAs) are growing in number, and they must be recovered to prevent loss and mismatch risk, and to improve their orbits, as they are likely to b…