activity
19992005
most citedISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared

85 citations · 337 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph2005★ 36 cited

Extinctions at 7um and 15um from the ISOGAL survey

B. W. Jiang, J. Gao, A. Omont +2

The extinction laws at 7um and 15um are derived for more than 120 sightlines in the inner Galactic plane based on the ISOGAL survey data and the near-infrared data from DENIS and 2…

astro-ph2003★ 85 cited

ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared

A. Omont, G. Gilmore, C. Alard +38

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss…

astro-ph2003★ 42 cited

Explanatory Supplement of the ISOGAL-DENIS Point Source Catalogue

F. Schuller, S. Ganesh, M. Messineo +10

We present version 1.0 of the ISOGAL-DENIS Point Source Catalogue (PSC), containing more than 100,000 point sources detected at 7 and/or 15 micron in the ISOGAL survey of the inner…

astro-ph2003★ 29 cited

Stellar sources in the ISOGAL intermediate bulge fields

D. K. Ojha, A. Omont, F. Schuller +3

We present a study of ISOGAL sources in the "intermediate" galactic bulge ( 2, 1--4), observed by ISOCAM at 7 and 15 . In…

astro-ph2003★ 21 cited

The ISOGAL field FC--01863+00035: Mid-IR interstellar extinction and stellar populations

B. W. Jiang, A. Omont, S. Ganesh +2

A 0.35\degr 0.29\degr field centered at =--18.63\degr, =0.35\degr was observed during the ISOGAL survey by ISOCAM imaging at 7m and 15{\rm m}. 648 objects were…

astro-ph2002★ 6 cited

Low resolution spectroscopy of ISOGAL sources: Search for early-type stars with infrared excess

M. Schultheis, M. Parthasarathy, A. Omont +4

An analysis of low resolution spectra and infared data of 29 ISOGAL-DENIS sources with mid-IR excess is presented. Eight ISOGAL sources from our sample with 7-15 micron excess are…