activity
19992011
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 · 500 across the 10 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 44 cited

Interstellar Extinction and Long-Period Variables in the Galactic Center

M. Schultheis, K. Sellgren, S. Ramirez +4

We use the Spitzer IRAC catalogue of the Galactic Center (GC) point sources (Ramirez et al. 2008) and combine it with new isochrones (Marigo et al. 2008) to derive extinctions base…

astro-ph2006★ 15 cited

Recent star formation in the inner Galactic Bulge seen by ISOGAL. I - Classification of bright mid-IR sources in a test field

F. Schuller, A. Omont, I. S. Glass +3

Context: The stellar populations in the central region of the Galaxy are poorly known because of the high visual extinction and very great source density in this direction. Aims: T…

astro-ph2004★ 55 cited

SiO Maser Survey of IRAS Sources in the Inner Galactic Disk

S. Deguchi, T. Fujii, I. S. Glass +7

We have surveyed 401 color selected IRAS sources in the Galactic disk in the SiO J=1--0 v= 1 and 2 maser lines at 43 GHz, resulting in 254 (239 new) detections. The observed source…

astro-ph2004★ 43 cited

SiO Maser Survey of the Large-Amplitude Variables in the Galactic Center

S. Deguchi, H. Imai, T. Fujii +7

We have surveyed ~400 known large-amplitude variables within 15' of the galactic center in the SiO J=1--0 v=1 and 2 maser lines at 43 GHz, resulting in 179 detections. SiO lines we…

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-ph2002★ 26 cited

Detections of SiO Masers from the Large-Amplitude Variables in the Galactic Nuclear Disk

H. Imai, S. Deguchi, T. Fujii +7

We have surveyed known large-amplitude variables within 15' of the Galactic center in the SiO J=1-0 v=1 and 2 maser lines at 43 GHz, resulting in 79 detections and 58 non-detection…