4 pages, 4 figures, accepted for publication in A&A as a letter, see also http://www-denis.iap.fr/articles/extinction/DENIS observations in the J (1.2 micron) and K_S (2.15 micron) bands together with isochrones calculated for the RGB and AGB phase are used to draw an extinction map of the inner Galactic Bulge. The uncertainty in this method is mainly limited by the optical depth of the Bulge itself. A comparison with fields of known extinction shows a very good agreement. We present an extinction map for the inner Galactic Bulge (approx. 20 sq. deg.
Galactic interstellar extinction maps are powerful and necessary tools for Milky Way structure and s...
Context. Three dimensional interstellar extinction maps provide a powerful tool for stellar populati...
Context. We have obtained BVRI photometry for 21 stellar fields located in directions towards the ce...
The past decade has seen rapid progress in studies on the Galactic bulge thanks to many large-scale ...
Context. Studies of the properties of the inner Galactic Bulge depend strongly on the assumptions ab...
We combine V I photometry from OGLE-III with V V V and 2MASS mea-surements of E(J −Ks) to resolve th...
Context. Studies of the properties of the inner Galactic bulge strongly depend on the assu...
We built K band extinction maps in the area of two candidate low-extinction windows in the inner Bul...
Photometry of the Galactic bulge, collected during the OGLE-II microlensing search, indicates high a...
We combine VI photometry from OGLE-III with VISTA Variables in The Via Lactea survey and Two Micron ...
We present J (1.2 microns) H (1-6 microns) K' (2.11 microns) and Br(gamma) (2.166 microns) images fr...
Context.We have obtained BVRI photometry for 21 stellar fields located in directions towards the ce...
Due to the very strong interstellar extinction in the inner Galaxy, the stellar complexities of this...
Context. It has been suggested that the ratio of total-to-selective extinction RV in dust in the int...
Recently Wo'zniak & Stanek (1996) proposed a new method to investigate interstellar extinct...
Galactic interstellar extinction maps are powerful and necessary tools for Milky Way structure and s...
Context. Three dimensional interstellar extinction maps provide a powerful tool for stellar populati...
Context. We have obtained BVRI photometry for 21 stellar fields located in directions towards the ce...
The past decade has seen rapid progress in studies on the Galactic bulge thanks to many large-scale ...
Context. Studies of the properties of the inner Galactic Bulge depend strongly on the assumptions ab...
We combine V I photometry from OGLE-III with V V V and 2MASS mea-surements of E(J −Ks) to resolve th...
Context. Studies of the properties of the inner Galactic bulge strongly depend on the assu...
We built K band extinction maps in the area of two candidate low-extinction windows in the inner Bul...
Photometry of the Galactic bulge, collected during the OGLE-II microlensing search, indicates high a...
We combine VI photometry from OGLE-III with VISTA Variables in The Via Lactea survey and Two Micron ...
We present J (1.2 microns) H (1-6 microns) K' (2.11 microns) and Br(gamma) (2.166 microns) images fr...
Context.We have obtained BVRI photometry for 21 stellar fields located in directions towards the ce...
Due to the very strong interstellar extinction in the inner Galaxy, the stellar complexities of this...
Context. It has been suggested that the ratio of total-to-selective extinction RV in dust in the int...
Recently Wo'zniak & Stanek (1996) proposed a new method to investigate interstellar extinct...
Galactic interstellar extinction maps are powerful and necessary tools for Milky Way structure and s...
Context. Three dimensional interstellar extinction maps provide a powerful tool for stellar populati...
Context. We have obtained BVRI photometry for 21 stellar fields located in directions towards the ce...