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Foreground Extinction to Extended Celestial Objects. I. New Extinction Maps. / Gontcharov, G. A.; Marchuk, A. A.; Savchenko, S. S.; Mosenkov, A. V.; Il'in, V. B.; Poliakov, D. M.; Smirnov, A. A.; Krayani, H.
в: Research in Astronomy and Astrophysics, Том 25, № 12, 125016, 01.12.2025.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Foreground Extinction to Extended Celestial Objects. I. New Extinction Maps
AU - Gontcharov, G. A.
AU - Marchuk, A. A.
AU - Savchenko, S. S.
AU - Mosenkov, A. V.
AU - Il'in, V. B.
AU - Poliakov, D. M.
AU - Smirnov, A. A.
AU - Krayani, H.
PY - 2025/12/1
Y1 - 2025/12/1
N2 - We present a new two-dimensional (2D) map of total Galactic extinction, AV, across the entire dust half-layer from the Sun to extragalactic space for Galactic latitudes ∣b∣ > 13°, as well as a three-dimensional (3D) map of AV within 2 kpc of the Sun. These maps are based on AV and distance estimates derived from a data set, which utilizes Gaia Data Release 3 parallaxes and multi-band photometry for nearly 100 million dwarf stars. We apply our own corrections to account for significant systematics in this data set. Our 2D map achieves an angular resolution of 6.'1, while the 3D map offers a transverse resolution of 3.56 pc—corresponding to variable angular resolution depending on distance—and a radial resolution of 50 pc. In constructing these maps, we pay particular attention to the solar neighborhood (within 200 pc) and to high Galactic latitudes. The 3D map predicts AV from the Sun to any extended object within the Galactic dust layer with an accuracy of σ(AV) = 0.1 mag. The 2D map provides AV estimates for the entire dust half-layer up to extragalactic distances with an accuracy of σ(AV) = 0.07 mag. We provide AV estimates from our maps for various classes of extended celestial objects with angular size primarily in the range of 2'─40', including 19,809 galaxies and quasars, 170 Galactic globular clusters, 458 open clusters, and several hundred molecular clouds from two lists. We also present extinction values for 8293 Type Ia supernovae. Comparison of our extinction estimates with those from previous maps and literature sources reveals systematic differences, indicating large-scale spatial variations in the extinction law and suggesting that earlier 2D reddening maps based on infrared dust emission tend to underestimate low extinction values.
AB - We present a new two-dimensional (2D) map of total Galactic extinction, AV, across the entire dust half-layer from the Sun to extragalactic space for Galactic latitudes ∣b∣ > 13°, as well as a three-dimensional (3D) map of AV within 2 kpc of the Sun. These maps are based on AV and distance estimates derived from a data set, which utilizes Gaia Data Release 3 parallaxes and multi-band photometry for nearly 100 million dwarf stars. We apply our own corrections to account for significant systematics in this data set. Our 2D map achieves an angular resolution of 6.'1, while the 3D map offers a transverse resolution of 3.56 pc—corresponding to variable angular resolution depending on distance—and a radial resolution of 50 pc. In constructing these maps, we pay particular attention to the solar neighborhood (within 200 pc) and to high Galactic latitudes. The 3D map predicts AV from the Sun to any extended object within the Galactic dust layer with an accuracy of σ(AV) = 0.1 mag. The 2D map provides AV estimates for the entire dust half-layer up to extragalactic distances with an accuracy of σ(AV) = 0.07 mag. We provide AV estimates from our maps for various classes of extended celestial objects with angular size primarily in the range of 2'─40', including 19,809 galaxies and quasars, 170 Galactic globular clusters, 458 open clusters, and several hundred molecular clouds from two lists. We also present extinction values for 8293 Type Ia supernovae. Comparison of our extinction estimates with those from previous maps and literature sources reveals systematic differences, indicating large-scale spatial variations in the extinction law and suggesting that earlier 2D reddening maps based on infrared dust emission tend to underestimate low extinction values.
KW - (ISM:) dust
KW - extinction
KW - (Galaxy:) local interstellar matter
KW - (Galaxy:) solar neighborhood
KW - (Galaxy:) globular clusters: general
KW - (Galaxy:) open clusters and associations: general
KW - galaxies: general
KW - (stars:) supernovae: general
KW - ISM: clouds
UR - https://www.mendeley.com/catalogue/6eafdad3-9102-3e3c-ae3a-23835eaeb79e/
U2 - 10.1088/1674-4527/ae12a6
DO - 10.1088/1674-4527/ae12a6
M3 - статья
VL - 25
JO - Research in Astronomy and Astrophysics
JF - Research in Astronomy and Astrophysics
SN - 1674-4527
IS - 12
M1 - 125016
ER -
ID: 144754008