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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 изданияхстатьяРецензирование

Harvard

Gontcharov, GA, Marchuk, AA, Savchenko, SS, Mosenkov, AV, Il'in, VB, Poliakov, DM, Smirnov, AA & Krayani, H 2025, 'Foreground Extinction to Extended Celestial Objects. I. New Extinction Maps', Research in Astronomy and Astrophysics, Том. 25, № 12, 125016. https://doi.org/10.1088/1674-4527/ae12a6

APA

Gontcharov, G. A., Marchuk, A. A., Savchenko, S. S., Mosenkov, A. V., Il'in, V. B., Poliakov, D. M., Smirnov, A. A., & Krayani, H. (2025). Foreground Extinction to Extended Celestial Objects. I. New Extinction Maps. Research in Astronomy and Astrophysics, 25(12), [125016]. https://doi.org/10.1088/1674-4527/ae12a6

Vancouver

Gontcharov GA, Marchuk AA, Savchenko SS, Mosenkov AV, Il'in VB, Poliakov DM и пр. Foreground Extinction to Extended Celestial Objects. I. New Extinction Maps. Research in Astronomy and Astrophysics. 2025 Дек. 1;25(12). 125016. https://doi.org/10.1088/1674-4527/ae12a6

Author

Gontcharov, G. A. ; Marchuk, A. A. ; Savchenko, S. S. ; Mosenkov, A. V. ; Il'in, V. B. ; Poliakov, D. M. ; Smirnov, A. A. ; Krayani, H. / Foreground Extinction to Extended Celestial Objects. I. New Extinction Maps. в: Research in Astronomy and Astrophysics. 2025 ; Том 25, № 12.

BibTeX

@article{aa8921aef0704ec7a1ff0404ffcc1845,
title = "Foreground Extinction to Extended Celestial Objects. I. New Extinction Maps",
abstract = "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.",
keywords = "(ISM:) dust, extinction, (Galaxy:) local interstellar matter, (Galaxy:) solar neighborhood, (Galaxy:) globular clusters: general, (Galaxy:) open clusters and associations: general, galaxies: general, (stars:) supernovae: general, ISM: clouds",
author = "Gontcharov, {G. A.} and Marchuk, {A. A.} and Savchenko, {S. S.} and Mosenkov, {A. V.} and Il'in, {V. B.} and Poliakov, {D. M.} and Smirnov, {A. A.} and H. Krayani",
year = "2025",
month = dec,
day = "1",
doi = "10.1088/1674-4527/ae12a6",
language = "русский",
volume = "25",
journal = "Research in Astronomy and Astrophysics",
issn = "1674-4527",
publisher = "IOP Publishing Ltd.",
number = "12",

}

RIS

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