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A Color-Excess Extinction map of the Southern Galactic disk from the VVV and GLIMPSE Surveys

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arxiv 1909.03131 v1 pith:EGS4KO27 submitted 2019-09-06 astro-ph.GA

classification astro-ph.GA
keywords circextinctionlesssimgalacticphotometrysurveydatadeep
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

An improved high-resolution and deep A$_{Ks}$ foreground dust extinction map is presented for the Galactic disk area within $295^{\circ} \lesssim l \lesssim 350^{\circ}$, $-1.0^{\circ} \lesssim b \lesssim +1.0^{\circ}$. At some longitudes the map reaches up to $|b|\sim2.25^{\circ}$, for a total of $\sim$148 deg$^2$. The map was constructed via the Rayleigh-Jeans Color Excess (RJCE) technique based on deep near-infrared (NIR) and mid-infrared (MIR) photometry. The new extinction map features a maximum bin size of 1', and relies on NIR observations from the Two Micron All-Sky Survey (2MASS) and new data from ESO's Vista Variables in the V\'ia L\'actea (VVV) survey, in concert with MIR observations from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE). The VVV photometry penetrates $\sim$4 magnitudes fainter than 2MASS, and provides enhanced sampling of the underlying stellar populations in this heavily obscured region. Consequently, the new results supersede existing RJCE maps tied solely to brighter photometry, revealing a systematic underestimation of extinction in prior work that was based on shallower data. The new high-resolution and large-scale extinction map presented here is readily available to the community through a web query interface.

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Cited by 1 Pith paper

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    First time-series detection of broad near-infrared water vapor emission bands in a classical T Tauri star during an EXor outburst, tracing a transient hot inner disk cooling from about 3000 K to 2000 K.

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