INTERSTELLAR EXTINCTION LAW TOWARD THE GALACTIC CENTER III: J, H, KS BANDS IN THE 2MASS AND THE MKO SYSTEMS, AND 3.6, 4.5, 5.8, 8.0 μm IN THE SPITZER/IRAC SYSTEM

@article{Nishiyama2009INTERSTELLAREL,
  title={INTERSTELLAR EXTINCTION LAW TOWARD THE GALACTIC CENTER III: J, H, KS BANDS IN THE 2MASS AND THE MKO SYSTEMS, AND 3.6, 4.5, 5.8, 8.0 $\mu$m IN THE SPITZER/IRAC SYSTEM},
  author={Shogo Nishiyama and Motohide Tamura and Hirofumi Hatano and Daisuke Kato and Toshihiko Tanab{\'e} and Koji Sugitani and Tetsuya Nagata},
  journal={The Astrophysical Journal},
  year={2009},
  volume={696},
  pages={1407-1417}
}
We have determined interstellar extinction law toward the Galactic center (GC) at the wavelength from 1.2 to 8.0 μm, using point sources detected in the IRSF/SIRIUS near-infrared (NIR) survey and those in the Two Micron All Sky Survey (2MASS) and Spitzer/IRAC/GLIMPSE II catalogs. The central region l 30 and b 10 has been surveyed in the J, H, and KS bands with the IRSF telescope and the SIRIUS camera whose filters are similar to the Mauna Kea Observatories (MKO) NIR photometric system. Combined… 
REDDENING AND EXTINCTION TOWARD THE GALACTIC BULGE FROM OGLE-III: THE INNER MILKY WAY'S RV ∼ 2.5 EXTINCTION CURVE*
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Interstellar extinction law toward the Galactic center. IV. J, H, and Ks bands from VVV red clump stars
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