S
Susan R. Stolovy
Researcher at El Camino College
Publications - 106
Citations - 13446
Susan R. Stolovy is an academic researcher from El Camino College. The author has contributed to research in topics: Star formation & Galactic Center. The author has an hindex of 44, co-authored 106 publications receiving 12882 citations. Previous affiliations of Susan R. Stolovy include California Institute of Technology.
Papers
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Journal ArticleDOI
The Multiband Imaging Photometer for Spitzer (MIPS)
George H. Rieke,Erick T. Young,Charles W. Engelbracht,D. M. Kelly,Frank J. Low,Eugene E. Haller,Jeffrey W. Beeman,Karl D. Gordon,John Stansberry,Karl Misselt,J. Cadien,Jane E. Morrison,Gil Rivlis,William B. Latter,Alberto Noriega-Crespo,Deborah Padgett,Karl R. Stapelfeldt,Dean C. Hines,Eiichi Egami,James Muzerolle,Almudena Alonso-Herrero,Myra Blaylock,Herve Dole,Joannah L. Hinz,E. Le Floc'h,Casey Papovich,Pablo G. Pérez-González,Paul S. Smith,Kate Y. L. Su,Lee Bennett,Dave Frayer,David A. Henderson,Nanyao Y. Lu,Frank J. Masci,M. Pesenson,Luisa Rebull,Jeonghee Rho,Jocelyn Keene,Susan R. Stolovy,Stefanie Wachter,W. A. Wheaton,Michael W. Werner,Paul L. Richards +42 more
TL;DR: The Multiband Imaging Photometer for Spitzer (MIPS) as discussed by the authors provides long-wavelength capability for the mission in imaging bands at 24, 70, and 160?m and measurements of spectral energy distributions between 52 and 100?m at a spectral resolution of about 7%.
Journal ArticleDOI
GLIMPSE. I. An SIRTF Legacy Project to Map the Inner Galaxy
Robert A. Benjamin,Ed Churchwell,Brian Babler,T. M. Bania,Dan P. Clemens,Martin Cohen,John M. Dickey,Remy Indebetouw,James M. Jackson,Henry A. Kobulnicky,Alex Lazarian,A. P. Marston,John S. Mathis,Marilyn R. Meade,Sara Seager,Susan R. Stolovy,C. Watson,Barbara A. Whitney,Michael J. Wolff,Mark G. Wolfire +19 more
TL;DR: The Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE), a Space Infrared Telescope Facility (SIRTF) Legacy Science Program, will be a fully sampled, confusion-limited infrared survey of the inner Galactic disk with a pixel resolution of ∼1 as mentioned in this paper.
Journal ArticleDOI
GLIMPSE: I. A SIRTF Legacy Project to Map the Inner Galaxy
Robert A. Benjamin,Ed Churchwell,Brian Babler,T. M. Bania,Dan P. Clemens,Martin Cohen,John M. Dickey,Remy Indebetouw,James M. Jackson,Henry A. Kobulnicky,Alex Lazarian,A. P. Marston,John S. Mathis,Marilyn R. Meade,Sara Seager,Susan R. Stolovy,C. Watson,Barbara A. Whitney,Michael J. Wolff,Mark G. Wolfire +19 more
TL;DR: Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) as discussed by the authors is a collection of images collected by the SIRTF Legacy Science Program with a pixel resolution of 1.2" using the Infrared Array Camera (IRAC).
Journal ArticleDOI
The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 μm Using GLIMPSE Data
Remy Indebetouw,Remy Indebetouw,John S. Mathis,Brian Babler,Marilyn R. Meade,Christer Watson,Barbara A. Whitney,M. J. Wolff,Mark G. Wolfire,Martin Cohen,T. M. Bania,Robert A. Benjamin,Dan P. Clemens,John M. Dickey,James M. Jackson,Henry A. Kobulnicky,A. P. Marston,E. P. Mercer,John R. Stauffer,Susan R. Stolovy,Ed Churchwell +20 more
TL;DR: In this paper, the extinction ratio between two of the filters, e.g., AJ/AK, is required to calculate A[λ]/AK from those measured ratios, which shows a flattening across the 3-8 μm wavelength range, roughly consistent with the extinction measurements derived by Lutz and coworkers for the sight line toward the Galactic center.
Journal ArticleDOI
The Wavelength Dependence of Interstellar Extinction from 1.25 to 8.0 microns Using GLIMPSE Data
Remy Indebetouw,John S. Mathis,Brian Babler,Marilyn R. Meade,C. Watson,B. A. Whitney,M. J. Wolff,Mark Wolfire,T. M. Bania,Robert A. Benjamin,Dan P. Clemens,Martin Cohen,John M. Dickey,James M. Jackson,Henry A. Kobulnicky,A. P. Marston,E. P. Mercer,John Stauffer,Susan R. Stolovy,Ed Churchwell +19 more
TL;DR: In this article, the extinction ratio between two filters, e.g. A(J)/A(K), is calculated from the color distributions of observed stars, and the mean values of the color excess ratios (A(λ)-A(k))/(A(J)-A (K)) are calculated from those measured ratios.