MIPSGAL: A Survey of the Inner Galactic Plane at 24 and 70 μm

By S. Carey, A. Noriega-Crespo, D. Mizuno, S. Shenoy, R. Paladini, K. Kraemer, S. Price, N. Flagey, E. Ryan, J. Ingalls and 17 more. 2005

534 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/996e84d361cbb9d664b6958b73ff6939f13fd6ff

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Citations in the corpus

A CLASS I AND CLASS II CH3OH MASER SURVEY OF EGOs FROM THE GLIMPSE SURVEY (2009, methodology): “42+0.33, the positions of 24 µm EGO counterparts and 6.7 GHz CH 3 OH masers from our survey are coincident within the combined uncertainties of the MIPS- GAL absolute astrometry (Carey et al. 2009) and our measurements of the 24 µm source positions – 12 – (see note (a) to Table 5).”
STAR FORMATION IN THE CENTRAL 400 PC OF THE MILKY WAY: EVIDENCE FOR A POPULATION OF MASSIVE YOUNG STELLAR OBJECTS (2009, methodology): “Our data are complemented by the Spitzer Legacy program MIPS Inner Galactic Plane Survey (MIPSGAL) which observed 220 deg2 of the inner Galactic plane, 65◦ > l > 10◦ and −10◦ > l > −65◦ for |b| < 1◦, at 24 and 70µm (Carey et al. 2009) which avoided duplicating coverage of the Galactic center region.”
A gallery of bubbles. The nature of the bubbles observed by Spitzer and what ATLASGAL tells us about the surrounding neutral material (2010, methodology): “We also use images at 24 μm from the Spitzer-MIPSGAL survey (Carey et al. 2009), which has the same Galactic coverage.”
THE WISE CATALOG OF GALACTIC H ii REGIONS (2013, methodology): “Anderson et al. (2012b) found that the WISE 22 μm flux of H ii regions is the same as the MIPSGAL 24 μm flux.”
The Milky Way Project First Data Release: a bubblier Galactic disc (2012, background): “Bania et al. (2010) later selected 24 µm diffuse emission sources from Spitzer/MIPSGAL survey images (Carey et al. 2009) with spatially coincident 21 cm continuum emission for a radio recombination line survey with the Green Bank Telescope, and discovered several hundred new Galactic H ii regions…”
SDC13 infrared dark clouds: longitudinally collapsing filaments? (2013, methodology): “We also make use of publicly available Spitzer GLIMPSE (Churchwell et al. 2009) and 24 µm MIPSGAL (Carey et al. 2009) data.”
A Herschel [C ii] Galactic plane survey - I. The global distribution of ISM gas components (2013, methodology): “Far-infrared dust continuum emission has been widely used as a mass tracer of the ISM, and several high-resolution, largescale, sensitive maps of the Galactic plane exist (Carey et al. 2009; Molinari et al. 2010).”
Characterizing precursors to stellar clusters with Herschel (2011, methodology): “We use the mid-IR data taken as part of the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE; 3.6, 4.5, 5.8, and 8.0 µm, Benjamin et al. 2003) and the MIPSGAL survey (24 µm; Carey et al. 2009).”
The RMS survey : Galactic distribution of massive star formation (2013, background): “…2MASS, UKIDSS, VVV, GLIMPSE, MIPSGAL, ATLASGAL and CORNISH; Skrutskie et al. 2006; Minniti et al. 2010; Lawrence et al. 2007; Benjamin et al. 2003; Carey et al. 2009; Schuller et al. 2009 and Hoare et al. 2012, respectively) of a mid-infrared colour selected sample of ∼5000 MSX sources (Lumsden…”
SURVEYING THE AGENTS OF GALAXY EVOLUTION IN THE TIDALLY STRIPPED, LOW METALLICITY SMALL MAGELLANIC CLOUD (SAGE-SMC). I. OVERVIEW (2011, result): “…the results from this SMC survey with the existing LMC (SAGE-LMC, Meixner et al. 2006) and Milky Way (GLIMPSE, MIPSGAL, Churchwell et al. 2009; Carey et al. 2009) surveys provides a foundation for understanding the physics of the ISM, current star formation, and evolved-star mass loss as a…”
EMU: Evolutionary Map of the Universe (2011, methodology): “The resolution of EMU is particularly well-matched to the MIPSGAL 24 mm (Carey et al. 2009) and Hi-GAL 70 mm (Molinari et al. 2010) survey images, of which the latter is an effective tracer of the intensity of the exciting radiation field (Compiègne et al. 2010).”
Ammonia from cold high-mass clumps discovered in the inner Galactic disk by the ATLASGAL survey (2012, background): “…plane surveys, conducted over a similar range, are the MSX survey covering 8 to 21 μm (Price et al. 2001), 2MASS around 2 μm (Skrutskie et al. 2006), GLIMPSE from 3 to 8 μm (Benjamin et al. 2003), MIPSGAL at 24 and 70 μm (Carey et al. 2009) and HiGAL from 70 to 500 μm (Molinari et al. 2010).”
THE GREEN BANK TELESCOPE H ii REGION DISCOVERY SURVEY. II. THE SOURCE CATALOG (2011, background): “…Stil et al. 2006), the NRAO VLA Sky Survey at 20 cm continuum (NVSS: Condon et al. 1998), the Southern Galactic Plane Survey at 21 cm H I and continuum (SGPS: Haverkorn et al. 2006), the VLA MAGPIS at 20 cm continuum (Helfand et al. 2006), and the Spitzer 24µm MIPSGAL survey (Carey et al. 2009).”
THE BOLOCAM GALACTIC PLANE SURVEY: SURVEY DESCRIPTION AND DATA REDUCTION (2010, background): “The BGPS maps in the first quadrant overlap with the VLA Galactic Plane Survey (VGPS) in H i and radio continuum (Stil et al. 2006), the Spitzer-GLIMPSE and GLIMPSE-II fields (Benjamin et al. 2003), MIPSGAL (Carey et al. 2009), the BU-FCRAO 13CO J = 1 → 0 Galactic Ring Survey (Jackson et al. 2006), ”
THE RED MSX SOURCE SURVEY: THE MASSIVE YOUNG STELLAR POPULATION OF OUR GALAXY (2013, background): “…fraction of the Galactic Plane are either of low spatial resolution (eg IRAS: cf Chan et al 1996, or Campbell et al. 1989) or lack the dynamic range required to study a wide mass range (eg GLIMPSE: Benjamin et al 2003, Churchwell et al 2009; MIPSGAL: Mizuno et al. 2008, Carey et al. 2009).”
The ATLASGAL survey: a catalog of dust condensations in the Galactic plane (2013, methodology): “MIPSGAL at 24µm has only a factor of 2 higher sensitivity and an angular resolution of 6′′ (Carey et al. 2009) compared to WISE at 22µm with 12′′ resolution.”
FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results (2017, background): “Recently, continuum surveys of the Galactic plane such as the GLIMPSE and MIPSGAL by Spitzer (Benjamin et al. 2003; Carey et al. 2009), the Hi-GAL survey by Herschel (Molinari et al. 2010) and the all-sky survey by AKARI (Doi et al. 2015) have been carried out at the mid- and far-infrared…”
Hi-GAL, the Herschel infrared Galactic Plane Survey: Photometric maps and compact source catalogues: First data release for the inner Milky Way: +68° ≥ l ≥ -70° (2016, methodology): “More complete statistics in this respect will be presented by Elia et al. (2016) and Martinavarro-Armengol et al. (2015) who will discuss the HiGAL photometric catalogues in the context of ancillary photometric Galactic Plane surveys like ATLASGAL (Schuller et al., 2009), MIPSGAL (Carey et al., 2009”