The New Near Infrared Array Camera at the University of Rochester

1985 ◽  
Vol 97 ◽  
pp. 183 ◽  
Author(s):  
W. J. Forrest ◽  
A. Moneti ◽  
C. E. Woodward ◽  
J. L. Pipher ◽  
A. Hoffman
Keyword(s):  
Near Infrared ◽  
The University ◽  
Array Camera ◽  
Infrared Array

scholarly journals The Morphology of MID-Infrared UIR Feature Emission in the PPN M 2–9 and IRAS 21282+5050

1993 ◽  
Vol 155 ◽  
pp. 344-344
Author(s):  
L. K. Deutsch ◽  
J. L. Hora ◽  
W. F. Hoffmann ◽  
G. G. Fazio ◽  
K. Shivanandan
Keyword(s):  
Near Infrared ◽  
Infrared Images ◽  
Mid Infrared ◽  
Nicmos 3 ◽  
Array Camera ◽  
Infrared Array

The carbon-rich PPN M 2–9 and IRAS 21282+5050 are known to exhibit UIR feature emission at 7.7, 8.6, and 11.22 μm. The two nebulae have been imaged in the mid-IR with the UA/SAO/NRL Mid-Infrared Array Camera (MIRAC) in bandpasses which include UIR feature emission (8.8 and 11.22 μm). Near-infrared images of the nebulae have also been taken with the NICMOS 3 Hg:Cd:Te array camera at J, H, and K for M 2–9 and at K for IRAS 21282+5050.

MANIAC: a new mid- and near-infrared array camera

1997 ◽  
Author(s):  
Torsten Boeker ◽  
T. Lehmann ◽  
John W. V. Storey ◽  
Alfred Krabbe
Keyword(s):  
Near Infrared ◽  
Array Camera ◽  
Infrared Array

scholarly journals Spitzer/Infrared Array Camera near-infrared features in the outer parts of S4G galaxies

2014 ◽  
Vol 444 (4) ◽  
pp. 3015-3039 ◽  
Author(s):  
Seppo Laine ◽  
Johan H. Knapen ◽  
Juan-Carlos Muñoz-Mateos ◽  
Taehyun Kim ◽  
Sébastien Comerón ◽  
...  
Keyword(s):  
Near Infrared ◽  
Array Camera ◽  
Infrared Array

scholarly journals The Extended Disc Galaxy Exploration Science Survey: description and surface brightness profile properties

2019 ◽  
Vol 486 (2) ◽  
pp. 1995-2010 ◽  
Author(s):  
Shawn M Staudaher ◽  
Daniel A Dale ◽  
Liese van Zee
Keyword(s):  
Surface Brightness ◽  
Near Infrared ◽  
Infrared Imaging ◽  
Large Range ◽  
Disc Galaxy ◽  
Full Sample ◽  
Wide Range ◽  
Tidal Stream ◽  
Array Camera ◽  
Infrared Array

Abstract The survey description and near-infrared properties for 92 galaxies are presented for the Extended Disc Galaxy Exploration Science (EDGES) Survey, along with an investigation into the properties of the stellar haloes of these galaxies. EDGES is a Spitzer Space Telescope Warm Mission program designed to reach the surface brightness limit (∼0.5 kJy sr−1 or 29 AB mag arcsec−2) of the Infrared Array Camera (IRAC) 3.6 and 4.5 ${\rm \mu}$m bands for a wide range of galaxy types found within the local volume. The surface brightness profiles exhibit a large range in disc scale length, with breaks more frequently seen than in previous studies, owing in large part to the extremely deep near-infrared imaging. A number of these surface brightness profile breaks may be due to stellar haloes, up to seven galaxies out of the full sample of 92 galaxies, and we explore these implications in relation to current cosmological models. We also report the discovery of a new tidal stream near NGC 3953.

scholarly journals Galaxy Stellar Mass Functions from z ∼ 10 to z ∼ 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of Galaxies in the First Gigayear of Cosmic Time

2021 ◽  
Vol 922 (1) ◽  
pp. 29
Author(s):  
Mauro Stefanon ◽  
Rychard J. Bouwens ◽  
Ivo Labbé ◽  
Garth D. Illingworth ◽  
Valentino Gonzalez ◽  
...  
Keyword(s):  
Star Formation ◽  
Near Infrared ◽  
Mass Density ◽  
Formation Rate ◽  
Stellar Mass ◽  
Wide Area ◽  
Space Telescope ◽  
Mass Functions ◽  
Array Camera ◽  
Infrared Array

Abstract We present new stellar mass functions at z ∼ 6, z ∼ 7, z ∼ 8, z ∼ 9 and, for the first time, z ∼ 10, constructed from ∼800 Lyman-break galaxies previously identified over the eXtreme Deep Field and Hubble Ultra-Deep Field parallel fields and the five Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey fields. Our study is distinctive due to (1) the much deeper (∼200 hr) wide-area Spitzer/Infrared Array Camera (IRAC) imaging at 3.6 μm and 4.5 μm from the Great Observatories Origins Deep Survey Re-ionization Era Wide-area Treasury from Spitzer program (GREATS) and (2) consideration of z ∼ 6–10 sources over a 3× larger area than those of previous Hubble Space Telescope+Spitzer studies. The Spitzer/IRAC data enable ≥2σ rest-frame optical detections for an unprecedented 50% of galaxies down to a stellar mass limit of ∼ 10 8  ⊙ across all redshifts. Schechter fits to our volume densities suggest a combined evolution in the characteristic mass  * and normalization factor ϕ * between z ∼ 6 and z ∼ 8. The stellar mass density (SMD) increases by ∼1000× in the ∼500 Myr between z ∼ 10 and z ∼ 6, with indications of a steeper evolution between z ∼ 10 and z ∼ 8, similar to the previously reported trend of the star formation rate density. Strikingly, abundance matching to the Bolshoi–Planck simulation indicates halo mass densities evolving at approximately the same rate as the SMD between z ∼ 10 and z ∼ 4. Our results show that the stellar-to-halo mass ratios, a proxy for the star formation efficiency, do not change significantly over the huge stellar mass buildup occurred from z ∼ 10 to z ∼ 6, indicating that the assembly of stellar mass closely mirrors the buildup in halo mass in the first ∼1 Gyr of cosmic history. The James Webb Space Telescope is poised to extend these results into the “first galaxy” epoch at z ≳ 10.

scholarly journals MANIAC--A New Mid- and Near-Infrared Array Camera

1997 ◽  
Vol 109 ◽  
pp. 827 ◽  
Author(s):  
T. Boeker ◽  
J. W. V. Storey ◽  
A. Krabbe ◽  
T. Lehmann
Keyword(s):  
Near Infrared ◽  
Array Camera ◽  
Infrared Array

scholarly journals Line observations of the 30-Dor complex and N159A5 with the MPE imaging NIR spectrometer FAST

1991 ◽  
Vol 148 ◽  
pp. 205-206 ◽  
Author(s):  
A. Krabbe ◽  
J. Storey ◽  
V. Rotaciuc ◽  
S. Drapatz ◽  
R. Genzel
Keyword(s):  
Spatial Resolution ◽  
Molecular Hydrogen ◽  
Near Infrared ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Emission Lines ◽  
Resolving Power ◽  
Max Planck ◽  
First Time ◽  
Infrared Array

Images with subarcsec spatial resolution in the light of near-infrared atomic (Bry) and molecular hydrogen H2 (S(1) v=1-0) emission lines were obtained for some extended, pointlike objects in the Large Magellanic Cloud (LMC) for the first time. We used the Max-Planck-Institut für extraterrestrische Physik (MPE) near-infrared array spectrometer FAST (image scale 0.8”/pix, spectral resolving power 950) at the ESO/MPI 2.2m telescope, La Silla. We present some results on the 30-Dor complex and N159A5.

scholarly journals MIRAC: a mid-infrared array camera for astronomy

1993 ◽  
Author(s):  
William F. Hoffmann ◽  
Giovanni G. Fazio ◽  
Kandiah Shivanandan ◽  
Joseph L. Hora ◽  
Lynne K. Deutsch
Keyword(s):  
Mid Infrared ◽  
Array Camera ◽  
Infrared Array

scholarly journals ERRATUM: “THE SPITZER SOUTH POLE TELESCOPE DEEP FIELD: SURVEY DESIGN AND INFRARED ARRAY CAMERA CATALOGS” (2013, ApJS, 209, 22)

2014 ◽  
Vol 212 (1) ◽  
pp. 16 ◽  
Author(s):  
M. L. N. Ashby ◽  
S. A. Stanford ◽  
M. Brodwin ◽  
A. H. Gonzalez ◽  
J. Martinez-Manso ◽  
...  
Keyword(s):  
Field Survey ◽  
Survey Design ◽  
South Pole ◽  
South Pole Telescope ◽  
Array Camera ◽  
Infrared Array
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