Rho, J., Kozasa, T., Reach, W. T., Rudnick, L., DeLaney, T., Smith, J. D., ...
We performed Spitzer Infrared Spectrograph mapping observations covering nearly the entire extent of the Cassiopeia A supernova remnant (SNR), producing mid-infrared (5.5-35 micron) spectra every...
Aromatic emission from the ionised mane of the Horsehead nebula (2007)
Compiegne, M., Abergel, A., Verstraete, L., Reach, W. T., Habart, E., Smith, J. D., ...
We study the evolution of the Aromatic Infrared Bands (AIBs) emitters across the illuminated edge of the Horsehead nebula and especially their survival and properties in the HII region. We present...
First Space-Based Microlens Parallax Measurement: Spitzer Observations of OGLE-2005-SMC-001 (2007)
Dong, Subo, Udalski, A., Gould, A., Reach, W. T., Christie, G. W., Boden, A. F., ...
We combine Spitzer and ground-based observations to measure the microlens parallax of OGLE-2005-SMC-001, the first such space-based determination since S. Refsdal proposed the idea in 1966. The...
Spitzer IRAC Images and Sample Spectra of Cassiopeia A's Explosion (2006)
Ennis, J. A., Rudnick, L., Reach, W. T., Smith, J. D., Rho, J., DeLaney, T., ...
We present Spitzer IRAC images, along with representative 5.27 to 38.5 micron IRS spectra of the Cassiopeia A supernova remnant. We find that various IRAC channels are each most sensitive to a...
Smith, Beverly J., Struck, C., Hancock, M., Appleton, P. N., Charmandaris, V., Reach, W. T.
We present Spitzer mid-infrared imaging of a sample of 35 tidally-distorted pre-merger interacting galaxy pairs selected from the Arp Atlas. We compare their global mid-infrared properties with those...
Tappe, A., Rho, J., Reach, W. T.
We observed the oxygen-rich Large Magellanic Cloud (LMC) supernova remnant N132D (SNR 0525-69.6), using all instruments onboard the Spitzer Space Telescope, IRS, IRAC, and MIPS (Infrared...
Dust in High-Velocity Clouds : relevance for Planck (2006)
Miville-Deschenes, M. -A., Boulanger, F., Martin, P. G., Lockman, F. J., Reach, W. T., Noriega-Crespo, A.
The recent detection of dust emission in Complex C, the largest High-Velocity Cloud (HVC) on the sky, opens a very interesting perspective for Planck. The HVC dust temperature determined using IRAS...
Flagey, N., Boulanger, F., Verstraete, L., Deschenes, M. A. Miville, Crespo, A. Noriega, Reach, W. T.
We measure IRAC colors of extended emission in several fields covering a range of Galactic latitudes and longitudes outside of star forming regions. We determine the nature of the Galactic diffuse...
Rho, J., Reach, W. T., Lefloch, B., Fazio, G.
Spitzer IRAC and MIPS images of the Trifid Nebula (M20) reveal its spectacular appearance in infrared light, highlighting the nebula's special evolutionary stage. The images feature recently-formed...
First detection of dust emission in a High-Velocity Cloud (2005)
Miville-Deschenes, M. -A., Boulanger, F., Reach, W. T., Noreiga-Crespo, A.
By comparing sensitive Spitzer Space Telescope (SST) infrared and Green Bank Telescope 21 cm observations, we are able to report the first detection of dust emission in Complex C, the largest High...
The 1997 Reference of Diffuse Night Sky Brightness (2004)
Leinert, C., Bowyer, S., Haikala, L. K., Hanner, M. S., Hauser, M. G., Levasseur-Regourd, A. C., ...
In the following we present material in tabular and graphical form, with the aim to allow the non specialist to obtain a realistic estimate of the diffuse night sky brightness over a wide range of...
Reach, W. T., Wall, W. F., Odegard, N.
We have created a map of the large-scale infrared surface bightness in excess of that associated with the atomic interstellar medium, using region-by-region correlations between the far-infrared and...
Excitation and Disruption of a Giant Molecular Cloud by the Sepurnova Remnant 3C 391 (2004)
The ambient molecular gas at the distance of the remnant comprises a giant molecular cloud whose edge is closely parallel to a ridge of bright non-thermal radio continuum, which evidently delineates...
Rho, J., Jarrett, T. H., Cutri, C. M., Reach, W. T.
We present near-infrared J (1.25 mum), H (1.65 mum), and K-s (2.17 mum) imaging of the entire supernova remnant IC 443 from the Two Micron All Sky Survey (2MASS), and Infrared Space Observatory (ISO)...
2MASS observation of RCW 103: evolution of young SNR in dense environment (2004)
Rho, J., Koo, B.-C., Reach, W. T., Jarrett, T. H., Cutri, R., Skrutsk, M.
We present near-infrared images of the supernova remnant RCW 103 from the Two Micron All Sky Survey (2MASS).
X-rays and protostars in the Trifid Nebula (2004)
Rho, J., Corcoran, M. F., Chu, Y.-H., Reach, W. T.
The Nature of Faint 24 micron Sources Seen in Spitzer Observations of ELAIS-N1 (2004)
Chary, R., Casertano, S., Dickinson, M. E., Ferguson, H. C., Eisenhardt, P. R. M., Elbaz, D., ...
The Spitzer Space Telescope has undertaken the deepest ever observations of the 24 micron sky in the ELAIS-N1 field as part of GOODS Science Verification observations. We present the shape of the 24...
The IRAC Shallow Survey (2004)
Eisenhardt, P. R., Stern, D., Brodwin, M., Fazio, G. G., Rieke, G. H., Rieke, M. J., ...
The IRAC shallow survey covers 8.5 square degrees in the NOAO Deep Wide-Field Survey in Bootes with 3 or more 30 second exposures per position. An overview of the survey design, reduction,...
Deep mid-infrared observations of Lyman-break galaxies (2004)
Barmby, P., Huang, J. -S., Fazio, G. G, Surace, J. A., Arendt, R. G., Hora, J. L., ...
As part of the In-Orbit Checkout activities for the Spitzer Space Telescope, the IRAC team carried out a deep observation (average integration time ~8 hours) of a field surrounding the bright QSO HS...
THE ASTROPHYSICAL JOURNAL, 555 563571, 2001 July 10 (2003)
L. Cambre, Sy And, W. T. Reach, C. A. Beichman, T. H. Jarrett
Using the 2MASS second incremental data release and the zodiacal subtracted mission average maps of COBE/DIRBE, we estimate the cosmic background in the J (1.25 km) and K (2.2 km) bands using...
Dole, Herve, Gispert, Richard, Lagache, Guilaine, Puget, Jean-Loup, Bouchet, F. R., Cesarsky, C., ...
The FIRBACK (Far Infrared BACKground) survey is one of the deepest imaging surveys carried out at 170 microns with ISOPHOT onboard ISO, and is aimed at the study of the structure of the Cosmic Far...
Cambresy, L., Reach, W. T., Beichman, C. A., Jarrett, T. H.
Using the 2MASS 2nd Incremental Data Release and the Zodiacal-Subtracted Mission Average maps of COBE/DIRBE, we estimate the cosmic background in the J (1.25 micron) and K (2.2 microns) bands using...
Near-infrared Imaging and [O~I] spectroscopy of IC 443 using 2MASS and ISO (2000)
Rho, Jeonghee, Jarrett, T. H., Cutri, R. M., Reach, W. T.
We present near-infrared J (1.25um), H (1.65um), and Ks (2.17um) imaging of the entire supernova remnant IC 443 from the Two Micron All Sky Survey (2MASS), and Infrared Space Observatory (ISO) LWS...
FIRBACK Source Counts and Cosmological Implications (2000)
Dole, Herve, Gispert, Richard, Lagache, Guilaine, Puget, Jean-Loup, Aussel, H., Bouchet, F. R., ...
FIRBACK is a one of the deepest surveys performed at 170 microns with ISOPHOT onboard ISO, and is aimed at the study of cosmic far infrared background sources. About 300 galaxies are detected in an...
The extragalactic background and its fluctuations in the far-infrared wavelengths (2000)
Lagache, G., Puget, J-L., Abergel, A., Bouchet, F. R., Boulanger, F., Ciliegi, P., ...
A Cosmic Far-InfraRed Background (CFIRB) has long been predicted that would traces the intial phases of galaxy formation. It has been first detected by Puget et al.(1996) using COBE data and has been...
Dust in the Local Interstellar Wind (1999)
Frisch, P. C., Dorschner, J. M., Geiss, J., Greenberg, J. M., Grün, E., Landgraf, M., ...
The gas-to-dust mass ratios found for interstellar dust within the Solar System, versus values determined astronomically for the cloud around the Solar System, suggest that large and small...
FIRBACK Far Infrared Survey with ISO: Data Reduction, Analysis and First Results (1999)
Dole, Herve, Lagache, Guilaine, Puget, Jean-Loup, Gispert, Richard, Aussel, H., Bouchet, F. R., ...
FIRBACK is one of the deepest cosmological surveys performed in the far infrared, using ISOPHOT. We describe this survey, its data reduction and analysis. We present the maps of fields at 175...
A Deep 12 Micron Survey with ISO (1999)
Clements, D. L., Desert, F-X., Franceschini, A., Reach, W. T., Baker, A. C., Davies, J. K., ...
We present the first results of a study of faint 12 micron sources detected with the Infrared Space Observatory (ISO) in four deep, high galactic latitude fields. The sample includes 50 such sources...
FIRBACK: I. A deep survey at 175 $\mu$m with ISO, preliminary results (1998)
Puget, J. L., Lagache, G., Clements, D. L, Reach, W. T., Aussel, H., Bouchet, F. R, ...
FIRBACK is a deep survey conducted with the ISOPHOT instrument aboard the Infrared Space Observatory (ISO) at an effective wavelength of 175 $\mu$m. We present here results we have obtained on the...
The FIRBACK 175 micron Survey (1998)
Clements, David L., Puget, J-L, Lagache, G., Dole, H., Cox, P., Gispert, R., ...
The FIRBACK project is a collaboration of eight institutes aimed at using long wavelength surveys with ISO to uncover the nature of the Cosmic Far-Infrared Background. We have surveyed nearly 4 sq....
Kelsall, T., Weiland, J. L., Franz, B. A., Reach, W. T., Arendt, R. G., Dwek, E., ...
The COBE Diffuse Infrared Background Experiment (DIRBE) was designed to search for the cosmic infrared background (CIB) radiation. Scattered light and thermal emission from the interplanetary dust...
Hauser, M. G., Arendt, R. G., Kelsall, T., Dwek, E., Odegard, N., Weiland, J. L., ...
The DIRBE on the COBE spacecraft was designed primarily to conduct systematic search for an isotropic CIB in ten photometric bands from 1.25 to 240 microns. The results of that search are presented...
Arendt, R. G., Odegard, N., Weiland, J. L., Sodroski, T. J., Hauser, M. G., Dwek, E., ...
The Cosmic Infrared Background (CIB) is hidden behind veils of foreground emission from our own solar system and Galaxy. This paper describes procedures for removing the Galactic IR emission from the...
High-Latitude Galactic Emission in the COBE DMR Two-Year Sky Maps (1995)
Kogut, A., Banday, A. J., Bennett, C. L., Gorski, K. M., Hinshaw, G., Reach, W. T.
We cross-correlate the COBE-DMR 2-year sky maps with spatial templates from long-wavelength radio surveys and the far-infrared COBE DIRBE maps. We place an upper limit on the spectral index of...
FAR-INFRARED SPECTRAL OBSERVATIONS OF THE GALAXY BY COBE (1995)
Reach, W. T., Dwek, E., Fixsen, D. J., Hewagama, T., Mather, J. C., Shafer, R. A., ...
We derive Galactic continuum spectra from 5-96/cm from COBE/FIRAS observations. The spectra are dominated by warm dust emission, which may be fit with a single temperature in the range 16-21 K (for...