Zobrazeno 1 - 10
of 451
pro vyhledávání: '"Stickel, M"'
Autor:
Leipski, C., Meisenheimer, K., Klaas, U., Walter, F., Nielbock, M., Krause, O., Dannerbauer, H., Bertoldi, F., Besel, M. -A., de Rosa, G., Fan, X., Haas, M., Hutsemekers, D., Jean, C., Lemke, D., Rix, H. -W., Stickel, M.
We present Herschel far-infrared (FIR) observations of two sub-mm bright quasars at high redshift: SDSS J1148+5251 (z=6.42) and BR 1202-0725 (z=4.69) obtained with the PACS instrument. Both objects are detected in the PACS photometric bands. The Hers
Externí odkaz:
http://arxiv.org/abs/1005.5016
Constraints on the density and thermal 3D structure of the dense molecular cloud core Rho Oph D are derived from a detailed 3D radiative transfer modeling. Two ISOCAM images at 7 and 15 micron are fitted simultaneously by representing the dust distri
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410635
Autor:
Heraudeau, Ph., Oliver, S., del Burgo, C., Kiss, C., Stickel, M., Mueller, T., Rowan-Robinson, M., Efstathiou, A., Surace, C., Toth, L. V., Serjeant, S., Alexander, D. M., Franceschini, A., Lemke, D., Perez-Fournon, I., Morel, T., Puget, J-L., Rigopoulou, D., Rocca-Volmerange, B., Verma, A.
We present a re--analysis of the European Large Area ISO Survey (ELAIS) 90mum observations carried out with ISOPHOT, an instrument on board the ESA's Infrared Space Observatory (ISO). With more than 12 sq. deg., the ELAIS survey is the largest area c
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410379
Autor:
Serjeant, S., Carraminana, A., Gonzales-Solares, E., Heraudeau, P., Mujica, R., Perez-Fournon, I., Sedgwick, N., Rowan-Robinson, M., Franceschini, A., Babbedge, T., del Burgo, C., Ciliegi, P., Efstathiou, A., La Franca, F., Gruppioni, C., Hughes, D., Lari, C., Oliver, S., Pozzi, F., Stickel, M., Vaccari, M.
We present the 90 micron luminosity function of the Final Analysis of the European Large Area ISO Survey (ELAIS), extending the sample size of our previous analysis (paper IV) by about a factor of 4. Our sample extends to z=1.1, around 50 times the c
Externí odkaz:
http://arxiv.org/abs/astro-ph/0401289
Publikováno v:
Astron.Astrophys.407:137-146,2003
The Sc galaxy M33 has been mapped with ISOPHOT in the far-infrared, at 60, 100, and 170mue. The spatial resolution of these FIR maps allows the separation of spiral arms and interarm regions and the isolation of a large number of star-forming regions
Externí odkaz:
http://arxiv.org/abs/astro-ph/0306558
Publikováno v:
Astron.Astrophys. 398 (2003) 1007-1020
We present a multi-wavelength study of the star forming region ISOSS J 20298+3559, which was identified by a cross-correlation of cold compact sources from the 170 micron ISOPHOT Serendipity Survey (ISOSS) database coinciding with objects detected by
Externí odkaz:
http://arxiv.org/abs/astro-ph/0209288
The ISOPHOT Serendipity Survey (ISOSS) covered approximately 15 % of the sky at a wavelength of 170 micron while the ISO satellite was slewing from one target to the next. By chance ISOSS slews went over many solar system objects (SSOs). We identifie
Externí odkaz:
http://arxiv.org/abs/astro-ph/0203216
Publikováno v:
Astron.Astrophys. 395 (2002) 663-668
A faint $I_{\rm 170}=4$ MJysr$^{-1}$ bipolar globule was discovered with the ISOPHOT 170 $\mu$m Serendipity Survey (ISOSS). ISOSS J 20246+6541 is a cold ($T_{\rm d}\approx 14.5$ K) FIR source without an IRAS pointsource counterpart. In the Digitized
Externí odkaz:
http://arxiv.org/abs/astro-ph/0202523
The ISOPHOT instrument aboard ISO has been used to observe extended FIR emission of six Abell clusters. The raw profiles of the I_(120 um) / I_(180 um) surface brightness ratio including zodiacal light show a bump towards Abell 1656 (Coma), dips towa
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112063
Autor:
Dole, Herve, Gispert, Richard, Lagache, Guilaine, Puget, Jean-Loup, Bouchet, F. R., Cesarsky, C., Ciliegi, P., Clements, D. L., Dennefeld, M., Desert, F-X, Elbaz, D., Franceschini, A., Guiderdoni, B., Harwit, M., Lemke, D., Moorwood, A. F. M., Oliver, S., Reach, W. T., Rowan-Robinson, M., Stickel, M.
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 Infrared Background. This paper provides the analysis
Externí odkaz:
http://arxiv.org/abs/astro-ph/0103434