Deep 15um AKARI observations in the CDFS: estimating dust

Nov 23, 2008 - We will try to understand better the physics of the two galaxy samples by analysing the f24/f15 ratio by a comparison with the models a...

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firmed by the SIMBAD astronomical database as stars or. QSOs, so we removed them from our catalogs, leaving 1678 sources for the photometric redshift algorithm ...... South (HDFS), and more similar to the value of ∼ 20% to ∼. 35% determined by Fo

Jun 1, 2007 - 2002). Ramdani and Jorissen (2001) observed outer regions of. NGC104, and Origlia et al. (2002) observed an area of about 5′ × 3′ centered on the cluster core. The IRC's wide field of view (10′ × 10′) enables us to cover both

Dec 3, 2016 - 2 Institut de Ci`encies del Cosmos (ICCUB), Universitat de Barcelona ..... 555, A43. Gilli, R., Comastri, A., & Hasinger, G. 2007, A&A, 463, 79.

Most of the SWIRE data are now in the public domain (see Here we use the SWIRE Public. Data Release 3. The IRAC and MIPS fluxes used here are, in the case of unresolved or noisy sourc

Jul 27, 2007 - ... Disc galaxy with star formation taking place around the cen- ... Disc galaxy with mild star formation taking place in knots.

( .... ( ...... This figure "fig12_1.jpg" is available in "jpg"format from:.

Feb 16, 2018 - Of particular interest are near- and mid-infrared (NIR and MIR) observations, as they trace the dust emission resulting from the heating by ...

Apr 1, 2015 - ferent IRC filters led us to perform a 8µm rest-frame selection. In Fig.8 is reported the IR luminosity (obtained with CIGALE) against redshift for our sample. We estimated the detection limit at 5σ using the flux limits of Murata et

Nov 25, 2008 - We investigate the photometric redshift accuracy achievable with the AKARI infrared data in deep multi-band surveys, such as in the North Ecliptic Pole field. We demon- strate that the passage of redshifted policyclic aromatic hydrocar

Aug 18, 2005 - ABSTRACT. We explore the evolution of field early-type galaxies on a sample extracted from the ACS images of the Southern GOODS field. The galaxies are selected by means of a non-parametric analysis followed by visual inspection of the

Nov 30, 2009 - 5 College of Inter-Faculty Individual Studies in Mathematics and ..... sources are summarized in the tables which are available online. ...... (upside-down red triangles) and UV: 1650, 2500, 3150 nm (full navy blue upside-down.

Mar 23, 2011 - In this paper, we present the first results of our search for AGNs based on ... heated by the central engine of the AGN, even though their optical spectra do not show ..... from the Japan Society for the Promotion of Science (No.

Mar 11, 2016 - 2015; Kondo et al. 2016). The DIRBE model cannot reproduce the real fine structure of the asteroidal dust-band components, because DIRBE operated with a large. 42′ × 42′ beam, and only a small fraction of the DIRBE data were used

Sep 17, 2010 - Typical total exposure time per map pixel after these observations were completed was 164s at 24µm and 73.7s at 70µm. The 24 and 70 micron images were created from raw data frames using the MIPS Data Analysis Tools (DAT) version 3.10

Sep 17, 2010 - Section 2 we describe the Spitzer observations and the data processing steps used to produce the reduced maps. In Sec- tion 3 we describe source extraction at 24µm and the pro- duction of the 24µm counts. Section 4 does the same at.

Jun 7, 2010 - Milton Keynes, MK7 6AA, UK. 2Space Science ... To interpret the CIRB in terms of galaxy formation and evolution models (e.g. Granato et al.

Jun 7, 2010 - Spitzer, SCUBA and BLAST data have shown, via stacking analysis of 24µm ..... Rush, B., Malkan, M. A., & Spinoglio, L. 1993, ApJS, 89, 1.

Feb 23, 2011 - For example, the absorption of various ice species ... detection of the CO2, XCN and CO ices was reported in the nucleus of NGC 4945 (Spoon ...

1Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1. Yoshinodai, Chuo-ku, Sagamihara, Kanagawa ...... thank an anonymous reviewer for their careful and constructive reviews, which helped us improve the manuscript

Oct 6, 2009 - nant G292.0+1.8 using six IRC and four FIS bands covering 2.7–26.5 µm and. 50–180 .... The IRC observations were conducted in the two-filter mode that ...... 26.8. 26.8. 44.2. 44.2. FWHM (′′). 4.0. 4.2. 5.1. 4.8. 5.7. 6.8. 37.

Feb 23, 2011 - the center of the galaxy, we clearly detect the absorption features of .... In addition, on the south side, the ices show peaks in the S3 and S4 ...

This procedure excluded most of the sources in the S7 and S11 bands: hence ... t0 is the time of maxi- mum light (either in V or I band) and P is the pulsational.

Oct 29, 2012 - 1Institute of Space and Astronautical Science, Japan Aerospace .... S cameras share the same field of view through a beam splitter, ... The data packages of the IRC slow-scan observations are stored in dedicated FITS file.

Jan 6, 2016 - arXiv:1601.01206v1 [astro-ph.GA] 6 Jan 2016. Publications of the Korean Astronomical Society. pISSN: 1225-1534 / eISSN: 2287-6936. 00: 1 ∼ 99, 2014 March ... lengths' will differ depending on the scientific goals of the survey. The la