IRAS 04384-4848 , the SIMBAD biblio

IRAS 04384-4848 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:32:59


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Title First 3 Authors
1988IRASP.C......0J viz 14       D               1 245223 ~ Infrared Astronomical Satellite Catalogs, 1988. The Point Source Catalog, version 2.0, NASA RP-1190 JOINT IRAS SCIENCE WORKING GROUP
1999MNRAS.308..897L viz 2404 75 The QDOT all-sky IRAS galaxy redshift survey. LAWRENCE A., ROWAN-ROBINSON M., ELLIS R.S., et al.
2000MNRAS.317...55S viz 14       D               1 16424 457 The PSCz catalogue. SAUNDERS W., SUTHERLAND W.J., MADDOX S.J., et al.
2000PYunO..83...15L 37 0 Preliminary results of 20 cm observations on an ultraluminous IRAS galaxy sample. LI Y.-S., SU B.-M. and NORRIS R.P.
2001AJ....122...63C 107 43 Statistical properties of ultraluminous IRAS galaxies from an HST imaging survey. CUI J., XIA X.-Y., DENG Z.-G., et al.
2001ApJ...552..527T 91 200 ISOCAM-CVF 5-12 micron spectroscopy of ultraluminous infrared galaxies. TRAN Q.D., LUTZ D., GENZEL R., et al.
2001MNRAS.326.1333F 1 26 98 HST/WFPC2 imaging of the QDOT ultraluminous infrared galaxy sample. FARRAH D., ROWAN-ROBINSON M., OLIVER S., et al.
2003A&A...412...45P viz 15       D               1 956189 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., et al.
2003ApJ...590..707M 97 25 A Hubble Space Telescope WFPC2 snapshot survey of 2MASS-selected red QSOs. MARBLE A.R., HINES D.C., SCHMIDT G.D., et al.
2003ApJS..147....1C viz 245 633 The relationship between stellar light distributions of galaxies and their formation histories. CONSELICE C.J.
2004AJ....128..163L viz 231 596 A new nonparametric approach to galaxy morphological classification. LOTZ J.M., PRIMACK J. and MADAU P.
2004ApJ...613..986P 122 348 Polycyclic aromatic hydrocarbons as a tracer of star formation? PEETERS E., SPOON H.W.W. and TIELENS A.G.G.M.
2004ApJS..150..343E viz 253 8 A uniform database of 2.2-16.5 µm spectra from the ISOCAM CVF spectrometer. ENGELKE C.W., KRAEMER K.E. and PRICE S.D.
2005A&A...441..999D 47 15 Follow-up near-infrared spectroscopy of ultraluminous infrared galaxies observed by ISO. DANNERBAUER H., RIGOPOULOU D., LUTZ D., et al.
2007ApJ...659..296L 24 46 Infrared molecular starburst fingerprints in deeply obscured (Ultra)Luminous infrared galaxy nuclei. LAHUIS F., SPOON H.W.W., TIELENS A.G.G.M., et al.
2009ApJ...700..395F 90       D         F     4 106 18 An evolutionary paradigm for dusty active galaxies at low redshift. FARRAH D., CONNOLLY B., CONNOLLY N., et al.
2009ApJ...701.1814V 15       D               1 262 71 A backward evolution model for infrared surveys: the role of AGN- and color-l TIRDistributions. VALIANTE E., LUTZ D., STURM E., et al.
2009ApJ...704.1506P 37           X         1 7 11 Paschen-α emission in the gravitationally lensed galaxy SMM J163554.2+661225. PAPOVICH C., RUDNICK G., RIGBY J.R., et al.
2010MNRAS.405.2505N viz 90       D         F     3 242 83 The role of nuclear activity as the power source of ultraluminous infrared galaxies. NARDINI E., RISALITI G., WATABE Y., et al.
2021A&A...651A.117T 17       D               2 125 4 A systematic study of silicate absorption features in heavily obscured AGNs observed by Spitzer/IRS. TSUCHIKAWA T., KANEDA H., OYABU S., et al.
2022ApJS..259...37S viz 17       D               1 3243 4 The Infrared Database of Extragalactic Observables from Spitzer. II. The Database and Diagnostic Power of Crystalline Silicate Features in Galaxy Spectra. SPOON H.W.W., HERNAN-CABALLERO A., RUPKE D., et al.
2022MNRAS.517.4162P 102       D         F     2 140 ~ Classification of local ultraluminous infrared galaxies and quasars with kernel principal component analysis. PAPAEFTHYMIOU E.S., MICHOS I., PAVLOU O., et al.
2022ApJ...941...50T 17       D               2 101 ~ Spitzer/IRS Full Spectral Modeling to Characterize Mineralogical Properties of Silicate Dust in Heavily Obscured AGNs. TSUCHIKAWA T., KANEDA H., OYABU S., et al.
2023ApJS..269....3M viz 17       D               1 356397 ~ Siena Galaxy Atlas 2020. MOUSTAKAS J., LANG D., DEY A., et al.

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