ATELAIS J003907.93-433205.8 , the SIMBAD biblio

ATELAIS J003907.93-433205.8 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST16:29:12


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Title First 3 Authors
1999MNRAS.305..297G viz 656 58 A 1.4-GHz survey of the southern European Large-Area ISO Survey region. GRUPPIONI C., CILIEGI P., ROWAN-ROBINSON M., et al.
2004MNRAS.351.1290R viz 15       D               3768 122 The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue. ROWAN-ROBINSON M., LARI C., PEREZ-FOURNON I., et al.
2008AJ....135.1276M viz 15       D               1 1225 51 Deep Australia Telescope Large Area Survey radio observations of the european large area ISO survey S1/Spitzer wide-area infrared extragalactic field. MIDDELBERG E., NORRIS R.P., CORNWELL T.J., et al.
2011A&A...526A...8M 38           X         1 33 25 The radio properties of infrared-faint radio sources. MIDDELBERG E., NORRIS R.P., HALES C.A., et al.
2011MNRAS.415..845C 15       D               1 24 3 Are the infrared-faint radio sources pulsars? CAMERON A.D., KEITH M., HOBBS G., et al.
2011A&A...531A..14Z 15       D               1 63 16 Infrared-faint radio sources: a cosmological view. AGN number counts, the cosmic X-ray background and SMBH formation. ZINN P.-C., MIDDELBERG E. and IBAR E.
2015A&A...580A...7H 135       D     X C       3 24 4 Infrared-faint radio sources remain undetected at far-infrared wavelengths. Deep photometric observations using the Herschel Space Observatory. HERZOG A., NORRIS R.P., MIDDELBERG E., et al.
2016A&A...593A.130H 40           X         1 46 4 The radio spectral energy distribution of infrared-faint radio sources. HERZOG A., NORRIS R.P., MIDDELBERG E., et al.
2018MNRAS.477..578C 16       D               1 11 3 High-resolution observations of low-luminosity gigahertz-peaked spectrum and compact steep-spectrum sources. COLLIER J.D., TINGAY S.J., CALLINGHAM J.R., et al.
2021A&A...655A..17S viz 17       D               1 338596 3 The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. STEIN Y., VOLLMER B., BOCH T., et al.

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