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| ATELAIS J002905.22-433403.9 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST15:21:12 |
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More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
2008AJ....135.1276M 
|
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. | ||
| 2011ApJ...736...55N | 15 | D | 2 | 59 | 25 | Deep Spitzer observations of infrared-faint radio sources: high-redshift radio-loud active galactic nuclei? | NORRIS R.P., AFONSO J., CAVA 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. | ||
|
2012MNRAS.421.1644R
|
93 | D | X | 3 | 20 | 30 | Spectral index properties of milliJansky radio sources. | RANDALL K.E., HOPKINS A.M., NORRIS R.P., et al. | |
| 2015A&A...580A...7H | 254 | D | X C | 6 | 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. | ||
|
2021A&A...655A..17S
|
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. |
