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IRAS F10119+1429 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST08:08:39 |
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 |
---|---|---|---|---|---|---|---|---|---|
2000MNRAS.316..885R | 1 | 47 | 167 | Hyperluminous infrared galaxies. | ROWAN-ROBINSON M. | ||||
2001ApJS..133....1U | 1480 | 79 | The ASCA medium sensitivity survey (the GIS catalog project): source catalog. | UEDA Y., ISHISAKI Y., TAKAHASHI T., et al. | |||||
2002MNRAS.335..574V | 35 | 32 | Observations of hyperluminous infrared galaxies with the Infrared Space Observatory : implications for the origin of their extreme luminosities. | VERMA A., ROWAN-ROBINSON M. and McMAHON R. | |||||
2002PASJ...54..327K | 83 | 218 | Study of the X-ray background spectrum and its large-scale fluctuation with ASCA. | KUSHINO A., ISHISAKI Y., MORITA U., et al. | |||||
2003A&A...411L..59E | 1017 | 51 | High-energy sources before INTEGRAL. INTEGRAL reference catalog. | EBISAWA K., BOURBAN G., BODAGHEE A., et al. | |||||
2003MNRAS.346L..51S | 37 | 11 | The K -band Hubble diagram of submillimetre galaxies and hyperluminous galaxies. | SERJEANT S., FARRAH D., GEACH J., et al. | |||||
2004MNRAS.349..518F | 8 | 17 | The environments of hyperluminous infrared galaxies at 0.44 < z < 1.55. | FARRAH D., GEACH J., FOX M., et al. | |||||
2009MNRAS.398..109W | 15 | D | 1 | 50356 | 37 | The imperial IRAS-FSC redshift catalogue. | WANG L. and ROWAN-ROBINSON M. | ||
2010A&A...511A..53V | 15 | D | 1 | 107940 | 39 | The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory. | VOLLMER B., GASSMANN B., DERRIERE S., et al. | ||
2018A&A...619A.169R | 16 | D | 2 | 53 | 6 | Extreme submillimetre starburst galaxies. | ROWAN-ROBINSON M., WANG L., FARRAH D., 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. |