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| NVSS J172508+370936 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST14:01:17 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
2000ApJS..131..185S 
|
109 | 55 | The FIRST sample of ultraluminous infrared galaxies at high redshift. I. Sample and near-infrared morphologies. | STANFORD S.A., STERN D., VAN BREUGEL W., et al. | |||||
| 2006ApJ...648..323H | 82 | 65 | A Spitzer Space Telescope Infrared Spectrograph Survey of warm molecular hydrogen in ultraluminous infrared galaxies. | HIGDON S.J.U., ARMUS L., HIGDON J.L., et al. | |||||
|
2008ApJ...683..114S
|
15 | D | 1 | 29 | 12 | Spitzer IRS spectra of optically faint IRAS sources. | SARGSYAN L., MICKAELIAN A., WEEDMAN D., et al. | ||
|
2009ApJ...698.1682W
|
15 | D | 2 | 178 | 9 | Evolution of the most luminous dusty galaxies. | WEEDMAN D.W. and HOUCK J.R. | ||
|
2009MNRAS.398..109W
|
15 | D | 1 | 22041 | 37 | The imperial IRAS-FSC redshift catalogue. | WANG L. and ROWAN-ROBINSON M. | ||
|
2010MNRAS.405.2505N
|
90 | D | F | 2 | 242 | 83 | The role of nuclear activity as the power source of ultraluminous infrared galaxies. | NARDINI E., RISALITI G., WATABE Y., et al. | |
|
2013A&A...550A..41C
|
16 | D | 1 | 39 | 108 | Gas fraction and star formation efficiency at z < 1.0. | COMBES F., GARCIA-BURILLO S., BRAINE J., et al. | ||
|
2019MNRAS.487.1823L
|
16 | D | 1 | 1896 | 23 | Mid-infrared spectroscopic evidence for AGN heating warm molecular gas. | LAMBRIDES E.L., PETRIC A.O., TCHERNYSHYOV K., et al. | ||
|
2022ApJS..259...37S
|
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. |
