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| US 3506 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:57:17 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1984ApJS...56..393H |
14 | D | 1316 | 21 | Faint blue objects at high galactic latitude. IV. Palomar Schmidt fields centered on selected areas 55 and 94. | HUANG K.-L. and USHER P.D. | |||
| 1986Ap&SS.125...85H | 282 | 4 | Optically selected QSO candidates in the field centered on selected Area 94. | HUANG K.-L. and HUANG J.-H. | |||||
| 1987A&AS...67..551B | 176 | 13 | Quasar candidates in the field of SA 94. II. Objective-prism classification of the US objects. | BARBIERI C., CRISTIANI S., IOVINO A., et al. | |||||
|
1995A&AS..112..347C |
567 | 40 | The ESO key-programme "A homogeneous bright QSO survey". I. The methods and the "deep" fields. | CRISTIANI S., LA FRANCA F., ANDREANI P., et al. | |||||
|
2002ApJS..141...23E |
330 | 5 | JHK' imaging photometry of Seyfert 1 active galactic nuclei and quasars. I. Multiaperture photometry. | ENYA K., YOSHII Y., KOBAYASHI Y., et al. | |||||
|
2004ApJS..153..119M |
15 | D | 654 | 2 | Faint blue objects at high galactic latitude. VIII. Performance characteristics of the US survey. | MITCHELL K.J. and USHER P.D. | |||
|
2006A&A...455..773V |
108223 | 628 | A catalogue of quasars and active nuclei: 12th edition. | VERON-CETTY M.-P. and VERON P. | |||||
|
2009A&A...505..385A |
15 | D | 1 | 99836 | 35 | The large quasar reference frame (LQRF). An optical representation of the ICRS. | ANDREI A.H., SOUCHAY J., ZACHARIAS N., et al. | ||
|
2010A&A...518A..10V |
15 | D | 1 | 168913 | 597 | A catalogue of quasars and active nuclei: 13th edition. | VERON-CETTY M.-P. and VERON P. | ||
|
2018AJ....155..189D |
16 | D | 1 | 18896 | 7 | The Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) Quasar Survey: quasar properties from data release two and three. | DONG X.Y., WU X.-B., AI Y.L., et al. |