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| SDSS J140447.40+363627.3 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:40:43 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1999A&A...350..414P | 55 | 22 | On the star-formation properties of emission-line galaxies in and around voids. | POPESCU C.C., HOPP U. and ROSA M.R. | |||||
| 2000A&AS..142..247P | 95 | 36 | A spectrophotometric catalogue of HII galaxies. | POPESCU C.C. and HOPP U. | |||||
|
2001A&A...374..907U |
194 | 10 | The Hamburg/SAO survey for emission-line galaxies. V. The fifth list of 161 galaxies. | UGRYUMOV A.V., ENGELS D., KNIAZEV A.Y., et al. | |||||
|
2006MNRAS.365..454H |
408 | 26 | The impact of the visibility of the [OIII]λ4363 line on the general properties of HII galaxies in the Local Universe. | HOYOS C. and DIAZ A.I. | |||||
|
2008A&A...485..657B |
15 | D | 578 | 188 | Galaxies with Wolf-Rayet signatures in the low-redshift Universe. A survey using the Sloan Digital Sky Survey. | BRINCHMANN J., KUNTH D. and DURRET F. | |||
|
2014ApJ...788...45T |
15 | D | 1 | 224166 | 54 | Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. | TOBA Y., OYABU S., MATSUHARA H., et al. | ||
|
2017A&A...599A..71D |
16 | D | 1 | 209271 | 41 | Aperture-free star formation rate of SDSS star-forming galaxies. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. | ||
|
2018AJ....155...17C |
16 | D | 1 | 802 | ~ | Infrared photometric study of Wolf-Rayet galaxies. | CHEN P.S., YANG X.H., LIU J.Y., et al. | ||
|
2018MNRAS.478.3447E |
16 | D | 2 | 107 | 64 | Enhanced atomic gas fractions in recently merged galaxies: quenching is not a result of post-merger gas exhaustion. | ELLISON S.L., CATINELLA B. and CORTESE L. | ||
|
2022A&A...666A.186D |
17 | D | 1 | 194359 | 6 | Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. | DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al. |