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[KLG2007] GC1 92 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST06:06:48 |
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 |
---|---|---|---|---|---|---|---|---|---|
2003AJ....126..175B | 15 | D | 270 | 44 | DIRECT distances to nearby galaxies using detached eclipsing binaries and cepheids. IX. Variables in the field M31Y discovered with image subtraction. | BONANOS A.Z., STANEK K.Z., SASSELOV D.D., et al. | |||
2006A&A...459..321V | 15 | D | 3968 | 33 | Eclipsing binaries suitable for distance determination in the Andromeda galaxy. | VILARDELL F., RIBAS I. and JORDI C. | |||
2007AJ....134..706K | 15 | D | 749 | 43 | Wide-field survey of globular clusters in M 31. I. A catalog of new clusters. | KIM S.C., LEE M.G., GEISLER D., et al. | |||
2010MNRAS.402..803P | 15 | D | 1 | 1599 | 87 | The M31 globular cluster system: ugriz and K-band photometry and structural parameters. | PEACOCK M.B., MACCARONE T.J., KNIGGE C., et al. | ||
2010ApJ...725..200F | 15 | D | 1 | 988 | 23 | An updated catalog of M31 globular-like clusters: UBVRI photometry, ages, and masses. | FAN Z., DE GRIJS R. and ZHOU X. | ||
2012ApJS..199...37K | 15 | D | 1 | 713 | 25 | A comprehensive GALEX ultraviolet catalog of star clusters in M31 and a study of the young clusters. | KANG Y., REY S.-C., BIANCHI L., et al. | ||
2012ApJ...752...95J | 15 | D | 1 | 1244 | 44 | PHAT stellar cluster survey. I. Year 1 catalog and integrated photometry. | JOHNSON L.C., SETH A.C., DALCANTON J.J., et al. | ||
2013AJ....145..106K | 16 | D | 1 | 2023 | 19 | Properties of M31. II. A Cepheid disk sample derived from the first year of PS1 PAndromeda data. | KODRIC M., RIFFESER A., HOPP U., et al. | ||
2013ApJ...769...10J | 16 | D | 1 | 470 | 11 | A survey for planetary nebulae in M31 globular clusters. | JACOBY G.H., CIARDULLO R., DE MARCO O., et al. | ||
2018ApJ...861...36A | 165 | X F | 3 | 180 | 38 | On Cepheid distance scale bias due to stellar companions and cluster populations. | ANDERSON R.I. and RIESS A.G. |