SV* HV 5655 , the SIMBAD biblio

SV* HV 5655 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.02.22CET01:14:29


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Title First 3 Authors
1979MNRAS.188..139M 71 156 Multicolour photoelectric photometry of Magellanic Cloud Cepheids. II. An analysis of BVRI observations in the LMC. MARTIN W.L., WARREN P.R. and FEAST M.W.
1979SAAOC...1...98M 70 35 Multicolour photoelectric photometry of Magellanic Cloud Cepheids. I: Individual UBVI observations. MARTIN W.L. and WARREN P.R.
1984A&AS...56..169W 176 17 Photometry of Cepheid variables in the Large Magellanic Cloud. WAYMAN P.A., STIFT M.J. and BUTLER C.J.
1985MNRAS.212..395D 118 11 Period change in Magellanic Cloud Cepheids. DEASY H.P. and WAYMAN P.A.
1996A&A...305....1K 50 8 On improved Cepheid distance estimators. KANBUR S.M. and HENDRY M.A.
2002ApJS..142...71S viz 15       D               616 36 The cepheid period-luminosity relation in the Large Magellanic Cloud. SEBO K.M., RAWSON D., MOULD J., et al.
2004A&A...424...43S 100 144 New period-luminosity and period-color relations of classical Cepheids. II. Cepheids in LMC. SANDAGE A., TAMMANN G.A. and REINDL B.
2004AJ....128.2239P viz 93 212 New cepheid period-luminosity relations for the Large Magellanic Cloud: 92 near-infrared light curves. PERSSON S.E., MADORE B.F., KRZEMINSKI W., et al.
2005MNRAS.363..831N 59 52 Further empirical evidence for the non-linearity of the period-luminosity relations as seen in the Large Magellanic Cloud Cepheids. NGEOW C.-C., KANBUR S.M., NIKOLAEV S., et al.
2008ApJ...679...71F viz 15       D               1 71 34 The Cepheid period-luminosity relation at mid-infrared wavelengths. I. First-epoch LMC data. FREEDMAN W.L., MADORE B.F., RIGBY J., et al.
2009ApJ...695..988M 15       D               2 74 26 The Cepheid period-luminosity relation (The Leavitt law) at mid-infrared wavelengths. II. Second-epoch LMC data. MADORE B.F., FREEDMAN W.L., RIGBY J., et al.
2008AcA....58..163S viz 15       D               1 3398 282 The Optical Gravitational Lensing Experiment. The OGLE-III catalog of variable stars. I. Classical Cepheids in the Large Magellanic Cloud. SOSZYNSKI I., POLESKI R., UDALSKI A., et al.
2008AcA....58..313P viz 15       D               1 2950 15 Period changes of LMC Cepheids in the OGLE and MACHO Data. POLESKI R.
2011A&A...534A..95S viz 16       D   O           2 43 108 Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC'. STORM J., GIEREN W., FOUQUE P., et al.
2011ApJ...743...76S viz 15       D               1 91 47 The Carnegie Hubble Program: the Leavitt law at 3.6 µm and 4.5 µm in the Large Magellanic Cloud. SCOWCROFT V., FREEDMAN W.L., MADORE B.F., et al.
2012ApJ...748..107P viz 15       D               1 291 30 A global physical model for cepheids. PEJCHA O. and KOCHANEK C.S.
2012MNRAS.421.2998F viz       D           *   2 56 20 The Cepheid distance to the Local Group galaxy NGC 6822. FEAST M.W., WHITELOCK P.A., MENZIES J.W., et al.
2012MNRAS.426.3148S 93       D     X         3 85 6 Binarity among Cepheids in the Magellanic Clouds. SZABADOS L. and NEHEZ D.
2013A&A...550A..70G viz 16       D               2 201 45 Baade-Wesselink distances to Galactic and Magellanic Cloud Cepheids and the effect of metallicity. GROENEWEGEN M.A.T.
2015MNRAS.447.3342B viz 16       D               5 2329 21 On the variation of Fourier parameters for Galactic and LMC Cepheids at optical, near-infrared and mid-infrared wavelengths. BHARDWAJ A., KANBUR S.M., SINGH H.P., et al.
2015AJ....149..117M viz 16       D               2 1486 89 Large Magellanic Cloud near-infrared synoptic survey. I. Cepheid variables and the calibration of the Leavitt Law. MACRI L.M., NGEOW C.-C., KANBUR S.M., et al.
2015A&A...576A..30I viz 16       D               1 289 30 New NIR light-curve templates for classical Cepheids. INNO L., MATSUNAGA N., ROMANIELLO M., et al.
2016MNRAS.459.1170S viz 16       D               1 219 6 The Carnegie Chicago Hubble Program: the mid-infrared colours of Cepheids and the effect of metallicity on the CO band-head at 4.6µm. SCOWCROFT V., SEIBERT M., FREEDMAN W.L., et al.
2016ApJ...832..176I viz 16       D               1 3931 41 The panchromatic view of the Magellanic Clouds from classical Cepheids. I. Distance, reddening, and geometry of the Large Magellanic Cloud disk. INNO L., BONO G., MATSUNAGA N., et al.
2017A&A...608A..18G 81         O X         2 47 13 Observational calibration of the projection factor of Cepheids. IV. Period-projection factor relation of Galactic and Magellanic Cloud Cepheids. GALLENNE A., KERVELLA P., MERAND A., et al.
2015AcA....65..297S viz 16       D               1 9695 105 The OGLE Collection of Variable Stars. Classical Cepheids in the Magellanic System. SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al.
2019A&A...622A..60C viz 17       D               1 150347 194 Gaia Data Release 2. Specific characterisation and validation of all-sky Cepheids and RR Lyrae stars. CLEMENTINI G., RIPEPI V., MOLINARO R., et al.
2019MNRAS.485..961J viz 17       D               1 814 116 The ASAS-SN catalogue of variable stars III: variables in the southern TESS continuous viewing zone. JAYASINGHE T., STANEK K.Z., KOCHANEK C.S., et al.
2020MNRAS.491.4752B viz 17       D               1 13884 ~ When a period is not a full stop: Light-curve structure reveals fundamental parameters of Cepheid and RR Lyrae stars. BELLINGER E.P., KANBUR S.M., BHARDWAJ A., et al.
2020AJ....160..120J viz 17       D               1 365761 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2021MNRAS.500..817C viz 17       D               1 5050 ~ The mid-infrared Leavitt law for classical Cepheids in the Magellanic Clouds. CHOWN A.H., SCOWCROFT V. and WUYTS S.
2021ApJ...913...38B viz 17       D               1 2043 32 The influence of metallicity on the Leavitt law from geometrical distances of Milky Way and Magellanic Cloud Cepheids. BREUVAL L., KERVELLA P., WIELGORSKI P., et al.

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