SV* HV 2463 , the SIMBAD biblio

SV* HV 2463 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST10:17:55

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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
1982ApJ...260..695B 193 10 The occurrence of carbon stars and Cepheid variables in common fields of the Magellanic Clouds. BECKE S.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.
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.
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.
2015MNRAS.447.3342B viz 16       D               7 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               1 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.
2016AJ....151...88B viz 16       D               1 1353 18 Large Magellanic Cloud near-infrared Synoptic Survey. II. The Wesenheit relations and their application to the distance scale. BHARDWAJ A., KANBUR S.M., MACRI L.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.
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.
2019ApJ...876...85R viz 37       D               1 75 1556 Large Magellanic Cloud Cepheid standards provide a 1% foundation for the determination of the Hubble constant and stronger evidence for physics beyond ΛCDM. RIESS A.G., CASERTANO S., YUAN W., 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.
2022A&A...658A..29R viz 18       D               1 72 23 The iron and oxygen content of LMC Classical Cepheids and its implications for the extragalactic distance scale and Hubble constant. Equivalent width analysis with Kurucz stellar atmosphere models. ROMANIELLO M., RIESS A., MANCINO S., et al.

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