SV* HV 938 , the SIMBAD biblio

SV* HV 938 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST12:57:01


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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.
1983AJ.....88..507H 38 35 Photometry of Cepheids in the LMC and Magellanic Cloud abundances HARRIS H.C.
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.
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.
2009AJ....137.3139V viz 15       D               1 1973 42 Variable evolved stars and young stellar objects discovered in the large Magellanic cloud using the SAGE survey. VIJH U.P., MEIXNER M., BABLER B., 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.
2011AcA....61..303K 92       D         F     2 69 3 Large Magellanic Cloud Cepheids in the ASAS Data. KARCZMAREK P., DZIEMBOWSKI W.A., LENZ P., et al.
2015MNRAS.447.3342B viz 16       D               3 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.
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.
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.
2013AcA....63..159U viz 16       D               1 769 16 Variable stars from the OGLE-III Shallow Survey in the Large Magellanic Cloud. ULACZYK K., SZYMANSKI M.K., UDALSKI 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.
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.
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...32D viz 17       D               1 5182 ~ Photometric classifications of evolved massive stars: preparing for the era of webb and roman with machine learning. DORN-WALLENSTEIN T.Z., DAVENPORT J.R.A., HUPPENKOTHEN D., et al.
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.
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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