HD 177128 , the SIMBAD biblio

HD 177128 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:48:47

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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
1993yCat.3135....0C viz 14       D               1 252979 52 VizieR Online Data Catalog: Henry Draper Catalogue and Extension, published in Ann. Harvard Obs. 91-100 (1918-1925) CANNON A.J. and PICKERING E.C.
2016ApJS..225...19E viz 16       D               1 6649 9 A catalog of 1.5273 um diffuse interstellar bands based on APOGEE hot telluric calibrators. ELYAJOURI M., MONREAL-IBERO A., REMY Q., et al.
2016A&A...594A..39F viz 16       D               2 51408 86 Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al.
2014ASPC..485..223B viz 15       D               1 465820 45 The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements BOURGES L., LAFRASSE S., MELLA G., et al.
2017MNRAS.467.1830B viz 16       D               1 642 26 Starspots on A stars. BALONA L.A.
2018A&A...619A..98H 337       D     X C       8 70 27 The Kepler view of magnetic chemically peculiar stars. HUMMERICH S., MIKULASEK Z., PAUNZEN E., et al.
2018A&A...620A.172Z viz 16       D               1 127610 99 3D mapping of young stars in the solar neighbourhood with Gaia DR2. ZARI E., HASHEMI H., BROWN A.G.A., et al.
2019ApJ...873L...5C viz 16       D               1 160 16 Discovery of resolved magnetically split lines in SDSS/APOGEE spectra of 157 Ap/Bp stars. CHOJNOWSKI S.D., HUBRIG S., HASSELQUIST S., et al.
2019A&A...628A..81S viz 16       D               1 245 ~ Strongly magnetic Ap stars in the Gaia DR2 Hertzsprung-Russell diagram. I. Selecting the most reliable astrometric and photometric data. SCHOLZ R.-D., CHOJNOWSKI S.D. and HUBRIG S.
2019MNRAS.490.2112B viz 16       D               1 2864 ~ Evidence for spots on hot stars suggests major revision of stellar physics. BALONA L.A.
2019MNRAS.490.3158C viz 16       D               1 465839 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al.
2020AJ....160..120J viz 16       D               1 365763 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.
2020A&A...640A..40H viz 16       D               1 1016 21 A plethora of new, magnetic chemically peculiar stars from LAMOST DR4. HUMMERICH S., PAUNZEN E. and BERNHARD K.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022ApJS..259...63S viz 17       D               1 10269 2 Objective Separation between CP1 and CP2 Based on Feature Extraction with Machine Learning. SHANG L.-H., LUO A.-L., WANG L., et al.
2022A&A...664A..78F viz 17       D               1 7452 7 Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., et al.
2023ApJS..264...17Z viz 17       D               6 31380 1 Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. ZHANG L.-Y., SU T., MISRA P., et al.
2023A&A...676A..55L viz 17       D               1 790 ~ Photometric variability of the LAMOST sample of magnetic chemically peculiar stars as seen by TESS. LABADIE-BARTZ J., HUMMERICH S., BERNHARD K., et al.
2024A&A...689A.208T 18       D               2 40 ~ Magnetism in LAMOST CP stars observed by TESS. THOMSON-PARESSANT K., NEINER C. and LABADIE-BARTZ J.

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