DENIS J231105.0-013705 , the SIMBAD biblio

DENIS J231105.0-013705 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.05.28CEST11:20:20


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Title First 3 Authors
2017MNRAS.472.4173R viz 16       D               2244 5 Multiband photometry and spectroscopy of an all-sky sample of bright white dwarfs. RADDI R., GENTILE FUSILLO N.P., PALA A.F., et al.
2019A&A...621A..38G viz 17       D               1 39805 ~ The population of hot subdwarf stars studied with Gaia. II. The Gaia DR2 catalogue of hot subluminous stars. GEIER S., RADDI R., GENTILE FUSILLO N.P., et al.
2019MNRAS.482.4570G viz 17       D               1 486647 ~ A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS. GENTILE FUSILLO N.P., TREMBLAY P.-E., GANSICKE B.T., et al.
2020MNRAS.499.3738O 1959 T K A D     X C F     43 19 ~
PHL 417: a zirconium-rich pulsating hot subdwarf (V366 Aquarid) discovered in K2 data.
OSTENSEN R.H., JEFFERY C.S., SAIO H., et al.
2021A&A...650A.205V viz 18       D               2 272 ~ A search for transiting planets around hot subdwarfs. I. Methods and performance tests on light curves from Kepler, K2, TESS, and CHEOPS. VAN GROOTEL V., POZUELOS F.J., THUILLIER A., et al.
2021MNRAS.506.5398D 45           X         1 3 ~ Electron-impact excitation of Ge III and photoionization of Ge II. DUNLEAVY N.L., BALLANCE C.P., RAMSBOTTOM C.A., et al.
2021A&A...653A.120D 45           X         1 29 ~ EC 22536-5304: a lead-rich and metal-poor long-period binary. DORSCH M., JEFFERY C.S., IRRGANG A., et al.
2022MNRAS.511L..60M 47           X         1 6 ~ An evolutionary channel for CO-rich and pulsating He-rich subdwarfs. MILLER BERTOLAMI M.M., BATTICH T., CORSICO A.H., et al.
2022A&A...663A..45K viz 19       D               1 147 ~ Discovery of new TESS pulsating hot subdwarfs. KRZESINSKI J. and BALONA L.A.
2023A&A...669A..48B viz 50           X         1 51 ~ Short-period pulsating hot-subdwarf stars observed by TESS I. Southern ecliptic hemisphere. BARAN A.S., VAN GROOTEL V., OSTENSEN R.H., et al.

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2023.05.28-11:20:20

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