Atels
E.g., 2025-03-18
to
E.g., 2025-03-18
Degrees (0..360, with decimal point) or sexagesimal: HH:MM:SS.SS / HH MM SS.SS
Degrees (-90..+90, with decimal point) or sexagesimal: ±DD:MM:SS.SS / ±DD MM SS.SS
Degrees (0..360, with decimal point) or sexagesimal: HH:MM:SS.SS / HH MM SS.SS
to
Degrees (0..360, with decimal point) or sexagesimal: HH:MM:SS.SS / HH MM SS.SS
Degrees (0..360, with decimal point) or sexagesimal: HH:MM:SS.SS / HH MM SS.SS
to
Degrees (-90..+90, with decimal point) or sexagesimal: ±DD:MM:SS.SS / ±DD MM SS.SS
Showing results 1 to 4 out of 4
Atel IDsort descendingAtel Date (UT)Coords X-RefsRADECTitleKeywordsAuthors
105522017-07-02 04:05:0018:31:45.918-14:18:55.57The likely progenitor of Nova ASASSN-17hx (=ASASSN-17ib) detected by the VVVX SurveyInfra-Red, Cataclysmic Variable, NovaR. K. Saito (Universidade Federal de Santa Catarina), M. Hempel (Pontificia Universidad Catolica de Chile, Millennium Institute of Astrophysics), D. Minniti (Universidad Andres Bello, Millennium Institute of Astrophysics, Vatican Observatory)
105522017-07-02 04:05:0018:31:45.860-14:18:55.40The likely progenitor of Nova ASASSN-17hx (=ASASSN-17ib) detected by the VVVX SurveyInfra-Red, Cataclysmic Variable, NovaR. K. Saito (Universidade Federal de Santa Catarina), M. Hempel (Pontificia Universidad Catolica de Chile, Millennium Institute of Astrophysics), D. Minniti (Universidad Andres Bello, Millennium Institute of Astrophysics, Vatican Observatory)
105272017-06-24 12:07:0018:31:45.918-14:18:55.57Spectral confirmation of galactic nova ASASSN-17hx (=ASASSN-17ib)Optical, Cataclysmic Variable, NovaA. Kurtenkov (Institute of Astronomy and NAO, Bulgaria), T. Tomov (Nicolaus Copernicus University, Torun, Poland), P. Pessev (GTC, IAC, ULL, Spain)
105232017-06-23 16:20:0018:31:45.918-14:18:55.57ASAS-SN Discovery of a Possible Galactic Nova ASASSN-17ib on the RiseOptical, NovaK. Z. Stanek, C. S. Kochanek (OSU), L. Chomiuk, J. Strader (MSU), J. S. Brown, T. W.-S. Holoien, J. V. Shields, T. A. Thompson (OSU), B. J. Shappee (Hubble Fellow, Carnegie Observatories), J. L. Prieto (Diego Portales; MAS), Subo Dong (KIAA-PKU)