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2019ApJ...887L..25B - Astrophys. J., 887, L25-L25 (2019/December-2)
Constraining the neutron star mass-radius relation and dense matter equation of state with NICER. I. The millisecond pulsar X-ray data set.
BOGDANOV S., GUILLOT S., RAY P.S., WOLFF M.T., CHAKRABARTY D., HO W.C.G., KERR M., LAMB F.K., LOMMEN A., LUDLAM R.M., MILBURN R., MONTANO S., MILLER M.C., BAUBOCK M., OZEL F., PSALTIS D., REMILLARD R.A., RILEY T.E., STEINER J.F., STROHMAYER T.E., WATTS A.L., WOOD K.S., ZELDES J., ENOTO T., OKAJIMA T., KELLOGG J.W., BAKER C., MARKWARDT C.B., ARZOUMANIAN Z. and GENDREAU K.C.
Abstract (from CDS):
Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.
Journal keyword(s): Neutron stars - Pulsars - Compact objects - Nuclear astrophysics - Millisecond pulsars - X-ray astronomy - X-ray observatories - Pulsar timing method - Spectroscopy - Astronomical techniques
Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR. // All or part of tables of objects could be ingested in SIMBAD with priority 2.
Simbad objects: 9
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