Dictionary of Nomenclature of Celestial Objects
(Last update: 18-Dec-2020)

Result of query: info cati WTS HHa-N-NNNNN$



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Details on Acronym:   WTS
   WTS (WFCAM Transit Survey) Write:<<WTS -N>>
<<WTS -Na>>
<<WTS HHa-N-NNNNN>>
<<WTS HHa_N_NNNN>> (not recognised by Simbad, but found in literature) N: 1+1+31+16+68 Object:* + Poss. Pl +V*  (SIMBAD class: Unknown = Object of unknown nature) Note:The WFCAM Transit Survey (WTS) is a photometric monitoring campaign using the UKIRT Wide Field Camera (WFCAM), cf. http://www.ast.cam.ac.uk/~sth/wts/
Formats -N and -Nb: for stars hosting exoplanets (only the first reference 2012MNRAS.427.1877C is given here).
Format HHa-N-NNNNN: for M dwarfs. In this format, HH stands for the four survey fields (03hr, 07hr, 17hr, 19hr). A field is observed through eight pointings, each labelled with a single letter (from "a" to "h"). The single digit N refers to one of the four detectors (paw print) of WFCAM. Rem:(a dash between the acronym and its contents is found in the literature) Ref:=2012MNRAS.425..950N byNEFS S.V. , BIRKBY J.L., SNELLEN I.A.G., HODGKIN S.T., PINFIELD D.J., SIPOCZ B., KOVACS G., MISLIS D., SAGLIA R.P., KOPPENHOEFER J., CRUZ P., BARRADO D., MARTIN E.L., GOULDING N., STOEV H., ZENDEJAS J., DEL BURGO C., CAPPETTA M., PAVLENKO Y.V. Mon. Not. R. Astron. Soc., 425, 950-968 (2012) Four ultra-short-period eclipsing M-dwarf binaries in the WFCAM Transit Survey. oTables 2+A1: <WTS HHa-N-NNNNN> N=31. Ref:=2012MNRAS.427.1877C byCAPPETTA M. , SAGLIA R.P., BIRKBY J.L., KOPPENHOEFER J., PINFIELD D.J., HODGKIN S.T., CRUZ P., KOVACS G., SIPOCZ B., BARRADO D., NEFS B., PAVLENKO Y.V., FOSSATI L., DEL BURGO C., MARTIN E.L., SNELLEN I., BARNES J., BAYO A., CAMPBELL D.A., CATALAN S., GALVEZ-ORTIZ M.C., GOULDING N., HASWELL C., IVANYUK O., JONES H.R., KUZNETSOV M., LODIEU N., MAROCCO F., MISLIS D., MURGAS F., NAPIWOTZKI R., PALLE E., POLLACCO D., SARRO BARO L., SOLANO E., STEELE P., STOEV H., TATA R., ZENDEJAS J. Mon. Not. R. Astron. Soc., 427, 1877-1890 (2012) The first planet detected in the WTS: an inflated hot Jupiter in a 3.35d orbit around a late F star. o(Erratum) errata vol. 444, p. 3150 (2014), vol. 497, p. 916 (2020) o<WTS-N> (No. 1), <WTS-Na> (No. 1b). Ref:=2012MNRAS.426.1507B byBIRKBY J. , NEFS B., HODGKIN S., KOVACS G., SIPOCZ B., PINFIELD D., SNELLEN I., MISLIS D., MURGAS F., LODIEU N., DE MOOIJ E., GOULDING N., CRUZ P., STOEV H., CAPPETTA M., PALLE E., BARRADO D., SAGLIA R., MARTIN E., PAVLENKO Y. Mon. Not. R. Astron. Soc., 426, 1507-1532 (2012) Discovery and characterization of detached M dwarf eclipsing binaries in the WFCAM Transit Survey. oTable A3: SDSS 0123 is SDSS J121258.25-012310.1. oTables 1-2+A2: <WTS HHa-N-NNNNN> N=3+13. Ref:=2012MNRAS.427.3358G byGOULDING N.T. , BARNES J.R., PINFIELD D.J., KOVACS G., BIRKBY J., HODGKIN S., CATALAN S., SIPOCZ B., JONES H.R.A., DEL BURGO C., JEFFERS S.V., NEFS S., GALVEZ-ORTIZ M.C., MARTIN E.L. Mon. Not. R. Astron. Soc., 427, 3358-3373 (2012) J-band variability of M dwarfs in the WFCAM Transit Survey. oTable A1: <WTS HHa-N-NNNNN> N=68 added. =E=Catalogue in electronic form as <J/MNRAS/426/1507/> Originof the Acronym: A = Assigned by the author(s)

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