Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Apr-2024)

Result of query: info cati WISP 64$
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Details on Acronym:   WISP
  
WISP (WFC3 Infrared Spectroscopic Parallel (WISP))
Write:<<WISP JHHMM+DDMM>>
<<WISP FFF NNNN>>
<<WISP HHMM+DDMM>> (not recognised by Simbad, but found in literature)
<<WISP FFF_NNNN>>
N: 3+?
Object:(NIR)  (SIMBAD class: NearIR = Near-IR Source (λ < 3 µm))
Note:HST slitless spectra over 0.8-1.7µm for more than 700 arcmin2 of sky using the two infrared grisms installed on the IR channel of WFC3.
Only the first references using these formats are listed here.
More information is available at http://wisps.ipac.caltech.edu
Ref:=2012ApJ...752L..14M
byMASTERS D. , McCARTHY P., BURGASSER A.J., HATHI N.P., MALKAN M., ROSS N.R., SIANA B., SCARLATA C., HENRY A., COLBERT J., ATEK H., RAFELSKI M., TEPLITZ H., BUNKER A., DRESSLER A.
 Astrophys. J., 752L, 14 (2012)
  Discovery of three distant, cold brown dwarfs in the WFC3 infrared spectroscopic parallels survey.
oTable 1: <WISP JHHMM+DDMM> N=3.
Ref:=2011ApJ...743..121A
byATEK H. , SIANA B., SCARLATA C., MALKAN M., McCARTHY P., TEPLITZ H., HENRY A., COLBERT J., BRIDGE C., BUNKER A.J., DRESSLER A., FOSBURY R.A.E., HATHI N.P., MARTIN C., ROSS N.R., SHIM H.
 Astrophys. J., 743, 121 (2011)
  Very strong emission-line galaxies in the WFC3 infrared spectroscopic parallel survey and implications for high-redshift galaxies.
oTable 2: <WISP FFF NNN> N=9.
Originof the Acronym: S = Created by Simbad, the CDS Database