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

Result of query: info cati ADW2016] MM$
.

Details on Acronym:   [ADW2016]
  
[ADW2016] (Aravena+Decarli+Walter+, 2016)= ([ADW2016a]) = (ASPECS)
Write:<<[ADW2016] CNN>>
<<[ADW2016] MM JHHMMSS.ss+DDMMSS.s>>
N: 16*2
Object:(mm)  (SIMBAD class: mmRad = Millimetric Radio Source)
Stat:is completely incorporated in Simbad
Note:ALMA 1.2mm continuum observations of N=16 sources, as part of the ALMA SPECtroscopic Survey in the Hubble Ultra-Deep Field (ASPECS).
See also [WDA2016] and [DWA2016].
in source:NAME Hubble Ultra Deep Field
Ref:=2016ApJ...833...68A
byARAVENA M. , DECARLI R., WALTER F., DA CUNHA E., BAUER F.E., CARILLI C.L., DADDI E., ELBAZ D., IVISON R.J., RIECHERS D.A., SMAIL I., SWINBANK A.M., WEISS A., ANGUITA T., ASSEF R.J., BELL E., BERTOLDI F., BACON R., BOUWENS R., CORTES P., COX P., GONZALEZ-LOPEZ J., HODGE J., IBAR E., INAMI H., INFANTE L., KARIM A., LE FEVRE O., MAGNELLI B., OTA K., POPPING G., SHETH K., VAN DER WERF P., WAGG J.
 Astrophys. J., 833, 68-68 (2016)
  The ALMA spectroscopic survey in the Hubble Ultra Deep Field: continuum number counts, resolved 1.2 mm extragalactic background, and properties of the faintest dusty star-forming galaxies.
oTable 1: <[ADW2016] CNN> = <[ADW2016] MM JHHMMSS.ss+DDMMSS.s> N=16.
Originof the Acronym: S = Created by Simbad, the CDS Database

Details on Acronym:   [ADW2016a]
  
[ADW2016a] (Aravena+Decarli+Walter+, 2016)
***** Avoid the usage of [ADW2016a], prefer [ADW2016]
Originof the Acronym: S = Created by Simbad, the CDS Database

Details on Acronym:   ASPECS
  
ASPECS (ALMA SPECtroscopic Survey)
***** Avoid the usage of ASPECS, prefer [ADW2016]
Originof the Acronym: A = Assigned by the author(s)