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 |
by | ARAVENA 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. | |
o | Table 1: <[ADW2016] CNN> = <[ADW2016] MM JHHMMSS.ss+DDMMSS.s> N=16. |
Origin | of 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] |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: ASPECS | |
ASPECS | (ALMA SPECtroscopic Survey) |
***** | Avoid the usage of ASPECS, prefer [ADW2016] |
Origin | of the Acronym: A = Assigned by the author(s) |