Dictionary of Nomenclature of Celestial Objects
(Last update: 10-Apr-2024)

Result of query: info cati ASPECS$

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

Details on Acronym:   ASPECS
  
ASPECS (ALMA SPECtroscopic Survey)
Write:<<ASPECS LP.3mm.NN>>
<<ASPECS LP.3mm.CNN>>
<<ASPECS LP-MP.3mm.NN>>
<<ASPECS LP.1mm.CNNa>>
<<ASPECS LP.1mm.Faint.CNN>>
<<ASPECS -LP.3mm.NN>> (not recognised by Simbad, but found in literature)
<<ASPECS -LP-3mm.CNN>>
<<ASPECS -LP-MP.3mm.NN>>
N: 16+6+2+36+26
Object:(mm)  (SIMBAD class: mmRad = Millimetric Radio Source)
Note:ALMA band 3 (3mm) and band 6 (1.2mm) observations of
N=16 CO-emitting galaxies (format LP.3mm.NN), N=6 continuum source candidates (format LP.3mm.CNN), and N=2 "MUSE prior" sources (format LP-MP.3mm.NN), and N=36+26 continuum sources candidates (formats LP.1mm.CNNa and LP.1mm.Faint.CNN),
as part of the ALMA Spectroscopic Survey Large Program (ASPECS-LP), targeting the Hubble Ultra Deep Field (HUDF).
See also [WDA2016] and [ADW2016] for the ASPECS pilot program.
Rem:(a dash between the acronym and its contents is found in the literature)
in source:NAME Hubble Ultra Deep Field
Ref:=2019ApJ...882..136A
byARAVENA M. , DECARLI R., GONZALEZ-LOPEZ J., BOOGAARD L., WALTER F., CARILLI C., POPPING G., WEISS A., ASSEF R.J., BACON R., BAUER F.E., BERTOLDI F., BOUWENS R., CONTINI T., CORTES P.C., COX P., DA CUNHA E., DADDI E., DIAZ-SANTOS T., ELBAZ D., HODGE J., INAMI H., IVISON R., LE FEVRE O., MAGNELLI B., OESCH P., RIECHERS D., SMAIL I., SOMERVILLE R.S., SWINBANK A.M., UZGIL B., VAN DER WERF P., WAGG J., WISOTZKI L.
 Astrophys. J., 882, 136-136 (2019)
  The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: evolution of the molecular gas in CO-selected galaxies.
oFig. 14, Tables 1-3: <ASPECS LP.3mm.NN> (Nos 1-16).
Ref:=2019ApJ...882..139G
byGONZALEZ-LOPEZ J. , DECARLI R., PAVESI R., WALTER F., ARAVENA M., CARILLI C., BOOGAARD L., POPPING G., WEISS A., ASSEF R.J., BAUER F.E., BERTOLDI F., BOUWENS R., CONTINI T., CORTES P.C., COX P., DA CUNHA E., DADDI E., DIAZ-SANTOS T., INAMI H., HODGE J., IVISON R., LE FEVRE O., MAGNELLI B., OESCH P., RIECHERS D., RIX H.-W., SMAIL I., SWINBANK A.M., SOMERVILLE R.S., UZGIL B., VAN DER WERF P.
 Astrophys. J., 882, 139-139 (2019)
  The Atacama Large Millimeter/submillimeter Array SPECtroscopic Survey in the Hubble Ultra Deep Field: CO emission lines and 3 mm continuum sources.
oTable 7: <ASPECS -LP.3mm.CNN> (Nos C01-C06).
Ref:=2019ApJ...882..140B
byBOOGAARD L.A. , DECARLI R., GONZALEZ-LOPEZ J., VAN DER WERF P., WALTER F., BOUWENS R., ARAVENA M., CARILLI C., BAUER F.E., BRINCHMANN J., CONTINI T., COX P., DA CUNHA E., DADDI E., DIAZ-SANTOS T., HODGE J., INAMI H., IVISON R., MASEDA M., MATTHEE J., OESCH P., POPPING G., RIECHERS D., SCHAYE J., SCHOUWS S., SMAIL I., WEISS A., WISOTZKI L., BACON R., CORTES P.C., RIX H.-W., SOMERVILLE R.S., SWINBANK M., WAGG J.
 Astrophys. J., 882, 140-140 (2019)
  The ALMA spectroscopic survey in the HUDF: nature and physical properties of gas-mass selected galaxies using MUSE spectroscopy.
oFig. 4, Table 2: <ASPECS LP-MP.3mm.NN> (Nos 01-02).
Ref:=2020ApJ...897...91G
byGONZALEZ-LOPEZ J. , NOVAK M., DECARLI R., WALTER F., ARAVENA M., CARILLI C., BOOGAARD L., POPPING G., WEISS A., ASSEF R.J., BAUER F.E., BOUWENS R., CORTES P.C., COX P., DADDI E., DA CUNHA E., DIAZ-SANTOS T., IVISON R., MAGNELLI B., RIECHERS D., SMAIL I., VAN DER WERF P., WAGG J.
 Astrophys. J., 897, 91-91 (2020)
  The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts.
oFig. 2, Table 1: <ASPECS LP.1mm.CNNa> (Nos C01-C13, C14a-C14b, C15-C34). Table 5: <ASPECS LP.1mm.Faint.CNN> (Nos C01-C26).
Originof the Acronym: A = Assigned by the author(s)

Details on Acronym:   ASPECS
  
ASPECS (ALMA SPECtroscopic Survey)
***** Avoid the usage of ASPECS, prefer [WDA2016]
Originof the Acronym: A = Assigned by the author(s)