ASPECS LP.3mm.12 , the SIMBAD biblio

ASPECS LP.3mm.12 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:09:55


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Title First 3 Authors
2019ApJ...882..136A 19       D               1 19 63 The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: evolution of the molecular gas in CO-selected galaxies. ARAVENA M., DECARLI R., GONZALEZ-LOPEZ J., et al.
2019ApJ...887...37U 16       D               1 17 ~ The ALMA Spectroscopic Survey in the HUDF: constraining cumulative CO emission at 1 <= z <= 4 with power spectrum analysis of ASPECS LP data from 84 to 115 GHz. UZGIL B.D., CARILLI C., LIDZ A., et al.
2020ApJ...896L..21R 18       D               2 16 47 VLA-ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (VLASPECS): total cold gas masses and CO line ratios for z = 2-3 main-sequence galaxies. RIECHERS D.A., BOOGAARD L.A., DECARLI R., et al.
2020ApJ...897...91G 17       D               1 40 53 The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm continuum number counts. GONZALEZ-LOPEZ J., NOVAK M., DECARLI R., et al.
2020ApJ...901...79A 17       D               1 38 44 The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: the nature of the faintest dusty star-forming galaxies. ARAVENA M., BOOGAARD L., GONZALEZ-LOPEZ J., et al.
2020ApJ...902..109B 389       D     X         10 26 59 The ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: CO excitation and atomic carbon in star-forming galaxies at z < 1-3. BOOGAARD L.A., VAN DER WERF P., WEISS A., et al.
2020ApJ...902..112B 20       D               1 22 90 The ALMA Spectroscopic Survey large program: the infrared excess of z = 1.5-10 UV-selected galaxies and the implied high-redshift star formation history. BOUWENS R., GONZALEZ-LOPEZ J., ARAVENA M., et al.
2023ApJ...942...24S 17       D               1 53 9 CO Emission, Molecular Gas, and Metallicity in Main-sequence Star-forming Galaxies at z ∼ 2.3. SANDERS R.L., SHAPLEY A.E., JONES T., et al.
2024ApJ...969...27B 18       D               2 37 ~ MIDIS: JWST/MIRI Reveals the Stellar Structure of ALMA-selected Galaxies in the Hubble Ultra Deep Field at Cosmic Noon. BOOGAARD L.A., GILLMAN S., MELINDER J., et al.

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