[TCB2007] 12004280 , the SIMBAD biblio

[TCB2007] 12004280 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST04:12:05


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Title First 3 Authors
2007MNRAS.382..109T viz 15       D               800 448 Strong size evolution of the most massive galaxies since z ∼ 2. TRUJILLO I., CONSELICE C.J., BUNDY K., et al.
2011ApJS..193...30B viz 15       D               1 7611 103 UV-to-FIR analysis of Spitzer/IRAC sources in the Extended Groth Strip. II. Photometric redshifts, stellar masses, and star formation rates. BARRO G., PEREZ-GONZALEZ P.G., GALLEGO J., et al.
2012ApJ...751...50G viz 15       D               1 8632 29 The DEEP2 Galaxy Redshift Survey: the Voronoi-Delaunay method catalog of galaxy groups. GERKE B.F., NEWMAN J.A., DAVIS M., et al.
2013ApJS..204...21M viz 15       D               1 34882 13 Extended photometry for the DEEP2 galaxy redshift survey: a testbed for photometric redshift experiments. MATTHEWS D.J., NEWMAN J.A., COIL A.L., et al.
2013ApJ...765..117E viz 15       D               1 440 19 X-ray groups of galaxies in the AEGIS deep and wide fields. ERFANIANFAR G., FINOGUENOV A., TANAKA M., et al.
2013ApJ...768...74T viz 19       D               2 82 774 PHIBSS: molecular gas content and scaling relations in z ∼ 1-3 massive, main-sequence star-forming galaxies. TACCONI L.J., NERI R., GENZEL R., et al.
2017A&A...602A..51V 16       D               2 77 7 Predicting HCN, HCO+, multi-transition CO, and dust emission of star-forming galaxies. From local spiral and ultraluminous infrared galaxies to high-z star-forming and submillimeter galaxies. VOLLMER B., GRATIER P., BRAINE J., et al.
2017MNRAS.467.4886C 79               F     1 23 10 PHIBSS: exploring the dependence of the CO-H2 conversion factor on total mass surface density at z<1.5. CARLETON T., COOPER M.C., BOLATTO A.D., et al.
2022A&A...667A..30V 17       D               1 72 5 Deciphering the radio-star formation correlation on kpc scales II. The integrated infrared-radio continuum and star formation-radio continuum correlations. VOLLMER B., SOIDA M. and DALLANT J.

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