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[MBR2003] CDFS-H 2707 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST19:27:47 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
---|---|---|---|---|---|---|---|---|---|
2003A&A...403..493M | 4820 | 24 | H-band observations of the Chandra Deep Field South. | MOY E., BARMBY P., RIGOPOULOU D., et al. | |||||
2009PASJ...61..177B | 15 | D | 1 | 258 | 10 | Deep 15 mu.m AKARI observations in the CDFS: Estimating dust luminosities for a MIR-selected sample and for Lyman Break Galaxies and the evolution of Ldust/LUV with the redshift. | BURGARELLA D., BUAT V., TAKEUCHI T.T., et al. | ||
2012MNRAS.425.2116C | 15 | D | 4 | 7382 | 55 | The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS spectroscopic survey of the Chandra Deep Field-South. | COOPER M.C., YAN R., DICKINSON M., et al. | ||
2012ApJS..203...15B | 15 | D | 1 | 894 | 38 | The sub-mJy radio population of the E-CDFS: optical and infrared counterpart identification. | BONZINI M., MAINIERI V., PADOVANI P., et al. | ||
2012ApJ...761..140C | 15 | D | 1 | 725 | 145 | A redshift survey of Herschel far-infrared selected starbursts and implications for obscured star formation. | CASEY C.M., BERTA S., BETHERMIN M., et al. | ||
2013ApJS..205...13M | 16 | D | 1 | 894 | 109 | The Very Large Array 1.4 GHz survey of the Extended Chandra Deep Field South: second data release. | MILLER N.A., BONZINI M., FOMALONT E.B., et al. | ||
2013MNRAS.436.3759B | 16 | D | 1 | 885 | 125 | The sub-mJy radio sky in the Extended Chandra Deep Field-South: source population. | BONZINI M., PADOVANI P., MAINIERI V., et al. | ||
2015MNRAS.453.1079B | 16 | D | 1 | 781 | 30 | Star formation properties of sub-mJy radio sources. | BONZINI M., MAINIERI V., PADOVANI P., et al. | ||
2017ApJ...840...78D | 16 | D | 1 | 925 | 95 | An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South: spectroscopic redshifts. | DANIELSON A.L.R., SWINBANK A.M., SMAIL I., et al. |