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| NAME Marano1 Field , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST03:49:49 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1988MNRAS.232..111M | 149 | 58 | A new sample of quasars to B=22.0. | MARANO B., ZAMORANI G. and ZITELLI V. | |||||
| 1997MNRAS.286..470G | 71 | T | 90 | 39 | Radio observations of the Marano Field and the faint radio galaxy population. | GRUPPIONI C., ZAMORANI G., DE RUITER H.R., et al. | |||
| 1999A&A...345...29P | 1 | 38 | 161 | FIRBACK. I. A deep survey at 175µm with ISO, preliminary results. | PUGET J.L., LAGACHE G., CLEMENTS D.L., et al. | ||||
| 1999A&A...346..731Z | 73 | T | 8 | 46 | The ROSAT Deep Survey. V. X-ray sources and optical identifications in the Marano field. | ZAMORANI G., MIGNOLI M., HASINGER G., et al. | |||
| 2000A&A...355...17L | 25 | 1 | 77 | Detection of the extra-Galactic background fluctuations at 170µm. | LAGACHE G. and PUGET J.L. | ||||
|
2007A&A...466...41K |
414 | 12 | The XMM-Newton survey in the Marano field. I. The X-ray data and optical follow-up. | KRUMPE M., LAMER G., SCHWOPE A.D., et al. | |||||
| 2007A&A...474..731G | 5 | 1 | 16 | Power spectrum analysis of far-IR background fluctuations in 160 µm maps from the multiband imaging photometer for Spitzer. | GROSSAN B. and SMOOT G.F. | ||||
| 2007A&A...475..801R | 74 | C | 1 | 7 | 13 | The 12 µm ISO-ESO-Sculptor and 24 µm Spitzer faint counts reveal a population of ULIRGs as dusty massive ellipticals. Evolution by types and cosmic star formation. | ROCCA-VOLMERANGE B., DE LAPPARENT V., SEYMOUR N., et al. | ||
| 2007A&A...475..901K | 521 | A | D | S X C | 13 | 9 | 60 | OVII and OVIII line emission in the diffuse soft X-ray background: heliospheric and galactic contributions. | KOUTROUMPA D., ACERO F., LALLEMENT R., et al. |
|
2007A&A...476.1191B |
37 | X | 1 | 343 | 35 | The XMM-Newton serendipitous survey. IV. Optical identification of the XMM-Newton medium sensitivity survey (XMS). | BARCONS X., CARRERA F.J., CEBALLOS M.T., et al. | ||
| 2008A&A...478..575K | 49 | X | 1 | 8 | 193 | The EPIC-MOS particle-induced background spectra. | KUNTZ K.D. and SNOWDEN S.L. | ||
| 2008A&A...483..415K | 37 | X | 1 | 11 | 17 | X-ray absorption in distant type II QSOs. | KRUMPE M., LAMER G., CORRAL A., et al. | ||
| 2008ApJS..177...14S | 47 | X | 1 | 7 | 140 | A new method to separate star-forming from AGN galaxies at intermediate redshift: the submillijansky radio population in the VLA-COSMOS survey. | SMOLCIC V., SCHINNERER E., SCODEGGIO M., et al. | ||
|
2008A&A...487..539W |
37 | X | 1 | 198 | 4 | A slitless spectroscopic survey for quasars near quasars. | WORSECK G., WISOTZKI L. and SELMAN F. | ||
| 2010A&A...514A...8P | 15 | D | 3 | 14 | 14 | Source counts at 15 microns from the AKARI NEP survey. | PEARSON C.P., OYABU S., WADA T., et al. | ||
| 2012ApJ...745..171S | 39 | X | 1 | 12 | 26 | Far-IR/Submillimeter spectroscopic cosmological surveys: predictions of infrared line luminosity functions for z < 4 galaxies. | SPINOGLIO L., DASYRA K.M., FRANCESCHINI A., et al. | ||
|
2015MNRAS.453.4020F |
157 | C F | 2 | 13 | 30 | ATLAS - I. Third release of 1.4 GHz mosaics and component catalogues. | FRANZEN T.M.O., BANFIELD J.K., HALES C.A., et al. | ||
|
2017A&A...602A...2S |
52 | X | 1 | 5 | 120 | The VLA-COSMOS 3 GHz Large Project: Multiwavelength counterparts and the composition of the faint radio population. | SMOLCIC V., DELVECCHIO I., ZAMORANI G., et al. | ||
|
2020A&A...635A...5D |
41 | X | 1 | 263 | 58 | Giant radio galaxies in the LOFAR Two-metre Sky Survey. I. Radio and environmental properties. | DABHADE P., ROTTGERING H.J.A., BAGCHI J., et al. | ||
|
2022ApJS..259...31S |
43 | X | 1 | 7 | 6 | A New Catalog of Head-Tail Radio Galaxies from the VLA FIRST Survey. | SASMAL T.K., BERA S., PAL S., et al. | ||
| 2024A&A...681A..78L | 45 | X | 1 | 11 | ~ | The warm-hot circumgalactic medium of the Milky Way as seen by eROSITA. | LOCATELLI N., PONTI G., ZHENG X., et al. |