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| NAME Pavo Field , the SIMBAD biblio (18 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST09:52:40 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1989BAAS...21.1168G | 1 | 0 | Correlated deep X-ray and optical imaging in Pavo. | GRIFFITHS R.E. and EWALD S.P. | |||||
| 1990MNRAS.247....1R | 8 | 6 | 201 | A sparse-sampled redshift survey of IRAS galaxies. I. The convergence of the IRAS dipole and the origin of our motion with respect to the microwave background. | ROWAN-ROBINSON M., LAWRENCE A., SAUNDERS W., et al. | ||||
| 1990PASAu...8..348B | 2 | 1 | Radio observations of the Einstein deep X-ray field in Pavo. | BEDDING T.R. and TURTLE A.J. | |||||
|
1991ApJ...374..440P |
31 | 37 | The CfA Eisntein observatory extended deep X-ray survey. | PRIMINI F.A., MURRAY S.S., HUCHRA J., et al. | |||||
| 1991ApJ...379..576H | 36 | 25 | Faint X-ray source counts and the origin of the X-ray background. | HAMILTON T.T., HELFAND D.J. and WU X. | |||||
| 1991MNRAS.250..780B | 10 | 18 | A model of the Galaxy in the ultraviolet. | BROSCH N. | |||||
| 1991IBVS.3681....1L | 132 | 3 | Improved positions of variable stars in northern Pavo. | LOPEZ C.E. and GIRARD T.M. | |||||
| 1993A&A...269L...9G | 7 | 4 | The motion of the Local group with respect to the microwave background frame : local anomaly and effect of clusters at distances >40h-1 Mpc. | GOICOECHEA L.J. | |||||
| 1993A&A...278..161C | 36 | 24 | The observability of old isolated neutron stars with ROSAT. II. Molecular clouds and deep fields. | COLPI M., CAMPANA S. and TREVES A. | |||||
| 1994AJ....107..582C | 1 | 9 | 67 | Powerful model for the point source sky: far-ultraviolet and enhanced midinfrared performance. | COHEN M. | ||||
| 1994ApJ...434L..39M | 1 | 6 | 25 | Large-scale streaming motions in the Local Universe. | MATHEWSON D.S. and FORD V.L. | ||||
|
1997A&A...319...18R |
484 | 51 | X-ray sources <1 degree from Seyfert galaxies. | RADECKE H.-D. | |||||
| 1997A&A...323...47D | 25 | 2 | The final optical identification content of the Einstein deep X-ray field in Pavo. | DANZIGER I.J. and GILMOZZI R. | |||||
| 1997MNRAS.292L..59W | 14 | 35 | The rms peculiar velocity of clusters. | WATKINS R. | |||||
|
2003SerAJ.166...13F |
73 | T | 3 | 0 |
A multi-frequency study of the deep Pavo field. |
FILIPOVIC M.D., ANDERSON M., EKERS R.D., et al. | |||
| 2009PZP.....9...22S | O | 5 | 0 | A new RR Lyrae variable near NGC 6744 in Pavo. | SAUER T. | ||||
| 2015A&A...576A.104P | 177 | D | X C | 4 | 28 | 332 | Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust. | PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al. | |
| 2015A&A...576A.105P | 488 | D | X C | 12 | 13 | 124 | Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence. | PLANCK COLLABORATION, ADE P.A.R., AGHANIM N., et al. |