RRF 2267 , the SIMBAD biblio

RRF 2267 , the SIMBAD biblio (26 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST08:48:11

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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
1959MmRAS..68...37E viz 475 264 A survey of radio sources at a frequency of 159 Mc/s. EDGE D.O., SHAKESHAFT J.R., McADAM W.B., et al.
1966ApJS...13...65P viz 736 224 Positions and flux densities of radio sources. PAULINY-TOTH I.I.K., WADE C.M. and HEESCHEN D.S.
1968AJ.....73..298K 640 89 Measurements of the flux density of discrete radio sources at centimeter wawelengths. I. Observations at 2695 MHz. (11.3cm). KELLERMANN K.I., PAULINY-TOTH I.I.K. and TYLER W.C.
1968MNRAS.139..289W 373 34 The radio spectra of sources in the fourth Cambridge catalogue -III. WILLIAMS P.J.S., COLLINS R.A., CASWELL J.L., et al.
1968MNRAS.141...57H 5 23 Some extended radio sources in Monoceros. HOLDEN D.J.
1968AuJPh..21..369K 88 82 A catalogue of galactic radio sources. KESTEVEN M.J.L.
1971MNRAS.151..385H 10 40 Observations of some extended galactic radio sources. HASLAM C.G.T. and SALTER C.J.
1972AuJPA..25....1D 384 74 A low-latitude galactic survey from lII = 46 to 61 and 190 to 290 at 2700 MHz. DAY G.A., CASWELL J.L. and COOKE D.J.
1973AJ.....78....1D 628 61 First results from the Texas interferometer: positions of 605 discrete sources. DOUGLAS J.N., BASH F.N., GHIGO F.D., et al.
1975AJ.....80..335S 1095 38 Positions and flux densities of 1075 radio sources at 365 MHz. SHARP J.R. and BASH F.N.
1979Ap&SS..64...73B viz 433 31 Decametric survey of discrete sources in the northern sky. V. Source catalogue in the range of declinations 0 to +10. BRAUDE S.Y., MEGN A.V., SOKOLOV K.P., et al.
1984Ap&SS.102...21D 9 3 Observatrions of the Rosette nebula using the decameter wave radio telescope at Gauribidanur. DESHPANDE A.A., SHEVGAONKAR R.K. and SASTRY C.V.
1986ApJ...301..813O 11 25 Decameter wavelength observations of the Rosette nebula and the Monoceros Loop supernova remnant. ODEGARD N.
1988ApJS...68..715K viz 715 33 The Clark Lake 30.9 MHz galactic plane survey. KASSIM N.E.
1989AJ.....98.1652H 52 6 A search for X-ray counterparts to small-diameter galactic radio sources. HELFAND D.J. and CHANAN G.A.
1995ApJS...97..347G viz 4381 198 The Parkes-MIT-NRAO (PMN) Surveys. VI. Source Catalog for the Equatorial Survey (-9.5 deg < Dec. < +10.0 deg) GRIFFITH M.R., WRIGHT A.E., BURKE B.F., et al.
1995AuJPh..48..143S viz 2214 69 Radio sources observed with the Culgoora circular array. SLEE O.B.
1997A&AS..126..413R viz 1829 86 The Effelsberg 21 cm radio continuum survey of the Galactic plane between l = 95.5deg and l = 240 deg. REICH P., REICH W. and FUERST E.
2003ApJ...586.1067H 1 84 486 The millennium Arecibo 21 centimeter absorption-line survey. II. Properties of the warm and cold neutral media. HEILES C. and TROLAND T.H.
2003ApJS..145..329H viz 74 137 The millennium Arecibo 21 centimeter absorption-line survey. I. Techniques and gaussian fits. HEILES C. and TROLAND T.H.
2010A&A...511A..53V viz 15       D               1 107940 39 The SPECFIND V2.0 catalogue of radio cross-identifications and spectra. SPECFIND meets the Virtual Observatory. VOLLMER B., GASSMANN B., DERRIERE S., et al.
2014ApJS..212...15F viz 16       D               1 24940 60 A broadband polarization catalog of extragalactic radio sources. FARNES J.S., GAENSLER B.M. and CARRETTI E.
2018ApJS..235....1L 17       D               2 24 46 Where is OH and does it trace the dark molecular gas (DMG)? LI D., TANG N., NGUYEN H., et al.
2018ApJ...862...49N 16       D               1 58 51 Dust-gas scaling relations and OH abundance in the galactic ISM. NGUYEN H., DAWSON J.R., MIVILLE-DESCHENES M.-A., et al.
2019ApJ...880..141N 17       D               2 90 21 Exploring the properties of warm and cold atomic hydrogen in the Taurus and Gemini regions. NGUYEN H., DAWSON J.R., LEE M.-Y., et al.
2021A&A...655A..17S viz 17       D               1 338596 3 The SPECFIND V3.0 catalog of radio continuum cross-identifications and spectra: Reaching lower frequencies. STEIN Y., VOLLMER B., BOCH T., et al.

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