other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
QSO B1713+218 , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST13:29:28 |
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 |
---|---|---|---|---|---|---|---|---|---|
1998MNRAS.294L...7H | 1 | 10 | 42 | Discovery of radio-loud quasars with z = 4.72 and z = 4.01. | HOOK I.M. and McMAHON R.G. | ||||
2000AJ....119.1526S | 42 | 71 | Radio properties of z>4 optically selected quasars. | STERN D., DJORGOVSKI S.G., PERLEY R.A., et al. | |||||
2001MNRAS.325.1167S | 32 | 16 | A search for distant radio-loud quasars in the CLASS survey: three new radio-selected quasars at z > 4. | SNELLEN I.A.G., McMAHON R.G., DENNETT-THORPE J., et al. | |||||
2002MNRAS.329..700S | 1288 | 23 | Automated optical identification of a large complete northern hemisphere sample of flat-spectrum radio sources with S6cm>200mJy. | SNELLEN I.A.G., McMAHON R.G., HOOK I.M., et al. | |||||
2003AJ....125..418V | 57 | 46 | X-ray lighthouses of the high-redshift universe: probing the most luminous z>4 Palomar digital sky survey quasars with Chandra. | VIGNALI C., BRANDT W.N., SCHNEIDER D.P., et al. | |||||
2004AJ....128..523B | 19 | 32 | Chandra observations of radio-loud quasars at z>4: x-rays from the radio beacons of the early universe. | BASSETT L.C., BRANDT W.N., SCHNEIDER D.P., et al. | |||||
2006A&A...455..773V | 108224 | 628 | A catalogue of quasars and active nuclei: 12th edition. | VERON-CETTY M.-P. and VERON P. | |||||
2008MNRAS.388.1349E | 151 | X F | 3 | 50 | 15 | A search for damped Lyman α systems towards radio-loud quasars I: the optical survey. | ELLISON S.L., YORK B.A., PETTINI M., et al. | ||
2010A&A...511A..53V | 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. | ||
2010AJ....139.1695L | 15 | D | 1 | 280 | 59 | The Celestial Reference Frame at 24 and 43 GHz. I. Astrometry. | LANYI G.E., BOBOLTZ D.A., CHARLOT P., et al. | ||
2010A&A...518A..10V | 15 | D | 1 | 168913 | 597 | A catalogue of quasars and active nuclei: 13th edition. | VERON-CETTY M.-P. and VERON P. | ||
2013ApJ...763..109W | 562 | D | X C | 14 | 33 | 20 | An X-ray and multiwavelength survey of highly radio-loud quasars at z > 4: jet-linked emission in the brightest radio beacons of the early universe. | WU J., BRANDT W.N., MILLER B.P., et al. | |
2015MNRAS.452.3457G | 453 | D | X C | 11 | 22 | 14 | CMB quenching of high-redshift radio-loud AGNs. | GHISELLINI G., HAARDT F., CIARDI B., et al. | |
2016MNRAS.461L..21G | 16 | D | 1 | 12 | 6 | Dark bubbles around high-redshift radio-loud active galactic nucleus. | GHISELLINI G. and SBARRATO T. | ||
2019MNRAS.482.2016Z | 17 | D | 1 | 49 | 3 | Investigating the X-ray enhancements of highly radio-loud quasars at z > 4. | ZHU S.F., BRANDT W.N., WU J., et al. | ||
2019MNRAS.484..204C | 17 | D | 1 | 45 | 22 | The space density of z > 4 blazars. | CACCIANIGA A., MORETTI A., BELLADITTA S., et al. | ||
2019MNRAS.489.2732I | 17 | D | 3 | 25 | 24 | X-ray properties of z > 4 blazars. | IGHINA L., CACCIANIGA A., MORETTI A., et al. | ||
2020ApJ...897..177P | 17 | D | 1 | 142 | 16 | Blazars at the cosmic dawn. | PALIYA V.S., AJELLO M., CAO H.-M., et al. | ||
2021MNRAS.508.2798S | 17 | D | 1 | 119 | 7 | High-redshift quasars at z >= 3 - I. Radio spectra. | SOTNIKOVA Y., MIKHAILOV A., MUFAKHAROV T., et al. | ||
2021A&A...655A..17S | 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. | ||
2022ApJS..260...49K | 18 | D | 1 | 87 | 4 | Radio-loud Quasars above Redshift 4: Very Long Baseline Interferometry (VLBI) Imaging of an Extended Sample. | KREZINGER M., PERGER K., GABANYI K.E., et al. |