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We present moderate- (1'') and high-resolution (02) observations of the CO (2–1) emission at 43 GHz and radio continuum emission at 1.47 GHz from the z = 4.7 QSO BRI 1202-0725 and the z = 4.4 QSO BRI ...
Searches for CO emission in high-redshift objects have traditionally suffered from the accuracy of optically derived redshifts for lack of bandwidth in correlators at radio observatories. This problem...
Despite decades of study, it remains unclear whether there are distinct radio-loud and radio-quiet populations of quasi-stellar objects (QSOs). Early studies were limited by inhomogeneous QSO samples,...
We report on the detection of bright CO(4-3) line emission in two powerful, obscured quasars discovered in the SWIRE survey, SW022513 and SW022550 at z>3.4. We analyze the line strength and profile to...
IR Spectroscopy in High Redshift QSOs
Low Redshift BAL QSOs in the Eigenvector 1 Context。
QSOs and the survey OTELO     QSOs  survey OTELO       2009/6/25
QSOs and the survey OTELO。
A Search for z 6 QSOs in the Palomar-Quest Sky Survey。
The puzzle of the lyman continuum polarization of qsos
A correlation between redshifts .z/ and apparent magnitudes .V / (Hubble relation) of Quasi Stellar Objects (QSOs) has long been sought. Such a correlation exists for galaxies whose redshifts are of...

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