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相关论文: Strong MgII Absorption Systems in QSOs from the Sl…

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We present the results of a MgII absorption-line survey using QSO spectra from the SDSS EDR. Over 1,300 doublets with rest equivalent widths greater than 0.3\AA and redshifts $0.366 \le z \le 2.269$ were identified and measured. We find…

天体物理学 · 物理学 2009-11-10 D. B. Nestor , D. A. Turnshek , S. M. Rao

We present the results of a search for metal absorption lines in the spectra of background QSOs whose sightlines pass close to foreground QSOs. We detect MgII(2796,2803) absorption in Sloan Digital Sky Survey (SDSS) spectra of four z>1.5…

We detail a powerful indirect method for the study of damped Lyman alpha systems (DLAs) at low redshift. We increase the probability of finding a low-redshift DLA to nearly 50% by targeting QSOs that are known to have strong low-redshift…

天体物理学 · 物理学 2016-01-27 Daniel B. Nestor , Sandhya Rao , David Turnshek

We present a detailed study of HI and metals for 110 MgII absorption systems discovered at 1.98 <= z <= 5.33 in the infrared spectra of high redshift QSOs. Using new measurements of rest-frame UV lines from optical spectra of the same…

宇宙学与河外天体物理 · 物理学 2015-06-05 Michael S. Matejek , Robert A. Simcoe , Kathy L. Cooksey , Eduardo N. Seyffert

Using a sample of nearly 700 quasars with strong (W_0(2796)>0.8 Angstrom) MgII absorption lines detected in the Early Data Release of the SDSS, we demonstrate the feasibility of measuring the photometric properties of the absorber systems…

天体物理学 · 物理学 2009-11-13 Stefano Zibetti , Brice Menard , Daniel Nestor , David Turnshek

We present a catalog of intervening MgII quasar absorption-line systems in the redshift interval 0.36 <= z <= 2.28. The catalog was built from Sloan Digital Sky Survey Data Release Four (SDSS DR4) quasar spectra. Currently, the catalog…

宇宙学与河外天体物理 · 物理学 2015-05-27 Anna M. Quider , Daniel B. Nestor , David A. Turnshek , Sandhya M. Rao , Eric M. Monier , Anja N. Weyant , Joseph R. Busche

We analyze the cross-correlation of 2,705 unambiguously intervening Mg II (2796,2803A) quasar absorption line systems with 1,495,604 luminous red galaxies (LRGs) from the Fifth Data Release of the Sloan Digital Sky Survey within the…

We discuss issues concerning the physical nature of intervening MgII quasar absorption systems in light of results from our recent surveys using SDSS EDR QSO spectra and data obtained at the MMT. These surveys indicate an excess of weak…

天体物理学 · 物理学 2009-11-11 D. B. Nestor , D. A. Turnshek , S. M. Rao

We present an initial survey of Mg II absorption characteristics in the halos of a carefully constructed, volume-limited subsample of galaxies embedded in the spectroscopic part of the Sloan Digital Sky Survey. We observed quasars near…

宇宙学与河外天体物理 · 物理学 2015-05-14 Elizabeth J. Barton , Jeff Cooke

We have performed an analysis of over 34,000 MgII doublets at 0.36 < z < 2.29 in Sloan Digital Sky Survey (SDSS) Data-Release 7 quasar spectra; the catalog, advanced data products, and tools for analysis are publicly available. The catalog…

宇宙学与河外天体物理 · 物理学 2014-01-20 Eduardo N. Seyffert , Kathy L. Cooksey , Robert A. Simcoe , John M. O'Meara , Melodie M. Kao , J. Xavier Prochaska

The XQ-100 survey provides optical and near infrared coverage of 36 blindly selected, intervening damped Lyman alpha systems (DLAs) at 2 < z < 4, simultaneously covering the MgII doublet at 2796A, 2803A, and the Ly-alpha transition. Using…

We present the catalogue of the Mg II absorption systems detected at a high significance level using an automated search algorithm in the spectra of quasars from the twelfth data release of the Sloan Digital Sky Survey. A total of 266,433…

We have discovered two dusty intervening MgII absorption systems at z~1.3 in the Sloan Digital Sky Survey (SDSS) database. The overall spectra of both QSOs are red (u-K>4.5 mag) and are well modelled by the composite QSO spectrum reddened…

天体物理学 · 物理学 2009-11-13 R. Srianand , N. Gupta , P. Petitjean , P. Noterdaeme , D. J. Saikia

We present a generic and fully-automatic method aimed at detecting absorption lines in the spectra of astronomical objects. The algorithm estimates the source continuum flux using a dimensionality reduction technique, nonnegative matrix…

宇宙学与河外天体物理 · 物理学 2015-06-12 Guangtun Zhu , Brice Ménard

We present a catalogue of MgII absorption systems obtained from high resolution UVES/VLT data of 77 QSOs in the redshift range 0.6 < z < 2.0, and down to an equivalent width W_0 > 0.1 \AA. The statistical properties of our sample are found…

宇宙学与河外天体物理 · 物理学 2015-05-18 M. L. Bernet , F. Miniati , S. J. Lilly

We present the results from a spectroscopic survey for intervening MgII absorption in the spectra of 381 background QSOs conducted at the Multiple Mirror Telescope. This survey complements our earlier SDSS EDR MgII survey, extending our…

天体物理学 · 物理学 2009-11-11 Daniel B. Nestor , David A. Turnshek , Sandhya M. Rao

We present a systematic search for molecular hydrogen absorption systems at high redshift in quasar spectra from the Sloan Digital Sky Survey (SDSS) II Data Release 7 and SDSS-III Data Release 9. We have selected candidates using a modified…

宇宙学与河外天体物理 · 物理学 2014-03-20 S. A. Balashev , V. V. Klimenko , A. V. Ivanchik , D. A. Varshalovich , P. Petitjean , P. Noterdaeme

We describe a search for MgII(2796,2803) absorption lines in Sloan Digital Sky Survey (SDSS) spectra of QSOs whose lines of sight pass within impact parameters of 200 kpc of galaxies with photometric redshifts of z=0.46-0.6 and redshift…

宇宙学与河外天体物理 · 物理学 2015-05-20 David V. Bowen , Doron Chelouche

We present a search for "weak" MgII absorbers [those with W_r(2796) < 0.3 A in the HIRES/Keck spectra of 26 QSOs. We found 30, of which 23 are newly discovered. The spectra are 80% complete to W_r(2796) = 0.02 A and have a cumulative…

天体物理学 · 物理学 2009-10-30 Christopher W. Churchill , Jane R. Rigby , Jane C. Charlton , Steven S. Vogt

We present extensive metal-line absorption properties for 45 absorption systems that were selected by their Mg II absorption at redshifts between 0.4 and 1.4. For each system the properties of several chemical species are determined,…

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