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相关论文: New searches for HI 21-cm in damped Lyman-alpha ab…

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We present deep GMRT 21cm absorption spectra of 10 damped Lyman-$\alpha$ systems (DLAs), of which 8 are at redshifts $z \ga 1.3$. HI absorption was detected in only one DLA, the $z = 0.5318$ absorber toward PKS 1629+12, which has been…

天体物理学 · 物理学 2008-11-26 Nissim Kanekar , Jayaram N Chengalur

In this paper we investigate the possible reasons why HI 21-cm absorption in damped Lyman-alpha systems (DLAs) has only been detected at low redshift... We suggest that the lack of 21-cm absorption detections at high redshift arises from…

天体物理学 · 物理学 2009-11-11 S. J. Curran , J. K. Webb

We investigate the practice of assigning high spin temperatures to damped Lyman-alpha absorption systems (DLAs) not detected in HI 21-cm absorption. In particular, Kanekar & Chengaulr (2003) have attributed the mix of 21-cm detections and…

天体物理学 · 物理学 2009-11-10 S. J. Curran , M. T. Murphy , Y. M. Pihlstroem , J. K. Webb , C. R. Purcell

We report Giant Metrewave Radio Telescope (GMRT) 21cm observations of two confirmed and one candidate low redshift damped Lyman-alpha systems (DLAS). HI absorption was detected in the two confirmed systems, at z=0.2378 and z=0.5247, with…

天体物理学 · 物理学 2009-11-06 Nissim Kanekar , Jayaram N. Chengalur

We present the results of a survey for 21-cm absorption in four never previously searched damped Lyman-alpha absorption systems (DLAs) with the Westerbork Synthesis Radio Telescope. We add our results to other recent studies in order to…

天体物理学 · 物理学 2009-11-13 S. J. Curran , P. Tzanavaris , Y. M. Pihlstroem , J. K. Webb

We report the detection of HI 21 cm absorption from the $z=2.289$ damped Lyman-$\alpha$ system (DLA) towards TXS 0311+430, with the Green Bank Telescope. The 21 cm absorption has a velocity spread (between nulls) of $\sim 110$ km s$^{-1}$…

天体物理学 · 物理学 2009-11-13 Brian A. York , Nissim Kanekar , Sara L. Ellison , Max Pettini

We report results from a deep search for redshifted HI 21cm absorption from eight damped Lyman-$\alpha$ absorbers (DLAs) detected in our earlier optical survey for DLAs towards radio-loud quasars. HI 21cm absorption was detected from the $z…

宇宙学与河外天体物理 · 物理学 2015-06-12 Nissim Kanekar , Sara L. Ellison , Emmanuel Momjian , Brian A. York , Max Pettini

We report the detection of redshifted HI~21cm absorption in the $z \sim 2.347$ damped Lyman-$\alpha$ absorber (DLA) towards PKS B0438-436, with the Green Bank Telescope. This is the second-highest redshift at which 21cm absorption has been…

天体物理学 · 物理学 2009-11-11 N. Kanekar , R. Subrahmanyan , S. L. Ellison , W. M. Lane , J. N. Chengalur

Damped Lyman-alpha systems (DLAs) seen in the spectra of high-z QSOs allow us to probe the physical conditions in protogalaxies. Our understanding of physical conditions in DLAs at high-z is primarily based on the absorption lines of H_2…

宇宙学与河外天体物理 · 物理学 2009-02-19 N. Gupta , R. Srianand , P. Petitjean , P. Noterdaeme , D. J. Saikia

We report the GMRT detection of HI 21cm absorption from the $z \sim 3.39$ damped Lyman-$\alpha$ absorber (DLA) towards PKS 0201+113, the highest redshift at which 21cm absorption has been detected in a DLA. The absorption is spread over…

天体物理学 · 物理学 2008-11-26 N. Kanekar , J. N. Chengalur , W. M. Lane

We report a deep search for redshifted HI 21 cm emission from three damped and sub-damped Lyman-$\alpha$ absorbers (DLAs) at $z \approx 0.1$ with the Green Bank Telescope (GBT). No evidence for a redshifted HI 21 cm emission signal was…

星系天体物理 · 物理学 2015-06-19 Parichay Mazumdar , Nissim Kanekar , J. Xavier Prochaska

(Abridged) We present the results of a systematic GBT and GMRT survey for 21-cm absorption in a sample of 10 DLAs at 2<z_abs<3.4. Analysis of L-band VLBA images of the background QSOs are also presented. We detect 21-cm absorption in only…

宇宙学与河外天体物理 · 物理学 2015-06-03 R. Srianand , N. Gupta , P. Petitjean , P. Noterdaeme , C. Ledoux , C. J. Salter , D. J. Saikia

Recent high redshift surveys for 21-cm absorption in damped Lyman-alpha absorption systems (DLAs) take the number of published searches at z > 2 to 25, the same number as at z < 2, although the detection rate at high redshift remains…

宇宙学与河外天体物理 · 物理学 2015-06-04 S. J. Curran

We present Giant Metrewave Radio Telescope HI 21cm absorption observations, of candidate and confirmed damped Lyman-$\alpha$ systems (DLAS). The derived spin temperatures (T_s) are in all cases $\sim 1000$ K or higher. We have also collated…

天体物理学 · 物理学 2015-06-24 Jayaram N Chengalur , Nissim Kanekar

I report the detection of HI 21cm absorption in two high column density damped Lyman-$\alpha$ absorbers (DLAs) at $z \approx 2$ using new wide-band $250-500$ MHz receivers onboard the Giant Metrewave Radio Telescope. The integrated HI 21cm…

星系天体物理 · 物理学 2015-06-23 Nissim Kanekar

As part of a larger program to identify low redshift radio analogues of the damped Lyman-alpha (DLA) absorbers seen in the spectra of high redshift quasars, Westerbork Synthesis Radio Telescope (WSRT) observations have discovered two new HI…

天体物理学 · 物理学 2009-11-07 W. M. Lane , F. H. Briggs

The HI 21cm absorption optical depth and the N(HI) derived from Lya absorption can be combined to yield the spin temperature (Ts) of DLAs. Although Ts measurements exist for samples of DLAs with z <0.6 and z >1.7, the intermediate redshift…

宇宙学与河外天体物理 · 物理学 2015-06-05 Sara L. Ellison , Nissim Kanekar , J. Xavier Prochaska , Emmanuel Momjian , Gabor Worseck

We report the discovery of two low redshift HI 21cm absorbers, one at z = 0.2212 towards the z_{em} = 0.630 quasar OI 363 (B0738+313), and the other at z = 0.3127 towards PKS B1127-145 (z_{em} = 1.187). Both were found during a survey of…

天体物理学 · 物理学 2009-10-30 W. Lane , A. Smette , F. Briggs , S. Rao , D. Turnshek , G. Meylan

We present the results of a blind search for intervening HI 21 cm absorption toward 260 radio sources in the redshift range 0<z<2.74 with the Green Bank Telescope. The survey has the sensitivity to detect sub-damped Lyman-alpha (DLA)…

星系天体物理 · 物理学 2020-08-25 Kathryn Grasha , Jeremy Darling , Adam K. Leroy , Alberto D. Bolatto

We have used the Very Long Baseline Array to image 18 quasars with foreground damped Lyman-$\alpha$ systems (DLAs) at 327, 610 or 1420 MHz, to measure the covering factor $f$ of each DLA at or near its redshifted HI 21cm line frequency.…

宇宙学与河外天体物理 · 物理学 2011-02-11 N. Kanekar , W. M. Lane , E. Momjian , F. H. Briggs , J. N. Chengalur
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