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Absorption due to HeII Ly-alpha has been detected at low resolution in the spectra of four quasars between redshifts z = 2.74-3.29. We assess these observations, giving particular attention to the radiative transfer of the ionizing…

天体物理学 · 物理学 2009-10-30 Mark A. Fardal , Mark L. Giroux , J. Michael Shull

We report on the detection of strongly varying intergalactic HeII absorption in HST/COS spectra of two z~3 quasars. From our homogeneous analysis of the HeII absorption in these and three archival sightlines, we find a marked increase in…

The Lyman alpha absorption from intergalactic, once-ionized helium (HeII) has been measured with HST in four quasars over the last few years, over the redshift range 2.4 < z < 3.2. These observations have indicated that the HeII…

天体物理学 · 物理学 2009-10-31 Jordi Miralda-Escude

We report on observations of redshifted HeII 304 A absorption in the QSO HE 2347-4342 (z=2.885, V=16.1) with the GHRS on board HST (FWHM=0.7 A). At the expected position of HeII 304 A absorption, HE 2347-4342 is the most UV-bright high…

天体物理学 · 物理学 2009-09-28 D. Reimers , S. Koehler , L. Wisotzki , D. Groote , P. Rodriguez-Pascual , W. Wamsteker

We present measurements of the large-scale (~40 comoving Mpc) effective optical depth of HeII Ly$\alpha$ absorption, $\tau_{\rm eff}$, at 2.54<z<3.86 toward 16 HeII-transparent quasars observed with the Cosmic Origins Spectrograph (COS) on…

星系天体物理 · 物理学 2019-05-01 Gábor Worseck , Frederick B. Davies , Joseph F. Hennawi , J. Xavier Prochaska

We measure the effective optical depth of HeII Ly\alpha\ absorption \tau$_\mathsf{eff,HeII}$ at 2.3<z<3.5 in 17 UV-transmitting quasars observed with UV spectrographs on the Hubble Space Telescope (HST). The median \tau$_\mathsf{eff,HeII}$…

宇宙学与河外天体物理 · 物理学 2017-08-30 Gábor Worseck , J. Xavier Prochaska , Joseph F. Hennawi , Matthew McQuinn

We obtained high-resolution VLT and FUSE spectra of the quasar HE2347-4342 to study the properties of the intergalactic medium between redshifts z=2.0-2.9. The high-quality optical spectrum allows us to identify approximately 850 HeII…

Many experts believe that the z ~ 3 HeII Ly-alpha forest will suffer from the same saturation issues as the z ~ 6 HI Ly-alpha forest and, therefore, will not be a sensitive probe of HeII reionization. However, there are several factors that…

宇宙学与河外天体物理 · 物理学 2009-10-06 Matthew McQuinn

We report the discovery of a further line of sight allowing detection of HeII Ly alpha absorption by the intergalactic medium. A HST/STIS survey of 32 bright z ~ 3 quasars selected from the Hamburg Quasar Surveys yielded one detection…

天体物理学 · 物理学 2016-08-30 D. Reimers , C. Fechner , H. -J. Hagen , P. Jakobsen , D. Tytler , D. Kirkman

We present a new, high resolution HST/GHRS spectrum of quasar Q0302-003, and use the HeII Lyman-$\alpha$ absorption, together with a high resolution Keck spectrum of the HI Lyman-$\alpha$ forest, to probe the distribution and ionization…

天体物理学 · 物理学 2009-09-28 Craig J. Hogan , Scott F. Anderson , Martin H. Rugers

Quasars that allow the study of IGM He II are very rare, since they must be at high redshift along sightlines free of substantial hydrogen absorption, but recent work has dramatically expanded the number of such quasars known. We analyze…

宇宙学与河外天体物理 · 物理学 2015-05-20 David Syphers , Scott F. Anderson , Wei Zheng , Avery Meiksin , Daryl Haggard , Donald P. Schneider , Donald G. York

The ultraviolet spectrum (1145--1720A) of the distant quasar Q 0302--003 (z=3.286) was observed at 1.8A resolution with the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope. A total integration time of 23,280 s was…

天体物理学 · 物理学 2007-05-23 S. R. Heap , G. M. Williger , A. Smette , I. Hubeny , M. Sahu , E. B. Jenkins , T. M. Tripp , J. N. Winkler

Intergalactic Ly-alpha opacity suggests that H I was reionized at z ~ 6, while He II reionization was delayed to z ~ 3. Both epochs are in conflict with inferences from CMB optical depth (WMAP) which suggest early reionization at z = 10-20.…

天体物理学 · 物理学 2007-05-23 J. Michael Shull

The large number of quasars found in the Sloan Digital Sky Survey has allowed searches for elusive, clear lines of sight towards HeII Ly-alpha absorption, a sensitive probe of the intergalactic medium. The few known systems indicate that…

天体物理学 · 物理学 2009-11-10 W. Zheng , K. Chiu , S. F. Anderson , D. P. Schneider , C. J. Hogan , D. G. York , S. Burles , J. V. Brinkmann

We present statistics of HeII Lya transmission spikes and large-scale absorption troughs using archival high-resolution ($R=\lambda /\Delta \lambda \simeq 12,500$-$18,000$) far-UV spectra of eight HeII-transparent quasars obtained with the…

宇宙学与河外天体物理 · 物理学 2022-03-30 Kirill Makan , Gábor Worseck , Frederick B. Davies , Joseph F. Hennawi , J. Xavier Prochaska , Philipp Richter

The neutral hydrogen and the ionized helium absorption in the spectra of quasars are unique probes of structure in the early universe. We present Far-Ultraviolet Spectroscopic Explorer observations of the line of sight to the quasar…

Observations of He II Ly{\alpha} Gunn-Peterson troughs have proved to be a valuable probe of the epoch of helium reionization at z~3. Since this optical depth can become unmeasurably large even for modest He II fractions, various alternate…

Observations from the HUT and the HST have recently detected HeII absorption along the lines of sight to two high redshift quasars. We use cosmological simulations with gas dynamics to investigate HeII absorption in the cold dark matter…

天体物理学 · 物理学 2009-10-28 Rupert A. C. Croft , David H. Weinberg , Neal Katz , Lars Hernquist

Recent observations of high redshift quasars at z~6 have finally revealed complete Gunn-Peterson absorption. However, this at best constrains the volume-weighted and mass-weighted hydrogen neutral fractions to be greater than 10^-3 and…

天体物理学 · 物理学 2009-11-07 S. Peng Oh

Three independent observational studies have now detected a narrow (\Delta z ~ 0.5) dip centred at z=3.2 in the otherwise smooth redshift evolution of the Lya forest effective optical depth. This feature has previously been interpreted as…

宇宙学与河外天体物理 · 物理学 2015-05-13 James S. Bolton , S. Peng Oh , Steven R. Furlanetto
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