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F. Briggs

5 papers hereh-index 7337 citations11 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3
  • last author1

Across the 4 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph4
  • astro-ph.CO1
same name
  • F. Briggs — 91 papers, h 49
  • F. Briggs — 6 papers, h 12
  • F. Briggs — 3 papers, h 4
  • F. Briggs — 1 paper
  • F. Briggs — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982009
collaborators

5 papers

astro-ph.CO2009

The covering factor of high redshift damped Lyman-α systems

N. Kanekar, W. M. Lane, E. Momjian +2

We have used the Very Long Baseline Array to image 18 quasars with foreground damped Lyman-α systems (DLAs) at 327, 610 or 1420 MHz, to measure the covering factor f of each DL…

astro-ph2001

Did VV~29 collide with a dark Dark-Matter halo?

F. H. Briggs, O. Moller, J. L. Higdon +2

Westerbork Radio Synthesis Telescope observation of the galaxy VV29=Arp188=UGC10214 shows that there are at least three distinct dynamical components whose kinematics can be traced…

astro-ph2001

Two New Low Redshift 21cm Absorbers

W. M. Lane, F. H. Briggs

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 Ra…

astro-ph1999

Detection of Warm and Cold Phases of the Neutral ISM in a Damped Ly-alpha Absorber

W. M. Lane, F. H. Briggs, A. Smette

We present a detailed study of the HI 21cm absorption system at z=0.0912 towards the radio quasar B0738+313. The uncommonly narrow main absorption line and weak secondary line are…

astro-ph1998

HI 21cm absoprtion in two low redshift damped Ly-alpha systems

W. Lane, A. Smette, F. Briggs +3

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…

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