Zobrazeno 1 - 10
of 104
pro vyhledávání: '"David V. Bowen"'
Autor:
Varsha P. Kulkarni, David V. Bowen, Lorrie A. Straka, Donald G. York, Neeraj Gupta, Pasquier Noterdaeme, Raghunathan Srianand
Publikováno v:
The Astrophysical Journal, 929(2):150
We report {\it HST} COS spectroscopy of 10 quasars with foreground star-forming galaxies at 0.02$
Comment: 51 pages, 12 figures. Submitted to the Astrophysical Journal
Comment: 51 pages, 12 figures. Submitted to the Astrophysical Journal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c393c6fdf7793e1bc18f1eeb73ed37e5
https://hdl.handle.net/1887/3562556
https://hdl.handle.net/1887/3562556
Autor:
Todd M. Tripp, Renyue Cen, Edward B. Jenkins, Donald G. York, David V. Bowen, Max Pettini, D. Chelouche
We present an HST Cosmic Origins Spectrograph (COS) spectrum of the QSO SDSS J095109.12+330745.8 ($z_{em} = 0.645$) whose sightline passes through the SMC-like dwarf galaxy UGC 5282 ($M_B = -16.0$, $cz = 1577$ km s$^{-1}$ ), 1.2 kpc in projection fro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::323d9d1c3d68258b84826c2b3bee43a9
http://arxiv.org/abs/2003.06429
http://arxiv.org/abs/2003.06429
Using Hubble Space Telescope/Space Telescope Imaging Spectrograph G140M spectroscopy, we investigate an absorption-line system at $z$=0.07489 in the spectrum of the quasi-stellar object PG 1543+489 ($z_{QSO}$=0.401). The sightline passes within $\rho
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4312e06512e9de204171760c9fbf9df0
http://arxiv.org/abs/1901.08147
http://arxiv.org/abs/1901.08147
Autor:
Nicolas Lehner, J. Christopher Howk, John M. O'Meara, Christopher B. Wotta, Molly S. Peeples, David V. Bowen, Michelle A. Berg, Nicolas Tejos, Joseph N. Burchett
We present a search for HI in the circumgalactic medium (CGM) of 21 massive ($\langle \log M_\star \rangle \sim 11.4$), luminous red galaxies (LRGs) at $z\sim0.5$. Using UV spectroscopy of QSO sightlines projected within 500 kpc ($\sim R_{vir}$) of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::193ff33568fddb9aeaedddae8d3c8222
http://arxiv.org/abs/1811.10717
http://arxiv.org/abs/1811.10717
Autor:
Christopher N. A. Willmer, Nicolas Lehner, Joseph N. Burchett, Molly S. Peeples, Edward B. Jenkins, Rongmon Bordoloi, Neal Katz, David V. Bowen, Jessica K. Werk, J. Christopher Howk, Jason Tumlinson, John M. O'Meara, J. Xavier Prochaska, Joseph D. Meiring, Todd M. Tripp, Nicolas Tejos
We survey the highly ionized circumgalactic media (CGM) of 29 blindly selected galaxies at 0.49 < z_(gal) < 1.44 based on high-S/N ultraviolet spectra of z > 1 QSOs and the galaxy database from the COS Absorption Survey of Baryon Harbors (CASBaH). We
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::72351255f06ff929ae4f5f9b9e8497dd
Autor:
Edward B. Jenkins, Todd M. Tripp, David V. Bowen, Joseph N. Burchett, Q. Daniel Wang, Christopher N. A. Willmer
We analyze the intracluster medium (ICM) and circumgalactic medium (CGM) in 7 X-ray detected galaxy clusters using spectra of background QSOs (HST-COS/STIS), optical spectroscopy of the cluster galaxies (MMT/Hectospec and SDSS), and X-ray imaging/spe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d091e0f390301b9dc2c0e4903457917a
http://arxiv.org/abs/1705.05892
http://arxiv.org/abs/1705.05892
Autor:
Zakary L. Whichard, Varsha P. Kulkarni, Lorrie A. Straka, Donald G. York, Pushpa Khare, Michael Bishof, David V. Bowen
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 436:3200-3223
We have improved upon our previous search technique of systematically searching QSO spectra for narrow galactic H-alpha emission, which indicates a foreground galaxy within the Sloan Digital Sky Survey (SDSS) spectral fiber. We now search for H-alpha
Autor:
Donald G. York, Michael Florian, Celine Peroux, Varsha P. Kulkarni, Sean D. Johnson, David V. Bowen, Britt Lundgren, Lorrie A. Straka
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2016, 458 (4), pp.3760--3772. ⟨10.1093/mnras/stw508⟩
Monthly Notices of the Royal Astronomical Society, 458(4), 3760-3772
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 458 (4), pp.3760--3772. ⟨10.1093/mnras/stw508⟩
NASA Astrophysics Data System
Monthly Notices of the Royal Astronomical Society, 2016, 458 (4), pp.3760--3772. ⟨10.1093/mnras/stw508⟩
Monthly Notices of the Royal Astronomical Society, 458(4), 3760-3772
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 458 (4), pp.3760--3772. ⟨10.1093/mnras/stw508⟩
NASA Astrophysics Data System
Using the Low Dispersion Survey Spectrograph 3 at the Magellan II Clay Telescope, we target {candidate absorption host galaxies} detected in deep optical imaging {(reaching limiting apparent magnitudes of 23.0-26.5 in $g, r, i,$ and $z$ filters) in t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::91441e9d51545785738cd9ad0740873e
https://hal.science/hal-01440088/document
https://hal.science/hal-01440088/document
Autor:
Timothy M. Heckman, Pushpa Khare, David V. Bowen, Lorrie A. Straka, Gordon T. Richards, Jean M. Quashnock, Daniel E. Vanden Berk, Donald G. York, Seth Kuttruff, Varsha P. Kulkarni, Patrick B. Hall, Michael Bishof, Lara Ghering, Mark SubbaRao, Sean D. Johnson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 423:3692-3708
A search for emission lines in foreground galaxies in quasar spectra (z(gal) < z(QSO)) of the Sloan Digital Sky Survey (SDSS) data release 5 (DR5) reveals 23 examples of quasars shining through low redshift, foreground galaxies at small impact parame
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 408:849-864
We present the results from our 21-cm absorption survey of a sample of 5 quasar-galaxy pairs (QGPs), with the redshift of the galaxies in the range 0.03