1-14 of 14
Authors: C. Papovich
Journal Article
[Ne v] emission from a faint epoch of reionization-era galaxy: evidence for a narrow-line intermediate-mass black hole Open Access
Monthly Notices of the Royal Astronomical Society, Volume 534, Issue 3, November 2024, Pages 2633–2652, https://doi.org/10.1093/mnras/stae2199
Published: 23 September 2024
Journal Article
The origin of large emission line widths in massive galaxies at redshifts z ∼ 3–4 Open Access
Monthly Notices of the Royal Astronomical Society, Volume 531, Issue 3, July 2024, Pages 3187–3202, https://doi.org/10.1093/mnras/stae1335
Published: 31 May 2024
Journal Article
x-cigale : fitting AGN/galaxy SEDs from X-ray to infrared
Free
Monthly Notices of the Royal Astronomical Society, Volume 491, Issue 1, January 2020, Pages 740–757, https://doi.org/10.1093/mnras/stz3001
Published: 24 October 2019
Journal Article
The VANDELS ESO public spectroscopic survey Free
Monthly Notices of the Royal Astronomical Society, Volume 479, Issue 1, September 2018, Pages 25–42, https://doi.org/10.1093/mnras/sty1213
Published: 15 May 2018
Journal Article
Decoupled black hole accretion and quenching: the relationship between BHAR, SFR and quenching in Milky Way- and Andromeda-mass progenitors since z = 2.5 Free
Monthly Notices of the Royal Astronomical Society, Volume 473, Issue 3, January 2018, Pages 3710–3716, https://doi.org/10.1093/mnras/stx2587
Published: 09 October 2017
Journal Article
A deep ALMA image of the Hubble Ultra Deep Field Free
Monthly Notices of the Royal Astronomical Society, Volume 466, Issue 1, April 2017, Pages 861–883, https://doi.org/10.1093/mnras/stw3088
Published: 30 November 2016
Journal Article
Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z = 2.25 Free
Monthly Notices of the Royal Astronomical Society, Volume 455, Issue 3, 21 January 2016, Pages 2731–2744, https://doi.org/10.1093/mnras/stv2468
Published: 25 November 2015
Journal Article
Detecting massive galaxies at high redshift using the Dark Energy Survey Free
Monthly Notices of the Royal Astronomical Society, Volume 434, Issue 1, 01 September 2013, Pages 296–312, https://doi.org/10.1093/mnras/stt1018
Published: 02 July 2013
Journal Article
The LABOCA survey of the Extended Chandra Deep Field-South – radio and mid-infrared counterparts to submillimetre galaxies Free
Monthly Notices of the Royal Astronomical Society, Volume 413, Issue 4, June 2011, Pages 2314–2338, https://doi.org/10.1111/j.1365-2966.2010.18132.x
Published: 20 May 2011
Journal Article
The Hubble Space Telescope GOODS NICMOS Survey: overview and the evolution of massive galaxies at 1.5< z< 3 Free
Monthly Notices of the Royal Astronomical Society, Volume 413, Issue 1, May 2011, Pages 80–100, https://doi.org/10.1111/j.1365-2966.2010.18113.x
Published: 14 April 2011
Journal Article
A submillimetre galaxy at z= 4.76 in the LABOCA survey of the Extended Chandra Deep Field-South Free
Monthly Notices of the Royal Astronomical Society, Volume 395, Issue 4, June 2009, Pages 1905–1914, https://doi.org/10.1111/j.1365-2966.2009.14700.x
Published: 15 May 2009
Journal Article
The properties and evolution of a K‐band selected sample of massive galaxies at z∼ 0.4–2 in the Palomar/DEEP2 survey Free
Monthly Notices of the Royal Astronomical Society, Volume 381, Issue 3, November 2007, Pages 962–986, https://doi.org/10.1111/j.1365-2966.2007.12316.x
Published: 10 October 2007
Journal Article
Environmental dependence of active galactic nuclei activity in the supercluster A901/2 Free
Monthly Notices of the Royal Astronomical Society, Volume 380, Issue 4, September 2007, Pages 1467–1487, https://doi.org/10.1111/j.1365-2966.2007.12127.x
Published: 05 September 2007
Journal Article
The SCUBA HAlf Degree Extragalactic Survey – III. Identification of radio and mid-infrared counterparts to submillimetre galaxies Free
Monthly Notices of the Royal Astronomical Society, Volume 380, Issue 1, 1 September 2007, Pages 199–228, https://doi.org/10.1111/j.1365-2966.2007.12044.x
Published: 13 August 2007
