activity
20102021
most citedHST imaging of four gravitationally lensed quasars

30 citations · 65 across the 10 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2021★ 3 cited

Star Formation in CALIFA survey perturbed galaxies. II. Star Formation Histories and Oxygen Abundances

A. Morales-Vargas, J. P. Torres-Papaqui, F. F. Rosales-Ortega +6

Galaxy evolution is generally affected by tidal interactions. Firstly, in this series, we reported several effects which suggest that tidal interactions contribute to regulating st…

astro-ph.GA2020★ 7 cited

Star Formation in CALIFA survey perturbed galaxies. I. Effects of Tidal Interactions

A. Morales-Vargas, J. P. Torres-Papaqui, F. F. Rosales-Ortega +7

We explore the effects of tidal interactions on star formation (SF) by analysing a sample of CALIFA survey galaxies. The sample consists of tidally and non-tidally perturbed galaxi…

astro-ph.GA2018★ 30 cited

HST imaging of four gravitationally lensed quasars

Nicholas F. Bate, Georgios Vernardos, Matthew J. O'Dowd +7

We present new HST WFPC3 imaging of four gravitationally lensed quasars: MG 0414+0534; RXJ 0911+0551; B 1422+231; WFI J2026-4536. In three of these systems we detect wavelength-dep…

astro-ph.GA2014★ 4 cited

A mid infrared study of low-luminosity AGNs with WISE

R. Coziol, J. P. Torres-Papaqui, I. Plauchu-Frayn +4

Using data from the Wide-field Infrared Survey Explorer (WISE) we show that the mid infrared (MIR) colors of low-luminosity AGNs (LLAGNs) are significanlty different from those of…

astro-ph.GA2010

Low Luminosity AGN candidates in SDSS

J. P. Torres-Papaqui, R. Coziol, J. M. Islas-Islas +2

In a sample of 476931 NELGs obtained from the SDSS DR5 data we find that in 22% of the galaxies the emission line [OIII]5007, H, or both, are missing. The nature of the activ…

astro-ph.GA2010

The signature of LLAGNs in the nearby universe

D. M. Neri-Larios, J. P. Torres-Papaqui, R. Coziol +2

We have used the diagnostic diagram that compares the ratio of emission lines [NII]\lambda6584/Hαwith the equivalent width of [NII]6584, as proposed by Coziol et al. (1998), to…