Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Juan Pablo Torres-Papaqui"'
Autor:
Juan Pablo Torres-Papaqui, Roger Coziol, Aitor C. Robleto-Orús, Karla A. Cutiva-Alvarez, Paulina Roco-Avilez
Publikováno v:
The Astronomical Journal, Vol 168, Iss 1, p 37 (2024)
Using Sloan Digital Sky Survey (SDSS) spectra, we applied an automatic method to search for outflows (OFs) in three large samples of narrow-line active galactic nuclei (AGN) at low redshifts ( z < 0.4), separated into three spectral activity classes:
Externí odkaz:
https://doaj.org/article/448ead74617b4dc4a89885418e6f1fe2
Autor:
Coziol, Roger, Andernach, Heinz, Ortega-Minakata, Juan Pablo Torres-Papaqui René Alberto, del Rio, Froylan Moreno
To better constrain the hypotheses proposed to explain why only a few quasars are radio loud (RL), we compare the characteristics of 1958 nearby $(z\le 0.3)$ SDSS quasars, covered by the FIRST and NVSS radio surveys. Only 22\% are RL with $\log(L_{1.
Externí odkaz:
http://arxiv.org/abs/1612.02655
Autor:
A. C. Robleto-Orús, Juan Pablo Torres-Papaqui, R. A. Ortega-Minakata, Yago Ascasibar, Lluís Galbany, A. Morales-Vargas, Karla A. Cutiva-Alvarez, E. Bellocchi, J. J. Trejo-Alonso, Sebastián F. Sánchez, F. J. Romero-Cruz, Roger Coziol, A. L. Longinotti, M. Chow-Martínez
Publikováno v:
Proceedings of the International Astronomical Union. 15:291-294
NGC 7469 is a well-known type 1 AGN with a cirumnuclear star formation ring. It has previous detections of X-rays warm absorbers and an infrared biconical outflow. We analysed archival MUSE/VLT observations of this galaxy in order to look for an opti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ea3b3b242dc9565e2d6b0987da73010f
https://doi.org/10.1017/s1743921320001593
https://doi.org/10.1017/s1743921320001593
Autor:
A. C. Robleto-Orús, D. M. Neri-Larios, J. J. Trejo-Alonso, F. F. Rosales-Ortega, Juan Pablo Torres-Papaqui, M. Chow-Martínez, F. J. Romero-Cruz, A. Morales-Vargas, R. A. Ortega-Minakata
Galaxy evolution is generally affected by tidal interactions. Firstly, in this series, we reported several effects which suggest that tidal interactions contribute to regulating star formation (SF). To confirm that so, we now compare stellar mass ass
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c309e97405cee0de554ed19246090a0b
http://arxiv.org/abs/2109.07731
http://arxiv.org/abs/2109.07731
Autor:
D. M. Neri-Larios, J. J. Trejo-Alonso, M. Chow-Martínez, A. C. Robleto-Orús, F. J. Romero-Cruz, Juan Pablo Torres-Papaqui, R. A. Ortega-Minakata, F. F. Rosales-Ortega, A. Morales-Vargas, Sebastián F. Sánchez
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 galaxies whose star-forming regions are paired at the closest stellar mass s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96a1c3a96524c3608ed2d6763a2ca47d
Autor:
A. C. Robleto-Orús, Juan Pablo Torres-Papaqui, H. Andernach, R. Coziol, Karla A. Cutiva-Alvarez
Publikováno v:
Proceedings of the International Astronomical Union. 15:33-34
Using WISE data, we calibrated the W2-W3 colors in terms of star formation rates (SFRs) and applied this calibration to a sample of 1285 QSOs with the highest flux quality, covering a range in redshift from z ˜ 0.3 to z ˜ 3.8. According to our cali
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1532d7805012aa378e7798bf6ba88fe9
https://doi.org/10.1017/s1743921320001659
https://doi.org/10.1017/s1743921320001659
Autor:
Jesús Falcón-Barroso, C. Añorve, Juan Pablo Torres-Papaqui, Jorge K. Barrera-Ballesteros, Sebastián F. Sánchez, Hector Ibarra-Medel, Omar López-Cruz, Mark Birkinshaw, Wayne A. Barkhouse
Publikováno v:
López-Cruz, O, Ibarra-Medel, H J, Sánchez, S F, Birkinshaw, M, Añorve, C, Barrera-Ballesteros, J K, Falcon-Barroso, J, Barkhouse, W A & Torres-Papaqui, J P 2019, ' Secondary Infall in the Seyfert's Sextet : A Plausible Way Out of the Short Crossing Time Paradox ', Astrophysical Journal Letters, vol. 886, no. 1, L2 . https://doi.org/10.3847/2041-8213/ab5117
We used integral field spectroscopy from CALIFA DR3 and multiwavelength publicly-available data to investigate the star-formation histories of galaxies in the Seyfert's Sextet (SS, HCG 79). The galaxies H79a, H79b, H79c, and H79f have low star-format
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a0de21f624d6b674f94bc9dbd4bbb8a0
https://research-information.bris.ac.uk/ws/files/219552715/untitled.pdf
https://research-information.bris.ac.uk/ws/files/219552715/untitled.pdf
Autor:
Hector Bravo-Alfaro, César A. Caretta, Elcia M. S. Brito, Juan Pablo Torres-Papaqui, Felipe Macias Gloria, Eloy Juarez Sandoval, Patricia Campos Rodríguez
Publikováno v:
EPJ Web of Conferences, Vol 200, p 01008 (2019)
We present the main results of a multidisciplinary project on education and outreach in Guanajuato (Mexico). This collaboration was initiated in the International Year of Astronomy (IYA09, IAU-UNESCO, 2009) and is led by a team including astronomers,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d94172ba54aaea633763b176f01737ed
https://www.epj-conferences.org/articles/epjconf/pdf/2019/05/epjconf_ise2a2017_01008.pdf
https://www.epj-conferences.org/articles/epjconf/pdf/2019/05/epjconf_ise2a2017_01008.pdf
Autor:
Juan Pablo Torres-Papaqui, M. Chow-Martínez, A. C. Robleto-Orús, F. J. Romero-Cruz, Karla A. Cutiva-Alvarez, Gabriela Escobar-Vásquez, J. J. Trejo-Alonso, Roger Coziol, A. Morales-Vargas
Publikováno v:
The Astronomical Journal. 160:176
The optical spectra of 3,896 Seyfert~1 (Sy1) galaxies detected with WISE at z < 0.4 were analyzed for evidence of outflows. In 37% of the Sy1s the outflows appear as broad, blue-shifted, of the [OIII]5007, with a mean maximum velocity V_max ~1014 km/
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::92dbb5baa7808449b04b4933fd2fff04
https://doi.org/10.3847/1538-3881/abae5a
https://doi.org/10.3847/1538-3881/abae5a
Autor:
Froylan Moreno del Rio, Roger Coziol, René Alberto Ortega-Minakata, Juan Pablo Torres-Papaqui, Heinz Andernach
To better constrain the hypotheses proposed to explain why only a few quasars are radio loud (RL), we compare the characteristics of 1958 nearby $(z\le 0.3)$ SDSS quasars, covered by the FIRST and NVSS radio surveys. Only 22\% are RL with $\log(L_{1.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77495110343308a2099571bea6db88f9
http://arxiv.org/abs/1612.02655
http://arxiv.org/abs/1612.02655