CONTENT - Statistical studies of AMIGA sample - Individual studies of isolated galaxies - Detailed studies of complemetary samples Star formation, in
CONTENT - Statistical studies of AMIGA sample - Individual studies of isolated galaxies - Detailed studies of complemetary samples Star formation, interstellar medium and nuclear activity in complementary environments Physico-chemical conditions of the molecular gas Interstellar medium and nuclear activity QSOs - Technical and software related works STATISTICAL STUDIES OF AMIGA SAMPLE The AMIGA Sample of Isolated Galaxies XI. Optical characterization of nuclear activity. J. Sabater, L. Verdes-Montenegro, S. Leon, P. Best, J. W. Sulentic 2012 A&A 545, A.15S Note.- The Figure 5 of the paper has been corrected to include the [OI] diagnostic diagram. Links to the updated figure:[png][pdf] ASCII tables The AMIGA sample of isolated galaxies X. A First Look at Isolated Galaxy Colors. M. Fernández Lorenzo, J. Sulentic, L. Verdes-Montenegro, J.E. Ruiz, J. Sabater and S. Sánchez 2012 A&A 540, A.47 ASCII tables The AMIGA sample of isolated galaxies IX. Molecular gas properties U. Lisenfeld, D. Espada, L. Verdes-Montenegro , N. Kuno, S. Leon, J. Sabater, N. Sato, J. Sulentic, S. Verley, and M. S. Yun 2011 A&A 534, A.102 ASCII tables The AMIGA Sample of Isolated Galaxies VIII. On the rate of asymmetric HI profiles in spiral galaxies. D. Espada, L. Verdes-Montenegro, W. K. Huchtmeier, E. Garcia, R. Fisher, S. Leon, U. Lisenfeld, J. Sabater, J. W. Sulentic, and S. Verley 2011 A&A 532, A.117 ASCII tables Fourier Photometric Analysis of Isolated Galaxies in the context of AMIGA project. A. Durbala , R. Buta, J. W. Sulentic, and L. Verdes-Montenegro. 2009 Monthly Notices of the Royal Astronomical Society, 397, 1756-1775 Photometric characterization of a well defined sample of isolated galaxies in the context of the AMIGA project. A. Durbala , J. W. Sulentic, R. Buta, and L. Verdes-Montenegro. 2008 Monthly Notices of the Royal Astronomical Society, 390, 881-905 The AMIGA sample of isolated galaxies VII. Far infrared and radio continuum study of nuclear activity. J. Sabater, S. Leon, L. Verdes-Montenegro, U. Lisenfeld, J. W. Sulentic, and S. Verley. 2008 A&A 486, 73-83 ASCII tables The AMIGA sample of isolated galaxies VI. Radio continuum properties of isolated galaxies: a very radio-quiet sample. S. Leon, L. Verdes-Montenegro, J. Sabater, D. Espada, U. Lisenfeld, A. Ballu, J. W. Sulentic, S. Verley, G. Bergond, and E. García. 2008 A&A 485, 475-486 ASCII tables The AMIGA sample of isolated galaxies V. Quantification of the isolation. S. Verley, S. Leon, L. Verdes-Montenegro, F. Combes, J. Sabater, J. W. Sulentic, G. Bergond, D. Espada, E. García, U. Lisenfeld, and S. C. Odewahn. 2007 A&A 472, 121-130 ASCII tables The AMIGA sample of isolated galaxies IV. A catalogue of neighbours around isolated galaxies. S. Verley, S. C. Odewahn, L. Verdes-Montenegro, S. Leon, F. Combes, J. W. Sulentic, G. Bergond, D. Espada, E. García, U. Lisenfeld, and J. Sabater. 2007 A&A 470, 505-513 ASCII tables The AMIGA sample of isolated galaxies III. IRAS data and infrared diagnostics. U. Lisenfeld, L. Verdes-Montenegro, J. W. Sulentic, S. Leon, D. Espada, G. Bergond, E. García, J. Sabater, J.D. Santander-Vela, and S. Verley. 2007 A&A 462,507-523 ASCII tables The AMIGA sample of isolated galaxies II. Morphological refinement. J. W. Sulentic, L. Verdes-Montenegro, G. Bergond, U. Lisenfeld, A. Durbala, D. Espada, E. Garcia, S. Leon, J. Sabater, S. Verley, V. Casanova, and A. Sota. 2006 A&A 449,937-949. ASCII tables The AMIGA project I. Optical characterization of the CIG catalog. L. Verdes-Montenegro, J. W. Sulentic, U. Lisenfeld, S. Leon, D. Espada, E. Garcia, J. Sabater, and S. Verley. 2005 A&A 436,443 ASCII tables Revised positions for CIG galaxies S. Leon and L. Verdes-Montenegro 2003 A&A 411,391-395 INDIVIDUAL STUDIES OF ISOLATED GALAXIES HI asymmetry in the isolated galaxy CIG 85 (UGC 1547) C. Sengupta, T. C. Scott, L. Verdes Montenegro, A. Bosma, S. Verley, J.M. Vilchez, A. Durbala, M. Fernández Lorenzo, D. Espada, M. S. Yun, E. Athanassoula, J. Sulentic, and A. Portas. 2012 A&A 546, A95 HI asymmetries in the isolated galaxy CIG 292 A. Portas, T. C. Scott, E. Brinks, A. Bosma, L. Verdes-Montenegro, V. Heesen, D. Espada, S. Verley, J. Sulentic, C. Sengupta, E. Athanassoula, M. Yun 2011 ApJ, 739, L27 Star formation in the extended gaseous disk of the isolated galaxy CIG 96. D. Espada, J. C. Muñoz-Mateos, A. Gil de Paz, J. Sabater, L. Atthanasoula, S. Boissier, A. Bosma, S. Leon, L. Verdes-Montenegro, S. Verley, and M. Yun. 2011 ApJ, 736, 20 HCN(1-0) enhancement in the bar of NGC 2903. S. Leon, S. Jeyakumar, D. Pérez-Ramírez, L. Verdes-Montenegro, S. W. Lee, and B. Ocaña Flaquer. 2008 A&A, 491, 703-711 Star formation in isolated AMIGA galaxies: dynamical influence of bars. S. Verley, F. Combes, L. Verdes-Montenegro, G. Bergond, and S. Leon. 2007 A&A, 474, 43-53 The large asymmetric HI envelope of the isolated galaxy NGC 864 (CIG 96). D. Espada, A. Bosma, L. Verdes-Montenegro, E. Athanassoula, S. Leon, J. W. Sulentic, and M. S. Yun. 2005 A&A, 442, 455-459 DETAILED STUDIES OF COMPLEMENTARY SAMPLES AMIGA project started as a need in order to understand the effects of environment in dense environments. Hence we continue to pursue detailed studies of samples of nurture effects in groups and pairs of galaxies. Star formation, interstellar medium and nuclear activity in complementary environments Enhanced Warm H2 Emission in the Compact Group Mid-Infrared "Green Valley". M.E. Cluver, P.N. Appleton, P. Ogle, T.H. Jarrett, J. Rasmussen, U. Lisenfeld, P. Guillard, L. Verdes-Montenegro, R. Antonucci, T. Bitsakis, V. Charmandaris, F. Boulanger, E. Egami, C.K. Xu, M.S. Yun. 2013, Apj 765, 93. Seyfert’s Sextet: where is the gas? S. Tamburri, G. Trinchieri, A. Wolter, J. Sulentic, A. Durbalaand M. Rosado 2012 A&A 541, A28 Molecular gas content and SFR in Hickson Compact Groups: enhanced or deficient? V. Martinez-Badenes, U. Lisenfeld, D. Espada, L. Verdes-Montenegro, S. García-Burillo, S. Leon, J. Sulentic, and M. S. Yun 2012 A&A 540, A96 ASCII tables New insights on Stephan's Quintet: exploring the shock in three dimensions J. Iglesias-Páramo, L. López-Martín, J. M. Vílchez, V. Petropoulou, and J.W. Sulentic. 2012 A&A 539, A127 Two long H I tails in the outskirts of Abell 1367 T. C. Scott, L. Cortese, E. Brinks, H. Bravo-Alfaro, R. Auld, R. Minchin. 2012 MNRAS 419, L19 Dust Emission and Star Formation in Stephan's Quintet G. Natale, R. J. Tuffs, C. K. Xu, C. C. Popescu, J. Fischera, U. Lisenfeld, N. Lu, P. Appleton, M. Dopita, P. -A. Duc, and 4 coauthors 2010, ApJ 725, 955 Probing evolutionary mechanisms in galaxy clusters: neutral atomic hydrogen in Abell1367 T. C. Scott, H. Bravo-Alfaro, E. Brinks, C.A. Caretta, L. Cortese, A. Boselli, M.J. Hardcastle, J.H. Croston, and I. Plauchu. 2010, MNRAS 403, 1175 Quantifying the importance of ram-pressure stripping in a galaxy group at 100 Mpc E. Freeland, C. Sengupta, and J.H. Croston. 2010 MNRAS 409, 1518 The curious case of J113924.74+164144.0: a possible new group of galaxies at z = 0.069 N. Roy, C. Sengupta, and N. G. Kantharia. 2010 Monthly Notices of the Royal Astronomical Society 407, L64-L68 Detection of Diffuse Neutral Intragroup Medium in Hickson Compact Groups. S. Borthakur, M. S. Yun, and L. Verdes-Montenegro. 2010 ApJ 710, 385.Erratum. HI content and star formation in the interacting galaxy Arp86. C. Sengupta, K. S. Dwarakanath, and D. J. Saikia. 2009 Monthly Notices of the Royal Astronomical Society 397, 548 Galaxy evolution in Abell 85. I. Cluster substructure and environmental effects on the blue galaxy population. H. Bravo-Alfaro, C. A. Caretta, C. Lobo, F. Durret, and T. Scott. 2009 A&A 495, p. 379-387 Small-scale systems of galaxies. IV. Searching for the faint galaxy population associated with X-ray detected isolated E+S pairs. R. Grützbauch, W. W. Zeilinger, R. Rampazzo, E. V. Held, J. W. Sulentic, and G. Trinchieri. 2009 A&A 502, 473-498 Galaxy evolution in Hickson compact groups: the role of ram-pressure stripping and strangulation. J. Rasmussen, T. J. Ponman, L. Verdes-Montenegro, M. S. Yun, and S. Borthakur. 2008 Monthly Notices of the Royal Astronomical Society 388, 1245 Seyfert's Sextet: a Slowly Dissolving Stephan's Quintet? A. Durbala et al. 2008 AJ 135, 130 HI imaging of galaxies in X-ray bright groups. C. Sengupta, R. Balasubramanyam, and K. S. Dwarakanath 2007 Monthly Notices of the Royal Astronomical Society 378, 137 Cold and hot gas in the most HI deficient compact groups. L. Verdes-Montenegro, M. S. Yun, S. Borthakur, J. Rasmussen, and T. Ponman 2007 New Astronomy Reviews, 51, 87 HI content in galaxies in loose groups. C. Sengupta, and R. Balasubramanyam. 2006 Monthly Notices of the Royal Astronomical Society 369, 360 The evolution of HCG 31: Optical and high-resolution HI study. L. Verdes-Montenegro , A. Del Olmo, M. S. Yun, and J. Perea 2005 A&A 430, 443 Physico-chemical conditions of the molecular gas We are performing studies of the physical, chemical and dynamical state properties of both extragalactic as well as Galactic Disk and Centre chemical templates, in order to complement the study of isolated galaxies. On the nature of faint mid-infrared sources in M 33 E. Corbelli, C. Giovanardi, F. Palla, and S. Verley. 2011, A&A 528, 116 CS, HC3N and CH3CCH multi-line analyses towards starburst galaxies. The evolution of cloud structures in the central regions of galaxies. R. Aladro, J. Martín-Pintado, S. Martín, R. Mauersberger, and E. Bayet 2011, A&A 525, 89 TANGO I: ISM in nearby radio galaxies. Molecular gas. B. Ocana Flaquer, S. Leon, J. Lim, and F. Combes 2010, A&A 518, 9 Properties of compact 250 μm emission and H II regions in M 33 (HERM33ES) S. Verley et al. 2010 A&A, 518, 68 Star formation in M 33: the radial and local relations with the gas. S. Verley, E. Corbelli, C. Giovanardi, and L. K. Hunt. 2010 A&A, 518, 64 Imaging Carbon Monoxide Emission in the Starburst Galaxy NGC 6000. S. Martin, M. R. George, D. J. Wilner, and D. Espada 2010 AJ 139, 2241-2248 Star formation in M 33: multiwavelength signatures across the disk. S. Verley, E. Corbelli, C. Giovanardi, and L. K. Hunt. 2009 A&A, 493, 453 The cluster birthline in M 33. E. Corbelli, S. Verley, B. G. Elmegreen, and C. Giovanardi 2009 A&A, 495, 479-490 Interstellar medium and nuclear activity Detailed molecular gas studies of the role of molecular gas in powering radio powerful AGNs, such as the closest radio-powerful galaxy, Centaurus A (NGC5128). Disentangling the Circumnuclear Environs of Centaurus A. II. On the Nature of the Broad Absorption Line. D. Espada et al. 2010 ApJ 720, 666 Disentangling the Circumnuclear Environs of Centaurus A. I. High-Resolution Molecular Gas Imaging. D. Espada et al. 2009 ApJ 695, 116 QSOs Black hole mass (MBH) estimation provides an important comparison with AMIGA galaxies which we expect to have the smallest MBH in any sample of massive (as massive as many quasar hosts) galaxies. Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities Paola Marziani, Jack W. Sulentic, Sebastian Zamfir, C. A. Negrete, and Deborah Dultzin. 2011 BaltA 20, 472 The Case for Two Quasar Populations Jack Sulentic, Paola Marziani, and Sebastian Zamfir. 2011 BaltA 20, 427 A Photo-Ionization Method for Black Hole Mass Estimation in Quasars Paola Marziani, C. Alenka Negrete, Deborah Dultzin, and Jack W. Sulentic. 2011 BaltA 20, 406 Broad-line region physical conditions along the quasar eigenvector 1 sequence P. Marziani, J. W. Sulentic, C. A. Negrete, D. Dultzin, S. Zamfir, and R. Bachev. 2010, MNRAS 409, 1033 Detailed characterization of Hβ emission line profile in low-z SDSS quasars. S. Zamfir, J. W. Sulentic, P. Marziani, and D. Dultzin. 2010 Monthly Notices of the Royal Astronomical Society 403, 1759-1786 VLT/ISAAC spectra of the Hβ region in intermediate-redshift quasars. III. Hβ broad-line profile analysis and inferences about BLR structure. P. Marziani, J. W. Sulentic, G. M. Stirpe, S. Zamfir, and M. Calvani. 2009 A&A 495, 83-112 Comparing Hβ line profiles in the 4D Eigenvector 1 context. J. W. Sulentic, P. Marziani, and S. Zamfir. 2009 New Astronomy Reviews 53, 198-201 SOFWARE RELATED PUBLICATIONS Building a VO-compliant Radio Astronomical DAta Model for Single-dish radio telescopes. J. D. Santander-Vela, E. Garcia, S. Leon, V. Espigares, J. E. Ruiz, L. Verdes-Montenegro, and E. Solano. 2012. Accepted and published by Springer in Experimental Astronomy. TAPAS, a VO radio archive at the IRAM-30m telescope. S. Leon, V. Espigares, J.E. Ruiz, L. Verdes-Montenegro, R. Mauersberger, W. Brunswig, C. Kramer, J.D. Santander-Vela, H. Ungerechts, and H. Wiesemeyer. 2012. Accepted and published by Springer in Experimental Astronomy. Radio Astronomy Data Model for Single-Dish Multiple-Feed Instruments, and Robledo Archive Architecture J.D Santander-Vela, E. García 2007 IVOA Note January 22
HI asymmetry in the isolated galaxy CIG 85 (UGC 1547)
C. Sengupta, T. C. Scott, L. Verdes Montenegro, A. Bosma, S. Verley, J.M. Vilchez, A. Durbala,
M. Fernández Lorenzo, D. Espada, M. S. Yun, E. Athanassoula, J. Sulentic, and A. Portas.
2012 A&A 546, A95
HI asymmetries in the isolated galaxy CIG 292
A. Portas, T. C. Scott, E. Brinks, A. Bosma, L. Verdes-Montenegro, V. Heesen, D. Espada, S. Verley, J. Sulentic, C. Sengupta, E. Athanassoula, M. Yun
2011 ApJ, 739, L27
AMIGA project started as a need in order to understand the effects of environment in dense environments. Hence we continue to pursue detailed studies of samples of nurture effects in groups and pairs of galaxies.
Star formation, interstellar medium and nuclear activity in complementary environments
Physico-chemical conditions of the molecular gas
We are performing studies of the physical, chemical and dynamical state properties of both extragalactic as well as Galactic Disk and Centre chemical templates, in order to complement the study of isolated galaxies.
Interstellar medium and nuclear activity
Detailed molecular gas studies of the role of molecular gas in powering radio powerful AGNs, such as the closest radio-powerful galaxy, Centaurus A (NGC5128).
QSOs
Black hole mass (MBH) estimation provides an important comparison with AMIGA galaxies which we expect to have the smallest MBH in any sample of massive (as massive as many quasar hosts) galaxies.