Zobrazeno 1 - 10
of 386
pro vyhledávání: '"Circosta P"'
Autor:
Pucha, Ragadeepika, Juneau, S., Dey, Arjun, Siudek, M., Mezcua, M., Moustakas, J., BenZvi, S., Hainline, K., Hviding, R., Mao, Yao-Yuan, Alexander, D. M., Alfarsy, R., Circosta, C., Guo, Wei-Jian, Manwadkar, V., Martini, P., Weaver, B. A., Aguilar, J., Ahlen, S., Bianchi, D., Brooks, D., Canning, R., Claybaugh, T., Dawson, K., de la Macorra, A., Dey, Biprateep, Doel, P., Font-Ribera, A., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Gutierrez, G., Honscheid, K., Kehoe, R., Koposov, S. E., Lambert, A., Landriau, M., Guillou, L. Le, Meisner, A., Miquel, R., Prada, F., Rossi, G., Sanchez, E., Schlegel, D., Schubnell, M., Seo, H., Sprayberry, D., Tarlé, G., Zou, H.
Using early data from the Dark Energy Spectroscopic Instrument (DESI) survey, we search for AGN signatures in 410,757 line-emitting galaxies. By employing the BPT emission-line ratio diagnostic diagram, we identify AGN in 75,928/296,261 ($\approx$25.
Externí odkaz:
http://arxiv.org/abs/2411.00091
Autor:
Siudek, M., Pucha, R., Mezcua, M., Juneau, S., Aguilar, J., Ahlen, S., Brooks, D., Circosta, C., Claybaugh, T., Cole, S., Dawson, K., de la Macorra, A., Dey, Arjun, Dey, Biprateep, Doel, P., Font-Ribera, A., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Gutierrez, G., Honscheid, K., Howlett, C., Ishak, M., Kehoe, R., Kirkby, D., Kisner, T., Kremin, A., Lambert, A., Landriau, M., Guillou, L. Le, Manera, M., Martini, P., Meisner, A., Miquel, R., Moustakas, J., Newman, J. A., Niz, G., Pan, Z., Percival, W. J., Poppett, C., Prada, F., Rossi, G., Saintonge, A., Sanchez, E., Schlegel, D., Scholte, D., Schubnell, M., Seo, H., Speranza, F., Sprayberry, D., Tarle, G., Weaver, B. A., Zou, H.
Aims. We present an extensive catalog of the physical properties of more than a million galaxies within the Dark Energy Spectroscopic Instrument (DESI), one of the largest spectroscopic surveys to date. Spanning over a full variety of target types, i
Externí odkaz:
http://arxiv.org/abs/2409.19066
Autor:
Sun, Yang, Lyu, Jianwei, Rieke, George H., Ji, Zhiyuan, Sun, Fengwu, Zhu, Yongda, Bunker, Andrew J., Cargile, Phillip A., Circosta, Chiara, D'Eugenio, Francesco, Egami, Eiichi, Hainline, Kevin, Helton, Jakob M., Rinaldi, Pierluigi, Robertson, Brant E., Scholtz, Jan, Shivaei, Irene, Stone, Meredith A., Tacchella, Sandro, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris
Over the past two decades, tight correlations between black hole masses ($M_\bullet$) and their host galaxy properties have been firmly established at low-$z$ ($z<1$), indicating coevolution of supermassive black holes and galaxies. However, the situ
Externí odkaz:
http://arxiv.org/abs/2409.06796
Autor:
Bertola, E., Circosta, C., Ginolfi, M., Mainieri, V., Vignali, C., Rivera, G. Calistro, Ward, S. R., Lopez, I. E., Pensabene, A., Alexander, D. M., Bischetti, M., Brusa, M., Cappi, M., Comastri, A., Contursi, A., Cicone, C., Cresci, G., Dadina, M., D'Amato, Q., Feltre, A., Harrison, C. M., Kakkad, D., Lamperti, I., Lanzuisi, G., Mannucci, F., Marconi, A., Perna, M., Piconcelli, E., Puglisi, A., Ricci, F., Scholtz, J., Tozzi, G., Vietri, G., Zamorani, G., Zappacosta, L.
The energy released by AGN has the potential to heat or remove the gas of the ISM, thus likely impacting the cold molecular gas reservoir of host galaxies at first, with star formation following on longer timescales. Previous works on high-z galaxies
Externí odkaz:
http://arxiv.org/abs/2408.16821
Autor:
Scholte, D., Saintonge, A., Moustakas, J., Catinella, B., Zou, H., Dey, B., Aguilar, J., Ahlen, S., Anand, A., Blum, R., Brooks, D., Circosta, C., Claybaugh, T., de la Macorra, A., Doel, P., Font-Ribera, A., Förster, P. U., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Juneau, S., Kehoe, R., Kisner, T., Koposov, S. E., Kremin, A., Lambert, A., Landriau, M., Maraston, C., Martini, P., Meisner, A., Mighty, A. S., Miquel, R., Myers, A. D., Nie, J., Poppett, C., Prada, F., Rezaie, M., Rossi, G., Sanchez, E., Schubnell, M., Silber, J., Sprayberry, D., Siudek, M., Speranza, F., Tarlé, G., Weaver, B. A.
Galaxy scaling relations provide insights into the processes that drive galaxy evolution. The extension of these scaling relations into the dwarf galaxy regime is of particular interest. This is because dwarf galaxies represent a crucial stage in gal
Externí odkaz:
http://arxiv.org/abs/2408.03996
Autor:
Tozzi, G., Cresci, G., Perna, M., Mainieri, V., Mannucci, F., Marconi, A., Kakkad, D., Marasco, A., Brusa, M., Bertola, E., Bischetti, M., Carniani, S., Cicone, C., Circosta, C., Fiore, F., Feruglio, C., Harrison, C. M., Lamperti, I., Netzer, H., Piconcelli, E., Puglisi, A., Scholtz, J., Vietri, G., Vignali, C., Zamorani, G.
Publikováno v:
A&A 690, A141 (2024)
We present spatially resolved VLT/SINFONI spectroscopy with adaptive optics of type-2 active galactic nuclei (AGN) from the SINFONI Survey for Unveiling the Physics and Effect of Radiative feedback (SUPER), which targeted X-ray bright ($L_{2-10 keV}\
Externí odkaz:
http://arxiv.org/abs/2407.04099
Autor:
Lamperti, Isabella, Arribas, Santiago, Perna, Michele, Del Pino, Bruno Rodríguez, Circosta, Chiara, Pérez-González, Pablo G., Bunker, Andrew J., Carniani, Stefano, Charlot, Stéphane, D'Eugenio, Francesco, Maiolino, Roberto, Übler, Hannah, Willott, Chris J., Bertola, Elena, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Jones, Gareth C., Kumari, Nimisha, Parlanti, Eleonora, Scholtz, Jan, Venturi, Giacomo
We present JWST NIRSpec observations in IFS mode of the galaxy GS5001 at redshift z=3.47, the brightest member of a candidate protocluster in the GOODS-S field. The data cover a field of view (FoV) of 4''$\times$4'' (~$30\times30$~kpc$^2$) and were o
Externí odkaz:
http://arxiv.org/abs/2406.10348
Autor:
Scholtz, Jan, D'Eugenio, Francesco, Maiolino, Roberto, Pérez-González, Pablo G., Circosta, Chiara, Tacchella, Sandro, Williams, Christina C., Alberts, Stacey, Arribas, Santiago, Baker, William M., Bertola, Elena, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Cresci, Giovanni, Jones, Gareth C., Kumari, Nimisha, Lamperti, Isabella, Looser, Tobias J., Del Pino, Bruno Rodríguez, Robertson, Brant, Parlanti, Eleonora, Perna, Michele, Übler, Hannah, Venturi, Giacomo, Witstok, Joris
JWST is discovering increasing numbers of quiescent galaxies 1--2 billion years after the Big Bang, whose redshift, high mass, and old stellar ages indicate that their formation and quenching were surprisingly rapid. This fast-paced evolution seems t
Externí odkaz:
http://arxiv.org/abs/2405.19401
Autor:
Juneau, S., Canning, R., Alexander, D. M., Pucha, R., Fawcett, V. A., Myers, A. D., Moustakas, J., Ruiz-Macias, O., Cole, S., Pan, Z., Aguilar, J., Ahlen, S., Alam, S., Bailey, S., Brooks, D., Chaussidon, E., Circosta, C., Claybaugh, T., Dawson, K., de la Macorra, A., Dey, Arjun, Doel, P., Fanning, K., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Gutierrez, G., Hahn, C., Honscheid, K., Kehoe, R., Kisner, T., Kremin, A., Lambert, A., Landriau, M., Guillou, L. Le, Manera, M., Martini, P., Meisner, A., Miquel, R., Muñoz-Gutiérrez, A., Nie, J., Palanque-Delabrouille, N., Percival, W. J., Poppett, C., Prada, F., Ravoux, C., Rezaie, M., Rossi, G., Sanchez, E., Schlafly, E. F., Schlegel, D., Schubnell, M., Seo, H., Silber, J., Siudek, M., Sprayberry, D., Tarlé, G., Zhou, Z., Zou, H.
The Dark Energy Spectroscopic Instrument (DESI) cosmology survey includes a Bright Galaxy Survey (BGS) which will yield spectra for over ten million bright galaxies (r<20.2 AB mag). The resulting sample will be valuable for both cosmological and astr
Externí odkaz:
http://arxiv.org/abs/2404.03621
Autor:
Arribas, Santiago, Perna, Michele, Del Pino, Bruno Rodríguez, Lamperti, Isabella, D'Eugenio, Francesco, Pérez-González, Pablo G., Jones, Gareth C., Crespo, Alejandro, Curti, Mirko, Lim, Seunghwan, Álvarez-Márquez, Javier, Bunker, Andrew J., Carniani, Stefano, Charlot, Stéphane, Jakobsen, Peter, Maiolino, Roberto, Übler, Hannah, Willott, Chris J., Böker, Torsten, Chevallard, Jacopo, Circosta, Chiara, Cresci, Giovanni, Kumari, Nimisha, Parlanti, Eleonora, Scholtz, Jan, Venturi, Giacomo, Witstok, Joris
Publikováno v:
A&A 688, A146 (2024)
The SPT0311-58 system resides in a massive dark matter halo at z ~ 6.9. It hosts two dusty galaxies (E and W) with a combined star formation rate of ~3500 Msun/yr. Its surrounding field exhibits an overdensity of sub-mm sources, making it a candidate
Externí odkaz:
http://arxiv.org/abs/2312.00899