Zobrazeno 1 - 10
of 863
pro vyhledávání: '"Baran N."'
Autor:
Berweger, Samuel, Prajapati, Nikunjkumar, Artusio-Glimpse, Alexandra B., Rotunno, Andrew P., Brown, Roger, Holloway, Christopher L., Simons, Matthew T., Imhof, Eric, Jefferts, Steven R., Kayim, Baran N., Viray, Michael A., Wyllie, Robert, Sawyer, Brian C., Walker, Thad G.
On-resonance Rydberg atom-based radio-frequency (RF) electric field sensing methods remain limited by the narrow frequency signal detection bands available by resonant transitions. The use of an additional RF tuner field to dress or shift a target Ry
Externí odkaz:
http://arxiv.org/abs/2209.14407
Autor:
Marić, I., Dražić, G., Radin, E., Peter, R., Škrabić, M., Jurkin, T., Pustak, A., Baran, N., Mikac, L., Ivanda, M., Petravić, M., Štefanić, G., Gotić, M.
Publikováno v:
In Applied Surface Science 1 January 2023 607
Autor:
Melnyk, O., Elyiv, A., Smolcic, V., Plionis, M., Koulouridis, E., Fotopoulou, S., Chiappetti, L., Adami, C., Baran, N., Butler, A., Delhaize, J., Delvecchio, I., Finet, F., Huynh, M., Lidman, C., Pierre, M., Pompei, E., Vignali, C., Surdej, J.
Publikováno v:
A&A 620, A6 (2018)
This work is part of a series of studies focusing on the environment and the properties of the X-ray selected active galactic nuclei (AGN) population from the XXL survey. The present survey, given its large area, continuity, extensive multiwavelength
Externí odkaz:
http://arxiv.org/abs/1712.01872
Autor:
Smolcic, V., Delvecchio, I., Zamorani, G., Baran, N., Novak, M., Delhaize, J., Schinnerer, E., Berta, S., Bondi, M., Ciliegi, P., Capak, P., Civano, F., Karim, A., Fevre, O. Le, Ilbert, O., Laigle, C., Marchesi, S., McCracken, H. J., Tasca, L., Salvato, M., Vardoulaki, E.
Publikováno v:
A&A 602, A2 (2017)
(abridged) We study the composition of the faint radio population selected from the VLA-COSMOS 3GHz Large Project. The survey covers a 2.6sq.deg. area with a mean rms of ~2.3uJy/b, cataloging 10830 sources (>5sigma). Combining these radio data with o
Externí odkaz:
http://arxiv.org/abs/1703.09719
Autor:
Novak, M., Smolcic, V., Delhaize, J., Delvecchio, I., Zamorani, G., Baran, N., Bondi, M., Capak, P., Carilli, C. L., Ciliegi, P., Civano, F., Ilbert, O., Karim, A., Laigle, C., Fevre, O. Le, Marchesi, S., McCracken, H., Miettinen, O., Salvato, M., Sargent, M., Schinnerer, E., Tasca, L.
Publikováno v:
A&A 602, A5 (2017)
We make use of the deep Karl G. Jansky Very Large Array (VLA) COSMOS radio observations at 3 GHz to infer radio luminosity functions of star-forming galaxies up to redshifts of z~5 based on approximately 6000 detections with reliable optical counterp
Externí odkaz:
http://arxiv.org/abs/1703.09724
Autor:
Delvecchio, I., Smolcic, V., Zamorani, G., Lagos, C. Del P., Berta, S., Delhaize, J., Baran, N., Rosario, D. J., Gonzalez-Perez, V., Ilbert, O., Lacey, C. G., Fevre, O. Le, Miettinen, O., Alexander, D. M., Aravena, M., Bondi, M., Carilli, C., Ciliegi, P., Mooley, K., Novak, M., Schinnerer, E., Capak, P., Civano, F., Fanidakis, N., Ruiz, N. Herrera, Karim, A., Laigle, C., Marchesi, S., McCracken, H. J., Middleberg, E., Salvato, M., Tasca, L.
Publikováno v:
A&A 602, A3 (2017)
We explore the multiwavelength properties of AGN host galaxies for different classes of radio-selected AGN out to z$\lesssim$6 via a multiwavelength analysis of about 7700 radio sources in the COSMOS field. The sources were selected with the Very Lar
Externí odkaz:
http://arxiv.org/abs/1703.09720
Autor:
Delhaize, J., Smolcic, V., Delvecchio, I., Novak, M., Sargent, M., Baran, N., Magnelli, B., Zamorani, G., Schinnerer, E., Murphy, E. J., Aravena, M., Berta, S., Bondi, M., Capak, P., Ciliegi, P., Civano, F., Ilbert, O., Karim, A., Laigle, C., Fevre, O. Le, Marchesi, S., McCracken, H. J., Salvato, M., Seymour, N., Tasca, L.
Publikováno v:
A&A 602, A4 (2017)
We examine the behaviour of the infrared-radio correlation (IRRC) over the range $0
Externí odkaz:
http://arxiv.org/abs/1703.09723
Autor:
Smolcic, V., Novak, M., Bondi, M., Ciliegi, P., Mooley, K. P., Schinnerer, E., Zamorani, G., Navarrete, F., Bourke, S., Karim, A., Vardoulaki, E., Leslie, S., Delhaize, J., Carilli, C. L., Myers, S. T., Baran, N., Delvecchio, I., Miettinen, O., Banfield, J., Balokovic, M., Bertoldi, F., Capak, P., Frail, D. A., Hallinan, G., Hao, H., Ruiz, N. Herrera, Horesh, A., Ilbert, O., Intema, H., Jelic, V., Kloeckner, H. R., Krpan, J., Kulkarni, S. R., McCracken, H., Laigle, C., Middleberg, E., Murphy, E. J., Sargent, M., Scoville, N. Z., Sheth, K.
We present the VLA-COSMOS 3 GHz Large Project based on 384 hours of observations with the Karl G. Jansky Very Large Array (VLA) at 3 GHz (10 cm) toward the two square degree Cosmic Evolution Survey (COSMOS) field. The final mosaic reaches a median rm
Externí odkaz:
http://arxiv.org/abs/1703.09713
Autor:
Rotunno, Andrew P., Holloway, Christopher L., Prajapati, Nikunjkumar, Berweger, Samuel, Artusio-Glimpse, Alexandra B., Brown, Roger, Simons, Matthew, Robinson, Amy K., Kayim, Baran N., Viray, Michael A., Jones, Jasmine F., Sawyer, Brian C., Wyllie, Robert, Walker, Thad, Ziolkowski, Richard W., Jefferts, Steven R., Geibel, Steven, Wheeler, Jonathan, Imhof, Eric
Publikováno v:
Journal of Applied Physics; 8/28/2023, Vol. 134 Issue 8, p1-14, 14p
Autor:
Pierre, M., Adami, C., Birkinshaw, M., Chiappetti, L., Ettori, S., Evrard, A., Faccioli, L., Gastaldello, F., Giles, P., Horellou, C., Iovino, A., Koulouridis, E., Lidman, C., Brun, A. Le, Maughan, B., Maurogordato, S., McCarthy, I., Miyazaki, S., Pacaud, F., Paltani, S., Plionis, M., Reiprich, T., Sadibekova, T., Smolcic, V., Snowden, S., Surdej, J., Tsirou, M., Vignali, C., Willis, J., Alis, S., Altieri, B., Baran, N., Benoist, C., Bongiorno, A., Bremer, M., Butler, A., Cappi, A., Caretta, C., Ciliegi, P., Clerc, N., Corasaniti, P. S., Coupon, J., Delhaize, J., Delvecchio, I., Democles, J., Desai, Sh., Devriendt, J., Dubois, Y., Eckert, D., Elyiv, A., Farahi, A., Ferrari, C., Fotopoulou, S., Forman, W., Georgantopoulos, I., Guglielmo, V., Huynh, M., Jerlin, N., Jones, Ch., Lavoie, S., Fevre, J. -P. Le, Lieu, M., Kilbinger, M., Marulli, F., Mantz, A., McGee, S., Melin, J. -B., Melnyk, O., Moscardini, L., Novak, M., Piconcelli, E., Poggianti, B., Pomarede, D., Pompei, E., Ponman, T., Ceja, M. E. Ramos, Ranalli, P., Rapetti, D., Raychaudhury, S., Ricci, M., Rottgering, H., Sahlén, M., Sauvageot, J. -L., Schimd, C., Sereno, M., Smith, G. P., Umetsu, K., Valageas, P., Valotti, A., Valtchanov, I., Veropalumbo, A., Ascaso, B., Barnes, D., De Petris, M., Durret, F., Donahue, M., Ithana, M., Jarvis, M., Johnston-Hollitt, M., Kalfountzou, E., Kay, S., La Franca, F., Okabe, N., Muzzin, A., Rettura, A., Ricci, F., Ridl, J., Risaliti, G., Takizawa, M., Thomas, P., Truong, N.
Publikováno v:
Astronomische Nachrichten, 2017 AN 338, 334
The XXL survey currently covers two 25 sq. deg. patches with XMM observations of ~10ks. We summarise the scientific results associated with the first release of the XXL data set, that occurred mid 2016. We review several arguments for increasing the
Externí odkaz:
http://arxiv.org/abs/1610.01781