Zobrazeno 1 - 10
of 617
pro vyhledávání: '"Andrianasolo A."'
Publikováno v:
Research Reports in Clinical Cardiology, Vol Volume 15, Pp 75-83 (2024)
Sitraka Angelo Raharinavalona,1 Rija Mikhaël Miandrisoa,1 Tsikinirina Valisoa Randrianomanana,2 Radonirina Lazasoa Andrianasolo,2 Andrianirina Dave Patrick Rakotomalala2 1Cardiovascular Diseases and Internal Medicine Departments, Soavinandriana Hosp
Externí odkaz:
https://doaj.org/article/1d581b2d43674994bc3d05ca1a7f7b47
Autor:
Kéruzoré F., Adam R., Ade P., André P., Andrianasolo A., Arnaud M., Aussel H., Bartalucci I., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Gomez A., Goupy J., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Mauskopf P., Mayet F., Monfardini A., Perotto L., Pisano G., Pointecouteau E., Ponthieu N., Pratt G.W., Revéret V., Ritacco A., Romero C., Roussel H., Ruppin F., Schuster K., Shu S., Sievers A., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00012 (2020)
High-resolution mapping of the hot gas in galaxy clusters is a key tool for cluster-based cosmological analyses. Taking advantage of the NIKA2 millimeter camera operated at the IRAM 30-m telescope, the NIKA2 SZ Large Program seeks to get a high-resol
Externí odkaz:
https://doaj.org/article/1b0be797f5a9465ea34409286c4f0d2a
Autor:
Mayet F., Adam R., Ade P., André P., Andrianasolo A., Arnaud M., Aussel H., Bartalucci I., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Gomez A., Goupy J., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Mauskopf P., Monfardini A., Perotto L., Pisano G., Pointecouteau E., Ponthieu N., Pratt G.W., Revéret V., Ritacco A., Romero C., Roussel H., Ruppin F., Schuster K., Shu S., Sievers A., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00017 (2020)
The main limiting factor of cosmological analyses based on thermal Sunyaev-Zel’dovich (SZ) cluster statistics comes from the bias and systematic uncertainties that affect the estimates of the mass of galaxy clusters. High-angular resolution SZ obse
Externí odkaz:
https://doaj.org/article/6b1ebc53a4f84fe383304ed37c227fc2
Autor:
Ajeddig H., Adam R., Ade P., André Ph., Andrianasolo A., Aussel H., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Gomez A., Goupy J., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Maury A., Mauskopf P., Mayet F., Monfardini A., Perotto L., Pisano G., Ponthieu N., Revéret V., Ritacco A., Romero C., Roussel H., Ruppin F., Schuster K., Shimajiri Y., Shu S., Sievers A., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00002 (2020)
Clarifying the role of magnetic fields in the star formation process is crucial. Observations have already shown that magnetic fields play an important role in the early stages of star formation. The high spatial resolution (∼0.01 to 0.05 pc) provi
Externí odkaz:
https://doaj.org/article/61ca0a7f3e6a4173869f6dcc79bd469a
Autor:
Roussel H., Ponthieu N., Adam R., Ade P., André P., Andrianasolo A., Aussel H., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E. F. C., Gomez A., Goupy J., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Mauskopf P., Mayet F., Monfardini A., Perotto L., Pisano G., Revéret V., Ritacco A., Romero C., Ruppin F., Schuster K., Shu S., Sievers A., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00024 (2020)
The steps taken to tailor to NIKA2 observations the Scanamorphos algorithm (initially developed to subtract low-frequency noise from Herschel on-the-fly observations) are described, focussing on the consequences of the different instrument architectu
Externí odkaz:
https://doaj.org/article/b10d3d78b2794ea0bf30a43e71f34fde
Autor:
Ritacco A., Adam R., Ade P., Ajeddig H., André P., Andrianasolo A., Aussel H., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Gomez A., Goupy J., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Mauskopf P., Maury A., Mayet F., Monfardini A., Perotto L., Pisano G., Ponthieu N., Revéret V., Romero C., Roussel H., Ruppin F., Schuster K., Shimajiri Y., Shu S., Sievers A., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00022 (2020)
The NIKA2 polarization channel at 260 GHz (1.15 mm) has been proposed primarily to observe galactic star-forming regions and probe the critical scales between 0.01-0.05 pc at which magnetic field lines may channel the matter of interstellar filaments
Externí odkaz:
https://doaj.org/article/ad606a2a26b04698829e078e9b4da810
Autor:
Macías-Pérez J.F., Adam R., Ade P., André P., Andrianasolo A., Aussel H., Arnaud M., Bartalucci I., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Gomez A., Goupy J., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Mauskopf P., Mayet F., Monfardini A., Perotto L., Pisano G., Pointecouteau E., Ponthieu N., Pratt G.W., Revéret V., Ritacco A., Romero C., Roussel H., Ruppin F., Schuster K., Shu S., Sievers A., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00016 (2020)
Clusters of galaxies, the largest bound objects in the Universe, constitute a cosmological probe of choice, which is sensitive to both dark matter and dark energy. Within this framework, the Sunyaev-Zel’dovich (SZ) effect has opened a new window fo
Externí odkaz:
https://doaj.org/article/b78e15360a7442b0899cb43b8d2a40ad
Autor:
Ruppin F., Adam R., Ade P., André P., Andrianasolo A., Arnaud M., Aussel H., Bartalucci I., Bautz M.W., Beelen A., Benoît A., Bideaud A., Bourrion O., Brodwin M., Calvo M., Catalano A., Comis B., Decker B., De Petris M., Désert F.-X., Doyle S., Driessen E. F. C., Eisenhardt P. R. M., Gomez A., Gonzalez A. H., Goupy J., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Mauskopf P., Mayet F., McDonald M., Monfardini A., Moravec E., Perotto L., Pisano G., Pointecouteau E., Ponthieu N., Pratt G. W., Revéret V., Ritacco A., Romero C., Roussel H., Schuster K., Shu S., Sievers A., Stanford S. A., Stern D., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00026 (2020)
We present the results of the analysis of the very massive cluster MOO J1142+1527 at a redshift z = 1.2 based on high angular resolution NIKA2 Sunyaev-Zel’dovich (SZ) and Chandra X-ray data. This multi-wavelength analysis enables us to estimate the
Externí odkaz:
https://doaj.org/article/cb316fb7863e4a43a286edff0c822152
Autor:
Lestrade J.-F., Augereau J.-C., Booth M., Adam R., Ade P., André P., Andrianasolo A., Aussel H., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Gomez A., Goupy J., Holland W., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lefèvre C., Macías-Pérez J.F., Mauskopf P., Mayet F., Monfardini A., Perotto L., Pisano G., Ponthieu N., Revéret V., Ritacco A., Romero C., Roussel H., Ruppin F., Schuster K., Shu S., Sievers A., Thébault P., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00015 (2020)
The new NIKA2 camera at the IRAM 30m radiotelescope was used to observe three known debris disks in order to constrain the SED of their dust emission in the millimeter wavelength domain. We have found that the spectral index between the two NIKA2 ban
Externí odkaz:
https://doaj.org/article/e18e5b5b94ed4ff594295df693b37299
Autor:
Ritacco A., Adam R., Ade P., André P., Andrianasolo A., Aussel H., Beelen A., Benoît A., Bideaud A., Bourrion O., Calvo M., Catalano A., Comis B., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Gomez A., Goupy J., Kéruzoré F., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Mauskopf P., Maury A., Mayet F., Monfardini A., Perotto L., Pisano G., Ponthieu N., Revéret V., Romero C., Roussel H., Ruppin F., Schuster K., Shu S., Sievers A., Tucker C., Zylka R.
Publikováno v:
EPJ Web of Conferences, Vol 228, p 00021 (2020)
We present here the polarization system of the NIKA camera and give a summary of the main results obtained and performed studies on Orion and the Crab nebula. The polarization system was equipped with a room temperature continuously rotating multi-me
Externí odkaz:
https://doaj.org/article/da46cdad57bc421aa97882af1a375013