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Search for Candidate Objects with the Sunyaev–Zeldovich Effect in the Radio Source Vicinities—galaxies: clusters: general
cosmic background radiation
A comparison of properties of different population radio galaxies based on the Planck mission microwave data
Verkhodanov O., Solovyov D., Ulakhovich O., Khabibullina M.
microwave background radiation (CMB) maps, constructed according to the Planck SpaceObservatory data
Circumzenithal sky region survey at the frequency of 30 GHz with 32-element radiometer matrix of the RATAN-600
Parijskij Y., Bursov N., Berlin A., Mingaliev M., Nizhelskij N., Stolyarov V., Tsybulev P., Semenova T., Khaikin V., Grechkin A.
of the anisotropy of background radiation at the scales of (l > 3000) and noise from discrete radio sources
A comparison of properties of different population radio galaxies based on the Planck mission microwave data
Verkhodanov O., Solovyov D., Ulakhovich O., Khabibullina M.
microwave background radiation (CMB) maps, constructed according to the Planck SpaceObservatory data
Circumzenithal sky region survey at the frequency of 30 GHz with 32-element radiometer matrix of the RATAN-600
Parijskij Y., Bursov N., Berlin A., Mingaliev M., Nizhelskij N., Stolyarov V., Tsybulev P., Semenova T., Khaikin V., Grechkin A.
of the anisotropy of background radiation at the scales of (l > 3000) and noise from discrete radio sources
Dependence of cosmic ray component in background of atmosphere surface from solar magnetic activity
Zelinskiy, A. S., Yakovlev, G. A.
with a contribution of radionuclides of the soil of flux density of secondary cosmic radiation about 0
Some remarks on topological defects and their gravitational consequences
Bezerra V., Marques G., Khusnutdinov N.
in the background spacetime of a cosmic string and we discuss the possibility that these shifts could provide a
Some remarks on topological defects and their gravitational consequences
Bezerra V., Marques G., Khusnutdinov N.
in the background spacetime of a cosmic string and we discuss the possibility that these shifts could provide a
Planck 2015 results: V. LFI calibration
Ade P., Aghanim N., Ashdown M., Aumont J., Baccigalupi C., Banday A., Barreiro R., Bartolo N., Battaglia P., Battaner E., Benabed K., Benoît A., Benoit-Lévy A., Bernard J., Bersanelli M., Bielewicz P., Bock J., Bonaldi A., Bonavera L., Bond J., Borrill J., Bouchet F., Bucher M., Burigana C., Butler R., Calabrese E., Cardoso J., Catalano A., Chamballu A., Christensen P., Colombi S., Colombo L., Crill B., Curto A., Cuttaia F., Danese L., Davies R., Davis R., De Bernardis P., De Rosa A., De Zotti G., Delabrouille J., Dickinson C., Diego J., Dole H., Donzelli S., Doré O., Douspis M., Ducout A., Dupac X., Efstathiou G., Elsner F., Enßlin T., Eriksen H., Fergusson J., Finelli F., Forni O., Frailis M., Franceschi E., Frejsel A., Galeotta S., Galli S., Ganga K., Giard M.
-synchronous modulation of the cosmic microwave background dipole, but we now use the orbital component, rather than
Planck 2015 results: I. Overview of products and scientific results
Adam R., Ade P., Aghanim N., Akrami Y., Alves M., Arguëso F., Arnaud M., Arroja F., Ashdown M., Aumont J., Baccigalupi C., Ballardini M., Banday A., Barreiro R., Bartlett J., Bartolo N., Basak S., Battaglia P., Battaner E., Battye R., Benabed K., Benoît A., Benoit-Lévy A., Bernard J., Bersanelli M., Bertincourt B., Bielewicz P., Bikmaev I., Bock J., Böhringer H., Bonaldi A., Bonavera L., Bond J., Borrill J., Bouchet F., Boulanger F., Bucher M., Burenin R., Burigana C., Butler R., Calabrese E., Cardoso J., Carvalho P., Casaponsa B., Castex G., Catalano A., Challinor A., Chamballu A., Chary R., Chiang H., Chluba J., Chon G., Christensen P., Church S., Clemens M., Clements D., Colombi S., Colombo L., Combet C., Comis B., Contreras D.
and papers. The data products include maps of the cosmic microwave background (CMB), the thermal Sunyaev

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