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Quantum Gravity without Quantization
Ivanov, M. A.
the classical model, but by introducing a graviton background, which has a low temperature but strongly
Three Different Effects of the Same Quantum Nature
Ivanov, M. A., Иванов, М. А.
of the background. A tentative detection of a diffuse cosmic optical background by the New Horizons mission may
The quantum nature of gravity seen in cosmological observations
Ivanov, M. A., Иванов, М. А.
darkening of distant objects and a diffuse cosmic optical background, presumably detected by the New
Planck intermediate results: XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect
Ade P., Aghanim N., Arnaud M., Ashdown M., Aubourg E., Aumont J., Baccigalupi C., Banday A., Barreiro R., Bartolo N., Battaner E., Benabed K., Benoit-Lévy A., Bersanelli M., Bielewicz P., Bock J., Bonaldi A., Bonavera L., Bond J., Borrill J., Bouchet F., Burigana C., Calabrese E., Cardoso J., Catalano A., Chamballu A., Chiang H., Christensen P., Clements D., Colombo L., Combet C., Crill B., Curto A., Cuttaia F., Danese L., Davies R., Davis R., De Bernardis P., De Zotti G., Delabrouille J., Dickinson C., Diego J., Dolag K., Donzelli S., Doré O., Douspis M., Ducout A., Dupac X., Efstathiou G., Elsner F., Enßlin T., Eriksen H., Finelli F., Forni O., Frailis M., Fraisse A., Franceschi E., Frejsel A., Galeotta S., Galli S., Ganga K., Génova-Santos R., Giard M., Gjerløw E.
as an effective optical depth to Thomson scattering. We find τT = (1.4 ± 0.5) × 10-4; the simplest interpretation
Planck intermediate results: XXXVII. Evidence of unbound gas from the kinetic Sunyaev-Zeldovich effect
Ade P., Aghanim N., Arnaud M., Ashdown M., Aubourg E., Aumont J., Baccigalupi C., Banday A., Barreiro R., Bartolo N., Battaner E., Benabed K., Benoit-Lévy A., Bersanelli M., Bielewicz P., Bock J., Bonaldi A., Bonavera L., Bond J., Borrill J., Bouchet F., Burigana C., Calabrese E., Cardoso J., Catalano A., Chamballu A., Chiang H., Christensen P., Clements D., Colombo L., Combet C., Crill B., Curto A., Cuttaia F., Danese L., Davies R., Davis R., De Bernardis P., De Zotti G., Delabrouille J., Dickinson C., Diego J., Dolag K., Donzelli S., Doré O., Douspis M., Ducout A., Dupac X., Efstathiou G., Elsner F., Enßlin T., Eriksen H., Finelli F., Forni O., Frailis M., Fraisse A., Franceschi E., Frejsel A., Galeotta S., Galli S., Ganga K., Génova-Santos R., Giard M., Gjerløw E.
as an effective optical depth to Thomson scattering. We find τT = (1.4 ± 0.5) × 10-4; the simplest interpretation
Planck 2015 results: X. Diffuse component separation: Foreground maps
Adam R., Ade P., Aghanim N., Alves M., Arnaud M., Ashdown M., Aumont J., Baccigalupi C., Banday A., Barreiro R., Bartlett J., Bartolo N., 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., Boulanger F., Bucher M., Burigana C., Butler R., Calabrese E., Cardoso J., Catalano A., Challinor A., Chamballu A., Chary R., Chiang H., Christensen P., Clements D., Colombi S., Colombo L., Combet C., Couchot F., Coulais A., Crill B., Curto A., Cuttaia F., Danese L., Davies R., Davis R., De Bernardis P., De Rosa A., De Zotti G., Delabrouille J., Désert F., Dickinson C., Diego J., Dole H., Donzelli S., Doré O., Douspis M., Ducout A., Dupac X., Efstathiou G.
maps. Component separation dedicated to cosmic microwave background (CMB) reconstruction is described
LONG-TERM RESULTS OF PERCUTANEOUS CORONARY INTERVENTIONS IN PATIENTS WITH DIFFUSE AND MULTIVESSEL CORONARY ARTERY DISEASES; [ОТДАЛЕННЫЕ РЕЗУЛЬТАТЫ ЧРЕСКОЖНЫХ КОРОНАРНЫХ ВМЕШАТЕЛЬСТВ У ПАЦИЕНТОВ С ДИФФУЗНЫМ И МНОГОСОСУДИСТЫМ ПОРАЖЕНИЕМ КОРОНАРНЫХ АРТЕРИЙ]
Maximkin D.A., Bolivogui J.M., Shugushev Z.Kh., Faybushevich A.G., Chepurnoy A.G., Gitelzon E.A.
) in diffusely altered arteries was performed against the background of maximum hyperemia between stenoses
Planck 2015 results: IX. Diffuse component separation: CMB maps
Adam R., Ade P., Aghanim N., Arnaud M., Ashdown M., Aumont J., Baccigalupi C., Banday A., Barreiro R., Bartlett J., Bartolo N., Basak S., 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., Boulanger F., Bucher M., Burigana C., Butler R., Calabrese E., Cardoso J., Casaponsa B., Castex G., Catalano A., Challinor A., Chamballu A., Chary R., Chiang H., Christensen P., Clements D., Colombi S., Colombo L., Combet C., Couchot F., Coulais A., Crill B., Curto A., Cuttaia F., Danese L., Davies R., Davis R., De Bernardis P., De Rosa A., De Zotti G., Delabrouille J., Désert F., Dickinson C., Diego J., Dole H., Donzelli S., Doré O., Douspis M., Ducout A., Dupac X., Efstathiou G.
© ESO, 2016.We present foreground-reduced cosmic microwave background (CMB) maps derived from
Search for Candidate Objects with the Sunyaev–Zeldovich Effect in the Radio Source Vicinities—galaxies: clusters: general
cosmic background radiation
Planck 2015 results: X. Diffuse component separation: Foreground maps
Adam R., Ade P., Aghanim N., Alves M., Arnaud M., Ashdown M., Aumont J., Baccigalupi C., Banday A., Barreiro R., Bartlett J., Bartolo N., 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., Boulanger F., Bucher M., Burigana C., Butler R., Calabrese E., Cardoso J., Catalano A., Challinor A., Chamballu A., Chary R., Chiang H., Christensen P., Clements D., Colombi S., Colombo L., Combet C., Couchot F., Coulais A., Crill B., Curto A., Cuttaia F., Danese L., Davies R., Davis R., De Bernardis P., De Rosa A., De Zotti G., Delabrouille J., Désert F., Dickinson C., Diego J., Dole H., Donzelli S., Doré O., Douspis M., Ducout A., Dupac X., Efstathiou G.
maps. Component separation dedicated to cosmic microwave background (CMB) reconstruction is described

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