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Monocyte chemoattractant protein-1 serum levels in ovarian cancer patients
Hefler L, Tempfer C, Heinze G, Mayerhofer K, Breitenecker G, Leodolter S, Reinthaller A, Kainz C
regression models revealed a significant influence of MCP-1 serum levels on the odds of presenting
The 72-h WEBT microvariability observation of blazar S5 0716 + 714 in 2009
Bhatta G., Webb J., Hollingsworth H., Dhalla S., Khanuja A., Bachev R., Blinov D., Bottcher M., Bravo Calle O., Calcidese P., Capezzali D., Carosati D., Chigladze R., Collins A., Coloma J., Efimov Y., Gupta A., Hu S., Kurtanidze O., Lamerato A., Larionov V., Lee C., Lindfors E., Murphy B., Nilsson K., Ohlert J., Oksanen A., Pääkkönen P., Pollock J., Rani B., Reinthal R., Rodriguez D., Ros J., Roustazadeh P., Sagar R., Sanchez A., Shastri P., Sillanpää A., Strigachev A., Takalo L., Vennes S., Villata M., Villforth C., Wu J., Zhou X.
the Blazar showed almost constant variability over a 0.5 mag range. The resulting light curve is presented
The 72-h WEBT microvariability observation of blazar S5 0716 + 714 in 2009
Bhatta G., Webb J., Hollingsworth H., Dhalla S., Khanuja A., Bachev R., Blinov D., Bottcher M., Bravo Calle O., Calcidese P., Capezzali D., Carosati D., Chigladze R., Collins A., Coloma J., Efimov Y., Gupta A., Hu S., Kurtanidze O., Lamerato A., Larionov V., Lee C., Lindfors E., Murphy B., Nilsson K., Ohlert J., Oksanen A., Pääkkönen P., Pollock J., Rani B., Reinthal R., Rodriguez D., Ros J., Roustazadeh P., Sagar R., Sanchez A., Shastri P., Sillanpää A., Strigachev A., Takalo L., Vennes S., Villata M., Villforth C., Wu J., Zhou X.
the Blazar showed almost constant variability over a 0.5 mag range. The resulting light curve is presented
Stochastic Modeling of Multiwavelength Variability of the Classical BL Lac Object OJ 287 on Timescales Ranging from Decades to Hours
Goyal A., Stawarz, Zola S., Marchenko V., Soida M., Nilsson K., Ciprini S., Baran A., Ostrowski M., Wiita P., Gopal-Krishna, Siemiginowska A., Sobolewska M., Jorstad S., Marscher A., Aller M., Aller H., Hovatta T., Caton D., Reichart D., Matsumoto K., Sadakane K., Gazeas K., Kidger M., Piirola V., Jermak H., Alicavus F., Baliyan K., Baransky A., Berdyugin A., Blay P., Boumis P., Boyd D., Bufan Y., Torrent M., Campos F., Gómez J., Dalessio J., Debski B., Dimitrov D., Drozdz M., Er H., Erdem A., Pérez A., Ramazani V., Filippenko A., Gafton E., Garcia F., Godunova V., Pinilla F., Gopinathan M., Haislip J., Haque S., Harmanen J., Hudec R., Hurst G., Ivarsen K., Joshi A., Kagitani M., Karaman N., Karjalainen R., Kaur N., Kozieł-Wierzbowska D., Kuligowska E., Kundera T., Kurowski S., Kvammen A., Lacluyze A., Lee B., Liakos A., Haro J., Moore J., Mugrauer M., Nogues R., Neely A., Ogloza W., Okano S., Pajdosz U., Pandey J., Perri M., Poyner G., Provencal J., Pursimo T., Raj A., Rajkumar B., Reinthal R., Reynolds T., Saario J., Sadegi S.
to construct for the first time the optical variability power spectrum of a blazar without any gaps across ∼6
Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using Its General Relativity Centenary Flare: Improved Orbital Parameters
Dey L., Valtonen M., Gopakumar A., Zola S., Hudec R., Pihajoki P., Ciprini S., Matsumoto K., Sadakane K., Kidger M., Nilsson K., Mikkola S., Sillanpää A., Takalo L., Lehto H., Berdyugin A., Piirola V., Jermak H., Baliyan K., Pursimo T., Caton D., Alicavus F., Baransky A., Blay P., Boumis P., Boyd D., Torrent M., Campos F., Gómez J., Chandra S., Chavushyan V., Dalessio J., Debski B., Drozdz M., Er H., Erdem A., Pérez A., Ramazani V., Filippenko A., Gafton E., Ganesh S., Garcia F., Gazeas K., Godunova V., Pinilla F., Gopinathan M., Haislip J., Harmanen J., Hurst G., Janík J., Jelinek M., Joshi A., Kagitani M., Karjalainen R., Kaur N., Keel W., Kouprianov V., Kundera T., Kurowski S., Kvammen A., Lacluyze A., Lee B., Liakos A., Lindfors E., De Haro J., Mugrauer M., Nogues R., Neely A., Nelson R., Ogloza W., Okano S., Pajdosz-Śmierciak U., Pandey J., Perri M., Poyner G., Provencal J., Raj A., Reichart D., Reinthal R., Reynolds T., Saario J., Sadegi S., Sakanoi T., González J., Sameer, Schweyer T., Simon A.
of the predicted 2019 impact flare should allow a test of the celebrated black hole "no-hair theorem" at the 10
Polarization angle swings in blazars: The case of 3C 279
Kiehlmann S., Savolainen T., Jorstad S., Sokolovsky K., Schinzel F., Marscher A., Larionov V., Agudo I., Akitaya H., Benítez E., Berdyugin A., Blinov D., Bochkarev N., Borman G., Burenkov A., Casadio C., Doroshenko V., Efimova N., Fukazawa Y., Gómez J., Grishina T., Hagen-Thorn V., Heidt J., Hiriart D., Itoh R., Joshi M., Kawabata K., Kimeridze G., Kopatskaya E., Korobtsev I., Krajci T., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Lindfors E., López J., McHardy I., Molina S., Moritani Y., Morozova D., Nazarov S., Nikolashvili M., Nilsson K., Pulatova N., Reinthal R., Sadun A., Sasada M., Savchenko S., Sergeev S., Sigua L., Smith P., Sorcia M., Spiridonova O., Takaki K., Takalo L., Taylor B., Troitsky I., Uemura M., Ugolkova L., Ui T., Yoshida M., Zensus J., Zhdanova V.
this behaviour. Aims. Our goal is to study the observed EVPA rotations and to distinguish between a stochastic
Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies
Raiteri C., Villata M., Smith P., Larionov V., Acosta-Pulido J., Aller M., D'Ammando F., Gurwell M., Jorstad S., Joshi M., Kurtanidze O., Lähteenmäki A., Mirzaqulov D., Agudo I., Aller H., Arévalo M., Arkharov A., Bach U., Benítez E., Berdyugin A., Blinov D., Blumenthal K., Buemi C., Bueno A., Carleton T., Carnerero M., Carosati D., Casadio C., Chen W., Di Paola A., Dolci M., Efimova N., Ehgamberdiev S., Gómez J., González A., Hagen-Thorn V., Heidt J., Hiriart D., Holikov S., Konstantinova T., Kopatskaya E., Koptelova E., Kurtanidze S., Larionova E., Larionova L., León-Tavares J., Leto P., Lin H., Lindfors E., Marscher A., McHardy I., Molina S., Morozova D., Mujica R., Nikolashvili M., Nilsson K., Ovcharov E., Panwar N., Pasanen M., Puerto-Gimenez I., Reinthal R., Richter G., Ros J., Sakamoto T., Schwartz R., Sillanpää A., Smith N., Takalo L., Tammi J., Taylor B., Thum C., Tornikoski M., Trigilio C., Troitsky I., Umana G., Valcheva A., Wehrle A.
+382) experienced a large outburst in 2011, which was detected throughout the entire electromagnetic spectrum
Polarization angle swings in blazars: The case of 3C 279
Kiehlmann S., Savolainen T., Jorstad S., Sokolovsky K., Schinzel F., Marscher A., Larionov V., Agudo I., Akitaya H., Benítez E., Berdyugin A., Blinov D., Bochkarev N., Borman G., Burenkov A., Casadio C., Doroshenko V., Efimova N., Fukazawa Y., Gómez J., Grishina T., Hagen-Thorn V., Heidt J., Hiriart D., Itoh R., Joshi M., Kawabata K., Kimeridze G., Kopatskaya E., Korobtsev I., Krajci T., Kurtanidze O., Kurtanidze S., Larionova E., Larionova L., Lindfors E., López J., McHardy I., Molina S., Moritani Y., Morozova D., Nazarov S., Nikolashvili M., Nilsson K., Pulatova N., Reinthal R., Sadun A., Sasada M., Savchenko S., Sergeev S., Sigua L., Smith P., Sorcia M., Spiridonova O., Takaki K., Takalo L., Taylor B., Troitsky I., Uemura M., Ugolkova L., Ui T., Yoshida M., Zensus J., Zhdanova V.
this behaviour. Aims. Our goal is to study the observed EVPA rotations and to distinguish between a stochastic
Variability of the blazar 4C 38.41 (B3 1633+382) from GHz frequencies to GeV energies
Raiteri C., Villata M., Smith P., Larionov V., Acosta-Pulido J., Aller M., D'Ammando F., Gurwell M., Jorstad S., Joshi M., Kurtanidze O., Lähteenmäki A., Mirzaqulov D., Agudo I., Aller H., Arévalo M., Arkharov A., Bach U., Benítez E., Berdyugin A., Blinov D., Blumenthal K., Buemi C., Bueno A., Carleton T., Carnerero M., Carosati D., Casadio C., Chen W., Di Paola A., Dolci M., Efimova N., Ehgamberdiev S., Gómez J., González A., Hagen-Thorn V., Heidt J., Hiriart D., Holikov S., Konstantinova T., Kopatskaya E., Koptelova E., Kurtanidze S., Larionova E., Larionova L., León-Tavares J., Leto P., Lin H., Lindfors E., Marscher A., McHardy I., Molina S., Morozova D., Mujica R., Nikolashvili M., Nilsson K., Ovcharov E., Panwar N., Pasanen M., Puerto-Gimenez I., Reinthal R., Richter G., Ros J., Sakamoto T., Schwartz R., Sillanpää A., Smith N., Takalo L., Tammi J., Taylor B., Thum C., Tornikoski M., Trigilio C., Troitsky I., Umana G., Valcheva A., Wehrle A.
+382) experienced a large outburst in 2011, which was detected throughout the entire electromagnetic spectrum
Impaired vocal communication, sleep-related discharges, and transient alteration of slow-wave sleep in developing mice lacking the GluN2A subunit of N-methyl-d-aspartate receptors
Salmi M., Del Gallo F., Minlebaev M., Zakharov A., Pauly V., Perron P., Pons-Bennaceur A., Corby-Pellegrino S., Aniksztejn L., Lenck-Santini P., Epsztein J., Khazipov R., Burnashev N., Bertini G., Szepetowski P.
-methyl-d-aspartate receptors (NMDARs) are instrumental to brain development and functioning. Defects in the GRIN2A gene

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