%0 Generic %1 qu2023atacama %A Qu, Frank J. %A Sherwin, Blake D. %A Madhavacheril, Mathew S. %A Han, Dongwon %A Crowley, Kevin T. %A Abril-Cabezas, Irene %A Ade, Peter A. R. %A Aiola, Simone %A Alford, Tommy %A Amiri, Mandana %A Amodeo, Stefania %A An, Rui %A Atkins, Zachary %A Austermann, Jason E. %A Battaglia, Nicholas %A Battistelli, Elia Stefano %A Beall, James A. %A Bean, Rachel %A Beringue, Benjamin %A Bhandarkar, Tanay %A Biermann, Emily %A Bolliet, Boris %A Bond, J Richard %A Cai, Hongbo %A Calabrese, Erminia %A Calafut, Victoria %A Capalbo, Valentina %A Carrero, Felipe %A Carron, Julien %A Challinor, Anthony %A Chesmore, Grace E. %A Cho, Hsiao-mei %A Choi, Steve K. %A Clark, Susan E. %A Rosado, Rodrigo Córdova %A Cothard, Nicholas F. %A Coughlin, Kevin %A Coulton, William %A Dalal, Roohi %A Darwish, Omar %A Devlin, Mark J. %A Dicker, Simon %A Doze, Peter %A Duell, Cody J. %A Duff, Shannon M. %A Duivenvoorden, Adriaan J. %A Dunkley, Jo %A Dünner, Rolando %A Fanfani, Valentina %A Fankhanel, Max %A Farren, Gerrit %A Ferraro, Simone %A Freundt, Rodrigo %A Fuzia, Brittany %A Gallardo, Patricio A. %A Garrido, Xavier %A Gluscevic, Vera %A Golec, Joseph E. %A Guan, Yilun %A Halpern, Mark %A Harrison, Ian %A Hasselfield, Matthew %A Healy, Erin %A Henderson, Shawn %A Hensley, Brandon %A Hervías-Caimapo, Carlos %A Hill, J. Colin %A Hilton, Gene C. %A Hilton, Matt %A Hincks, Adam D. %A Hložek, Renée %A Ho, Shuay-Pwu Patty %A Huber, Zachary B. %A Hubmayr, Johannes %A Huffenberger, Kevin M. %A Hughes, John P. %A Irwin, Kent %A Isopi, Giovanni %A Jense, Hidde T. %A Keller, Ben %A Kim, Joshua %A Knowles, Kenda %A Koopman, Brian J. %A Kosowsky, Arthur %A Kramer, Darby %A Kusiak, Aleksandra %A La Posta, Adrien %A Lague, Alex %A Lakey, Victoria %A Lee, Eunseong %A Li, Zack %A Li, Yaqiong %A Limon, Michele %A Lokken, Martine %A Louis, Thibaut %A Lungu, Marius %A MacCrann, Niall %A MacInnis, Amanda %A Maldonado, Diego %A Maldonado, Felipe %A Mallaby-Kay, Maya %A Marques, Gabriela A. %A McMahon, Jeff %A Mehta, Yogesh %A Menanteau, Felipe %A Moodley, Kavilan %A Morris, Thomas W. %A Mroczkowski, Tony %A Naess, Sigurd %A Namikawa, Toshiya %A Nati, Federico %A Newburgh, Laura %A Nicola, Andrina %A Niemack, Michael D. %A Nolta, Michael R. %A Orlowski-Scherer, John %A Page, Lyman A. %A Pandey, Shivam %A Partridge, Bruce %A Prince, Heather %A Puddu, Roberto %A Radiconi, Federico %A Robertson, Naomi %A Rojas, Felipe %A Sakuma, Tai %A Salatino, Maria %A Schaan, Emmanuel %A Schmitt, Benjamin L. %A Sehgal, Neelima %A Shaikh, Shabbir %A Sierra, Carlos %A Sievers, Jon %A Sifón, Cristóbal %A Simon, Sara %A Sonka, Rita %A Spergel, David N. %A Staggs, Suzanne T. %A Storer, Emilie %A Switzer, Eric R. %A Tampier, Niklas %A Thornton, Robert %A Trac, Hy %A Treu, Jesse %A Tucker, Carole %A Ulluom, Joel %A Vale, Leila R. %A Van Engelen, Alexander %A Van Lanen, Jeff %A van Marrewijk, Joshiwa %A Vargas, Cristian %A Vavagiakis, Eve M. %A Wagoner, Kasey %A Wang, Yuhan %A Wenzl, Lukas %A Wollack, Edward J. %A Xu, Zhilei %A Zago, Fernando %A Zhang, Kaiwen %D 2023 %K tifr %T The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth %U http://arxiv.org/abs/2304.05202 %X We present new measurements of cosmic microwave background (CMB) lensing over $9400$ sq. deg. of the sky. These lensing measurements are derived from the Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) CMB dataset, which consists of five seasons of ACT CMB temperature and polarization observations. We determine the amplitude of the CMB lensing power spectrum at $2.3\%$ precision ($43\sigma$ significance) using a novel pipeline that minimizes sensitivity to foregrounds and to noise properties. To ensure our results are robust, we analyze an extensive set of null tests, consistency tests, and systematic error estimates and employ a blinded analysis framework. The baseline spectrum is well fit by a lensing amplitude of $A_lens=1.013\pm0.023$ relative to the Planck 2018 CMB power spectra best-fit $Łambda$CDM model and $A_lens=1.005\pm0.023$ relative to the $ACT DR4 + WMAP$ best-fit model. From our lensing power spectrum measurement, we derive constraints on the parameter combination $S^CMBL_8 \sigma_8 łeft(Ømega_m/0.3\right)^0.25$ of $S^CMBL_8= 0.818\pm0.022$ from ACT DR6 CMB lensing alone and $S^CMBL_8= 0.813\pm0.018$ when combining ACT DR6 and Planck NPIPE CMB lensing power spectra. These results are in excellent agreement with $Łambda$CDM model constraints from Planck or $ACT DR4 + WMAP$ CMB power spectrum measurements. Our lensing measurements from redshifts $z\sim0.5$--$5$ are thus fully consistent with $Łambda$CDM structure growth predictions based on CMB anisotropies probing primarily $z\sim1100$. We find no evidence for a suppression of the amplitude of cosmic structure at low redshifts

@misc{qu2023atacama, abstract = {We present new measurements of cosmic microwave background (CMB) lensing over $9400$ sq. deg. of the sky. These lensing measurements are derived from the Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) CMB dataset, which consists of five seasons of ACT CMB temperature and polarization observations. We determine the amplitude of the CMB lensing power spectrum at $2.3\%$ precision ($43\sigma$ significance) using a novel pipeline that minimizes sensitivity to foregrounds and to noise properties. To ensure our results are robust, we analyze an extensive set of null tests, consistency tests, and systematic error estimates and employ a blinded analysis framework. The baseline spectrum is well fit by a lensing amplitude of $A_{\mathrm{lens}}=1.013\pm0.023$ relative to the Planck 2018 CMB power spectra best-fit $\Lambda$CDM model and $A_{\mathrm{lens}}=1.005\pm0.023$ relative to the $\text{ACT DR4} + \text{WMAP}$ best-fit model. From our lensing power spectrum measurement, we derive constraints on the parameter combination $S^{\mathrm{CMBL}}_8 \equiv \sigma_8 \left({\Omega_m}/{0.3}\right)^{0.25}$ of $S^{\mathrm{CMBL}}_8= 0.818\pm0.022$ from ACT DR6 CMB lensing alone and $S^{\mathrm{CMBL}}_8= 0.813\pm0.018$ when combining ACT DR6 and Planck NPIPE CMB lensing power spectra. These results are in excellent agreement with $\Lambda$CDM model constraints from Planck or $\text{ACT DR4} + \text{WMAP}$ CMB power spectrum measurements. Our lensing measurements from redshifts $z\sim0.5$--$5$ are thus fully consistent with $\Lambda$CDM structure growth predictions based on CMB anisotropies probing primarily $z\sim1100$. We find no evidence for a suppression of the amplitude of cosmic structure at low redshifts}, added-at = {2023-04-12T08:12:27.000+0200}, author = {Qu, Frank J. and Sherwin, Blake D. and Madhavacheril, Mathew S. and Han, Dongwon and Crowley, Kevin T. and Abril-Cabezas, Irene and Ade, Peter A. R. and Aiola, Simone and Alford, Tommy and Amiri, Mandana and Amodeo, Stefania and An, Rui and Atkins, Zachary and Austermann, Jason E. and Battaglia, Nicholas and Battistelli, Elia Stefano and Beall, James A. and Bean, Rachel and Beringue, Benjamin and Bhandarkar, Tanay and Biermann, Emily and Bolliet, Boris and Bond, J Richard and Cai, Hongbo and Calabrese, Erminia and Calafut, Victoria and Capalbo, Valentina and Carrero, Felipe and Carron, Julien and Challinor, Anthony and Chesmore, Grace E. and Cho, Hsiao-mei and Choi, Steve K. and Clark, Susan E. and Rosado, Rodrigo Córdova and Cothard, Nicholas F. and Coughlin, Kevin and Coulton, William and Dalal, Roohi and Darwish, Omar and Devlin, Mark J. and Dicker, Simon and Doze, Peter and Duell, Cody J. and Duff, Shannon M. and Duivenvoorden, Adriaan J. and Dunkley, Jo and Dünner, Rolando and Fanfani, Valentina and Fankhanel, Max and Farren, Gerrit and Ferraro, Simone and Freundt, Rodrigo and Fuzia, Brittany and Gallardo, Patricio A. and Garrido, Xavier and Gluscevic, Vera and Golec, Joseph E. and Guan, Yilun and Halpern, Mark and Harrison, Ian and Hasselfield, Matthew and Healy, Erin and Henderson, Shawn and Hensley, Brandon and Hervías-Caimapo, Carlos and Hill, J. Colin and Hilton, Gene C. and Hilton, Matt and Hincks, Adam D. and Hložek, Renée and Ho, Shuay-Pwu Patty and Huber, Zachary B. and Hubmayr, Johannes and Huffenberger, Kevin M. and Hughes, John P. and Irwin, Kent and Isopi, Giovanni and Jense, Hidde T. and Keller, Ben and Kim, Joshua and Knowles, Kenda and Koopman, Brian J. and Kosowsky, Arthur and Kramer, Darby and Kusiak, Aleksandra and La Posta, Adrien and Lague, Alex and Lakey, Victoria and Lee, Eunseong and Li, Zack and Li, Yaqiong and Limon, Michele and Lokken, Martine and Louis, Thibaut and Lungu, Marius and MacCrann, Niall and MacInnis, Amanda and Maldonado, Diego and Maldonado, Felipe and Mallaby-Kay, Maya and Marques, Gabriela A. and McMahon, Jeff and Mehta, Yogesh and Menanteau, Felipe and Moodley, Kavilan and Morris, Thomas W. and Mroczkowski, Tony and Naess, Sigurd and Namikawa, Toshiya and Nati, Federico and Newburgh, Laura and Nicola, Andrina and Niemack, Michael D. and Nolta, Michael R. and Orlowski-Scherer, John and Page, Lyman A. and Pandey, Shivam and Partridge, Bruce and Prince, Heather and Puddu, Roberto and Radiconi, Federico and Robertson, Naomi and Rojas, Felipe and Sakuma, Tai and Salatino, Maria and Schaan, Emmanuel and Schmitt, Benjamin L. and Sehgal, Neelima and Shaikh, Shabbir and Sierra, Carlos and Sievers, Jon and Sifón, Cristóbal and Simon, Sara and Sonka, Rita and Spergel, David N. and Staggs, Suzanne T. and Storer, Emilie and Switzer, Eric R. and Tampier, Niklas and Thornton, Robert and Trac, Hy and Treu, Jesse and Tucker, Carole and Ulluom, Joel and Vale, Leila R. and Van Engelen, Alexander and Van Lanen, Jeff and van Marrewijk, Joshiwa and Vargas, Cristian and Vavagiakis, Eve M. and Wagoner, Kasey and Wang, Yuhan and Wenzl, Lukas and Wollack, Edward J. and Xu, Zhilei and Zago, Fernando and Zhang, Kaiwen}, biburl = {https://www.bibsonomy.org/bibtex/2fb4406fa38e27cb9ebf7bf89ea6fe233/citekhatri}, description = {The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth}, interhash = {d206de5562e6c7779b41c884235374e2}, intrahash = {fb4406fa38e27cb9ebf7bf89ea6fe233}, keywords = {tifr}, note = {cite arxiv:2304.05202Comment: 45+21 pages, 50 figures. Prepared for submission to ApJ. Also see companion papers Madhavacheril et al and MacCrann et al}, timestamp = {2023-04-12T08:12:27.000+0200}, title = {The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth}, url = {http://arxiv.org/abs/2304.05202}, year = 2023 }