Search

Your search keyword '"Rosado, Rodrigo Córdova"' showing total 10 results
Start Over Author "Rosado, Rodrigo Córdova"
10 results on '"Rosado, Rodrigo Córdova"'

1. The Atacama Cosmology Telescope: Galactic Dust Structure and the Cosmic PAH Background in Cross-correlation with WISE

Author

Rosado, Rodrigo Córdova, Hensley, Brandon S., Clark, Susan E., Duivenvoorden, Adriaan J., Atkins, Zachary, Battistelli, Elia Stefano, Choi, Steve K., Dunkley, Jo, Hervías-Caimapo, Carlos, Li, Zack, Louis, Thibaut, Naess, Sigurd, Page, Lyman A., Partridge, Bruce, Sifón, Cristóbal, Staggs, Suzanne T., Vargas, Cristian, and Wollack, Edward J.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present a cross-correlation analysis between $1'$ resolution total intensity and polarization observations from the Atacama Cosmology Telescope (ACT) at 150 and 220 GHz and 15$''$ mid-infrared photometry from the Wide-field Infrared Survey Explorer (WISE) over 107 12.5$^\circ\times$12.5$^\circ$ patches of sky. We detect a spatially isotropic signal in the WISE$\times$ACT $TT$ cross power spectrum at 30$\sigma$ significance that we interpret as the correlation between the cosmic infrared background at ACT frequencies and polycyclic aromatic hydrocarbon (PAH) emission from galaxies in WISE, i.e., the cosmic PAH background. Within the Milky Way, the Galactic dust $TT$ spectra are generally well-described by power laws in $\ell$ over the range 10$^3 < \ell < $10$^4$, but there is evidence both for variability in the power law index and for non-power law behavior in some regions. We measure a positive correlation between WISE total intensity and ACT $E$-mode polarization at 1000$ < \ell \lesssim $6000 at $>$3$\sigma$ in each of 35 distinct $\sim$100 deg$^2$ regions of the sky, suggesting alignment between Galactic density structures and the local magnetic field persists to sub-parsec physical scales in these regions. The distribution of $TE$ amplitudes in this $\ell$ range across all 107 regions is biased to positive values, while there is no evidence for such a bias in the $TB$ spectra. This work constitutes the highest-$\ell$ measurements of the Galactic dust $TE$ spectrum to date and indicates that cross-correlation with high-resolution mid-infrared measurements of dust emission is a promising tool for constraining the spatial statistics of dust emission at millimeter wavelengths., Comment: 20 pages, 14 figures, submitted to ApJ

Published
2023

2. The Atacama Cosmology Telescope: High-resolution component-separated maps across one-third of the sky

Author

Coulton, William R., Madhavacheril, Mathew S., Duivenvoorden, Adriaan J., Hill, J. Colin, Abril-Cabezas, Irene, Ade, Peter A. R., Aiola, Simone, Alford, Tommy, Amiri, Mandana, Amodeo, Stefania, An, Rui, Atkins, Zachary, Austermann, Jason E., Battaglia, Nicholas, Battistelli, Elia Stefano, Beall, James A., Bean, Rachel, Beringue, Benjamin, Bhandarkar, Tanay, Biermann, Emily, Bolliet, Boris, Bond, J Richard, Cai, Hongbo, Calabrese, Erminia, Calafut, Victoria, Capalbo, Valentina, Carrero, Felipe, Chesmore, Grace E., Cho, Hsiao-mei, Choi, Steve K., Clark, Susan E., Rosado, Rodrigo Córdova, Cothard, Nicholas F., Coughlin, Kevin, Crowley, Kevin T., Devlin, Mark J., Dicker, Simon, Doze, Peter, Duell, Cody J., Duff, Shannon M., Dunkley, Jo, Dünner, Rolando, Fanfani, Valentina, Fankhanel, Max, Farren, Gerrit, Ferraro, Simone, Freundt, Rodrigo, Fuzia, Brittany, Gallardo, Patricio A., Garrido, Xavier, Givans, Jahmour, Gluscevic, Vera, Golec, Joseph E., Guan, Yilun, Halpern, Mark, Han, Dongwon, Hasselfield, Matthew, Healy, Erin, Henderson, Shawn, Hensley, Brandon, Hervías-Caimapo, Carlos, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Irwin, Kent, Isopi, Giovanni, Jense, Hidde T., Keller, Ben, Kim, Joshua, Knowles, Kenda, Koopman, Brian J., Kosowsky, Arthur, Kramer, Darby, Kusiak, Aleksandra, La Posta, Adrien, Lakey, Victoria, Lee, Eunseong, Li, Zack, Li, Yaqiong, Limon, Michele, Lokken, Martine, Louis, Thibaut, Lungu, Marius, MacCrann, Niall, MacInnis, Amanda, Maldonado, Diego, Maldonado, Felipe, Mallaby-Kay, Maya, Marques, Gabriela A., van Marrewijk, Joshiwa, McCarthy, Fiona, McMahon, Jeff, Mehta, Yogesh, Menanteau, Felipe, Moodley, Kavilan, Morris, Thomas W., Mroczkowski, Tony, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nicola, Andrina, Niemack, Michael D., Nolta, Michael R., Orlowski-Scherer, John, Page, Lyman A., Pandey, Shivam, Partridge, Bruce, Prince, Heather, Puddu, Roberto, Qu, Frank J., Radiconi, Federico, Robertson, Naomi, Rojas, Felipe, Sakuma, Tai, Salatino, Maria, Schaan, Emmanuel, Schmitt, Benjamin L., Sehgal, Neelima, Shaikh, Shabbir, Sherwin, Blake D., Sierra, Carlos, Sievers, Jon, Sifón, Cristóbal, Simon, Sara, Sonka, Rita, Spergel, David N., Staggs, Suzanne T., Storer, Emilie, Switzer, Eric R., Tampier, Niklas, Thornton, Robert, Trac, Hy, Treu, Jesse, Tucker, Carole, Ullom, Joel, Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, Vargas, Cristian, Vavagiakis, Eve M., Wagoner, Kasey, Wang, Yuhan, Wenzl, Lukas, Wollack, Edward J., Xu, Zhilei, Zago, Fernando, and Zheng, Kaiwen

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Observations of the millimeter sky contain valuable information on a number of signals, including the blackbody cosmic microwave background (CMB), Galactic emissions, and the Compton-$y$ distortion due to the thermal Sunyaev-Zel'dovich (tSZ) effect. Extracting new insight into cosmological and astrophysical questions often requires combining multi-wavelength observations to spectrally isolate one component. In this work, we present a new arcminute-resolution Compton-$y$ map, which traces out the line-of-sight-integrated electron pressure, as well as maps of the CMB in intensity and E-mode polarization, across a third of the sky (around 13,000 sq.~deg.). We produce these through a joint analysis of data from the Atacama Cosmology Telescope (ACT) Data Release 4 and 6 at frequencies of roughly 93, 148, and 225 GHz, together with data from the \textit{Planck} satellite at frequencies between 30 GHz and 545 GHz. We present detailed verification of an internal linear combination pipeline implemented in a needlet frame that allows us to efficiently suppress Galactic contamination and account for spatial variations in the ACT instrument noise. These maps provide a significant advance, in noise levels and resolution, over the existing \textit{Planck} component-separated maps and will enable a host of science goals including studies of cluster and galaxy astrophysics, inferences of the cosmic velocity field, primordial non-Gaussianity searches, and gravitational lensing reconstruction of the CMB., Comment: The Compton-y map and associated products will be made publicly available upon publication of the paper. The CMB T and E mode maps will be made available when the DR6 maps are made public

Published
2023

3. The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing

Author

Luo, Yifei, Leauthaud, Alexie, Greene, Jenny, Huang, Song, Kado-Fong, Erin, Danieli, Shany, Li, Ting S., Li, Jiaxuan, Blanco, Diana, Wasleske, Erik J., Wick, Joseph, Mintz, Abby, Guan, Runquan, Peter, Annika H. G., Baldassare, Vivienne, Brooks, Alyson, Banerjee, Arka, Bhattacharyya, Joy, Cai, Zheng, Chen, Xinjun, Gunn, Jim, Johnson, Sean D., Kelvin, Lee S., Li, Mingyu, Lin, Xiaojing, Lupton, Robert, Mace, Charlie, Medina, Gustavo E., Read, Justin, Rosado, Rodrigo Cordova, and Seifert, Allen

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Merian survey is mapping $\sim$ 850 degrees$^2$ of the Hyper Suprime-Cam Strategic Survey Program (HSC-SSP) wide layer with two medium-band filters on the 4-meter Victor M. Blanco telescope at the Cerro Tololo Inter-American Observatory, with the goal of carrying the first high signal-to-noise (S/N) measurements of weak gravitational lensing around dwarf galaxies. This paper presents the design of the Merian filter set: N708 ($\lambda_c = 7080 \unicode{x212B}$, $\Delta\lambda = 275\unicode{x212B}$) and N540 ($\lambda_c = 5400\unicode{x212B}$, $\Delta\lambda = 210\unicode{x212B}$). The central wavelengths and filter widths of N708 and N540 were designed to detect the $\rm H\alpha$ and $\rm [OIII]$ emission lines of galaxies in the mass range $8<\rm \log M_*/M_\odot<9$ by comparing Merian fluxes with HSC broad-band fluxes. Our filter design takes into account the weak lensing S/N and photometric redshift performance. Our simulations predict that Merian will yield a sample of $\sim$ 85,000 star-forming dwarf galaxies with a photometric redshift accuracy of $\sigma_{\Delta z/(1+z)}\sim 0.01$ and an outlier fraction of $\eta=2.8\%$ over the redshift range $0.058

Published
2023
Full Text
View/download PDF

4. The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

Author

Madhavacheril, Mathew S., Qu, Frank J., Sherwin, Blake D., MacCrann, Niall, Li, Yaqiong, Abril-Cabezas, Irene, Ade, Peter A. R., Aiola, Simone, Alford, Tommy, Amiri, Mandana, Amodeo, Stefania, An, Rui, Atkins, Zachary, Austermann, Jason E., Battaglia, Nicholas, Battistelli, Elia Stefano, Beall, James A., Bean, Rachel, Beringue, Benjamin, Bhandarkar, Tanay, Biermann, Emily, Bolliet, Boris, Bond, J Richard, Cai, Hongbo, Calabrese, Erminia, Calafut, Victoria, Capalbo, Valentina, Carrero, Felipe, Challinor, Anthony, Chesmore, Grace E., Cho, Hsiao-mei, Choi, Steve K., Clark, Susan E., Rosado, Rodrigo Córdova, Cothard, Nicholas F., Coughlin, Kevin, Coulton, William, Crowley, Kevin T., Dalal, Roohi, Darwish, Omar, Devlin, Mark J., Dicker, Simon, Doze, Peter, Duell, Cody J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Fanfani, Valentina, Fankhanel, Max, Farren, Gerrit, Ferraro, Simone, Freundt, Rodrigo, Fuzia, Brittany, Gallardo, Patricio A., Garrido, Xavier, Givans, Jahmour, Gluscevic, Vera, Golec, Joseph E., Guan, Yilun, Hall, Kirsten R., Halpern, Mark, Han, Dongwon, Harrison, Ian, Hasselfield, Matthew, Healy, Erin, Henderson, Shawn, Hensley, Brandon, Hervías-Caimapo, Carlos, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Irwin, Kent, Isopi, Giovanni, Jense, Hidde T., Keller, Ben, Kim, Joshua, Knowles, Kenda, Koopman, Brian J., Kosowsky, Arthur, Kramer, Darby, Kusiak, Aleksandra, La Posta, Adrien, Lague, Alex, Lakey, Victoria, Lee, Eunseong, Li, Zack, Limon, Michele, Lokken, Martine, Louis, Thibaut, Lungu, Marius, MacInnis, Amanda, Maldonado, Diego, Maldonado, Felipe, Mallaby-Kay, Maya, Marques, Gabriela A., McMahon, Jeff, Mehta, Yogesh, Menanteau, Felipe, Moodley, Kavilan, Morris, Thomas W., Mroczkowski, Tony, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nicola, Andrina, Niemack, Michael D., Nolta, Michael R., Orlowski-Scherer, John, Page, Lyman A., Pandey, Shivam, Partridge, Bruce, Prince, Heather, Puddu, Roberto, Radiconi, Federico, Robertson, Naomi, Rojas, Felipe, Sakuma, Tai, Salatino, Maria, Schaan, Emmanuel, Schmitt, Benjamin L., Sehgal, Neelima, Shaikh, Shabbir, Sierra, Carlos, Sievers, Jon, Sifón, Cristóbal, Simon, Sara, Sonka, Rita, Spergel, David N., Staggs, Suzanne T., Storer, Emilie, Switzer, Eric R., Tampier, Niklas, Thornton, Robert, Trac, Hy, Treu, Jesse, Tucker, Carole, Ullom, Joel, Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, van Marrewijk, Joshiwa, Vargas, Cristian, Vavagiakis, Eve M., Wagoner, Kasey, Wang, Yuhan, Wenzl, Lukas, Wollack, Edward J., Xu, Zhilei, Zago, Fernando, and Zheng, Kaiwen

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, High Energy Physics - Phenomenology
Abstract

We present cosmological constraints from a gravitational lensing mass map covering 9400 sq. deg. reconstructed from CMB measurements made by the Atacama Cosmology Telescope (ACT) from 2017 to 2021. In combination with BAO measurements (from SDSS and 6dF), we obtain the amplitude of matter fluctuations $\sigma_8 = 0.819 \pm 0.015$ at 1.8% precision, $S_8\equiv\sigma_8({\Omega_{\rm m}}/0.3)^{0.5}=0.840\pm0.028$ and the Hubble constant $H_0= (68.3 \pm 1.1)\, \text{km}\,\text{s}^{-1}\,\text{Mpc}^{-1}$ at 1.6% precision. A joint constraint with CMB lensing measured by the Planck satellite yields even more precise values: $\sigma_8 = 0.812 \pm 0.013$, $S_8\equiv\sigma_8({\Omega_{\rm m}}/0.3)^{0.5}=0.831\pm0.023$ and $H_0= (68.1 \pm 1.0)\, \text{km}\,\text{s}^{-1}\,\text{Mpc}^{-1}$. These measurements agree well with $\Lambda$CDM-model extrapolations from the CMB anisotropies measured by Planck. To compare these constraints to those from the KiDS, DES, and HSC galaxy surveys, we revisit those data sets with a uniform set of assumptions, and find $S_8$ from all three surveys are lower than that from ACT+Planck lensing by varying levels ranging from 1.7-2.1$\sigma$. These results motivate further measurements and comparison, not just between the CMB anisotropies and galaxy lensing, but also between CMB lensing probing $z\sim 0.5-5$ on mostly-linear scales and galaxy lensing at $z\sim 0.5$ on smaller scales. We combine our CMB lensing measurements with CMB anisotropies to constrain extensions of $\Lambda$CDM, limiting the sum of the neutrino masses to $\sum m_{\nu} < 0.13$ eV (95% c.l.), for example. Our results provide independent confirmation that the universe is spatially flat, conforms with general relativity, and is described remarkably well by the $\Lambda$CDM model, while paving a promising path for neutrino physics with gravitational lensing from upcoming ground-based CMB surveys., Comment: 32 pages, 17 figures, replaced with version accepted in ApJ (Feb 2024). Cosmological likelihood data and mass maps are public here: https://lambda.gsfc.nasa.gov/product/act/actadv_prod_table.html ; likelihood software is here: https://github.com/ACTCollaboration/act_dr6_lenslike . Also see companion papers Qu et al and MacCrann et al

Published
2023
Full Text
View/download PDF

5. The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth

Author

Qu, Frank J., Sherwin, Blake D., Madhavacheril, Mathew S., Han, Dongwon, Crowley, Kevin T., Abril-Cabezas, Irene, Ade, Peter A. R., Aiola, Simone, Alford, Tommy, Amiri, Mandana, Amodeo, Stefania, An, Rui, Atkins, Zachary, Austermann, Jason E., Battaglia, Nicholas, Battistelli, Elia Stefano, Beall, James A., Bean, Rachel, Beringue, Benjamin, Bhandarkar, Tanay, Biermann, Emily, Bolliet, Boris, Bond, J Richard, Cai, Hongbo, Calabrese, Erminia, Calafut, Victoria, Capalbo, Valentina, Carrero, Felipe, Carron, Julien, Challinor, Anthony, Chesmore, Grace E., Cho, Hsiao-mei, Choi, Steve K., Clark, Susan E., Rosado, Rodrigo Córdova, Cothard, Nicholas F., Coughlin, Kevin, Coulton, William, Dalal, Roohi, Darwish, Omar, Devlin, Mark J., Dicker, Simon, Doze, Peter, Duell, Cody J., Duff, Shannon M., Duivenvoorden, Adriaan J., Dunkley, Jo, Dünner, Rolando, Fanfani, Valentina, Fankhanel, Max, Farren, Gerrit, Ferraro, Simone, Freundt, Rodrigo, Fuzia, Brittany, Gallardo, Patricio A., Garrido, Xavier, Gluscevic, Vera, Golec, Joseph E., Guan, Yilun, Halpern, Mark, Harrison, Ian, Hasselfield, Matthew, Healy, Erin, Henderson, Shawn, Hensley, Brandon, Hervías-Caimapo, Carlos, Hill, J. Colin, Hilton, Gene C., Hilton, Matt, Hincks, Adam D., Hložek, Renée, Ho, Shuay-Pwu Patty, Huber, Zachary B., Hubmayr, Johannes, Huffenberger, Kevin M., Hughes, John P., Irwin, Kent, Isopi, Giovanni, Jense, Hidde T., Keller, Ben, Kim, Joshua, Knowles, Kenda, Koopman, Brian J., Kosowsky, Arthur, Kramer, Darby, Kusiak, Aleksandra, La Posta, Adrien, Lague, Alex, Lakey, Victoria, Lee, Eunseong, Li, Zack, Li, Yaqiong, Limon, Michele, Lokken, Martine, Louis, Thibaut, Lungu, Marius, MacCrann, Niall, MacInnis, Amanda, Maldonado, Diego, Maldonado, Felipe, Mallaby-Kay, Maya, Marques, Gabriela A., McMahon, Jeff, Mehta, Yogesh, Menanteau, Felipe, Moodley, Kavilan, Morris, Thomas W., Mroczkowski, Tony, Naess, Sigurd, Namikawa, Toshiya, Nati, Federico, Newburgh, Laura, Nicola, Andrina, Niemack, Michael D., Nolta, Michael R., Orlowski-Scherer, John, Page, Lyman A., Pandey, Shivam, Partridge, Bruce, Prince, Heather, Puddu, Roberto, Radiconi, Federico, Robertson, Naomi, Rojas, Felipe, Sakuma, Tai, Salatino, Maria, Schaan, Emmanuel, Schmitt, Benjamin L., Sehgal, Neelima, Shaikh, Shabbir, Sierra, Carlos, Sievers, Jon, Sifón, Cristóbal, Simon, Sara, Sonka, Rita, Spergel, David N., Staggs, Suzanne T., Storer, Emilie, Switzer, Eric R., Tampier, Niklas, Thornton, Robert, Trac, Hy, Treu, Jesse, Tucker, Carole, Ulluom, Joel, Vale, Leila R., Van Engelen, Alexander, Van Lanen, Jeff, van Marrewijk, Joshiwa, Vargas, Cristian, Vavagiakis, Eve M., Wagoner, Kasey, Wang, Yuhan, Wenzl, Lukas, Wollack, Edward J., Xu, Zhilei, Zago, Fernando, and Zhang, Kaiwen

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
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, Comment: 45+22 pages, 50 figures. v2 matches with published version in ApJ. Cosmological likelihood data and lensing maps are here: https://lambda.gsfc.nasa.gov/product/act/actadv_prod_table.html ; likelihood software is here: https://github.com/ACTCollaboration/act_dr6_lenslike . Also see companion papers Madhavacheril et al and MacCrann et al

Published
2023
Full Text
View/download PDF

6. Evaluation of New Submillimeter VLBI Sites for the Event Horizon Telescope

Author

Raymond, Alexander W., Palumbo, Daniel, Paine, Scott N., Blackburn, Lindy, Rosado, Rodrigo Córdova, Doeleman, Sheperd S., Farah, Joseph R., Johnson, Michael D., Roelofs, Freek, Tilanus, Remo P. J., and Weintroub, Jonathan

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The Event Horizon Telescope (EHT) is a very long baseline interferometer built to image supermassive black holes on event-horizon scales. In this paper, we investigate candidate sites for an expanded EHT array with improved imaging capabilities. We use historical meteorology and radiative transfer analysis to evaluate site performance. Most of the existing sites in the EHT array have median zenith opacity less than 0.2 at 230 GHz during the March/April observing season. Seven of the existing EHT sites have 345 GHz opacity less than 0.5 during observing months. Out of more than forty candidate new locations analyzed, approximately half have 230 GHz opacity comparable to the existing EHT sites, and at least seventeen of the candidate sites would be comparably good for 345 GHz observing. A group of new sites with favorable transmittance and geographic placement leads to greatly enhanced imaging and science on horizon scales.

Published
2021
Full Text
View/download PDF

7. The Merian survey: design, construction, and characterization of a filter set optimized to find dwarf galaxies and measure their dark matter halo properties with weak lensing

Author

Luo, Yifei, primary, Leauthaud, Alexie, additional, Greene, Jenny, additional, Huang, Song, additional, Kado-Fong, Erin, additional, Danieli, Shany, additional, Li, Ting S, additional, Li, Jiaxuan, additional, Blanco, Diana, additional, Wasleske, Erik J, additional, Wick, Joseph, additional, Mintz, Abby, additional, Guan, Runquan, additional, Peter, Annika H G, additional, Baldassare, Vivienne, additional, Brooks, Alyson, additional, Banerjee, Arka, additional, Bhattacharyya, Joy, additional, Cai, Zheng, additional, Chen, Xinjun, additional, Gunn, Jim, additional, Johnson, Sean D, additional, Kelvin, Lee S, additional, Li, Mingyu, additional, Lin, Xiaojing, additional, Lupton, Robert, additional, Mace, Charlie, additional, Medina, Gustavo E, additional, Read, Justin, additional, Rosado, Rodrigo Córdova, additional, and Seifert, Allen, additional

Published
2024
Full Text
View/download PDF

8. Atacama Cosmology Telescope: High-resolution component-separated maps across one third of the sky

Author

Coulton, William, primary, Madhavacheril, Mathew S., additional, Duivenvoorden, Adriaan J., additional, Hill, J. Colin, additional, Abril-Cabezas, Irene, additional, Ade, Peter A. R., additional, Aiola, Simone, additional, Alford, Tommy, additional, Amiri, Mandana, additional, Amodeo, Stefania, additional, An, Rui, additional, Atkins, Zachary, additional, Austermann, Jason E., additional, Battaglia, Nicholas, additional, Battistelli, Elia Stefano, additional, Beall, James A., additional, Bean, Rachel, additional, Beringue, Benjamin, additional, Bhandarkar, Tanay, additional, Biermann, Emily, additional, Bolliet, Boris, additional, Bond, J. Richard, additional, Cai, Hongbo, additional, Calabrese, Erminia, additional, Calafut, Victoria, additional, Capalbo, Valentina, additional, Carrero, Felipe, additional, Chesmore, Grace E., additional, Cho, Hsiao-mei, additional, Choi, Steve K., additional, Clark, Susan E., additional, Rosado, Rodrigo Córdova, additional, Cothard, Nicholas F., additional, Coughlin, Kevin, additional, Crowley, Kevin T., additional, Devlin, Mark J., additional, Dicker, Simon, additional, Doze, Peter, additional, Duell, Cody J., additional, Duff, Shannon M., additional, Dunkley, Jo, additional, Dünner, Rolando, additional, Fanfani, Valentina, additional, Fankhanel, Max, additional, Farren, Gerrit, additional, Ferraro, Simone, additional, Freundt, Rodrigo, additional, Fuzia, Brittany, additional, Gallardo, Patricio A., additional, Garrido, Xavier, additional, Givans, Jahmour, additional, Gluscevic, Vera, additional, Golec, Joseph E., additional, Guan, Yilun, additional, Halpern, Mark, additional, Han, Dongwon, additional, Hasselfield, Matthew, additional, Healy, Erin, additional, Henderson, Shawn, additional, Hensley, Brandon, additional, Hervías-Caimapo, Carlos, additional, Hilton, Gene C., additional, Hilton, Matt, additional, Hincks, Adam D., additional, Hložek, Renée, additional, Ho, Shuay-Pwu Patty, additional, Huber, Zachary B., additional, Hubmayr, Johannes, additional, Huffenberger, Kevin M., additional, Hughes, John P., additional, Irwin, Kent, additional, Isopi, Giovanni, additional, Jense, Hidde T., additional, Keller, Ben, additional, Kim, Joshua, additional, Knowles, Kenda, additional, Koopman, Brian J., additional, Kosowsky, Arthur, additional, Kramer, Darby, additional, Kusiak, Aleksandra, additional, La Posta, Adrien, additional, Lakey, Victoria, additional, Lee, Eunseong, additional, Li, Zack, additional, Li, Yaqiong, additional, Limon, Michele, additional, Lokken, Martine, additional, Louis, Thibaut, additional, Lungu, Marius, additional, MacCrann, Niall, additional, MacInnis, Amanda, additional, Maldonado, Diego, additional, Maldonado, Felipe, additional, Mallaby-Kay, Maya, additional, Marques, Gabriela A., additional, van Marrewijk, Joshiwa, additional, McCarthy, Fiona, additional, McMahon, Jeff, additional, Mehta, Yogesh, additional, Menanteau, Felipe, additional, Moodley, Kavilan, additional, Morris, Thomas W., additional, Mroczkowski, Tony, additional, Naess, Sigurd, additional, Namikawa, Toshiya, additional, Nati, Federico, additional, Newburgh, Laura, additional, Nicola, Andrina, additional, Niemack, Michael D., additional, Nolta, Michael R., additional, Orlowski-Scherer, John, additional, Page, Lyman A., additional, Pandey, Shivam, additional, Partridge, Bruce, additional, Prince, Heather, additional, Puddu, Roberto, additional, Qu, Frank J., additional, Radiconi, Federico, additional, Robertson, Naomi, additional, Rojas, Felipe, additional, Sakuma, Tai, additional, Salatino, Maria, additional, Schaan, Emmanuel, additional, Schmitt, Benjamin L., additional, Sehgal, Neelima, additional, Shaikh, Shabbir, additional, Sherwin, Blake D., additional, Sierra, Carlos, additional, Sievers, Jon, additional, Sifón, Cristóbal, additional, Simon, Sara, additional, Sonka, Rita, additional, Spergel, David N., additional, Staggs, Suzanne T., additional, Storer, Emilie, additional, Switzer, Eric R., additional, Tampier, Niklas, additional, Thornton, Robert, additional, Trac, Hy, additional, Treu, Jesse, additional, Tucker, Carole, additional, Ullom, Joel, additional, Vale, Leila R., additional, Van Engelen, Alexander, additional, Van Lanen, Jeff, additional, Vargas, Cristian, additional, Vavagiakis, Eve M., additional, Wagoner, Kasey, additional, Wang, Yuhan, additional, Wenzl, Lukas, additional, Wollack, Edward J., additional, Xu, Zhilei, additional, Zago, Fernando, additional, and Zheng, Kaiwen, additional

Published
2024
Full Text
View/download PDF

9. The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters

Author

Madhavacheril, Mathew S., primary, Qu, Frank J., additional, Sherwin, Blake D., additional, MacCrann, Niall, additional, Li, Yaqiong, additional, Abril-Cabezas, Irene, additional, Ade, Peter A. R., additional, Aiola, Simone, additional, Alford, Tommy, additional, Amiri, Mandana, additional, Amodeo, Stefania, additional, An, Rui, additional, Atkins, Zachary, additional, Austermann, Jason E., additional, Battaglia, Nicholas, additional, Battistelli, Elia Stefano, additional, Beall, James A., additional, Bean, Rachel, additional, Beringue, Benjamin, additional, Bhandarkar, Tanay, additional, Biermann, Emily, additional, Bolliet, Boris, additional, Bond, J Richard, additional, Cai, Hongbo, additional, Calabrese, Erminia, additional, Calafut, Victoria, additional, Capalbo, Valentina, additional, Carrero, Felipe, additional, Challinor, Anthony, additional, Chesmore, Grace E., additional, Cho, Hsiao-mei, additional, Choi, Steve K., additional, Clark, Susan E., additional, Rosado, Rodrigo Córdova, additional, Cothard, Nicholas F., additional, Coughlin, Kevin, additional, Coulton, William, additional, Crowley, Kevin T., additional, Dalal, Roohi, additional, Darwish, Omar, additional, Devlin, Mark J., additional, Dicker, Simon, additional, Doze, Peter, additional, Duell, Cody J., additional, Duff, Shannon M., additional, Duivenvoorden, Adriaan J., additional, Dunkley, Jo, additional, Dünner, Rolando, additional, Fanfani, Valentina, additional, Fankhanel, Max, additional, Farren, Gerrit, additional, Ferraro, Simone, additional, Freundt, Rodrigo, additional, Fuzia, Brittany, additional, Gallardo, Patricio A., additional, Garrido, Xavier, additional, Givans, Jahmour, additional, Gluscevic, Vera, additional, Golec, Joseph E., additional, Guan, Yilun, additional, Hall, Kirsten R., additional, Halpern, Mark, additional, Han, Dongwon, additional, Harrison, Ian, additional, Hasselfield, Matthew, additional, Healy, Erin, additional, Henderson, Shawn, additional, Hensley, Brandon, additional, Hervías-Caimapo, Carlos, additional, Hill, J. Colin, additional, Hilton, Gene C., additional, Hilton, Matt, additional, Hincks, Adam D., additional, Hložek, Renée, additional, Ho, Shuay-Pwu Patty, additional, Huber, Zachary B., additional, Hubmayr, Johannes, additional, Huffenberger, Kevin M., additional, Hughes, John P., additional, Irwin, Kent, additional, Isopi, Giovanni, additional, Jense, Hidde T., additional, Keller, Ben, additional, Kim, Joshua, additional, Knowles, Kenda, additional, Koopman, Brian J., additional, Kosowsky, Arthur, additional, Kramer, Darby, additional, Kusiak, Aleksandra, additional, La Posta, Adrien, additional, Lague, Alex, additional, Lakey, Victoria, additional, Lee, Eunseong, additional, Li, Zack, additional, Limon, Michele, additional, Lokken, Martine, additional, Louis, Thibaut, additional, Lungu, Marius, additional, MacInnis, Amanda, additional, Maldonado, Diego, additional, Maldonado, Felipe, additional, Mallaby-Kay, Maya, additional, Marques, Gabriela A., additional, McMahon, Jeff, additional, Mehta, Yogesh, additional, Menanteau, Felipe, additional, Moodley, Kavilan, additional, Morris, Thomas W., additional, Mroczkowski, Tony, additional, Naess, Sigurd, additional, Namikawa, Toshiya, additional, Nati, Federico, additional, Newburgh, Laura, additional, Nicola, Andrina, additional, Niemack, Michael D., additional, Nolta, Michael R., additional, Orlowski-Scherer, John, additional, Page, Lyman A., additional, Pandey, Shivam, additional, Partridge, Bruce, additional, Prince, Heather, additional, Puddu, Roberto, additional, Radiconi, Federico, additional, Robertson, Naomi, additional, Rojas, Felipe, additional, Sakuma, Tai, additional, Salatino, Maria, additional, Schaan, Emmanuel, additional, Schmitt, Benjamin L., additional, Sehgal, Neelima, additional, Shaikh, Shabbir, additional, Sierra, Carlos, additional, Sievers, Jon, additional, Sifón, Cristóbal, additional, Simon, Sara, additional, Sonka, Rita, additional, Spergel, David N., additional, Staggs, Suzanne T., additional, Storer, Emilie, additional, Switzer, Eric R., additional, Tampier, Niklas, additional, Thornton, Robert, additional, Trac, Hy, additional, Treu, Jesse, additional, Tucker, Carole, additional, Ullom, Joel, additional, Vale, Leila R., additional, Van Engelen, Alexander, additional, Van Lanen, Jeff, additional, van Marrewijk, Joshiwa, additional, Vargas, Cristian, additional, Vavagiakis, Eve M., additional, Wagoner, Kasey, additional, Wang, Yuhan, additional, Wenzl, Lukas, additional, Wollack, Edward J., additional, Xu, Zhilei, additional, Zago, Fernando, additional, and Zheng, Kaiwen, additional

Published
2024
Full Text
View/download PDF

10. The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and Its Implications for Structure Growth

Author

Qu, Frank J., primary, Sherwin, Blake D., additional, Madhavacheril, Mathew S., additional, Han, Dongwon, additional, Crowley, Kevin T., additional, Abril-Cabezas, Irene, additional, Ade, Peter A. R., additional, Aiola, Simone, additional, Alford, Tommy, additional, Amiri, Mandana, additional, Amodeo, Stefania, additional, An, Rui, additional, Atkins, Zachary, additional, Austermann, Jason E., additional, Battaglia, Nicholas, additional, Battistelli, Elia Stefano, additional, Beall, James A., additional, Bean, Rachel, additional, Beringue, Benjamin, additional, Bhandarkar, Tanay, additional, Biermann, Emily, additional, Bolliet, Boris, additional, Bond, J Richard, additional, Cai, Hongbo, additional, Calabrese, Erminia, additional, Calafut, Victoria, additional, Capalbo, Valentina, additional, Carrero, Felipe, additional, Carron, Julien, additional, Challinor, Anthony, additional, Chesmore, Grace E., additional, Cho, Hsiao-mei, additional, Choi, Steve K., additional, Clark, Susan E., additional, Rosado, Rodrigo Córdova, additional, Cothard, Nicholas F., additional, Coughlin, Kevin, additional, Coulton, William, additional, Dalal, Roohi, additional, Darwish, Omar, additional, Devlin, Mark J., additional, Dicker, Simon, additional, Doze, Peter, additional, Duell, Cody J., additional, Duff, Shannon M., additional, Duivenvoorden, Adriaan J., additional, Dunkley, Jo, additional, Dünner, Rolando, additional, Fanfani, Valentina, additional, Fankhanel, Max, additional, Farren, Gerrit, additional, Ferraro, Simone, additional, Freundt, Rodrigo, additional, Fuzia, Brittany, additional, Gallardo, Patricio A., additional, Garrido, Xavier, additional, Gluscevic, Vera, additional, Golec, Joseph E., additional, Guan, Yilun, additional, Halpern, Mark, additional, Harrison, Ian, additional, Hasselfield, Matthew, additional, Healy, Erin, additional, Henderson, Shawn, additional, Hensley, Brandon, additional, Hervías-Caimapo, Carlos, additional, Hill, J. Colin, additional, Hilton, Gene C., additional, Hilton, Matt, additional, Hincks, Adam D., additional, Hložek, Renée, additional, Ho, Shuay-Pwu Patty, additional, Huber, Zachary B., additional, Hubmayr, Johannes, additional, Huffenberger, Kevin M., additional, Hughes, John P., additional, Irwin, Kent, additional, Isopi, Giovanni, additional, Jense, Hidde T., additional, Keller, Ben, additional, Kim, Joshua, additional, Knowles, Kenda, additional, Koopman, Brian J., additional, Kosowsky, Arthur, additional, Kramer, Darby, additional, Kusiak, Aleksandra, additional, La Posta, Adrien, additional, Lague, Alex, additional, Lakey, Victoria, additional, Lee, Eunseong, additional, Li, Zack, additional, Li, Yaqiong, additional, Limon, Michele, additional, Lokken, Martine, additional, Louis, Thibaut, additional, Lungu, Marius, additional, MacCrann, Niall, additional, MacInnis, Amanda, additional, Maldonado, Diego, additional, Maldonado, Felipe, additional, Mallaby-Kay, Maya, additional, Marques, Gabriela A., additional, McMahon, Jeff, additional, Mehta, Yogesh, additional, Menanteau, Felipe, additional, Moodley, Kavilan, additional, Morris, Thomas W., additional, Mroczkowski, Tony, additional, Naess, Sigurd, additional, Namikawa, Toshiya, additional, Nati, Federico, additional, Newburgh, Laura, additional, Nicola, Andrina, additional, Niemack, Michael D., additional, Nolta, Michael R., additional, Orlowski-Scherer, John, additional, Page, Lyman A., additional, Pandey, Shivam, additional, Partridge, Bruce, additional, Prince, Heather, additional, Puddu, Roberto, additional, Radiconi, Federico, additional, Robertson, Naomi, additional, Rojas, Felipe, additional, Sakuma, Tai, additional, Salatino, Maria, additional, Schaan, Emmanuel, additional, Schmitt, Benjamin L., additional, Sehgal, Neelima, additional, Shaikh, Shabbir, additional, Sierra, Carlos, additional, Sievers, Jon, additional, Sifón, Cristóbal, additional, Simon, Sara, additional, Sonka, Rita, additional, Spergel, David N., additional, Staggs, Suzanne T., additional, Storer, Emilie, additional, Switzer, Eric R., additional, Tampier, Niklas, additional, Thornton, Robert, additional, Trac, Hy, additional, Treu, Jesse, additional, Tucker, Carole, additional, Ullom, Joel, additional, Vale, Leila R., additional, Van Engelen, Alexander, additional, Van Lanen, Jeff, additional, van Marrewijk, Joshiwa, additional, Vargas, Cristian, additional, Vavagiakis, Eve M., additional, Wagoner, Kasey, additional, Wang, Yuhan, additional, Wenzl, Lukas, additional, Wollack, Edward J., additional, Xu, Zhilei, additional, Zago, Fernando, additional, and Zheng, Kaiwen, additional

Published
2024
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results