Search Results - "CAPAK, Peter L"

The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Survey Overview and Data Release 1 by Masters, Daniel C., Stern, Daniel K., Cohen, Judith G., Capak, Peter L., Rhodes, Jason D., Castander, Francisco J., Paltani, Stéphane

“…A key goal of the Stage IV dark energy experiments Euclid, LSST, and WFIRST is to measure the growth of structure with cosmic time from weak lensing analysis…”
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COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe by Riechers, Dominik A., Pavesi, Riccardo, Sharon, Chelsea E., Hodge, Jacqueline A., Decarli, Roberto, Walter, Fabian, Carilli, Christopher L., Aravena, Manuel, da Cunha, Elisabete, Daddi, Emanuele, Dickinson, Mark, Smail, Ian, Capak, Peter L., Ivison, Rob J., Sargent, Mark, Scoville, Nicholas Z., Wagg, Jeff

“…We report the first detailed measurement of the shape of the CO luminosity function at high redshift, based on >320 hr of the NSF's Karl G. Jansky Very Large…”
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The Complete Calibration of the Color-Redshift Relation (C3R2) Survey: Analysis and Data Release 2 by Masters, Daniel C., Stern, Daniel K., Cohen, Judith G., Capak, Peter L., Stanford, S. Adam, Hernitschek, Nina, Galametz, Audrey, Davidzon, Iary, Rhodes, Jason D., Sanders, Dave, Mobasher, Bahram, Castander, Francisco, Pruett, Kerianne, Fotopoulou, Sotiria

“…The Complete Calibration of the Color-Redshift Relation (C3R2) survey is a multi-institution, multi-instrument survey that aims to map the empirical relation…”
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COLDz: A High Space Density of Massive Dusty Starburst Galaxies ∼1 Billion Years after the Big Bang by Riechers, Dominik A., Hodge, Jacqueline A., Pavesi, Riccardo, Daddi, Emanuele, Decarli, Roberto, Ivison, Rob J., Sharon, Chelsea E., Smail, Ian, Walter, Fabian, Aravena, Manuel, Capak, Peter L., Carilli, Christopher L., Cox, Pierre, Cunha, Elisabete da, Dannerbauer, Helmut, Dickinson, Mark, Neri, Roberto, Wagg, Jeff

“…We report the detection of CO(J = 2 → 1) emission from three massive dusty starburst galaxies at z > 5 through molecular line scans in the NSF's Karl G. Jansky…”
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Low Star Formation Efficiency in Typical Galaxies at z = 5-6 by Pavesi, Riccardo, Riechers, Dominik A., Faisst, Andreas L., Stacey, Gordon J., Capak, Peter L.

“…Using the Very Large Array and ALMA, we have obtained CO(2-1), [C ii], and [N ii] line emission and multiple dust continuum measurements in a sample of…”
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Hidden in Plain Sight: A Massive, Dusty Starburst in a Galaxy Protocluster at z = 5.7 in the COSMOS Field by Pavesi, Riccardo, Riechers, Dominik A., Sharon, Chelsea E., Smol i, Vernesa, Faisst, Andreas L., Schinnerer, Eva, Carilli, Christopher L., Capak, Peter L., Scoville, Nick, Stacey, Gordon J.

“…We report the serendipitous discovery of a dusty, starbursting galaxy at z = 5.667 (hereafter called CRLE) in close physical association with the "normal"…”
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The redshift evolution of rest-UV spectroscopic properties to z ∼ 5 by Pahl, Anthony J, Shapley, Alice, Faisst, Andreas L, Capak, Peter L, Du, Xinnan, Reddy, Naveen A, Laursen, Peter, Topping, Michael W

“…ABSTRACT We perform a comprehensive analysis of the redshift evolution of the rest-UV spectra of star-forming galaxies out to z ∼ 5. We combine new z ∼ 5…”
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ALMA REVEALS WEAK [N ii] EMISSION IN "TYPICAL" GALAXIES AND INTENSE STARBURSTS AT z = 5-6 by Pavesi, Riccardo, Riechers, Dominik A., Capak, Peter L., Carilli, Christopher L., Sharon, Chelsea E., Stacey, Gordon J., Karim, Alexander, Scoville, Nicholas Z., Smol i, Vernesa

“…ABSTRACT We report interferometric measurements of [N ii] 205 m fine-structure line emission from a representative sample of three galaxies at z = 5-6 using…”
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A massive protocluster of galaxies at a redshift of z ≈ 5.3 by Capak, Peter L., Riechers, Dominik, Scoville, Nick Z., Carilli, Chris, Cox, Pierre, Neri, Roberto, Robertson, Brant, Salvato, Mara, Schinnerer, Eva, Yan, Lin, Wilson, Grant W., Yun, Min, Civano, Francesca, Elvis, Martin, Karim, Alexander, Mobasher, Bahram, Staguhn, Johannes G.

“…An early look at a galactic cluster A 'protocluster' of massive galaxies at a redshift z = 5.3, dating to only a billion years after the Big Bang, has been…”
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Galaxy–Galaxy lensing in HSC: Validation tests and the impact of heterogeneous spectroscopic training sets by Speagle, Joshua S, Leauthaud, Alexie, Huang, Song, Bradshaw, Christopher P, Ardila, Felipe, Capak, Peter L, Eisenstein, Daniel J, Masters, Daniel C, Mandelbaum, Rachel, More, Surhud, Simet, Melanie, Sifón, Cristóbal

“…Although photometric redshifts (photo-z’s) are crucial ingredients for current and upcoming large-scale surveys, the high-quality spectroscopic redshifts…”
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LARGE-SCALE STRUCTURE AROUND A z = 2.1 CLUSTER by Hung (洪肇伶), Chao-Ling, Casey, Caitlin M., Chiang, Yi-Kuan, Capak, Peter L., Cowley, Michael J., Darvish, Behnam, Kacprzak, Glenn G., Kova, K., Lilly, Simon J., Nanayakkara, Themiya, Spitler, Lee R., Tran, Kim-Vy H., Yuan, Tiantian

“…ABSTRACT The most prodigious starburst galaxies are absent in massive galaxy clusters today, but their connection with large-scale environments is less clear…”
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The stellar mass, star formation rate and dark matter halo properties of LAEs at z ∼ 2 by Kusakabe, Haruka, Shimasaku, Kazuhiro, Ouchi, Masami, Nakajima, Kimihiko, Goto, Ryosuke, Hashimoto, Takuya, Konno, Akira, Harikane, Yuichi, Silverman, John D, Capak, Peter L

“…Abstract We present average stellar population properties and dark matter halo masses of z ∼ 2 Lyα emitters (LAEs) from spectral energy distribution fitting…”
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Large-scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4 by Taamoli, Sina, Mobasher, Bahram, Chartab, Nima, Darvish, Behnam, Weaver, John R., Hemmati, Shoubaneh, Casey, Caitlin M., Sattari, Zahra, Brammer, Gabriel, Capak, Peter L., Ilbert, Olivier, Kartaltepe, Jeyhan S., McCracken, Henry J., Moneti, Andrea, Sanders, David B., Scoville, Nicholas, Steinhardt, Charles L., Toft, Sune

“…To study the role of environment in galaxy evolution, we reconstruct the underlying density field of galaxies based on COSMOS2020 (The Farmer catalog) and…”
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A Machine-learning Approach to Predict Missing Flux Densities in Multiband Galaxy Surveys by Chartab, Nima, Mobasher, Bahram, Cooray, Asantha R., Hemmati, Shoubaneh, Sattari, Zahra, Ferguson, Henry C., Sanders, David B., Weaver, John R., Stern, Daniel K., McCracken, Henry J., Masters, Daniel C., Toft, Sune, Capak, Peter L., Davidzon, Iary, Dickinson, Mark E., Rhodes, Jason, Moneti, Andrea, Ilbert, Olivier, Zalesky, Lukas, McPartland, Conor J. R., Szapudi, István, Koekemoer, Anton M., Teplitz, Harry I., Giavalisco, Mauro

“…We present a new method based on information theory to find the optimal number of bands required to measure the physical properties of galaxies with desired…”
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An Alternate Approach to Measure Specific Star Formation Rates at by Davidzon, Iary, Ilbert, Olivier, Faisst, Andreas L., Sparre, Martin, Capak, Peter L.

“…We trace the specific star formation rate (sSFR) of massive star-forming galaxies ( ) from to 7. Our method is substantially different from previous analyses,…”
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The Recent Burstiness of Star Formation in Galaxies at z ∼ 4.5 from Hα Measurements by Faisst, Andreas L., Capak, Peter L., Emami, Najmeh, Tacchella, Sandro, Larson, Kirsten L.

“…The redshift range z  = 4–6 marks a transition phase between primordial and mature galaxy formation in which galaxies considerably increase their stellar mass,…”
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Are High-redshift Galaxies Hot? Temperature of z > 5 Galaxies and Implications for Their Dust Properties by Faisst, Andreas L., Capak, Peter L., Yan, Lin, Pavesi, Riccardo, Riechers, Dominik A., Bariši, Ivana, Cooke, Kevin C., Kartaltepe, Jeyhan S., Masters, Daniel C.

“…Recent studies have found a significant evolution and scatter in the relationship between the UV spectral slope (βUV) and the infrared excess (IRX; LIR/LUV) at…”
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SILVERRUSH. V. Census of Lyα, [O iii] λ5007, Hα, and [C ii] 158 μm Line Emission with ∼1000 LAEs at z = 4.9–7.0 Revealed with Subaru/HSC by Harikane, Yuichi, Ouchi, Masami, Shibuya, Takatoshi, Kojima, Takashi, Zhang, Haibin, Itoh, Ryohei, Ono, Yoshiaki, Higuchi, Ryo, Inoue, Akio K., Chevallard, Jacopo, Capak, Peter L., Nagao, Tohru, Onodera, Masato, Faisst, Andreas L., Martin, Crystal L., Rauch, Michael, Bruzual, Gustavo A., Charlot, Stephane, Davidzon, Iary, Fujimoto, Seiji, Hilmi, Miftahul, Ilbert, Olivier, Lee, Chien-Hsiu, Matsuoka, Yoshiki, Silverman, John D., Toft, Sune

“…We investigate Ly α , [O iii ] λ 5007, H α , and [C ii ] 158 μ m emission from 1124 galaxies at z  = 4.9–7.0. Our sample is composed of 1092 Ly α emitters…”
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The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array by Pavesi, Riccardo, Sharon, Chelsea E., Riechers, Dominik A., Hodge, Jacqueline A., Decarli, Roberto, Walter, Fabian, Carilli, Chris L., Daddi, Emanuele, Smail, Ian, Dickinson, Mark, Ivison, Rob J., Sargent, Mark, Cunha, Elisabete da, Aravena, Manuel, Darling, Jeremy, Smol i, Vernesa, Scoville, Nicholas Z., Capak, Peter L., Wagg, Jeff

“…We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line deep field targeting CO(1-0) emission from galaxies at z = 1.95-2.85…”
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ALMA IMAGING OF GAS AND DUST IN A GALAXY PROTOCLUSTER AT REDSHIFT 5.3: [C II] EMISSION IN “TYPICAL” GALAXIES AND DUSTY STARBURSTS ≈1 BILLION YEARS AFTER THE BIG BANG by Riechers, Dominik A., Carilli, Christopher L., Capak, Peter L., Scoville, Nicholas Z., Smolčić, Vernesa, Schinnerer, Eva, Yun, Min, Cox, Pierre, Bertoldi, Frank, Karim, Alexander, Yan, Lin

“…We report interferometric imaging of [C II]({sup 2} P {sub 3/2}→{sup 2} P {sub 1/2}) and OH({sup 2}Π{sub 1/2} J = 3/2→1/2) emission toward the center of the…”
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