Zobrazeno 1 - 10
of 23
pro vyhledávání: '"Kremin, Anthony"'
Autor:
Guo, Wei-Jian, Zou, Hu, Fawcett, Victoria Anne, Canning, Rebecca, Juneau, Stephanie, Davis, Tamara M., Alexander, David M., Jiang, Linhua, Aguilar, Jessica Nicole, Ahlen, Steven, Brooks, David, Claybaugh, Todd, de la Macorra, Axel, Doel, Peter, Fanning, Kevin, Forero-Romero, Jaime E., Gontcho, Satya Gontcho A, Honscheid, Klaus, Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Nie, Jundan, Pan, Zhiwei, Poppett, Claire, Prada, Francisco, Rezaie, Mehdi, Rossi, Graziano, Siudek, Małgorzata, Sanchez, Eusebio, Schubnell, Michael, Seo, Hee-Jong, Sui, Jipeng, Tarlé, Gregory, Zhou, Zhiming
Changing-look Active Galactic Nuclei (CL AGN) can be generally confirmed by the emergence (turn-on) or disappearance (turn-off) of broad emission lines, associated with a transient timescale (about $100\sim5000$ days) that is much shorter than predic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::12c0ebb810d1bc0809b80d456d3fe879
http://arxiv.org/abs/2307.08289
http://arxiv.org/abs/2307.08289
Autor:
Yu, Jiaxi, Zhao, Cheng, Gonzalez-Perez, Violeta, Chuang, Chia-Hsun, Brodzeller, Allyson, de Mattia, Arnaud, Kneib, Jean-Paul, Krolewski, Alex, Rocher, Antoine, Ross, Ashley, Wang, Yunchong, Yuan, Sihan, Zhang, Hanyu, Zhou, Rongpu, Aguilar, Jessica Nicole, Ahlen, Steven, Brooks, David, Dawson, Kyle, de la Macorra, Alex, Doel, Peter, Fanning, Kevin, Font-Ribera, Andreu, Forero-Romero, Jaime, Gontcho, Satya Gontcho A, Honscheid, Klaus, Kehoe, Robert, Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Manera, Marc, Martini, Paul, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Nie, Jundan, Percival, Will, Poppett, Claire, Raichoor, Anand, Rossi, Graziano, Seo, Hee-Jong, Tarlé, Gregory, Zhou, Zhimin, Zou, Hu
International audience; We perform a SubHalo Abundance Matching (SHAM) study with two algorithms: {$\sigma, V_{\rm ceil}, v_{\rm smear}$}-SHAM and {$\sigma, V_{\rm ceil},f_{\rm sat}$}-SHAM. These are designed to reproduce the clustering on 5--30$\,h^
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98425d6298e77e9403149416bc326588
https://hal.science/hal-04152145
https://hal.science/hal-04152145
Autor:
Miller, Timothy N., Doel, Peter, Gutierrez, Gaston, Besuner, Robert, Brooks, David, Gallo, Giuseppe, Heetderks, Henry, Jelinsky, Patrick, Kent, Stephen M., Lampton, Michael, Levi, Michael, Liang, Ming, Meisner, Aaron, Sholl, Michael J., Silber, Joseph Harry, Sprayberry, David, Aguilar, Jessica Nicole, de la Macorra, Axel, Eisenstein, Daniel, Fanning, Kevin, Font-Ribera, Andreu, Gaztanaga, Enrique, Gontcho, Satya Gontcho A, Honscheid, Klaus, Jimenez, Jorge, Joyce, Dick, Kehoe, Robert, Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Guillou, Laurent Le, Magneville, Christophe, Martini, Paul, Miquel, Ramon, Moustakas, John, Nie, Jundan, Percival, Will, Poppett, Claire, Prada, Francisco, Rossi, Graziano, Schlegel, David, Schubnell, Michael, Seo, Hee-Jong, Sharples, Ray, Tarle, Gregory, Vargas-Magana, Mariana, Zhou, Zhimin
The Dark Energy Spectroscopic Instrument (DESI) is currently measuring the spectra of 40\,million galaxies and quasars, the largest such survey ever made to probe the nature of cosmological dark energy. The 4-meter Mayall telescope at Kitt Peak Natio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a0a7968e1c2af3c85c0ccbed1e3ef79a
https://hal.science/hal-04143309
https://hal.science/hal-04143309
Autor:
Hahn, ChangHoon, Aguilar, Jessica Nicole, Alam, Shadab, Ahlen, Steven, Brooks, David, Cole, Shaun, de la Macorra, Axel, Doel, Peter, Font-Ribera, Andreu A., Forero-Romero, Jaime E., Gontcho, Satya Gontcho A, Honscheid, Klaus, Huang, Song, Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Manera, Marc, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Nie, Jundan, Poppett, Claire, Rossi, Graziano, Saintonge, Amélie, Sanchez, Eusebio, Saulder, Christoph, Schubnell, Michael, Seo, Hee-Jong, Siudek, Małgorzata, Speranza, Federico, Tarlé, Gregory, Weaver, Benjamin A., Wechsler, Risa H., Yuan, Sihan, Zhou, Zhimin, Zou, Hu
We present the probabilistic stellar mass function (pSMF) of galaxies in the DESI Bright Galaxy Survey (BGS), observed during the One-Percent Survey. The One-Percent Survey was one of DESI's survey validation programs conducted from April to May 2021
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f08484f5ab9057dcb893728fa692e23d
http://arxiv.org/abs/2306.06318
http://arxiv.org/abs/2306.06318
Autor:
Brodzeller, Allyson, Dawson, Kyle, Bailey, Stephen, Yu, Jiaxi, Ross, A. J., Bault, A., Filbert, S., Aguilar, J., Ahlen, S., Alexander, David M., Armengaud, E., Berti, A., Brooks, D., Chaussidon, E., de la Macorra, A., Doel, P., Fanning, K., Fawcett, V. A., Font-Ribera, A., Gontcho, S. Gontcho A, Guy, J., Honscheid, K., Juneau, S., Kehoe, R., Kisner, T., Kremin, Anthony, Lan, Ting-Wen, Landriau, M., Levi, Michael E., Magneville, C., Martini, Paul, Meisner, Aaron M., Miquel, R., Moustakas, J., Palanque-Delabrouille, N., Percival, W. J., Prada, F., Ravoux, C., Rossi, Graziano, Saulder, C., Siudek, M., Tarlé, Gregory, Weaver, B. A., Youles, S., Zheng, Zheng, Zhou, Rongpu, Zhou, Zhimin
Publikováno v:
Astron.J.
Astron.J., 2023, 166 (2), pp.66. ⟨10.3847/1538-3881/ace35d⟩
Astron.J., 2023, 166 (2), pp.66. ⟨10.3847/1538-3881/ace35d⟩
Millions of quasar spectra will be collected by the Dark Energy Spectroscopic Instrument (DESI), leading to a four-fold increase in the number of known quasars. High accuracy quasar classification is essential to tighten constraints on cosmological p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f06a36a12c58b4d359e30e92e3868472
https://hal.science/hal-04111799
https://hal.science/hal-04111799
Autor:
Krolewski, Alex, Percival, Will J., Ferraro, Simone, Chaussidon, Edmond, Rezaie, Mehdi, Aguilar, Jessica Nicole, Ahlen, Steven, Brooks, David, Dawson, Kyle, de la Macorra, Axel, Doel, Peter, Fanning, Kevin, Font-Ribera, Andreu, Gontcho, Satya Gontcho A, Guy, Julien, Honscheid, Klaus, Kehoe, Robert, Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Levi, Michael E., Martini, Paul, Meisner, Aaron M., Miquel, Ramon, Nie, Jundan, Poppett, Claire, Ross, Ashley J., Rossi, Graziano, Schubnell, Michael, Seo, Hee-Jong, Tarle, Gregory, Vargas-Magana, Mariana, Weaver, Benjamin Alan, Yeche, Christophe, Zhou, Rongpu, Zhou, Zhimin
We detect the cross-correlation between 2.7 million DESI quasar targets across 14,700 deg$^2$ (180 quasars deg$^{-2}$) and Planck 2018 CMB lensing at $\sim$30$\sigma$. We use the cross-correlation on very large scales to constrain local primordial no
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f3079423ac6a32e9c1df1fc356b926f
https://hal.science/hal-04110273
https://hal.science/hal-04110273
Autor:
Saulder, Christoph, Howlett, Cullan, Douglass, Kelly A., Said, Khaled, BenZvi, Segev, Ahlen, Steven, Aldering, Greg, Bailey, Stephen, Brooks, David, Davis, Tamara, de la Macorra, Axel, Dey, Arjun, Font-Ribera, Andreu, Forero-Romero, Jaime E., Gontcho, Satya Gontcho A, Honscheid, Klaus, Kim, Alex G., Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Levi, Michael E., Lucey, John, Meisner, Aaron M., Miquel, Ramon, Moustakas, John, Myers, Adam D., Palanque-Delabrouille, Nathalie, Percival, Will, Poppett, Claire, Prada, Francisco, Qin, Fei, Schubnell, Michael, Tarlé, Gregory, Magaña, Mariana Vargas, Weaver, Benjamin Alan, Zhou, Rongpu, Zhou, Zhimin, Zou, Hu
We describe the target selection and characteristics of the DESI Peculiar Velocity Survey, the largest survey of peculiar velocities (PVs) using both the fundamental plane (FP) of galaxies and the Tully-Fisher (TF) relationship planned to date. We de
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d3678db50700d1b6b3c206933cff5c39
https://hal.science/hal-04028629
https://hal.science/hal-04028629
Autor:
Yang, Jinyi, Fan, Xiaohui, Gupta, Ansh, Myers, Adam, Palanque-Delabrouille, Nathalie, Wang, Feige, Yèche, Christophe, Aguilar, Jessica Nicole, Ahlen, Steven, Alexander, David, Brooks, David, Dawson, Kyle, de la Macorra, Axel, Dey, Arjun, Dhungana, Govinda, Fanning, Kevin, Font-Ribera, Andreu, Gontcho, Satya, Guy, Julien, Honscheid, Klaus, Juneau, Stephanie, Kisner, Theodore, Kremin, Anthony, Le Guillou, Laurent, Levi, Michael, Magneville, Christophe, Martini, Paul, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Nie, Jundan, Percival, Will, Poppett, Claire, Prada, Francisco, Schlafly, Edward, Tarlé, Gregory, Magana, Mariana Vargas, Weaver, Benjamin Alan, Wechsler, Risa, Zhou, Rongpu, Zhou, Zhimin, Zou, Hu
We report the first results of a high-redshift ($z$ >~ 5) quasar survey using the Dark Energy Spectroscopic Instrument (DESI). As a DESI secondary target program, this survey is designed to carry out a systematic search and investigation of quasars a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_dedup_::28a91414bbe85cf19aa87259a60226cc
http://arxiv.org/abs/2302.01777
http://arxiv.org/abs/2302.01777
Autor:
Darragh-Ford, Elise, Wu, John F., Mao, Yao-Yuan, Wechsler, Risa H., Geha, Marla, Forero-Romero, Jaime E., Hahn, Changhoon, Kallivayalil, Nitya, Moustakas, John, Nadler, Ethan O., Nowotka, Marta, Peek, J.E.G., Tollerud, Erik J., Weiner, Benjamin, Aguilar, J., Ahlen, S., Brooks, D., Cooper, A.P., de la Macorra, A., Dey, A., Fanning, K., Font-Ribera, A., Gontcho A. Gontcho, S., Honscheid, K., Kisner, T., Kremin, Anthony, Landriau, M., Levi, Michael E., Martini, P., Meisner, Aaron M., Miquel, R., Myers, Adam D., Nie, Jundan, Palanque-Delabrouille, N., Percival, W.J., Prada, F., Schlegel, D., Schubnell, M., Tarlé, Gregory, Vargas-Magaña, M., Zhou, Zhimin, Zou, And H.
We introduce the DESI LOW-Z Secondary Target Survey, which combines the wide-area capabilities of the Dark Energy Spectroscopic Instrument (DESI) with an efficient, low-redshift target selection method. Our selection consists of a set of color and su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0b37d6f208d56c4b0ee00e115a587ce
https://hal.science/hal-03924230
https://hal.science/hal-03924230
Autor:
Moon, Jeongin, Valcin, David, Rashkovetskyi, Michael, Saulder, Christoph, Aguilar, Jessica Nicole, Ahlen, Steven, Alam, Shadab, Bailey, Stephen, Baltay, Charles, Blum, Robert, Brooks, David, Burtin, Etienne, Chaussidon, Edmond, Dawson, Kyle, de la Macorra, Axel, de Mattia, Arnaud, Dhungana, Govinda, Eisenstein, Daniel, Flaugher, Brenna, Font-Ribera, Andreu, Garcia-Quintero, Cristhian, Guy, Julien, Hanif, Malik Muhammad Sikandar, Honscheid, Klaus, Ishak, Mustapha, Kehoe, Robert, Kim, Sumi, Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Guillou, Laurent Le, Levi, Michael, Martini, Paul, McDonald, Patrick, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Myers, Adam, Nadathur, Seshadri, Neveux, Richard, Newman, Jeffrey A., Nie, Jundan, Padmanabhan, Nikhil, Palanque-Delabrouille, Nathalie, Percival, Will, Fernández, Alejandro Pérez, Poppett, Claire, Prada, Francisco, Ross, Ashley J., Rossi, Graziano, Seo, Hee-Jong, Tarlé, Gregory, Magana, Mariana Vargas, Variu, Andrei, Weaver, Benjamin Alan, White, Martin J., Yuan, Sihan, Zhao, Cheng, Zhou, Rongpu, Zhou, Zhimin, Zou, Hu
We present the first detection of the baryon acoustic oscillations (BAO) signal obtained using unblinded data collected during the initial two months of operations of the Stage-IV ground-based Dark Energy Spectroscopic Instrument (DESI). From a selec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b67e786eff86561c5f7263a5c0ee710