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1. ForestFlow: cosmological emulation of Lyman-$\alpha$ forest clustering from linear to nonlinear scales

Author: Chaves-Montero, J., Cabayol-Garcia, L., Lokken, M., Font-Ribera, A., Aguilar, J., Ahlen, S., Bianchi, D., Brooks, D., Claybaugh, T., Cole, S., de la Macorra, A., Ferraro, S., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Gutierrez, G., Honscheid, K., Kehoe, R., Kirkby, D., Kremin, A., Lambert, A., Landriau, M., Manera, M., Martini, P., Miquel, R., Muñoz-Gutiérrez, A., Niz, G., Pérez-Ràfols, I., Rossi, G., Sanchez, E., Schubnell, M., Sprayberry, D., Tarlé, G., and Weaver, B. A.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: On large scales, measurements of the Lyman-$\alpha$ forest offer insights into the expansion history of the Universe, while on small scales, these impose strict constraints on the growth history, the nature of dark matter, and the sum of neutrino masses. This work introduces ForestFlow, a cosmological emulator designed to bridge the gap between large- and small-scale Lyman-$\alpha$ forest analyses. Using conditional normalizing flows, ForestFlow emulates the 2 Lyman-$\alpha$ linear biases ($b_\delta$ and $b_\eta$) and 6 parameters describing small-scale deviations of the 3D flux power spectrum ($P_\mathrm{3D}$) from linear theory. These 8 parameters are modeled as a function of cosmology $\unicode{x2013}$ the small-scale amplitude and slope of the linear power spectrum $\unicode{x2013}$ and the physics of the intergalactic medium. Thus, in combination with a Boltzmann solver, ForestFlow can predict $P_\mathrm{3D}$ on arbitrarily large (linear) scales and the 1D flux power spectrum ($P_\mathrm{1D}$) $\unicode{x2013}$ the primary observable for small-scale analyses $\unicode{x2013}$ without the need for interpolation or extrapolation. Consequently, ForestFlow enables for the first time multiscale analyses. Trained on a suite of 30 fixed-and-paired cosmological hydrodynamical simulations spanning redshifts from $z=2$ to $4.5$, ForestFlow achieves $3$ and $1.5\%$ precision in describing $P_\mathrm{3D}$ and $P_\mathrm{1D}$ from linear scales to $k=5\,\mathrm{Mpc}^{-1}$ and $k_\parallel=4\,\mathrm{Mpc}^{-1}$, respectively. Thanks to its parameterization, the precision of the emulator is also similar for both ionization histories and two extensions to the $\Lambda$CDM model $\unicode{x2013}$ massive neutrinos and curvature $\unicode{x2013}$ not included in the training set. ForestFlow will be crucial for the cosmological analysis of Lyman-$\alpha$ forest measurements from the DESI survey., Comment: 17 pages, 11 figures. Submitted to A&A
Published: 2024

2. The Early Data Release of the Dark Energy Spectroscopic Instrument

Author: Collaboration, DESI, Adame, AG, Aguilar, J, Ahlen, S, Alam, S, Aldering, G, Alexander, DM, Alfarsy, R, Prieto, C Allende, Alvarez, M, Alves, O, Anand, A, Andrade-Oliveira, F, Armengaud, E, Asorey, J, Avila, S, Aviles, A, Bailey, S, Balaguera-Antolínez, A, Ballester, O, Baltay, C, Bault, A, Bautista, J, Behera, J, Beltran, SF, BenZvi, S, Silva, L Beraldo E, Bermejo-Climent, JR, Berti, A, Besuner, R, Beutler, F, Bianchi, D, Blake, C, Blum, R, Bolton, AS, Brieden, S, Brodzeller, A, Brooks, D, Brown, Z, Buckley-Geer, E, Burtin, E, Cabayol-Garcia, L, Cai, Z, Canning, R, Cardiel-Sas, L, Rosell, A Carnero, Castander, FJ, Cervantes-Cota, JL, Chabanier, S, Chaussidon, E, Chaves-Montero, J, Chen, S, Chen, X, Chuang, C, Claybaugh, T, Cole, S, Cooper, AP, Cuceu, A, Davis, TM, Dawson, K, de Belsunce, R, de la Cruz, R, de la Macorra, A, Della Costa, J, de Mattia, A, Demina, R, Demirbozan, U, DeRose, J, Dey, A, Dey, B, Dhungana, G, Ding, J, Ding, Z, Doel, P, Doshi, R, Douglass, K, Edge, A, Eftekharzadeh, S, Eisenstein, DJ, Elliott, A, Ereza, J, Escoffier, S, Fagrelius, P, Fan, X, Fanning, K, Fawcett, VA, Ferraro, S, Flaugher, B, Font-Ribera, A, Forero-Romero, JE, Forero-Sánchez, D, Frenk, CS, Gänsicke, BT, García, LÁ, García-Bellido, J, Garcia-Quintero, C, Garrison, LH, Gil-Marín, H, Golden-Marx, J, and Gontcho, S Gontcho A
Subjects: Astronomical Sciences, Physical Sciences, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics
Abstract: The Dark Energy Spectroscopic Instrument (DESI) completed its 5 month Survey Validation in 2021 May. Spectra of stellar and extragalactic targets from Survey Validation constitute the first major data sample from the DESI survey. This paper describes the public release of those spectra, the catalogs of derived properties, and the intermediate data products. In total, the public release includes good-quality spectral information from 466,447 objects targeted as part of the Milky Way Survey, 428,758 as part of the Bright Galaxy Survey, 227,318 as part of the Luminous Red Galaxy sample, 437,664 as part of the Emission Line Galaxy sample, and 76,079 as part of the Quasar sample. In addition, the release includes spectral information from 137,148 objects that expand the scope beyond the primary samples as part of a series of secondary programs. Here, we describe the spectral data, data quality, data products, Large-Scale Structure science catalogs, access to the data, and references that provide relevant background to using these spectra.
Published: 2024

3. DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Author: DESI Collaboration, Adame, A. G., Aguilar, J., Ahlen, S., Alam, S., Alexander, D. M., Alvarez, M., Alves, O., Anand, A., Andrade, U., Armengaud, E., Avila, S., Aviles, A., Awan, H., Bahr-Kalus, B., Bailey, S., Baltay, C., Bault, A., Behera, J., BenZvi, S., Bera, A., Beutler, F., Bianchi, D., Blake, C., Blum, R., Brieden, S., Brodzeller, A., Brooks, D., Buckley-Geer, E., Burtin, E., Calderon, R., Canning, R., Rosell, A. Carnero, Cereskaite, R., Cervantes-Cota, J. L., Chabanier, S., Chaussidon, E., Chaves-Montero, J., Chen, S., Chen, X., Claybaugh, T., Cole, S., Cuceu, A., Davis, T. M., Dawson, K., de la Macorra, A., de Mattia, A., Deiosso, N., Dey, A., Dey, B., Ding, Z., Doel, P., Edelstein, J., Eftekharzadeh, S., Eisenstein, D. J., Elliott, A., Fagrelius, P., Fanning, K., Ferraro, S., Ereza, J., Findlay, N., Flaugher, B., Font-Ribera, A., Forero-Sánchez, D., Forero-Romero, J. E., Frenk, C. S., Garcia-Quintero, C., Gaztañaga, E., Gil-Marín, H., Gontcho, S. Gontcho A, Gonzalez-Morales, A. X., Gonzalez-Perez, V., Gordon, C., Green, D., Gruen, D., Gsponer, R., Gutierrez, G., Guy, J., Hadzhiyska, B., Hahn, C., Hanif, M. M. S, Herrera-Alcantar, H. K., Honscheid, K., Howlett, C., Huterer, D., Iršič, V., Ishak, M., Juneau, S., Karaçaylı, N. G., Kehoe, R., Kent, S., Kirkby, D., Kremin, A., Krolewski, A., Lai, Y., Lan, T. -W., Landriau, M., Lang, D., Lasker, J., Goff, J. M. Le, Guillou, L. Le, Leauthaud, A., Levi, M. E., Li, T. S., Linder, E., Lodha, K., Magneville, C., Manera, M., Margala, D., Martini, P., Maus, M., McDonald, P., Medina-Varela, L., Meisner, A., Mena-Fernández, J., Miquel, R., Moon, J., Moore, S., Moustakas, J., Mudur, N., Mueller, E., Muñoz-Gutiérrez, A., Myers, A. D., Nadathur, S., Napolitano, L., Neveux, R., Newman, J. A., Nguyen, N. M., Nie, J., Niz, G., Noriega, H. E., Padmanabhan, N., Paillas, E., Palanque-Delabrouille, N., Pan, J., Penmetsa, S., Percival, W. J., Pieri, M. M., Pinon, M., Poppett, C., Porredon, A., Prada, F., Pérez-Fernández, A., Pérez-Ràfols, I., Rabinowitz, D., Raichoor, A., Ramírez-Pérez, C., Ramirez-Solano, S., Ravoux, C., Rashkovetskyi, M., Rezaie, M., Rich, J., Rocher, A., Rockosi, C., Roe, N. A., Rosado-Marin, A., Ross, A. J., Rossi, G., Ruggeri, R., Ruhlmann-Kleider, V., Samushia, L., Sanchez, E., Saulder, C., Schlafly, E. F., Schlegel, D., Schubnell, M., Seo, H., Shafieloo, A., Sharples, R., Silber, J., Slosar, A., Smith, A., Sprayberry, D., Tan, T., Tarlé, G., Taylor, P., Trusov, S., Ureña-López, L. A., Vaisakh, R., Valcin, D., Valdes, F., Vargas-Magaña, M., Verde, L., Walther, M., Wang, B., Wang, M. S., Weaver, B. A., Weaverdyck, N., Wechsler, R. H., Weinberg, D. H., White, M., Yu, J., Yu, Y., Yuan, S., Yèche, C., Zaborowski, E. A., Zarrouk, P., Zhang, H., Zhao, C., Zhao, R., Zhou, R., Zhuang, T., and Zou, H.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present cosmological results from the measurement of baryon acoustic oscillations (BAO) in galaxy, quasar and Lyman-$\alpha$ forest tracers from the first year of observations from the Dark Energy Spectroscopic Instrument (DESI), to be released in the DESI Data Release 1. DESI BAO provide robust measurements of the transverse comoving distance and Hubble rate, or their combination, relative to the sound horizon, in seven redshift bins from over 6 million extragalactic objects in the redshift range $0.1-1$ and $w_a<0$. This preference is 2.6$\sigma$ for the DESI+CMB combination, and persists or grows when SN~Ia are added in, giving results discrepant with the $\Lambda$CDM model at the $2.5\sigma$, $3.5\sigma$ or $3.9\sigma$ levels for the addition of Pantheon+, Union3, or DES-SN5YR datasets respectively. For the flat $\Lambda$CDM model with the sum of neutrino mass $\sum m_\nu$ free, combining the DESI and CMB data yields an upper limit $\sum m_\nu < 0.072$ $(0.113)$ eV at 95% confidence for a $\sum m_\nu>0$ $(\sum m_\nu>0.059)$ eV prior. These neutrino-mass constraints are substantially relaxed in models beyond $\Lambda$CDM. [Abridged.], Comment: This DESI Collaboration Key Publication is part of the 2024 publication series using the first year of observations (see https://data.desi.lbl.gov/doc/papers). 68 pages, 15 figures. Version accepted for publication in JCAP
Published: 2024

4. DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Author: DESI Collaboration, Adame, A. G., Aguilar, J., Ahlen, S., Alam, S., Alexander, D. M., Alvarez, M., Alves, O., Anand, A., Andrade, U., Armengaud, E., Avila, S., Aviles, A., Awan, H., Bailey, S., Baltay, C., Bault, A., Bautista, J., Behera, J., BenZvi, S., Beutler, F., Bianchi, D., Blake, C., Blum, R., Brieden, S., Brodzeller, A., Brooks, D., Buckley-Geer, E., Burtin, E., Calderon, R., Canning, R., Rosell, A. Carnero, Cereskaite, R., Cervantes-Cota, J. L., Chabanier, S., Chaussidon, E., Chaves-Montero, J., Chen, S., Chen, X., Claybaugh, T., Cole, S., Cuceu, A., Davis, T. M., Dawson, K., de la Cruz, R., de la Macorra, A., de Mattia, A., Deiosso, N., Dey, A., Dey, B., Ding, J., Ding, Z., Doel, P., Edelstein, J., Eftekharzadeh, S., Eisenstein, D. J., Elliott, A., Fagrelius, P., Fanning, K., Ferraro, S., Ereza, J., Findlay, N., Flaugher, B., Font-Ribera, A., Forero-Sánchez, D., Forero-Romero, J. E., Garcia-Quintero, C., Gaztañaga, E., Gil-Marín, H., Gontcho, S. Gontcho A, Gonzalez-Morales, A. X., Gonzalez-Perez, V., Gordon, C., Green, D., Gruen, D., Gsponer, R., Gutierrez, G., Guy, J., Hadzhiyska, B., Hahn, C., Hanif, M. M. S, Herrera-Alcantar, H. K., Honscheid, K., Howlett, C., Huterer, D., Iršič, V., Ishak, M., Juneau, S., Karaçayli, N. G., Kehoe, R., Kent, S., Kirkby, D., Kremin, A., Krolewski, A., Lai, Y., Lan, T. -W., Landriau, M., Lang, D., Lasker, J., Goff, J. M. Le, Guillou, L. Le, Leauthaud, A., Levi, M. E., Li, T. S., Linder, E., Lodha, K., Magneville, C., Manera, M., Margala, D., Martini, P., Maus, M., McDonald, P., Medina-Varela, L., Meisner, A., Mena-Fernández, J., Miquel, R., Moon, J., Moore, S., Moustakas, J., Mueller, E., Muñoz-Gutiérrez, A., Myers, A. D., Nadathur, S., Napolitano, L., Neveux, R., Newman, J. A., Nguyen, N. M., Nie, J., Niz, G., Noriega, H. E., Padmanabhan, N., Paillas, E., Palanque-Delabrouille, N., Pan, J., Penmetsa, S., Percival, W. J., Pieri, M. M., Pinon, M., Poppett, C., Porredon, A., Prada, F., Pérez-Fernández, A., Pérez-Ràfols, I., Rabinowitz, D., Raichoor, A., Ramírez-Pérez, C., Ramirez-Solano, S., Rashkovetskyi, M., Ravoux, C., Rezaie, M., Rich, J., Rocher, A., Rockosi, C., Roe, N. A., Rosado-Marin, A., Ross, A. J., Rossi, G., Ruggeri, R., Ruhlmann-Kleider, V., Samushia, L., Sanchez, E., Saulder, C., Schlafly, E. F., Schlegel, D., Schubnell, M., Seo, H., Sharples, R., Silber, J., Sinigaglia, F., Slosar, A., Smith, A., Sprayberry, D., Tan, T., Tarlé, G., Trusov, S., Vaisakh, R., Valcin, D., Valdes, F., Vargas-Magaña, M., Verde, L., Walther, M., Wang, B., Wang, M. S., Weaver, B. A., Weaverdyck, N., Wechsler, R. H., Weinberg, D. H., White, M., Yu, J., Yu, Y., Yuan, S., Yèche, C., Zaborowski, E. A., Zarrouk, P., Zhang, H., Zhao, C., Zhao, R., Zhou, R., and Zou, H.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the measurement of Baryon Acoustic Oscillations (BAO) from the Lyman-$\alpha$ (Ly$\alpha$) forest of high-redshift quasars with the first-year dataset of the Dark Energy Spectroscopic Instrument (DESI). Our analysis uses over $420\,000$ Ly$\alpha$ forest spectra and their correlation with the spatial distribution of more than $700\,000$ quasars. An essential facet of this work is the development of a new analysis methodology on a blinded dataset. We conducted rigorous tests using synthetic data to ensure the reliability of our methodology and findings before unblinding. Additionally, we conducted multiple data splits to assess the consistency of the results and scrutinized various analysis approaches to confirm their robustness. For a given value of the sound horizon ($r_d$), we measure the expansion at $z_{\rm eff}=2.33$ with 2\% precision, $H(z_{\rm eff}) = (239.2 \pm 4.8) (147.09~{\rm Mpc} /r_d)$ km/s/Mpc. Similarly, we present a 2.4\% measurement of the transverse comoving distance to the same redshift, $D_M(z_{\rm eff}) = (5.84 \pm 0.14) (r_d/147.09~{\rm Mpc})$ Gpc. Together with other DESI BAO measurements at lower redshifts, these results are used in a companion paper to constrain cosmological parameters., Comment: This DESI Collaboration Key Publication is part of the 2024 publication series using the first year of observations (see https://data.desi.lbl.gov/doc/papers). Minor changes in v4, version accepted for publication in JCAP
Published: 2024

5. DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

Author: DESI Collaboration, Adame, A. G., Aguilar, J., Ahlen, S., Alam, S., Alexander, D. M., Alvarez, M., Alves, O., Anand, A., Andrade, U., Armengaud, E., Avila, S., Aviles, A., Awan, H., Bailey, S., Baltay, C., Bault, A., Behera, J., BenZvi, S., Beutler, F., Bianchi, D., Blake, C., Blum, R., Brieden, S., Brodzeller, A., Brooks, D., Buckley-Geer, E., Burtin, E., Calderon, R., Canning, R., Rosell, A. Carnero, Cereskaite, R., Cervantes-Cota, J. L., Chabanier, S., Chaussidon, E., Chaves-Montero, J., Chen, S., Chen, X., Claybaugh, T., Cole, S., Cuceu, A., Davis, T. M., Dawson, K., de la Macorra, A., de Mattia, A., Deiosso, N., Dey, A., Dey, B., Ding, Z., Doel, P., Edelstein, J., Eftekharzadeh, S., Eisenstein, D. J., Elliott, A., Fagrelius, P., Fanning, K., Ferraro, S., Ereza, J., Findlay, N., Flaugher, B., Font-Ribera, A., Forero-Sánchez, D., Forero-Romero, J. E., Garcia-Quintero, C., Gaztañaga, E., Gil-Marín, H., Gontcho, S. Gontcho A, Gonzalez-Morales, A. X., Gonzalez-Perez, V., Gordon, C., Green, D., Gruen, D., Gsponer, R., Gutierrez, G., Guy, J., Hadzhiyska, B., Hahn, C., Hanif, M. M. S, Herrera-Alcantar, H. K., Honscheid, K., Howlett, C., Huterer, D., Iršič, V., Ishak, M., Juneau, S., Karaçaylı, N. G., Kehoe, R., Kent, S., Kirkby, D., Kremin, A., Krolewski, A., Lai, Y., Lan, T. -W., Landriau, M., Lang, D., Lasker, J., Goff, J. M. Le, Guillou, L. Le, Leauthaud, A., Levi, M. E., Li, T. S., Linder, E., Lodha, K., Magneville, C., Manera, M., Margala, D., Martini, P., Maus, M., McDonald, P., Medina-Varela, L., Meisner, A., Mena-Fernández, J., Miquel, R., Moon, J., Moore, S., Moustakas, J., Mudur, N., Mueller, E., Muñoz-Gutiérrez, A., Myers, A. D., Nadathur, S., Napolitano, L., Neveux, R., Newman, J. A., Nguyen, N. M., Nie, J., Niz, G., Noriega, H. E., Padmanabhan, N., Paillas, E., Palanque-Delabrouille, N., Pan, J., Penmetsa, S., Percival, W. J., Pieri, M., Pinon, M., Poppett, C., Porredon, A., Prada, F., Pérez-Fernández, A., Pérez-Ràfols, I., Rabinowitz, D., Raichoor, A., Ramírez-Pérez, C., Ramirez-Solano, S., Rashkovetskyi, M., Rezaie, M., Rich, J., Rocher, A., Rockosi, C., Roe, N. A., Rosado-Marin, A., Ross, A. J., Rossi, G., Ruggeri, R., Ruhlmann-Kleider, V., Samushia, L., Sanchez, E., Saulder, C., Schlafly, E. F., Schlegel, D., Schubnell, M., Seo, H., Sharples, R., Silber, J., Slosar, A., Smith, A., Sprayberry, D., Swanson, J., Tan, T., Tarlé, G., Trusov, S., Vaisakh, R., Valcin, D., Valdes, F., Vargas-Magaña, M., Verde, L., Walther, M., Wang, B., Wang, M. S., Weaver, B. A., Weaverdyck, N., Wechsler, R. H., Weinberg, D. H., White, M., Yu, J., Yu, Y., Yuan, S., Yèche, C., Zaborowski, E. A., Zarrouk, P., Zhang, H., Zhao, C., Zhao, R., Zhou, R., and Zou, H.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present the DESI 2024 galaxy and quasar baryon acoustic oscillations (BAO) measurements using over 5.7 million unique galaxy and quasar redshifts in the range 0.1
Published: 2024

6. Impact of Systematic Redshift Errors on the Cross-correlation of the Lyman-$\alpha$ Forest with Quasars at Small Scales Using DESI Early Data

Author: Bault, Abby, Kirkby, David, Guy, Julien, Brodzeller, Allyson, Aguilar, J., Ahlen, S., Bailey, S., Brooks, D., Cabayol-Garcia, L., Chaves-Montero, J., Claybaugh, T., Cuceu, A., Dawson, K., de la Cruz, R., de la Macorra, A., Dey, A., Doel, P., Filbert, S., Font-Ribera, A., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Gordon, C., Herrera-Alcantar, H. K., Honscheid, K., Iršič, V., Karaçaylı, N. G., Kehoe, R., Kisner, T., Kremin, A., Lambert, A., Landriau, M., Guillou, L. Le, Levi, M. E., Manera, M., Martini, P., Meisner, A., Miquel, R., Montero-Camacho, P., Moustakas, J., Muñoz-Gutiérrez, A., Nie, J., Niz, G., Palanque-Delabrouille, N., Percival, W. J., Poppett, C., Prada, F., Pérez-Ràfols, I., Ramírez-Pérez, C., Ravoux, C., Rezaie, M., Rossi, G., Sanchez, E., Schlafly, E. F., Schlegel, D., Schubnell, M., Silber, J., Tan, T., Tarlé, G., Walther, M., Weaver, B. A., and Zhou, Z.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Dark Energy Spectroscopic Instrument (DESI) will measure millions of quasar spectra by the end of its 5 year survey. Quasar redshift errors impact the shape of the Lyman-$\alpha$ forest correlation functions, which can affect cosmological analyses and therefore cosmological interpretations. Using data from the DESI Early Data Release and the first two months of the main survey, we measure the systematic redshift error from an offset in the cross-correlation of the Lyman-$\alpha$ forest with quasars. We find evidence for a redshift dependent bias causing redshifts to be underestimated with increasing redshift, stemming from improper modeling of the Lyman-$\alpha$ optical depth in the templates used for redshift estimation. New templates were derived for the DESI Year 1 quasar sample at $z > 1.6$ and we found the redshift dependent bias, $\Delta r_\parallel$, increased from $-1.94 \pm 0.15$ $h^{-1}$ Mpc to $-0.08 \pm 0.04$ $h^{-1}$ Mpc ($-205 \pm 15~\text{km s}^{-1}$ to $-9.0 \pm 4.0~\text{km s}^{-1}$). These new templates will be used to provide redshifts for the DESI Year 1 quasar sample., Comment: 29 pages, 9 figures, 5 tables
Published: 2024

7. Synthetic spectra for Lyman-$\alpha$ forest analysis in the Dark Energy Spectroscopic Instrument

Author: Herrera-Alcantar, Hiram K., Muñoz-Gutiérrez, Andrea, Tan, Ting, González-Morales, Alma X., Font-Ribera, Andreu, Guy, Julien, Moustakas, John, Kirkby, David, Armengaud, E., Bault, A., Cabayol-Garcia, L., Chaves-Montero, J., Cuceu, A., de la Cruz, R., García, L. Á., Gordon, C., Iršič, V., Karaçaylı, N. G., Goff, J. M. Le, Montero-Camacho, P., Niz, G., Pérez-Ràfols, I., Ramírez-Pérez, C., Ravoux, C., Walther, M., Aguilar, J., Ahlen, S., Brooks, D., Claybaugh, T., Dawson, K., de la Macorra, A., Doel, P., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Honscheid, K., Kehoe, R., Kisner, T., Landriau, M., Levi, Michael E., Manera, M., Martini, P., Meisner, A., Miquel, R., Nie, J., Palanque-Delabrouille, N., Poppett, C., Rezaie, M., Rossi, G., Sanchez, E., Seo, H., Tarlé, G., Weaver, B. A., and Zhou, Z.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Synthetic data sets are used in cosmology to test analysis procedures, to verify that systematic errors are well understood and to demonstrate that measurements are unbiased. In this work we describe the methods used to generate synthetic datasets of Lyman-$\alpha$ quasar spectra aimed for studies with the Dark Energy Spectroscopic Instrument (DESI). In particular, we focus on demonstrating that our simulations reproduces important features of real samples, making them suitable to test the analysis methods to be used in DESI and to place limits on systematic effects on measurements of Baryon Acoustic Oscillations (BAO). We present a set of mocks that reproduce the statistical properties of the DESI early data set with good agreement. Additionally, we use full survey synthetic data to forecast the BAO scale constraining power with DESI., Comment: 42 pages, 17 figures, 7 tables
Published: 2023

8. The miniJPAS survey: Maximising the photo-z accuracy from multi-survey datasets with probability conflation

Author: Hernán-Caballero, A., Akhlaghi, M., López-Sanjuan, C., Vázquez-Ramió, H., Laur, J., Varela, J., Civera, T., Muniesa, D., Finoguenov, A., Fernández-Ontiveros, J. A., Domínguez-Sánchez, H., Chaves-Montero, J., Fernández-Soto, A., Lumbreras-Calle, A., Díaz-García, L. A., del Pino, A., Delgado, R. M. González, Hernández-Monteagudo, C., Coelho, P., Jiménez-Teja, Y., Lopes, P. A. A., Marra, V., Tempel, E., Vílchez, J. M., Abramo, R., Alcaniz, J., Benítez, N., Bonoli, S., Carneiro, S., Cenarro, J., Cristóbal-Hornillos, D., Dupke, R., Ederoclite, A., Marín-Franch, A., de Oliveira, C. Mendes, Moles, M., Sodré Jr., L., and Taylor, K.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a new method for obtaining photometric redshifts (photo-z) for sources observed by multiple photometric surveys using a combination (conflation) of the redshift probability distributions (PDZs) obtained independently from each survey. The conflation of the PDZs has several advantages over the usual method of modelling all the photometry together, including modularity, speed, and accuracy of the results. Using a sample of galaxies with narrow-band photometry in 56 bands from J-PAS and deeper grizy photometry from the Hyper-SuprimeCam Subaru Strategic program (HSC-SSP), we show that PDZ conflation significantly improves photo-z accuracy compared to fitting all the photometry or using a weighted average of point estimates. The improvement over J-PAS alone is particularly strong for i>22 sources, which have low signal-to-noise ratio in the J-PAS bands. For the entire i<22.5 sample, we obtain a 64% (45%) increase in the number of sources with redshift errors |Dz|<0.003, a factor 3.3 (1.9) decrease in the normalised median absolute deviation of the errors (sigma_NMAD), and a factor 3.2 (1.3) decrease in the outlier rate compared to J-PAS (HSC-SSP) alone. The photo-z accuracy gains from combining the PDZs of J-PAS with a deeper broadband survey such as HSC-SSP are equivalent to increasing the depth of J-PAS observations by ~1.2--1.5 magnitudes. These results demonstrate the potential of PDZ conflation and highlight the importance of including the full PDZs in photo-z catalogues., Comment: 15 pages, 16 figures, 1 table. Accepted for publication in A&A
Published: 2023
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9. Optimal 1D Ly α forest power spectrum estimation – III. DESI early data

Author: Karaçaylı, Naim Göksel, Martini, Paul, Guy, Julien, Ravoux, Corentin, Karim, Marie Lynn Abdul, Armengaud, Eric, Walther, Michael, Aguilar, J, Ahlen, S, Bailey, S, Bautista, J, Beltran, SF, Brooks, D, Cabayol-Garcia, L, Chabanier, S, Chaussidon, E, Chaves-Montero, J, Dawson, K, de la Cruz, R, de la Macorra, A, Doel, P, Font-Ribera, A, Forero-Romero, JE, Gontcho, S Gontcho A, Gonzalez-Morales, AX, Gordon, C, Herrera-Alcantar, HK, Honscheid, K, Iršič, V, Ishak, M, Kehoe, R, Kisner, T, Kremin, A, Landriau, M, Le Guillou, L, Levi, ME, Lukić, Z, Meisner, A, Miquel, R, Moustakas, J, Mueller, E, Muñoz-Gutiérrez, A, Napolitano, L, Nie, J, Niz, G, Palanque-Delabrouille, N, Percival, WJ, Pieri, M, Poppett, C, Prada, F, Pérez-Ràfols, I, Ramírez-Pérez, C, Rossi, G, Sanchez, E, Seo, H, Sinigaglia, F, Tan, T, Tarlé, G, Wang, B, Weaver, BA, Yéche, C, and Zhou, Z
Subjects: Astronomical Sciences, Physical Sciences, methods: data analysis, intergalactic medium, quasars: absorption lines, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics, Space sciences
Abstract: The 1D power spectrum P1D of the Ly α forest provides important information about cosmological and astrophysical parameters, including constraints on warm dark matter models, the sum of the masses of the three neutrino species, and the thermal state of the intergalactic medium. We present the first measurement of P1D with the quadratic maximum likelihood estimator (QMLE) from the Dark Energy Spectroscopic Instrument (DESI) survey early data sample. This early sample of 54 600 quasars is already comparable in size to the largest previous studies, and we conduct a thorough investigation of numerous instrumental and analysis systematic errors to evaluate their impact on DESI data with QMLE. We demonstrate the excellent performance of the spectroscopic pipeline noise estimation and the impressive accuracy of the spectrograph resolution matrix with 2D image simulations of raw DESI images that we processed with the DESI spectroscopic pipeline. We also study metal line contamination and noise calibration systematics with quasar spectra on the red side of the Ly α emission line. In a companion paper, we present a similar analysis based on the Fast Fourier Transform estimate of the power spectrum. We conclude with a comparison of these two approaches and discuss the key sources of systematic error that we need to address with the upcoming DESI Year 1 analysis.
Published: 2024

10. Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument

Author: Collaboration, DESI, Adame, AG, Aguilar, J, Ahlen, S, Alam, S, Aldering, G, Alexander, DM, Alfarsy, R, Prieto, C Allende, Alvarez, M, Alves, O, Anand, A, Andrade-Oliveira, F, Armengaud, E, Asorey, J, Avila, S, Aviles, A, Bailey, S, Balaguera-Antolínez, A, Ballester, O, Baltay, C, Bault, A, Bautista, J, Behera, J, Beltran, SF, BenZvi, S, Silva, L Beraldo E, Bermejo-Climent, JR, Berti, A, Besuner, R, Beutler, F, Bianchi, D, Blake, C, Blum, R, Bolton, AS, Brieden, S, Brodzeller, A, Brooks, D, Brown, Z, Buckley-Geer, E, Burtin, E, Cabayol-Garcia, L, Cai, Z, Canning, R, Cardiel-Sas, L, Rosell, A Carnero, Castander, FJ, Cervantes-Cota, JL, Chabanier, S, Chaussidon, E, Chaves-Montero, J, Chen, S, Chen, X, Chuang, C, Claybaugh, T, Cole, S, Cooper, AP, Cuceu, A, Davis, TM, Dawson, K, de Belsunce, R, de la Cruz, R, de la Macorra, A, de Mattia, A, Demina, R, Demirbozan, U, DeRose, J, Dey, A, Dey, B, Dhungana, G, Ding, J, Ding, Z, Doel, P, Doshi, R, Douglass, K, Edge, A, Eftekharzadeh, S, Eisenstein, DJ, Elliott, A, Escoffier, S, Fagrelius, P, Fan, X, Fanning, K, Fawcett, VA, Ferraro, S, Ereza, J, Flaugher, B, Font-Ribera, A, Forero-Sánchez, D, Forero-Romero, JE, Frenk, CS, Gänsicke, BT, García, LÁ, García-Bellido, J, Garcia-Quintero, C, Garrison, LH, Gil-Marín, H, Golden-Marx, J, Gontcho, S Gontcho A, and Gonzalez-Morales, AX
Subjects: Astronomical Sciences, Physical Sciences, Astronomical and Space Sciences, Astronomy & Astrophysics, Astronomical sciences, Particle and high energy physics
Abstract: The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a survey covering 14,000 deg2 over 5 yr to constrain the cosmic expansion history through precise measurements of baryon acoustic oscillations (BAO). The scientific program for DESI was evaluated during a 5 month survey validation (SV) campaign before beginning full operations. This program produced deep spectra of tens of thousands of objects from each of the stellar Milky Way Survey (MWS), Bright Galaxy Survey (BGS), luminous red galaxy (LRG), emission line galaxy (ELG), and quasar target classes. These SV spectra were used to optimize redshift distributions, characterize exposure times, determine calibration procedures, and assess observational overheads for the 5 yr program. In this paper, we present the final target selection algorithms, redshift distributions, and projected cosmology constraints resulting from those studies. We also present a One-Percent Survey conducted at the conclusion of SV covering 140 deg2 using the final target selection algorithms with exposures of a depth typical of the main survey. The SV indicates that DESI will be able to complete the full 14,000 deg2 program with spectroscopically confirmed targets from the MWS, BGS, LRG, ELG, and quasar programs with total sample sizes of 7.2, 13.8, 7.46, 15.7, and 2.87 million, respectively. These samples will allow exploration of the Milky Way halo, clustering on all scales, and BAO measurements with a statistical precision of 0.28% over the redshift interval z < 1.1, 0.39% over the redshift interval 1.1 < z < 1.9, and 0.46% over the redshift interval 1.9 < z < 3.5.
Published: 2024

11. Optimal 1D Ly$\alpha$ Forest Power Spectrum Estimation -- III. DESI early data

Author: Karaçaylı, Naim Göksel, Martini, Paul, Guy, Julien, Ravoux, Corentin, Karim, Marie Lynn Abdul, Armengaud, Eric, Walther, Michael, Aguilar, J., Ahlen, S., Bailey, S., Bautista, J., Beltran, S. F., Brooks, D., Cabayol-Garcia, L., Chabanier, S., Chaussidon, E., Chaves-Montero, J., Dawson, K., de la Cruz, R., de la Macorra, A., Doel, P., Font-Ribera, A., Forero-Romero, J. E., Gontcho, S. Gontcho A, Gonzalez-Morales, A. X., Gordon, C., Herrera-Alcantar, H. K, Honscheid, K., Iršič, V., Ishak, M., Kehoe, R., Kisner, T., Kremin, A., Landriau, M., Guillou, L. Le, Levi, M. E., Lukić, Z., Meisner, A., Miquel, R., Moustakas, J., Mueller, E., Muñoz-Gutiérrez, A., Napolitano, L., Nie, J., Niz, G., Palanque-Delabrouille, N., Percival, W. J., Pieri, M., Poppett, C., Prada, F., Pérez-Ràfols, I., Ramírez-Pérez, C., Rossi, G., Sanchez, E., Seo, H., Sinigaglia, F., Tan, T., Tarlé, G., Wang, B., Weaver, B. A., Yèche, C., and Zhou, Z.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The one-dimensional power spectrum $P_{\mathrm{1D}}$ of the Ly$\alpha$ forest provides important information about cosmological and astrophysical parameters, including constraints on warm dark matter models, the sum of the masses of the three neutrino species, and the thermal state of the intergalactic medium. We present the first measurement of $P_{\mathrm{1D}}$ with the quadratic maximum likelihood estimator (QMLE) from the Dark Energy Spectroscopic Instrument (DESI) survey early data sample. This early sample of $54~600$ quasars is already comparable in size to the largest previous studies, and we conduct a thorough investigation of numerous instrumental and analysis systematic errors to evaluate their impact on DESI data with QMLE. We demonstrate the excellent performance of the spectroscopic pipeline noise estimation and the impressive accuracy of the spectrograph resolution matrix with two-dimensional image simulations of raw DESI images that we processed with the DESI spectroscopic pipeline. We also study metal line contamination and noise calibration systematics with quasar spectra on the red side of the Ly$\alpha$ emission line. In a companion paper, we present a similar analysis based on the Fast Fourier Transform estimate of the power spectrum. We conclude with a comparison of these two approaches and implications for the upcoming DESI Year 1 analysis., Comment: 23 pages, 20 figures. To be published in MNRAS
Published: 2023

12. The Lyman-$\alpha$ forest catalog from the Dark Energy Spectroscopic Instrument Early Data Release

Author: Ramírez-Pérez, César, Pérez-Ràfols, Ignasi, Font-Ribera, Andreu, Karim, M. Abdul, Armengaud, E., Bautista, J., Beltran, S. F., Cabayol-Garcia, L., Cai, Z., Chabanier, S., Chaussidon, E., Chaves-Montero, J., Cuceu, A., de la Cruz, R., García-Bellido, J., Gonzalez-Morales, A. X., Gordon, C., Herrera-Alcantar, H. K., Iršič, V., Ishak, M., Karaçaylı, N. G., Lukić, Zarija, Manser, C. J., Montero-Camacho, P., Napolitano, L., Niz, G., Pieri, M., Ravoux, C., Sinigaglia, F., Tan, T., Walther, M., Wang, B., Aguilar, J., Ahlen, S., Bailey, S., Brooks, D., Claybaugh, T., Dawson, K., de la Macorra, A., Dhungana, G., Doel, P., Fanning, K., Forero-Romero, J. E., Gontcho, S. Gontcho A, Guy, J., Honscheid, K., Kehoe, R., Kisner, T., Landriau, M., Guillou, L. Le, Levi, M. E., Magneville, C., Martini, P., Meisner, A., Miquel, R., Moustakas, J., Mueller, E., Muñoz-Gutiérrez, A., Nie, J., Palanque-Delabrouille, N., Percival, W. J., Rossi, G., Sanchez, E., Schlafly, E. F., Schlegel, D., Seo, H., Tarlé, G., Weaver, B. A., Yèche, C., and Zhou, Z.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present and validate the catalog of Lyman-$\alpha$ forest fluctuations for 3D analyses using the Early Data Release (EDR) from the Dark Energy Spectroscopic Instrument (DESI) survey. We used 88,511 quasars collected from DESI Survey Validation (SV) data and the first two months of the main survey (M2). We present several improvements to the method used to extract the Lyman-$\alpha$ absorption fluctuations performed in previous analyses from the Sloan Digital Sky Survey (SDSS). In particular, we modify the weighting scheme and show that it can improve the precision of the correlation function measurement by more than 20%. This catalog can be downloaded from https://data.desi.lbl.gov/public/edr/vac/edr/lya/fuji/v0.3 and it will be used in the near future for the first DESI measurements of the 3D correlations in the Lyman-$\alpha$ forest.
Published: 2023

13. The Early Data Release of the Dark Energy Spectroscopic Instrument

Author: DESI Collaboration, Adame, A. G., Aguilar, J., Ahlen, S., Alam, S., Aldering, G., Alexander, D. M., Alfarsy, R., Prieto, C. Allende, Alvarez, M., Alves, O., Anand, A., Andrade-Oliveira, F., Armengaud, E., Asorey, J., Avila, S., Aviles, A., Bailey, S., Balaguera-Antolínez, A., Ballester, O., Baltay, C., Bault, A., Bautista, J., Behera, J., Beltran, S. F., BenZvi, S., Silva, L. Beraldo e, Bermejo-Climent, J. R., Berti, A., Besuner, R., Beutler, F., Bianchi, D., Blake, C., Blum, R., Bolton, A. S., Brieden, S., Brodzeller, A., Brooks, D., Brown, Z., Buckley-Geer, E., Burtin, E., Cabayol-Garcia, L., Cai, Z., Canning, R., Cardiel-Sas, L., Rosell, A. Carnero, Castander, F. J., Cervantes-Cota, J. L., Chabanier, S., Chaussidon, E., Chaves-Montero, J., Chen, S., Chen, X., Chuang, C., Claybaugh, T., Cole, S., Cooper, A. P., Cuceu, A., Davis, T. M., Dawson, K., de Belsunce, R., de la Cruz, R., de la Macorra, A., Della Costa, J., de Mattia, A., Demina, R., Demirbozan, U., DeRose, J., Dey, A., Dey, B., Dhungana, G., Ding, J., Ding, Z., Doel, P., Doshi, R., Douglass, K., Edge, A., Eftekharzadeh, S., Eisenstein, D. J., Elliott, A., Escoffier, S., Fagrelius, P., Fan, X., Fanning, K., Fawcett, V. A., Ferraro, S., Ereza, J., Flaugher, B., Font-Ribera, A., Forero-Sánchez, D., Forero-Romero, J. E., Frenk, C. S., Gänsicke, B. T., García, L. Á., García-Bellido, J., Garcia-Quintero, C., Garrison, L. H., Gil-Marín, H., Golden-Marx, J., Gontcho, S. Gontcho A, Gonzalez-Morales, A. X., Gonzalez-Perez, V., Gordon, C., Graur, O., Green, D., Gruen, D., Guy, J., Hadzhiyska, B., Hahn, C., Han, J. J., Hanif, M. M. S, Herrera-Alcantar, H. K., Honscheid, K., Hou, J., Howlett, C., Huterer, D., Iršič, V., Ishak, M., Jacques, A., Jana, A., Jiang, L., Jimenez, J., Jing, Y. P., Joudaki, S., Jullo, E., Juneau, S., Kizhuprakkat, N., Karaçaylı, N. G., Karim, T., Kehoe, R., Kent, S., Khederlarian, A., Kim, S., Kirkby, D., Kisner, T., Kitaura, F., Kneib, J., Koposov, S. E., Kovács, A., Kremin, A., Krolewski, A., L'Huillier, B., Lahav, O., Lambert, A., Lamman, C., Lan, T. -W., Landriau, M., Lang, D., Lange, J. U., Lasker, J., Leauthaud, A., Guillou, L. Le, Levi, M. E., Li, T. S., Linder, E., Lyons, A., Magneville, C., Manera, M., Manser, C. J., Margala, D., Martini, P., McDonald, P., Medina, G. E., Medina-Varela, L., Meisner, A., Mena-Fernández, J., Meneses-Rizo, J., Mezcua, M., Miquel, R., Montero-Camacho, P., Moon, J., Moore, S., Moustakas, J., Mueller, E., Mundet, J., Muñoz-Gutiérrez, A., Myers, A. D., Nadathur, S., Napolitano, L., Neveux, R., Newman, J. A., Nie, J., Nikutta, R., Niz, G., Norberg, P., Noriega, H. E., Paillas, E., Palanque-Delabrouille, N., Palmese, A., Zhiwei, P., Parkinson, D., Penmetsa, S., Percival, W. J., Pérez-Fernández, A., Pérez-Ràfols, I., Pieri, M., Poppett, C., Porredon, A., Pothier, S., Prada, F., Pucha, R., Raichoor, A., Ramírez-Pérez, C., Ramirez-Solano, S., Rashkovetskyi, M., Ravoux, C., Rocher, A., Rockosi, C., Ross, A. J., Rossi, G., Ruggeri, R., Ruhlmann-Kleider, V., Sabiu, C. G., Said, K., Saintonge, A., Samushia, L., Sanchez, E., Saulder, C., Schaan, E., Schlafly, E. F., Schlegel, D., Scholte, D., Schubnell, M., Seo, H., Shafieloo, A., Sharples, R., Sheu, W., Silber, J., Sinigaglia, F., Siudek, M., Slepian, Z., Smith, A., Soumagnac, M. T., Sprayberry, D., Stephey, L., Suárez-Pérez, J., Sun, Z., Tan, T., Tarlé, G., Tojeiro, R., Ureña-López, L. A., Vaisakh, R., Valcin, D., Valdes, F., Valluri, M., Vargas-Magaña, M., Variu, A., Verde, L., Walther, M., Wang, B., Wang, M. S., Weaver, B. A., Weaverdyck, N., Wechsler, R. H., White, M., Xie, Y., Yang, J., Yèche, C., Yu, J., Yuan, S., Zhang, H., Zhang, Z., Zhao, C., Zheng, Z., Zhou, R., Zhou, Z., Zou, H., Zou, S., and Zu, Y.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Dark Energy Spectroscopic Instrument (DESI) completed its five-month Survey Validation in May 2021. Spectra of stellar and extragalactic targets from Survey Validation constitute the first major data sample from the DESI survey. This paper describes the public release of those spectra, the catalogs of derived properties, and the intermediate data products. In total, the public release includes good-quality spectral information from 466,447 objects targeted as part of the Milky Way Survey, 428,758 as part of the Bright Galaxy Survey, 227,318 as part of the Luminous Red Galaxy sample, 437,664 as part of the Emission Line Galaxy sample, and 76,079 as part of the Quasar sample. In addition, the release includes spectral information from 137,148 objects that expand the scope beyond the primary samples as part of a series of secondary programs. Here, we describe the spectral data, data quality, data products, Large-Scale Structure science catalogs, access to the data, and references that provide relevant background to using these spectra., Comment: 43 pages, 7 figures, 17 tables, accepted for publication in the Astronomical Journal
Published: 2023
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14. Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument

Author: DESI Collaboration, Adame, A. G., Aguilar, J., Ahlen, S., Alam, S., Aldering, G., Alexander, D. M., Alfarsy, R., Prieto, C. Allende, Alvarez, M., Alves, O., Anand, A., Andrade-Oliveira, F., Armengaud, E., Asorey, J., Avila, S., Aviles, A., Bailey, S., Balaguera-Antolínez, A., Ballester, O., Baltay, C., Bault, A., Bautista, J., Behera, J., Beltran, S. F., BenZvi, S., Silva, L. Beraldo e, Bermejo-Climent, J. R., Berti, A., Besuner, R., Beutler, F., Bianchi, D., Blake, C., Blum, R., Bolton, A. S., Brieden, S., Brodzeller, A., Brooks, D., Brown, Z., Buckley-Geer, E., Burtin, E., Cabayol-Garcia, L., Cai, Z., Canning, R., Cardiel-Sas, L., Rosell, A. Carnero, Castander, F. J., Cervantes-Cota, J. L., Chabanier, S., Chaussidon, E., Chaves-Montero, J., Chen, S., Chuang, C., Claybaugh, T., Cole, S., Cooper, A. P., Cuceu, A., Davis, T. M., Dawson, K., de Belsunce, R., de la Cruz, R., de la Macorra, A., de Mattia, A., Demina, R., Demirbozan, U., DeRose, J., Dey, A., Dey, B., Dhungana, G., Ding, J., Ding, Z., Doel, P., Doshi, R., Douglass, K., Edge, A., Eftekharzadeh, S., Eisenstein, D. J., Elliott, A., Escoffier, S., Fagrelius, P., Fan, X., Fanning, K., Fawcett, V. A., Ferraro, S., Ereza, J., Flaugher, B., Font-Ribera, A., Forero-Sánchez, D., Forero-Romero, J. E., Frenk, C. S., Gänsicke, B. T., García, L. Á., García-Bellido, J., Garcia-Quintero, C., Garrison, L. H., Gil-Marín, H., Golden-Marx, J., Gontcho, S. Gontcho A, Gonzalez-Morales, A. X., Gonzalez-Perez, V., Gordon, C., Graur, O., Green, D., Gruen, D., Guy, J., Hadzhiyska, B., Hahn, C., Han, J. J., Hanif, M. M. S, Herrera-Alcantar, H. K., Honscheid, K., Hou, J., Howlett, C., Huterer, D., Iršič, V., Ishak, M., Jana, A., Jiang, L., Jimenez, J., Jing, Y. P., Joudaki, S., Joyce, R., Jullo, E., Juneau, S., Kizhuprakkat, N., Karaçaylı, N. G., Karim, T., Kehoe, R., Kent, S., Khederlarian, A., Kim, S., Kirkby, D., Kisner, T., Kitaura, F., Kneib, J., Koposov, S. E., Kovács, A., Kremin, A., Krolewski, A., L'Huillier, B., Lahav, O., Lambert, A., Lamman, C., Lan, T. -W., Landriau, M., Lang, D., Lange, J. U., Lasker, J., Guillou, L. Le, Leauthaud, A., Levi, M. E., Li, T. S., Linder, E., Lyons, A., Magneville, C., Manera, M., Manser, C. J., Margala, D., Martini, P., McDonald, P., Medina, G. E., Medina-Varela, L., Meisner, A., Mena-Fernández, J., Meneses-Rizo, J., Mezcua, M., Miquel, R., Montero-Camacho, P., Moon, J., Moore, S., Moustakas, J., Mueller, E., Mundet, J., Muñoz-Gutiérrez, A., Myers, A. D., Nadathur, S., Napolitano, L., Neveux, R., Newman, J. A., Nie, J., Niz, G., Norberg, P., Noriega, H. E., Paillas, E., Palanque-Delabrouille, N., Palmese, A., Zhiwei, P., Parkinson, D., Penmetsa, S., Percival, W. J., Pérez-Fernández, A., Pérez-Ràfols, I., Pieri, M., Poppett, C., Porredon, A., Prada, F., Pucha, R., Raichoor, A., Ramírez-Pérez, C., Ramirez-Solano, S., Rashkovetskyi, M., Ravoux, C., Rocher, A., Rockosi, C., Ross, A. J., Rossi, G., Ruggeri, R., Ruhlmann-Kleider, V., Sabiu, C. G., Said, K., Saintonge, A., Samushia, L., Sanchez, E., Saulder, C., Schaan, E., Schlafly, E. F., Schlegel, D., Scholte, D., Schubnell, M., Seo, H., Shafieloo, A., Sharples, R., Sheu, W., Silber, J., Sinigaglia, F., Siudek, M., Slepian, Z., Smith, A., Sprayberry, D., Stephey, L., Suárez-Pérez, J., Sun, Z., Tan, T., Tarlé, G., Tojeiro, R., Ureña-López, L. A., Vaisakh, R., Valcin, D., Valdes, F., Valluri, M., Vargas-Magaña, M., Variu, A., Verde, L., Walther, M., Wang, B., Wang, M. S., Weaver, B. A., Weaverdyck, N., Wechsler, R. H., White, M., Xie, Y., Yang, J., Yèche, C., Yu, J., Yuan, S., Zhang, H., Zhang, Z., Zhao, C., Zheng, Z., Zhou, R., Zhou, Z., Zou, H., Zou, S., and Zu, Y.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a survey covering 14,000 deg$^2$ over five years to constrain the cosmic expansion history through precise measurements of Baryon Acoustic Oscillations (BAO). The scientific program for DESI was evaluated during a five month Survey Validation (SV) campaign before beginning full operations. This program produced deep spectra of tens of thousands of objects from each of the stellar (MWS), bright galaxy (BGS), luminous red galaxy (LRG), emission line galaxy (ELG), and quasar target classes. These SV spectra were used to optimize redshift distributions, characterize exposure times, determine calibration procedures, and assess observational overheads for the five-year program. In this paper, we present the final target selection algorithms, redshift distributions, and projected cosmology constraints resulting from those studies. We also present a `One-Percent survey' conducted at the conclusion of Survey Validation covering 140 deg$^2$ using the final target selection algorithms with exposures of a depth typical of the main survey. The Survey Validation indicates that DESI will be able to complete the full 14,000 deg$^2$ program with spectroscopically-confirmed targets from the MWS, BGS, LRG, ELG, and quasar programs with total sample sizes of 7.2, 13.8, 7.46, 15.7, and 2.87 million, respectively. These samples will allow exploration of the Milky Way halo, clustering on all scales, and BAO measurements with a statistical precision of 0.28% over the redshift interval $z<1.1$, 0.39% over the redshift interval $1.1
Published: 2023
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15. Active galactic nuclei and gravitational redshifts

Author: Padilla, N. D., Carneiro, S., Chaves-Montero, J., Donzelli, C. J., Pigozzo, C., Colazo, P., and Alcaniz, J. S.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Context: Gravitational redshift is a classical effect of Einstein's General Relativity, already measured in stars, quasars and clusters of galaxies. Aims: We here aim to identify the signature of gravitational redshift in the emission lines of active galaxies due to supermassive black holes, and compare to what is found for inactive galaxies. Methods: Using the virial theorem, we estimate gravitational redshifts for quasars from the 14th data release of the Sloan Digital Sky Survey, and compare these with measured ones from the difference between the redshifts of emission lines of Sydney Australian Astronomical Observatory Multi-object Integral Field (SAMI) galaxies in central and outer annuli of their integral field spectra. Results: Firstly, from the full width at half maximum of $H_\beta$ lines of 57 Seyfert type I galaxies of the AGN Black Hole Mass Database, we derive a median gravitational redshift $z_g = 1.18 \times 10^{-4}$. Expanding this analysis to 86755 quasars from DR14 of SDSS we have a median value $z_g = 1.52 \times 10^{-4}$. Then, by comparing the redshifts of $34$ lines measured at central and outer regions of LINER galaxies in the SAMI survey we obtain $z_g = (0.68 \pm 0.09) \times 10^{-4}$, which increases to $z_g = (1.0 \pm 0.1) \times 10^{-4}$ when using $H_\alpha$ and $H_\beta$ lines. These numbers are compatible with central black holes of $\approx 10^9$ solar masses and broad line regions of $\approx 1$pc. For non-AGN galaxies the gravitational redshift is compatible with zero., Comment: Accepted for publication in A&A, 7 pages, 6 figures
Published: 2023
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16. The miniJPAS survey: AGN & host galaxy co-evolution of X-ray selected sources

Author: López, I. E., Brusa, M., Bonoli, S., Shankar, F., Acharya, N., Laloux, B., Dolag, K., Georgakakis, A., Lapi, A., Almeida, C. Ramos, Salvato, M., Chaves-Montero, J., Coelho, P., Díaz-García, L. A., Fernández-Ontiveros, J. A., Hernán-Caballero, A., Delgado, R. M. González, Marquez, I., Pović, M., Soria, R., Queiroz, C., Rahna, P. T., Abramo, R., Alcaniz, J., Benitez, N., Carneiro, S., Cenarro, J., Cristóbal-Hornillos, D., Dupke, R., Ederoclite, A., López-Sanjuan, C., Marín-Franch, A., de Oliveira, C. Mendes, Moles, M., Sodré Jr, L., Taylor, K., Varela, J., and Ramió, H. V.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Studies indicate strong evidence of a scaling relation in the local Universe between the supermassive black hole mass ($M_\rm{BH}$) and the stellar mass of their host galaxies ($M_\star$). They even show similar histories across cosmic times of their differential terms: star formation rate (SFR) and black hole accretion rate (BHAR). However, a clear picture of this coevolution is far from being understood. We select an X-ray sample of active galactic nuclei (AGN) up to $z=2.5$ in the miniJPAS footprint. Their X-ray to infrared spectral energy distributions (SEDs) have been modeled with CIGALE, constraining the emission to 68 bands. For a final sample of 308 galaxies, we derive their physical properties (e.g., $M_\star$, $\rm{SFR}$, $\rm{SFH}$, and $L_\rm{AGN}$). We also fit their optical spectra for a subsample of 113 sources to estimate the $M_\rm{BH}$. We calculate the BHAR depending on two radiative efficiency regimes. We find that the Eddington ratios ($\lambda$) and its popular proxy ($L_\rm{X}$/$M_\star$) have 0.6 dex of difference, and a KS-test indicates that they come from different distributions. Our sources exhibit a considerable scatter on the $M_\rm{BH}$-$M_\star$ relation, which can explain the difference between $\lambda$ and its proxy. We also model three evolution scenarios to recover the integral properties at $z=0$. Using the SFR and BHAR, we show a notable diminution in the scattering between $M_\rm{BH}$-$M_\star$. For the last scenario, we consider the SFH and a simple energy budget for the AGN accretion, obtaining a relation similar to the local Universe. Our study covers $\sim 1$ deg$^2$ in the sky and is sensitive to biases in luminosity. Nevertheless, we show that, for bright sources, the link between SFR and BHAR, and their decoupling based on an energy limit is the key that leads to the local $M_\rm{BH}$-$M_\star$ scaling relation., Comment: Accepted for publication in A&A
Published: 2023
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17. J-NEP: 60-band photometry and photometric redshifts for the James Webb Space Telescope North Ecliptic Pole Time-Domain Field

Author: Hernán-Caballero, A., Willmer, C. N. A., Varela, J., López-Sanjuan, C., Marín-Franch, A., Ramió, H. Vázquez, Civera, T., Ederoclite, A., Muniesa, D., Cenarro, J., Bonoli, S., Dupke, R., Lim, J., Chaves-Montero, J., Laur, J., Hernández-Monteagudo, C., Fernández-Ontiveros, J. A., Fernández-Soto, A., Díaz-García, L. A., Delgado, R. M. González, Queiroz, C., Vílchez, J. M., Abramo, R., Alcaniz, J., Benítez, N., Carneiro, S., Cristóbal-Hornillos, D., de Oliveira, C. Mendes, Moles, M., Sodré Jr., L., and Taylor, K.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: The J-PAS survey will observe ~1/3 of the northern sky with a set of 56 narrow-band filters using the dedicated 2.55 m JST telescope at the Javalambre Astrophysical Observatory. Prior to the installation of the main camera, in order to demonstrate the scientific potential of J-PAS, two small surveys were performed with the single-CCD Pathfinder camera: miniJPAS (~1 deg2 along the Extended Groth Strip), and J-NEP (~0.3 deg2 around the JWST North Ecliptic Pole Time Domain Field), including all 56 J-PAS filters as well as u, g, r, and i. J-NEP is ~0.5-1.0 magnitudes deeper than miniJPAS, providing photometry for 24,618 r-band detected sources and photometric redshifts (photo-z) for the 6,662 sources with r<23. In this paper we describe the photometry and photo-z of J-NEP and demonstrate a new method for the removal of systematic offsets in the photometry based on the median colours of galaxies, dubbed "galaxy locus recalibration". This method does not require spectroscopic observations except in a few reference pointings and, unlike previous methods, is applicable to the whole J-PAS survey. We use a spectroscopic sample of 787 galaxies to test the photo-z performance for J-NEP and in comparison to miniJPAS. We find that the deeper J-NEP observations result in a factor ~1.5-2 decrease in sigma_NMAD (a robust estimate of the standard deviation of the photo-z error) and the outlier rate relative to miniJPAS for r>21.5 sources, but no improvement in brighter ones. We find the same relation between sigma_NMAD and odds in J-NEP and miniJPAS, suggesting sigma_NMAD can be predicted for any set of J-PAS sources from their odds distribution alone, with no need for additional spectroscopy to calibrate the relation. We explore the causes for photo-z outliers and find that colour-space degeneracy at low S/N, photometry artifacts, source blending, and exotic spectra are the most important factors., Comment: 16 pages, 25 figures, accepted for publication in Astronomy and Astrophysics
Published: 2023
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18. TOPz: Photometric redshifts for J-PAS

Author: Laur, J., Tempel, E., Tamm, A., Kipper, R., Liivamägi, L. J., Hernán-Caballero, A., Muru, M. M., Chaves-Montero, J., Díaz-García, L. A., Turner, S., Tuvikene, T., Queiroz, C., Bom, C. R., Fernández-Ontiveros, J. A., Delgado, R. M. González, Civera, T., Abramo, R., Alcaniz, J., Benitez, N., Bonoli, S., Carneiro, S., Cenarro, J., Cristóbal-Hornillos, D., Dupke, R., Ederoclite, A., López-Sanjuan, C., Marín-Franch, A., de Oliveira, C. M., Moles, M., Sodré Jr, L., Taylor, K., Varela, J., and Ramió, H. V.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The importance of photometric galaxy redshift estimation is rapidly increasing with the development of specialised powerful observational facilities. We develop a new photometric redshift estimation workflow TOPz to provide reliable and efficient redshift estimations for the upcoming large-scale survey J-PAS which will observe 8500 deg2 of the northern sky through 54 narrow-band filters. TOPz relies on template-based photo-z estimation with some added J-PAS specific features and possibilities. We present TOPz performance on data from the miniJPAS survey, a precursor to the J-PAS survey with an identical filter system. First, we generated spectral templates based on the miniJPAS sources using the synthetic galaxy spectrum generation software CIGALE. Then we applied corrections to the input photometry by minimising systematic offsets from the template flux in each filter. To assess the accuracy of the redshift estimation, we used spectroscopic redshifts from the DEEP2, DEEP3, and SDSS surveys, available for 1989 miniJPAS galaxies with r < 22 magAB. We also tested how the choice and number of input templates, photo-z priors, and photometric corrections affect the TOPz redshift accuracy. The general performance of the combination of miniJPAS data and the TOPz workflow fulfills the expectations for J-PAS redshift accuracy. Similarly to previous estimates, we find that 38.6% of galaxies with r < 22 mag reach the J-PAS redshift accuracy goal of dz/(1 + z) < 0.003. Limiting the number of spectra in the template set improves the redshift accuracy up to 5%, especially for fainter, noise-dominated sources. Further improvements will be possible once the actual J-PAS data become available., Comment: 20 pages, 24 figures
Published: 2022
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19. CDK9 inhibition as an effective therapy for small cell lung cancer

Author: Valdez Capuccino, L., Kleitke, T., Szokol, B., Svajda, L., Martin, F., Bonechi, F., Krekó, M., Azami, S., Montinaro, A., Wang, Y., Nikolov, V., Kaiser, L., Bonasera, D., Saggau, J., Scholz, T., Schmitt, A., Beleggia, F., Reinhardt, H. C., George, J., Liccardi, G., Walczak, H., Tóvári, J., Brägelmann, J., Montero, J., Sos, M. L., Őrfi, L., and Peltzer, N.
Published: 2024
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20. The miniJPAS survey: the photometric redshift catalogue

Author: Hernán-Caballero, A., Varela, J., López-Sanjuan, C., Muniesa, D., Civera, T., Chaves-Montero, J., Díaz-García, L. A., Laur, J., Hernández-Monteagudo, C., Abramo, R., Angulo, R., Cristóbal-Hornillos, D., González-Delgado, R. M., Greisel, N., Orsi, A., Queiroz, C., Sobral, D., Tamm, A., Tempel, E., Vázquez-Ramió, H., Alcaniz, J., Benítez, N., Bonoli, S., Carneiro, S., Cenarro, J., Dupke, R., Ederoclite, A., Marín-Frach, A., de Oliveira, C. Mendes, Moles, M., Sodr, L., Taylor, K., and Cypriano, E. S.
Subjects: Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: MiniJPAS is a ~1 deg^2 imaging survey of the AEGIS field in 60 bands, performed to demonstrate the scientific potential of the upcoming JPAS survey. Full coverage of the 3800-9100 \AA range with 54 narrow and 6 broad optical filters allow for extremely accurate photo-z, which applied over 1000s of deg^2 will enable new applications of the photo-z technique such as measurement of baryonic acoustic oscillations. In this paper we describe the method used to obtain the photo-z included in the publicly available miniJPAS catalogue, and characterise the photo-z performance. We build 100 \AA resolution photo-spectra from the PSF-corrected forced-aperture photometry. Systematic offsets in the photometry are corrected by applying magnitude shifts obtained through iterative fitting with stellar population synthesis models. We compute photo-z with a customised version of LePhare, using a set of templates optimised for the J-PAS filter-set. We analyse the accuracy of miniJPAS photo-z and their dependence on multiple quantities using a subsample of 5,266 galaxies with spectroscopic redshifts from SDSS and DEEP, that we find to be representative of the whole r<23 miniJPAS sample. Formal uncertainties for the photo-z that are calculated with the \delta\chi^2 method underestimate the actual redshift errors. The odds parameter has the stronger correlation with |Dz|, and accurately reproduces the probability of a redshift outlier (|Dz|>0.03) irrespective of the magnitude, redshift, or spectral type of the sources. We show that the two main summary statistics characterising the photo-z accuracy for a population of galaxies (snmad and \eta) can be predicted by the distribution of odds in such population, and use this to estimate them for the whole miniJPAS sample. At r<23 there are 17,500 galaxies/deg^2 with valid photo-z estimates, of which 4,200 are expected to have |Dz|<0.003 (abridged)., Comment: 25 pages, 32 figures, 5 tables, accepted for publication in A&A
Published: 2021
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21. Clozapine but not lithium reverses aberrant tyrosine uptake in patients with bipolar disorder

Author: Tabrisi, R, Harun-Rashid, MD, Montero, J, Venizelos, N, and Msghina, M
Published: 2023
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22. Reinforcement corrosion in self-compacting concrete made with waste filler of bituminous mixtures

Author: Martinez-Echevarria, M.J., Del Castillo, J.P., Rodríguez Montero, J., and López-Alonso, M.
Published: 2024
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23. Encuesta nacional sobre cambios en las políticas de comunicación, visitas y cuidados al final de la vida en las unidades de cuidados intensivos durante las diferentes olas de la pandemia de COVID-19 (estudio COVIFAUCI)

Author: Fernández-Castillo, R.J., González-Caro, M.D., Arroyo-Muñoz, F.J., and Garnacho-Montero, J.
Published: 2024
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24. National survey on changes in visitation, communication and end-of-life care policies in intensive care units through the different COVID-19 pandemic’s waves (COVIFAUCI study)

Author: Fernández-Castillo, R.-J., González-Caro, M.-D., Arroyo-Muñoz, F.-J., and Garnacho-Montero, J.
Published: 2024
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25. Metal (boro-) hydrides for high energy density storage and relevant emerging technologies

Author: Bannenberg, L. J., Heere, M., Benzidi, H., Montero, J., Dematteis, E. M., Suwarno, S., Jaroń, T., Winny, M., Orłowski, P. A., Wegner, W., Starobrat, A., Fijałkowski, K. J., Grochala, W., Qian, Z., Bonnet, J. -P., Nuta, I., Lohstroh, W., Zlotea, C., Mounkachi, O., Cuevas, F., Chatillon, C., Latroche, M., Fichtner, M., Baricco, M., Hauback, B. C., and Kharbachi, A. El
Subjects: Condensed Matter - Materials Science
Abstract: The current energy transition imposes a rapid implementation of energy storage systems with high energy density and eminent regeneration and cycling efficiency. Metal hydrides are potential candidates for generalized energy storage, when coupled with fuel cell units and/or batteries. An overview of ongoing research is reported and discussed in this review work on the light of application as hydrogen and heat storage matrices, as well as thin films for hydrogen optical sensors. These include a selection of single-metal hydrides, Ti-V(Fe) based intermetallics, multi-principal element alloys (high-entropy alloys), and a series of novel synthetically accessible metal borohydrides. Metal hydride materials can be as well of important usefulness for MH-based electrodes with high capacity (e.g. MgH2 ~ 2000 mAh g-1) and solid-state electrolytes displaying high ionic conductivity suitable, respectively, for Li-ion and Li/Mg battery technologies. To boost further research and development directions some characterization techniques dedicated to the study of M-H interactions, their equilibrium reactions, and additional quantification of hydrogen concentration in thin film and bulk hydrides are presented at the end of this manuscript.
Published: 2020
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26. Cirugía radioguiada de tumores mesenquimales con semilla de 125I

Author: Barranquero, A.G., Corral Moreno, S., Martínez Lorca, A., Hernández-Cosido, L., Rioja Martín, M.E., Mena Mateos, A., Cabañas Montero, J., and Fernández-Cebrián, J.M.
Published: 2023
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27. Validation of two complementary oral-health related quality of life indicators (OIDP and OSS 0-10 ) in two qualitatively distinct samples of the Spanish population

Author: Albaladejo A, Bravo M, and Montero J
Subjects: Computer applications to medicine. Medical informatics, R858-859.7
Abstract: Abstract Background Oral health-related quality of life can be assessed positively, by measuring satisfaction with mouth, or negatively, by measuring oral impact on the performance of daily activities. The study objective was to validate two complementary indicators, i.e., the OIDP (Oral Impacts on Daily Performances) and Oral Satisfaction 0–10 Scale (OSS), in two qualitatively different socio-demographic samples of the Spanish adult population, and to analyse the factors affecting both perspectives of well-being. Methods A cross-sectional study was performed, recruiting a Validation Sample from randomly selected Health Centres in Granada (Spain), representing the general population (n = 253), and a Working Sample (n = 561) randomly selected from active Regional Government staff, i.e., representing the more privileged end of the socio-demographic spectrum of this reference population. All participants were examined according to WHO methodology and completed an in-person interview on their oral impacts and oral satisfaction using the OIDP and OSS 0–10 respectively. The reliability and validity of the two indicators were assessed. An alternative method of describing the causes of oral impacts is presented. Results The reliability coefficient (Cronbach's alpha) of the OIDP was above the recommended 0.7 threshold in both Validation and Occupational samples (0.79 and 0.71 respectively). Test-retest analysis confirmed the external reliability of the OSS (Intraclass Correlation Coefficient, 0.89; p < 0.001) Some subjective factors (perceived need for dental treatment, complaints about mouth and intermediate impacts) were strongly associated with both indicators, supporting their construct and criterion validity. The main cause of oral impact was dental pain. Several socio-demographic, behavioural and clinical variables were identified as modulating factors. Conclusion OIDP and OSS are valid and reliable subjective measures of oral impacts and oral satisfaction, respectively, in an adult Spanish population. Exploring simultaneously these issues may provide useful insights into how satisfaction and impact on well-being are constructed.
Published: 2008
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28. Modeling the observations of GRB 180720B: From radio to sub-TeV gamma-rays

Author: Fraija, N., Dichiara, S., Pedreira, A. C. Caligula do E. S., Galvan-Gamez, A., Becerra, R. L., Montalvo, A., Montero, J., Kamenetskaia, B. Betancourt, and Zhang, B. B.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Early and late multiwavelength observations play an important role in determining the nature of the progenitor, circumburst medium, physical processes and emitting regions associated to the spectral and temporal features of bursts. GRB 180720B is a long and powerful burst detected by a large number of observatories in multiwavelenths that range from radio bands to sub-TeV gamma-rays. The simultaneous multiwavelength observations were presented over multiple periods of time beginning just after the trigger time and extending for more than 30 days. The temporal and spectral analysis of Fermi LAT observations suggests that it presents similar characteristics to other bursts detected by this instrument. Coupled with X-ray and optical observations, the standard external-shock model in a homogeneous medium is favored by this analysis. The X-ray flare is consistent with the synchrotron self-Compton (SSC) model from the reverse-shock region evolving in a thin shell and long-lived LAT, X-ray and optical data with the standard synchrotron forward-shock model. The best-fit parameters derived with the Markov chain Monte Carlo simulations indicate that the outflow is endowed with magnetic fields and that the radio observations are in the self-absorption regime. The SSC forward-shock model with our parameters can explain the LAT photons beyond the synchrotron limit as well as the emission recently reported by the HESS Collaboration., Comment: 18 pages, 9 figures. Minor changes. Accepted for publication in ApJ
Published: 2019
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29. Light-induced breathing in photochromic yttrium oxy-hydrides

Author: Baba, E. M., Montero, J., Strugovshchikov, E., Zayim, E. Ö., and Karazhanov, E. Zh.
Subjects: Condensed Matter - Materials Science
Abstract: When exposed to air, metallic yttrium dihydride YH2films turn into insulating and transparent yttrium oxy-hydride (YHO). The incorporation of oxygen causes the lattice expansion of YH2 and the emergence of photochromic properties. However, the oxidation of YH2 is not completely irreversible: under illumination some oxygen atoms move towards the YHO surface, leaving behind an oxygen-deficient bulk (responsible for the photochromic darkening and observed lattice contraction). Under illumination, and according to experimental evidence, some oxygen atoms can effectively leave the film, being replaced by other oxygen atoms once the illumination has stopped, i.e., YHO "breathes" when subjected to illumination/darkness cycling. Based on this "breathing", YHO films become more hydrophobic under illumination conditions than when kept in darkness. Ab-initio calculations point to the light-induced weakening of the Y-O bond as the possible mechanism for explaining these experimental observations.
Published: 2019
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30. Determinants of mortality in cancer patients with unscheduled admission to the Intensive Care Unit: A prospective multicenter study

Author: Cantón-Bulnes, M.L., Jiménez-Sánchez, M., Alcántara-Carmona, S., Gimeno-Costa, R., Berezo-García, J.Á., Beato, C., Álvarez-Lerma, F., Mojal, S., Olaechea, P., Gordo-Vidal, F., and Garnacho-Montero, J.
Published: 2022
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31. High redshift galaxies in the ALHAMBRA survey: II. strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z <= 4.5 by PDF analysis

Author: Viironen, K., López-Sanjuan, C., Hernández-Monteagudo, C., Chaves-Montero, J., Ascaso, B., Bonoli, S., Cristóbal-Hornillos, D., Díaz-García, L. A., Fernández-Soto, A., Márquez, I., Masegosa, J., Pović, M., Varela, J., Cenarro, A. J., Aguerri, J. A. L., Alfaro, E., Aparicio-Villegas, T., Benítez, N., Broadhurst, T., Cabrera-Caño, J., Castander, F. J., Cepa, J., Cerviño, M., Delgado, R. M. González, Husillos, C., Infante, L., Martínez, V. J., Moles, M., Molino, A., del Olmo, A., Perea, J., Prada, F., and Quintana, J. M.
Subjects: Astrophysics - Astrophysics of Galaxies
Abstract: Context. Knowing the exact shape of the UV luminosity function of high-redshift galaxies is important in order to understand the star formation history of the early universe. However, the uncertainties, especially at the faint and bright ends of the LFs, are still significant. Aims. In this paper, we study the UV luminosity function of redshift z = 2.5 - 4.5 galaxies in 2.38 deg^2 of ALHAMBRA data with I <= 24. Thanks to the large area covered by ALHAMBRA, we particularly constrain the bright end of the luminosity function. We also calculate the cosmic variance and the corresponding bias values for our sample and derive their host dark matter halo masses. Methods. We use a novel methodology based on redshift and magnitude probability distribution functions (PDFs). This methodology robustly takes into account the uncertainties due to redshift and magnitude errors, shot noise and cosmic variance, and models the luminosity function in two dimensions (z; M_UV ). Results. We find an excess of bright ~ M*_UV galaxies as compared to the studies based on broad-band photometric data. However, our results agree well with the luminosity function of the magnitude-selected spectroscopic VVDS data. We measure high bias values, b ~ 8 - 10, that are compatible with the previous measurements considering the redshifts and magnitudes of our galaxies and further reinforce the real high-redshift nature of our bright galaxies. Conclusions. We call into question the shape of the luminosity function at its bright end; is it a double power-law as suggested by the recent broad-band photometric studies or rather a brighter Schechter function, as suggested by our multi-filter analysis and the spectroscopic VVDS data., Comment: 16 pages, 12 figures
Published: 2017
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32. Predictive factors of six-week mortality in critically ill patients with SARS-CoV-2: A multicenter prospective study

Author: Estella, Á., Garcia Garmendia, J.L., de la Fuente, C., Machado Casas, J.F., Yuste, M.E., Amaya Villar, R., Estecha, M.A., Yaguez Mateos, L., Cantón Bulnes, M.L., Loza, A., Mora, J., Fernández Ruiz, L., Díez del Corral Fernández, B., Rojas Amezcua, M., Rodriguez Higueras, M.I., Díaz Torres, I., Recuerda Núñez, M., Zaheri Beryanaki, M., Rivera Espinar, F., Matallana Zapata, D.F., Moreno Cano, S.G., Gimenez Beltrán, B., Muñoz, N., Sainz de Baranda Piñero, A., Bustelo Bueno, P., Moreno Barriga, E., Rios Toro, J.J., Pérez Ruiz, M., Gómez González, C., Breval Flores, A., de San José Bermejo Gómez, A., Ruiz Cabello Jimenez, M.A., Guerrero Marín, M., Ortega Ordiales, A., Tejero-Aranguren, J., Rodriguez Mejías, C., Gomez de Oña, J., de la Hoz, C., Ocaña Fernández, D., Ibañez Cuadros, S., and Garnacho Montero, J.
Published: 2022
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33. Axion dark matter in a $3-3-1$ model

Author: Montero, J. C., Castellanos, Ana R. Romero, and Sánchez-Vega, B. L.
Subjects: High Energy Physics - Phenomenology
Abstract: Slightly extending a right-handed neutrino version of the $3-3-1$ model, we show that it is not only possible to solve the strong CP problem but also to give the total dark matter abundance reported by the Planck collaboration. Specifically, we consider the possibility of introducing a $3-3-1$ scalar singlet to implement a gravity stable Peccei-Quinn mechanism in this model. Remarkably, for allowed regions of the parameter space, the arising axions with masses $m_a\approx$ meV can both make up the total dark matter relic density through non-thermal production mechanisms and be very close to the region to be explored by the IAXO helioscope., Comment: 21 pages, 4 figures
Published: 2017
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34. New constraints on the 3-3-1 model with right-handed neutrinos

Author: Sánchez-Vega, B. L., Schmitz, E. R., and Montero, J. C.
Subjects: High Energy Physics - Phenomenology
Abstract: In the framework of a 3-3-1 model with right-handed neutrinos and three scalar triplets we consider different spontaneous symmetry breaking patterns seeking for a non-linear realization of accidental symmetries of the model, which will produce physical Nambu-Goldstone (NG) bosons in the neutral scalar spectrum. We make a detailed study of the safety of the model concerning the NG boson emission in energy loss processes which could affect the standard evolution of astrophysical objects. We consider the model with a $\mathbb{Z}_2$ symmetry, conventionally used in the literature, finding that in all of the symmetry breaking patterns the model is excluded. Additionally, looking for solutions for that problem, we introduce soft $\mathbb{Z}_2$-breaking terms in the scalar potential in order to remove the extra accidental symmetries and at the same time maintain the model as simple as possible. We find that there is only one soft $\mathbb{Z}_2$-violating term that can get rid of the problematic NG bosons., Comment: 16 pages
Published: 2016
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35. Recommendations for the management of critically ill patients with COVID-19 in Intensive Care Units

Author: Vidal-Cortés, P., Díaz Santos, E., Aguilar Alonso, E., Amezaga Menéndez, R., Ballesteros, M.Á., Bodí, M.A., Bordejé Laguna, M.L., Garnacho Montero, J., García Sánchez, M., López Sánchez, M., Martín-Loeches, I., Ochagavía Calvo, A., Ramírez Galleymore, P., Alcántara Carmona, S., Andaluz Ojeda, D., Badallo Arébalo, O., Barrasa González, H., Borges Sa, M., Castellanos-Ortega, Á., Estella, Á., Ferrer Roca, R., Fraile Gutiérrez, V., Fuset Cabanes, M., Giménez-Esparza Vich, C., González Iglesias, C., Hernández-Tejedor, A., Igeño Cano, J.C., Iglesias Posadilla, D., Jiménez Rivera, J.J., Llanos Jorge, C., Llompart-Pou, J.A., López Camps, V., Lorencio Cárdenas, C., Marcos Neira, P., Martín Delgado, M.C., Martín-Macho González, M., Martín Villén, L., Nuvials Casals, X., Ortiz Suñer, A., Quintana Díaz, M., Rascado Sedes, P., Recuerda Núñez, M., del Río Carbajo, L., Rodríguez Aguirregabiria, M., Rodríguez Oviedo, A., Seijas Betolaza, I., Soriano Cuesta, C., Suberviola Cañas, B., Vera Ching, C., Vidal González, Á., Zapata Fenor, L., and Zaragoza Crespo, R.
Published: 2022
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36. Feasibility and safety of physiologic pacing post-TAVR

Author: Pajaro Merino, P A, primary, Del Valle Montero, J A, additional, Moraleda Salas, M T, additional, Luque Perez, M, additional, Arce Leon, A, additional, Esteve Ruiz, I, additional, Carreno Lineros, J M, additional, Gomez Menchero, A E, additional, and Morina Vazquez, P, additional
Published: 2024
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37. Longitudinal outcomes of obeticholic acid therapy in ursodiol‐nonresponsive primary biliary cholangitis: Stratifying the impact of add‐on fibrates in real‐world practice

Author: Gómez, E., primary, Montero, J. L., additional, Molina, E., additional, García‐Buey, L., additional, Casado, M., additional, Fuentes, J., additional, Simón, M. A., additional, Díaz‐González, A., additional, Jorquera, F., additional, Morillas, R. M., additional, Presa, J., additional, Berenguer, M., additional, Conde, M. I., additional, Olveira, A., additional, Macedo, G., additional, Garrido, I., additional, Hernández‐Guerra, M., additional, Olivas, I., additional, Rodríguez‐Taje, S., additional, Londoño, M., additional, Sousa, J. M., additional, Ampuero, J., additional, Romero‐González, E., additional, González‐Padilla, Sh., additional, Escudero‐García, D., additional, Carvalho, A., additional, Santos, A., additional, Gutiérrez, M. L., additional, Pérez‐Fernández, E., additional, Aburruza, L., additional, Uriz, J., additional, Gomes, D., additional, Santos, L., additional, Martínez‐González, J., additional, Albillos, A., additional, and Fernández‐Rodríguez, C. M., additional
Published: 2024
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38. The miniJPAS survey: Maximising the photo-z accuracy from multi-survey datasets with probability conflation

Author: Hernán-Caballero, A., primary, Akhlaghi, M., additional, López-Sanjuan, C., additional, Vázquez Ramió, H., additional, Laur, J., additional, Varela, J., additional, Civera, T., additional, Muniesa, D., additional, Finoguenov, A., additional, Fernández-Ontiveros, J. A., additional, Domínguez Sánchez, H., additional, Chaves-Montero, J., additional, Fernández-Soto, A., additional, Lumbreras-Calle, A., additional, Díaz-García, L. A., additional, del Pino, A., additional, González Delgado, R. M., additional, Hernández-Monteagudo, C., additional, Coelho, P., additional, Jiménez-Teja, Y., additional, Lopes, P. A. A., additional, Marra, V., additional, Tempel, E., additional, Vílchez, J. M., additional, Abramo, R., additional, Alcaniz, J., additional, Benítez, N., additional, Bonoli, S., additional, Carneiro, S., additional, Cenarro, J., additional, Cristóbal-Hornillos, D., additional, Dupke, R., additional, Ederoclite, A., additional, Marín-Franch, A., additional, Mendes de Oliveira, C., additional, Moles, M., additional, Sodré, L., additional, and Taylor, K., additional
Published: 2024
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39. Active galactic nuclei and gravitational redshifts

Author: Padilla, N., primary, Carneiro, S., additional, Chaves-Montero, J., additional, Donzelli, C. J., additional, Pigozzo, C., additional, Colazo, P., additional, and Alcaniz, J. S., additional
Published: 2024
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40. WEAVE-QSO: A Massive Intergalactic Medium Survey for the William Herschel Telescope

Author: Pieri, M. M., Bonoli, S., Chaves-Montero, J., Paris, I., Fumagalli, M., Bolton, J. S., Viel, M., Noterdaeme, P., Miralda-Escudé, J., Busca, N. G., Rahmani, H., Peroux, C., Font-Ribera, A., Trager, S. C., and Collaboration, The WEAVE
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: In these proceedings we describe the WEAVE-QSO survey, which will observe around 400,000 high redshift quasars starting in 2018. This survey is part of a broader WEAVE survey to be conducted at the 4.2m William Herschel Telescope. We will focus on chiefly on the science goals, but will also briefly summarise the target selection methods anticipated and the expected survey plan. Understanding the apparent acceleration in the expansion of the Universe is one of the key scientific challenges of our time. Many experiments have been proposed to study this expansion, using a variety of techniques. Here we describe a survey that can measure this acceleration and therefore help elucidate the nature of dark energy: a survey of the Lyman-alpha forest (and quasar absorption in general) in spectra towards z>2 quasars (QSOs). Further constraints on neutrino masses and warm dark matter are also anticipated. The same data will also shed light on galaxy formation via study of the properties of inflowing/outflowing gas associated with nearby galaxies and in a cosmic web context. Gas properties are sensitive to density, temperature, UV radiation, metallicity and abundance pattern, and so constraint galaxy formation in a variety of ways. WEAVE-QSO will study absorbers with a dynamic range spanning more than 8 orders of magnitude in column density, their thermal broadening, and a host of elements and ionization species. A core principal of the WEAVE-QSO survey is the targeting of QSOs with near 100% efficiency principally through use of the J-PAS (r < 23.2) and Gaia (r < 20) data., Comment: 8 pages, 2 figures, proceedings of the SF2A conference, Lyon, 2016
Published: 2016

41. Synthesis of photochromic oxygen-containing yttrium hydride

Author: Montero, J., Martinsen, F. A., Lelis, M., Karazhanov, S. Zh., Hauback, B. C., and Marstein, E. S.
Subjects: Condensed Matter - Materials Science
Abstract: Photochromic oxygen-containing yttrium hydride has been synthesized using a two step process. The process consists of an initial sputter deposition of oxygen-free yttrium hydride YH$_\mathrm{x}$, followed by a controlled reaction with air that causes incorporation of oxygen into the material. An in-situ study of the YH$_\mathrm{x}$ as it reacted with oxygen was made possible by applying an aluminium capping layer with a low but non-zero oxygen permeability prior to air exposure. During the reaction, the visual appearance of the YH$_\mathrm{x}$ went from dark and opaque to transparent and yellowish. This transition was accredited incorporation of oxygen into the material, as shown through analysis with energy dispersive x-ray spectroscopy (EDS) and x-ray photoemission spectroscopy (XPS). Grazing incidence x-ray diffraction (GIXRD) studies revealed an fcc structure both before and after oxygen exposure, with a lattice parameter that increased from 5.2 {\AA} to 5.4 {\AA} during the reaction. With the lattice parameter in the oxygen free YH$_\mathrm{x}$ being equal to that reported earlier for YH$_\mathrm{2}$, our findings suggest that the non-reacted YH$_\mathrm{x}$ in this study is in-fact YH$_\mathrm{2}$.
Published: 2016
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42. Supersymmetric $U(1)_{Y^{\prime}}\otimes U(1)_{B-L}$ extension of the standard model

Author: Montero, J. C., Pleitez, V., Rodriguez, M. C., and Sánchez-Vega, B. L.
Subjects: High Energy Physics - Phenomenology
Abstract: We build a supersymmetric version with $SU(3)_C\otimes SU(2)_L\otimes U(1)_{Y^\prime}\otimes U(1)_{B-L}$ gauge symmetry, where $Y^\prime$ is a new charge and $B$ and $L$ are the usual baryonic and leptonic numbers. The model has three right-handed neutrinos with identical $B-L$ charges, and can accommodate all fermion masses at the tree level. In particular, the type-I seesaw mechanism is implemented for the generation of the active neutrino masses. We obtain the mass spectra of all sectors and for the scalar one we also give the flat directions allowed by the model., Comment: Version submitted for publication. 29 pages
Published: 2016
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43. New insights into the photochromic mechanism in oxygen-containing yttrium hydride thin films: an optical perspective

Author: Montero, J., Martinsen, F. A., Karazhanov, S. Zh., Hauback, B. C., and Marstein, E. S.
Subjects: Condensed Matter - Materials Science
Abstract: Oxygen-containing yttrium hydride thin films exhibit a photochromic behavior: transparent thin films switch from a transparent state to a photodarkened state after being illuminated with UV or blue light. This feature has attracted much attention in recent years due to its potential applications in smart fenestration or in any device in which a response to intense light radiation is needed. However, the process responsible for the reversible change of the optical properties upon illumination is still not well understood. The objective of the present work is to shed some light on the photochromic mechanism by using an optical approach. On this basis, the optical properties of oxygen-containing yttrium hydride thin films have been studied by optical spectrophotometry and ellipsometry before (transparent state) and after UV illumination (dark state). According to the observed results, the photochromic optical change of the films can be explained quantitatively by the gradual growth, under illumination, of metallic phases within the initial wide-band gap semiconducting lattice., Comment: 5 pages 5 figures
Published: 2016
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44. Epidemiology and prognosis of patients with a history of cancer admitted to intensive care. A multicenter observational study

Author: Durá Navarro, Raquel, Ruano Suarez, María Carmen, Alonso Araujo, Inmaculada, Arenzana Seisdedos, Ángel, Córdoba López, Alberto, Camino Redondo, Nuria, Barbadillo Ansorregui, Sandra, Mouriz Fernández, Lorena, Vilas Otero, Maria Elena, Márquez Alonso, José Antonio, Bueno Blázquez, Adoración Gema, Abella Alvarez, Ana, Lobo Palanco, Joaquín, Cofiño Castañeda, Luis, Montejo González, J.C., García García, Miguel Ángel, Sandar Núñez, María Dolores, Tebar Soto, María Teresa, Cabadas Avión, Rafael, Gimeno Costa, Ricardo, Berezo García, José Ángel, García López, Fernando, López Matamala, Blanca, Colomar Ferrá, Asunción, Rey García, María Sopetrán, Cidoncha Calderón, Belén, Alcántara Carmona, Sara, Manteiga Riestra, Eva, Gil Rueda, Bernardo, Gallego González, Carlos, Jiménez Sánchez, Roberto, de Toro Martín-Consuegra, Ismael López, Souto Higueras, Jessica, Lander Azcona, Arantxa, Fuster Lozano, José María, Vera Artázcoz, Paula, Castro Orjales, María José, Arquitecto Marcide, H., Asensio Martín, María José, Estecha Foncea, María Antonia, Reig Valero, Roberto, Priego Sanz, Jesús, Vallés Daunis, Jordi, Ezpeleta Galindo, Ana Isabel, Álvarez Martínez, Braulio, Bobillo de Lamo, Felipe, Margarit Ribas, Antoni, Olaechea Astigarraga, Pedro M., Ballesteros Herráez, Juan Carlos, Saldaña Fernández, María Teresa, Sánchez Miralles, Ángel, Amaya Villar, Rosario, López-Cuervo, Juan Fajardo, Socias, Antonia, Bonet Saris, Alfons, Díaz Lamas, Ana María, Iruretagoyena Amiano, José Ramón, Acosta Rivera, Ingrid, Cerón García, María, Moradillo González, Susana, Rodríguez Pedreira, Paula, Palencia Herrejón, Eduardo, López Núñez, Carlos, Mas Lodo, Margarita, Pardo Talavera, Juan Carlos, Luisa Mora, María, Ferrer Roca, Ricard, de La Fuente Óconnor, Eugenia, Sánchez García, Miguel, Blanco Huelga, Carmen, Garijo Catalina, María Ángeles, Alcalá López, Adoración, Ugalde Gutierrez, Marta, Navarro Ruiz, María Rosa, Román Millan, María José, Lara Aguayo, Pedro, Herreros Gonzalo, María, Claverias Cabrera, Laura, Martos López, José, Valdovinos Mahave, María Concepción, Fontaneda López, Daniel, Matachana Martínez, María, García Sánchez, Esther, Santarrufina Lluch, Carmen, Garcés González, Rafael, Gallego Lara, Sonia, Martinez Trivez, Pilar, Vilanova Pàmies, Cecília, Llanos Jorge, Celina, Montejo Gonzalez, Juan Carlos, Alemparte Pardavila, Enrique, Olaechea Astigarraga, P.M., Álvarez Lerma, F., Beato Zambrano, C., Gimeno Costa, R., Gordo Vidal, F., Durá Navarro, R., Ruano Suarez, C., Aldabó Pallás, T., and Garnacho Montero, J.
Published: 2021
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45. Fate of rejected manuscripts in the journal Medicina Intensiva during 2015–2017 period

Author: García-Garmendia, J.L., Gordo-Vidal, F., Leal-Noval, S.R., Amaya-Villar, R., Raimondi, N., Ochagavía-Calvo, A., and Garnacho-Montero, J.
Published: 2021
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46. A multicenter and observational study of the Ambu™ AuraGain™ laryngeal mask in adult patients

Author: Zaballos, M., Escribá, F., López, S., Zaballos, J., Montero, J., Fernández, I., and López, A.M.
Published: 2021
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47. Estudio multicéntrico observacional de la mascarilla Ambu® AuraGain® en pacientes adultos

Author: Zaballos, M., Escribá, F., López, S., Zaballos, J., Montero, J., Fernández, I., and López, A.M.
Published: 2021
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48. Automated identification of leukocyte subsets improves standardization of database-guided expert-supervised diagnostic orientation in acute leukemia: a EuroFlow study

Author: Lhermitte, Ludovic, Barreau, Sylvain, Morf, Daniela, Fernandez, Paula, Grigore, Georgiana, Barrena, Susana, de Bie, Maaike, Flores-Montero, Juan, Brüggemann, Monika, Mejstrikova, Ester, Nierkens, Stefan, Burgos, Leire, Caetano, Joana, Gaipa, Giuseppe, Buracchi, Chiara, da Costa, Elaine Sobral, Sedek, Lukasz, Szczepański, Tomasz, Aanei, Carmen-Mariana, van der Sluijs-Gelling, Alita, Delgado, Alejandro Hernández, Fluxa, Rafael, Lecrevisse, Quentin, Pedreira, Carlos E., van Dongen, Jacques J.M., Orfao, Alberto, van der Velden, Vincent H.J., van Dongen, J. J.M., Bitter, W.M., Lubbers, B.R., Teodosio, C.I., Zlei, M., van der Sluijs-Gelling, A.J., de Bie, F., de Bruin-Versteeg, S., van der Burg, M., Schilham, M.W., van der Velden, V. H.J., Langerak, A.W., te Marvelde, J., Bras, A.E., Schilperoord-Vermeulen, J., Jugooa, R., Heezen, K.C., Orfao, A., Almeida, J., Vidriales, M.B., Flores-Montero, J., Pérez-Andrés, M., Matarraz, S., Martín, L., Lecrevisse, Q., Pérez-Morán, J.J., Puig, N., Almeida, A. Medina, Gomes da Silva, M., Faria, T., Brüggemann, M., Ritgen, M., Szczepanowski, M., Kohlscheen, S., Laqua, A., Harbst, E., Finke, J., Asnafi, V., Lhermitte, L., Duroyon, E., Trka, J., Hrusak, O., Kalina, T., Mejstrikova, E., Novakova, M., Thurner, D., Kanderova, V., Szczepanski, T., Sędek, L., Bulsa, J., Slota, L., Kulis, J., Pedreira, C.E., da Costa, E. Sobral, Nierkens, S., de Jong, A., de Koning, A., Lima, M., Santos, A.H., Böttcher, S., Lange, S., Engelmann, R., Paape, D., Machka, C., Gaipa, G., Burracchi, C., Bugarin, C., Lopez-Granados, E., del Pino Molina, L., Campos-Guyotat, L., Aanei, C., Miguel, J. F. San, Paiva, B., Burgos, L., Villamor-Casas, N., Magnano, L., Philippé, J., Bonroy, C., Denys, B., Willems, A., Breughe, P., de Wolf, J., Sousa, A.E., Silva, S.L., Fernandez, P., and Morf, D.
Published: 2021
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49. Global age-sex-specific mortality, life expectancy, and population estimates in 204 countries and territories and 811 subnational locations, 1950–2021, and the impact of the COVID-19 pandemic : a comprehensive demographic analysis for the Global Burden of Disease Study 2021

Author: Schumacher, A. E., Kyu, H. H., Antony, C. M., Aravkin, A. Y., Azhar, G. S., Bisignano, C., Burkart, K., Cercy, K. M., Chung, E., Coberly, K., Comfort, H., Cousin, E., Culbreth, G. T., Cunningham, M., Weaver, N. D., Degenhardt, L., Deitesfeld, L., Dirac, M. A., Estep, K., Feigin, V. L., Flaxman, A. D., Flor, L. S., Force, L. M., Fuller, J. E., Gakidou, E., Hay, S. I., Ikuta, K. S., Jones, D. P., Kassebaum, N. J., Kassel, M. B., Keller, C., Kinzel, K. E., Krohn, K. J., Lozano, R., May, E. A., McKowen, A. W., McLaughlin, S. A., Mehlman, M. L., Mestrovic, T., Mokdad, A. H., Mosser, J. F., Mougin, V., Naghavi, M., Nesbit, O. D., Novotney, A., Ozten, Y., Pease, S. A., Pigott, D. M., Reiner, R. C., Robinson-Oden, H. E., Shaw, D. H., Slepak, E. L. N., Sorensen, R. J. D., Verghese, N. A., Vollset, S., Vongpradith, A., Vos, T., Wang, D., Watson, S., Weaver, M. R., Wells, K. M., Wilson, S., Wool, E. E., Zheng, P., Lim, S. S., Murray, C. J. L., Boyko, E. J., Chahine, Y., Kalani, R., Krishnamoorthy, V., Khalil, I. A., Minja, N. W., Morrison, S. D., Nafukho, F. M., Olivas-Martinez, A., Orellana, E., Tram, K., Aali, A., Rahnavard, N., Ahmadzade, A., Mohammad-Pour, S., Morovatdar, N., Pourali, G., Zafari, N., Abbafati, C., Cattaruzza, M. S., Abbas, J., Phillips, M. R., Abbasgholizadeh, R., Emamverdi, M., Friedman, J., Abbasi, M. A., Daneshvar, S., Dashti, M., Ghasemzadeh, A., Mirza-Aghazadeh-Attari, M., Doshmangir, L., Ghafourifard, M., Lotfi, M., Hosseini, M., Jadidi-Niaragh, F., Kalankesh, L. R., Karimi, S., Mohammad-Alizadeh-Charandabi, S., Khalafi, M., Mirghafourvand, M., Mirinezhad, S., Heris, R. M., Mousavi, S., Kafil, H. S., Abbasian, M., Momenzadeh, K., Santos, F. C. D., Carr, S., Chi, G., Elgendy, I. Y., Feroze, A. H., Kempen, J. H., Kubeisy, C. M., Li, Z., Rohloff, P., Liu, X., Natto, Z. S., Olanipekun, T. O., Pigeolet, M., Pradhan, P. M. S., Zweck, E., Sharfaei, S., Sheikh, A., Abtahi, D., Salimi, S., Shakeri, A., Tajbakhsh, A., Aghamiri, S., Ahmadzade, M., Hashemi, M. B., Ajami, M., Asgary, S., Ghasemi, M., Hassanian-Moghaddam, H., Kolahi, A., Nikoobar, A., Heidari-Foroozan, M., Montazeri, F., Nejadghaderi, S., Rahmani, S., Ziaeefar, P., Hesami, H., Zahir, M., Jahankhani, K., Rasouli-Saravani, A., Jahanmehr, N., Kashani, H. K., Nasiri, M., Raee, P., Rezaee, M., Safi, S., Shool, S., Tabatabai, S., ElHafeez, S. A., Tantawi, M. E., Elmeligy, O. A. A., Ghazy, R. M., Talaat, I. M., Abdelmasseh, M., Sanabria, J., Abd-Elsalam, S., Abdelwahab, A., Abdollahi, M., Abolhassani, H., Rezaei, N., Saghazadeh, A., Ala, M., Noroozi, N., Bahri, R. A., Khatami, F., Ayyoubzadeh, S., Azadnajafabad, S., Keykhaei, M., Momtazmanesh, S., Mousavi, P., Behnoush, A., Farrokhpour, H., Karimi, H., Khalaji, A., Khanmohammadi, S., Mayeli, M., Mohammadi, S., Eskandarieh, S., Sahraian, M., Fahimi, S., Malekzadeh, R., Mansouri, V., Sepanlou, S. G., Ghassemi, F., Haddadi, M., Kazemian, S., Khadembashiri, M., Khamesipour, F., Khavandegar, A., Khormali, M., Salamati, P., Kompani, F., Larijani, B., Mirdamadi, N., Seyedi, S., Malazy, O. T., Mahmoudi, E., Rashedi, S., Rad, E. M., Mansournia, M., Nasab, E. M., Mohammadshahi, M., Mostafavi, H., SeyedAlinaghi, S., Shafie, M., Shahbandi, A., Vahdani, A. M., Sharifan, A., Shirkoohi, R., Sohrabi, H., Tavangar, S., Heidari-Soureshjani, R., Abdoun, M., Abdullahi, A., Awotidebe, A. W., Borodo, S. B., Gadanya, M. A., Ladan, M., Ali, M. U., Tyrovolas, S., Abdurehman, A. M., Debele, A. T., Getachew, T., Gudeta, M. D., Misgana, T., Sertsu, A., Abebe, M., Ayele, G. M., Afework, A., Lerango, T. L., Tebeje, T. M., Sibhat, M. M., Tesfaye, S. H., Abedi, A., Gholamrezanezhad, A., Salehi, S., Athari, S., Hanifi, N., Abegaz, T. M., Kifle, Z. D., Zuñiga, R. A. A., Abhilash, E. S., Abiodun, O. O., Aboagye, R. G., Amu, H., Ayanore, M. A., Dowou, R. K., Immurana, M., Klu, D., Orish, V. N., Carrero, J. J., Cederroth, C. R., Deuba, K., Laflamme, L., Fereshtehnejad, S., Kauppila, J. H., Abouzid, M., Abreu, L. G., Malta, D. C., Prates, E. J. S., Nascimento, B. R., Abrha, W. A., Weldemariam, A. H., Girmay, A., Abrigo, M. R. M., Rumeileh, S. A., Abu-Rmeileh, N. M., Aburuz, S., Ahmed, L. A., Alam, Z., Elbarazi, I., Grivna, M., Nauman, J., Khan, G., Khan, M. A., Zaki, N., Ahmad, M. M., Abu-Zaid, A., Temsah, R. M. H., Zand, R., Acuna, J. M., Gautam, P., Chowdhury, R., Adair, T., Jiang, H., Babu, A. S., Borschmann, R., Meretoja, A., Wijeratne, T., Addo, I. Y., Okeke, S. R., Dai, Z., Xu, X., Huda, M., Mitchell, P. B., Peden, A. E., Resnikoff, S., Sharma, S., Si, Y., Sitas, F., Ye, P., Adebayo, O. M., Aladelusi, T. O., Salami, A. A., Ilesanmi, O. S., Owolabi, M. O., Adegboye, O. A., Adekanmbi, V., AlBataineh, M. T., Almahmeed, W., Aden, B., Adepoju, A. V., Adetunji, C. O., Adeyeoluwa, T. E., Oyeyemi, I. T., Oyeyemi, O. T., Udoakang, A. J., Adeyomoye, O. I., Anuoluwa, I. A., Bello, O. O., Oluwafemi, Y. D., Ekundayo, T. C., Idowu, O. O., Oluwatunase, G. O., Afolabi, A. A., Ekholuenetale, M., Fagbamigbe, A. F., Olufadewa, I. I., Ibitoye, S. E., Okekunle, A. P., Adha, R., Adikusuma, W., Adibi, A., Chen, M., Hossain, M., Rasali, D. P., Pashaei, A., Adnani, Q. E. S., Postma, M. J., Adra, S., Barqawi, H. J., Dash, N. R., Halwani, R., Maghazachi, A. A., Saber-Ayad, M. M., Sharif-Askari, N. S., Ahmad, F., Saddik, B., Saleh, M. A., Alzoubi, K. H., Omar, H. A., Arumugam, A., Bustanji, Y., Elemam, N. M., Faris, M. E. M., Karim, A., Qaisar, R., Semreen, M. H., Soliman, S. S. M., Altirkawi, K. A., Afraz, A., Ilaghi, M., Nematollahi, M., Afyouni, S., Amindarolzarbi, A., Zandieh, G. G. Z., Columbus, A., Kamireddy, A., Shafaat, O., Kazemi, F., Vervoort, D., Zhang, H., Jamshidi, E., Afzal, S., Agasthi, P., Agodi, A., Barchitta, M., D'Amico, E., Maugeri, A., Veroux, M., Biondi, A., Isola, G., Vacante, M., Falzone, L., Libra, M., Agyemang-Duah, W., Nikpoor, A., Ahinkorah, B. O., Demant, D., Ahmad, A., Mustafa, G., Pathan, A. R., Tabish, M., Ahmad, D., Bagheri, N., Burns, R. A., Cherbuin, N., Ahmad, T., Ahmadi, K., Saxena, S., Beaney, T., Palladino, R., Rawaf, S., Mossialos, E., Rawaf, D. L., Ahmed, A., Siddig, E. E., Ahmed, H., Ahmed, M. B., Shiferaw, D., Ashemo, M. Y., Gerema, U., Getachew, M. E., Bayileyegn, N. S., Mohamed, A. I., Eshetie, T. C., Tiruye, T. Y., Ahmed, S., Ali, H., Bodunrin, A. O., Tumurkhuu, M., Tung, K., Ubah, C. S., Aruleba, R. T., Aji, B., Ajumobi, O., Akalu, G. T., Beyene, H. B., Deribe, K., Ijo, D., Kassaw, N. A., Akara, E., Akinosoglou, K., Akkala, S., Asaad, M., Hassan, A. M., Bleyer, A., Akyirem, S., Bell, M. L., Song, Y., Etaee, F., Goldust, M., Li, W., Pawar, S., Hamad, H. A., Sathian, B., Hasan, S. A., Homsi, A. A., Almidani, O., Göbölös, L., Qadire, M. A., AL-Ahdal, T. M. A., Chen, S., Moazen, B., Alalalmeh, S. O., Hegazi, O. E., Shahwan, M. J., Shamsi, M. A., Zyoud, S. 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A., Zaman, S., Zamora, N., Zanghì, A., Zare, I., Zeng, Y., Zhai, C., Zhang, Y., Zhao, H., Zhao, Y., Zhou, J., and Zhu, B.
Abstract: Background: Estimates of demographic metrics are crucial to assess levels and trends of population health outcomes. The profound impact of the COVID-19 pandemic on populations worldwide has underscored the need for timely estimates to understand this unprecedented event within the context of long-term population health trends. The Global Burden of Diseases, Injuries, and Risk Factors Study (GBD) 2021 provides new demographic estimates for 204 countries and territories and 811 additional subnational locations from 1950 to 2021, with a particular emphasis on changes in mortality and life expectancy that occurred during the 2020–21 COVID-19 pandemic period. Methods: 22 223 data sources from vital registration, sample registration, surveys, censuses, and other sources were used to estimate mortality, with a subset of these sources used exclusively to estimate excess mortality due to the COVID-19 pandemic. 2026 data sources were used for population estimation. Additional sources were used to estimate migration; the effects of the HIV epidemic; and demographic discontinuities due to conflicts, famines, natural disasters, and pandemics, which are used as inputs for estimating mortality and population. Spatiotemporal Gaussian process regression (ST-GPR) was used to generate under-5 mortality rates, which synthesised 30 763 location-years of vital registration and sample registration data, 1365 surveys and censuses, and 80 other sources. ST-GPR was also used to estimate adult mortality (between ages 15 and 59 years) based on information from 31 642 location-years of vital registration and sample registration data, 355 surveys and censuses, and 24 other sources. Estimates of child and adult mortality rates were then used to generate life tables with a relational model life table system. For countries with large HIV epidemics, life tables were adjusted using independent estimates of HIV-specific mortality generated via an epidemiological analysis of HIV prevalence surveys, ant
Published: 2024
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50. Global age-sex-specific mortality, life expectancy, and population estimates in 204 countries and territories and 811 subnational locations, 1950–2021, and the impact of the COVID-19 pandemic: a comprehensive demographic analysis for the Global Burden of Disease Study 2021

Author: Schumacher, A, Kyu, H, Aali, A, Abbafati, C, Abbas, J, Abbasgholizadeh, R, Abbasi, M, Abbasian, M, Abd ElHafeez, S, Abdelmasseh, M, Abd-Elsalam, S, Abdelwahab, A, Abdollahi, M, Abdoun, M, Abdullahi, A, Abdurehman, A, Abebe, M, Abedi, A, Abegaz, T, Abeldaño Zuñiga, R, Abhilash, E, Abiodun, O, Aboagye, R, Abolhassani, H, Abouzid, M, Abreu, L, Abrha, W, Abrigo, M, Abtahi, D, Abu Rumeileh, S, Abu-Rmeileh, N, Aburuz, S, Abu-Zaid, A, Acuna, J, Adair, T, Addo, I, Adebayo, O, Adegboye, O, Adekanmbi, V, Aden, B, Adepoju, A, Adetunji, C, Adeyeoluwa, T, Adeyomoye, O, Adha, R, Adibi, A, Adikusuma, W, Adnani, Q, Adra, S, Afework, A, Afolabi, A, Afraz, A, Afyouni, S, Afzal, S, Agasthi, P, Aghamiri, S, Agodi, A, Agyemang-Duah, W, Ahinkorah, B, Ahmad, A, Ahmad, D, Ahmad, F, Ahmad, M, Ahmad, T, Ahmadi, K, Ahmadzade, A, Ahmadzade, M, Ahmed, A, Ahmed, H, Ahmed, L, Ahmed, M, Ahmed, S, Ajami, M, Aji, B, Ajumobi, O, Akalu, G, Akara, E, Akinosoglou, K, Akkala, S, Akyirem, S, Al Hamad, H, Al Hasan, 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Shubha, Jeganathan, Jayakumar, Jema, Alelign Tasew, Jemere, Digisie Mequanint, Jeong, Wonjeong, Jha, Anil K, Jha, Ravi Prakash, Ji, John S, Jiang, Heng, Jin, Yingzhao, Jin, Yinzi, Johnson, Olatunji, Jomehzadeh, Nabi, Jones, Darwin Phan, Joo, Tamas, Joseph, Abel, Joseph, Nitin, Joshua, Charity Ehimwenma, Jozwiak, Jacek Jerzy, Jürisson, Mikk, Kaambwa, Billingsley, Kabir, Ali, Kabir, Hannaneh, Kabir, Zubair, Kadashetti, Vidya, Kahe, Farima, Kakodkar, Pradnya Vishal, Kalani, Rizwan, Kalankesh, Leila R, Kaliyadan, Feroze, Kalra, Sanjay, Kamath, Ashwin, Kamireddy, Arun, Kanagasabai, Thanigaivelan, Kandel, Himal, Kanmiki, Edmund Wedam, Kanmodi, Kehinde Kazeem, Kantar, Rami S, Kapoor, Neeti, Karajizadeh, Mehrdad, Karami Matin, Behzad, Karanth, Shama D, Karaye, Ibraheem M, Karim, Asima, Karimi, Hanie, Karimi, Salah Eddin, Karimi Behnagh, Arman, Karkhah, Samad, Karna, Ajit K, Kashoo, Faizan Zaffar, Kasraei, Hengameh, Kassaw, Nigussie Assefa, Kassebaum, Nicholas J, Kassel, Molly B, Katamreddy, 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Sun, Jing, Sunkersing, David, Susanty, Sri, Swain, Chandan Kumar, Sykes, Bryan L, Szarpak, Lukasz, Szeto, Mindy D, Szócska, Miklós, Tabaee Damavandi, Payam, Tabatabaei Malazy, Ozra, Tabatabaeizadeh, Seyed-Amir, Tabatabai, Shima, Tabb, Karen M, Tabish, Mohammad, Taborda-Barata, Luis M, Tabuchi, Takahiro, Tadesse, Birkneh Tilahun, Taheri, Amirmasoud, Taheri Abkenar, Yasaman, Taheri Soodejani, Moslem, Taherkhani, Amir, Taiba, Jabeen, Tajbakhsh, Ardeshir, Talaat, Iman M, Talukder, Ashis, Tamuzi, Jacques Lukenze, Tan, Ker-Kan, Tang, Haosu, Tang, Hong K, Tat, Nathan Y, Tat, Vivian Y, Tavakoli Oliaee, Razieh, Tavangar, Seyed Mohammad, Taveira, Nuno, Tebeje, Tsion Mulat, Tefera, Yibekal Manaye, Teimoori, Mojtaba, Temsah, Mohamad-Hani, Temsah, Reem Mohamad Hani, Teramoto, Masayuki, Tesfaye, Solomon Hailemariam, Thangaraju, Pugazhenthan, Thankappan, Kavumpurathu Raman, Thapa, Rajshree, Thapar, Rekha, Thomas, Nihal, Thrift, Amanda G, Thum, Chern Choong Chern, Tian, Jing, Tichopad, Ales, Ticoalu, Jansje Henny Vera, Tiruye, Tenaw Yimer, Tohidast, Seyed Abolfazl, Tonelli, Marcello, Touvier, Mathilde, Tovani-Palone, Marcos Roberto, Tram, Khai Hoan, Tran, Nghia Minh, Trico, Domenico, Trihandini, Indang, Tromans, Samuel Joseph, Truong, Vien T, Truyen, Thien Tan Tri Tai, Tsermpini, Evangelia Eirini, Tumurkhuu, Munkhtuya, Tung, Kang, Tyrovolas, Stefanos, Ubah, Chukwudi S, Udoakang, Aniefiok John, Udoh, Arit, Ulhaq, Inam, Ullah, Saeed, Ullah, Sana, Umair, Muhammad, Umar, Tungki Pratama, Umeokonkwo, Chukwuma David, Umesh, Anushri, Unim, Brigid, Unnikrishnan, Bhaskaran, Upadhyay, Era, Urso, Daniele, Vacante, Marco, Vahdani, Amir Mohammad, Vaithinathan, Asokan Govindaraj, Valadan Tahbaz, Sahel, Valizadeh, Rohollah, Van den Eynde, Jef, Varavikova, Elena, Varga, Orsolya, Varma, Siddhartha Alluri, Vart, Priya, Varthya, Shoban Babu, Vasankari, Tommi Juhani, Veerman, Lennert J, Venketasubramanian, Narayanaswamy, Venugopal, Deneshkumar, Verghese, Nicholas Alexander, Verma, Madhur, Verma, Pratibha, Veroux, Massimiliano, Verras, Georgios-Ioannis, Vervoort, Dominique, Vieira, Rafael José, Villafañe, Jorge Hugo, Villani, Leonardo, Villanueva, Gabriela Ines, Villeneuve, Paul J, Violante, Francesco S, Visontay, Rachel, Vlassov, Vasily, Vo, Bay, Vollset, Stein Emil, Volovat, Simona Ruxandra, Volovici, Victor, Vongpradith, Avina, Vos, Theo, Vujcic, Isidora S, Vukovic, Rade, Wado, Yohannes Dibaba, Wafa, Hatem A, Waheed, Yasir, Wamai, Richard G, Wang, Cong, Wang, Denny, Wang, Fang, Wang, Shu, Wang, Song, Wang, Yanzhong, Wang, Yuan-Pang, Ward, Paul, Watson, Stefanie, Weaver, Marcia R, Weerakoon, Kosala Gayan, Weiss, Daniel J, Weldemariam, Abrha Hailay, Wells, Katherine M, Wen, Yi Feng, Werdecker, Andrea, Westerman, Ronny, Wickramasinghe, Dakshitha Praneeth, Wickramasinghe, Nuwan Darshana, Wijeratne, Tissa, Wilson, Shadrach, Wojewodzic, Marcin W, Wool, Eve E, Woolf, Anthony D, Wu, Dongze, Wulandari, Ratna Dwi, Xiao, Hong, Xu, Bin, Xu, Xiaoyue, Yadav, Lalit, Yaghoubi, Sajad, Yang, Lin, Yano, Yuichiro, Yao, Yao, Ye, Pengpeng, Yesera, Gesila Endashaw, Yesodharan, Renjulal, Yesuf, Subah Abderehim, Yiğit, Arzu, Yiğit, Vahit, Yip, Paul, Yon, Dong Keon, Yonemoto, Naohiro, You, Yuyi, Younis, Mustafa Z, Yu, Chuanhua, Zadey, Siddhesh, Zadnik, Vesna, Zafari, Nima, Zahedi, Mohammad, Zahid, Muhammad Nauman, Zahir, Mazyar, Zakham, Fathiah, Zaki, Nazar, Zakzuk, Josefina, Zamagni, Giulia, Zaman, Burhan Abdullah, Zaman, Sojib Bin, Zamora, Nelson, Zand, Ramin, Zandi, Milad, Zandieh, Ghazal G Z, Zanghì, Aurora, Zare, Iman, Zastrozhin, Mikhail Sergeevich, Zeariya, Mohammed G M, Zeng, Youjie, Zhai, Chunxia, Zhang, Chen, Zhang, Haijun, Zhang, Hongwei, Zhang, Yunquan, Zhang, Zhaofeng, Zhang, Zhenyu, Zhao, Hanqing, Zhao, Yang, Zhao, Yong, Zheng, Peng, Zhong, Chenwen, Zhou, Juexiao, Zhu, Bin, Zhu, Zhaohua, Ziaeefar, Pardis, Zielińska, Magdalena, Zou, Zhiyong, Zumla, Alimuddin, Zweck, Elric, Zyoud, Samer H, Lim, Stephen S, and Murray, Christopher J L
Published: 2024

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