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1. z-GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies: I. Overview

Author: Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-Fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiab, A., Van Der Werf, P., Yang, C., Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-Fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiab, A., Van Der Werf, P., and Yang, C.
Abstract: Using the IRAM NOrthern Extended Millimetre Array (NOEMA), we conducted a Large Programme (z-GAL) to measure redshifts for 126 bright galaxies detected in the Herschel Astrophysical Large Area Survey (H-ATLAS), the HerMES Large Mode Survey (HeLMS), and the Herschel Stripe 82 (HerS) Survey. We report reliable spectroscopic redshifts for a total of 124 of the Herschel-selected galaxies. The redshifts are estimated from scans of the 3 and 2-mm bands (and, for one source, the 1-mm band), covering up to 31 GHz in each band, and are based on the detection of at least two emission lines. Together with the Pilot Programme, where 11 sources had their spectroscopic redshifts measured, our survey has derived precise redshifts for 135 bright Herschel-selected galaxies, making it the largest sample of high-z galaxies with robust redshifts to date. Most emission lines detected are from 12CO (mainly from J = 2 1 to 5 4), with some sources seen in [CI] and H2O emission lines. The spectroscopic redshifts are in the range 0.8 < z < 6.55 with a median value of z = 2.56 ± 0.10, centred on the peak epoch of galaxy formation. The linewidths of the sources are large, with a mean value for the full width at half maximum I- V of 590 ± 25 km s-1 and with 35% of the sources having widths of 700 km s-1 < I- V < 1800 km s-1. Most of the sources are unresolved or barely resolved on scales of ∼2 to 3; (or linear sizes of ∼15 - 25 kpc, unlensed). Some fields reveal double or multiple sources in line emission and the underlying dust continuum and, in some cases, sources at different redshifts. Taking these sources into account, there are, in total, 165 individual sources with robust spectroscopic redshifts, including lensed galaxies, binary systems, and over-densities. This paper presents an overview of the z-GAL survey and provides the observed properties of the emission lines, the derived spectroscopic redshifts, and a catalogu
Published: 2023

2. z -GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies: III. Physical properties

Author: Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J.L.C., Beelen, A., Weib, A., Nanni, A., Omont, A., Van Der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C., Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J.L.C., Beelen, A., Weib, A., Nanni, A., Omont, A., Van Der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., and Vlahakis, C.
Abstract: The z-GAL survey observed 137 bright Herschel-selected targets with the IRAM Northern Extended Millimeter Array, with the aim to measure their redshift and study their properties. Several of them have been resolved into multiple sources. Consequently, robust spectroscopic redshifts have been measured for 165 individual galaxies in the range 0.8., <., z., <., 6.5. In this paper we analyse the millimetre spectra of the z-GAL sources, using both their continuum and line emission to derive their physical properties. At least two spectral lines are detected for each source, including transitions of 12CO, [CI], and H2O. The observed 12CO line ratios and spectral line energy distributions of individual sources resemble those of local starbursts. In seven sources the para-H2O (211-202) transition is detected and follows the IR versus H2O luminosity relation of sub-millimetre galaxies. The molecular gas mass of the z-GAL sources is derived from their 12CO, [CI], and sub-millimetre dust continuum emission. The three tracers lead to consistent results, with the dust continuum showing the largest scatter when compared to 12CO. The gas-to-dust mass ratio of these sources was computed by combining the information derived from 12CO and the dust continuum and has a median value of 107, similar to star-forming galaxies of near-solar metallicity. The same combined analysis leads to depletion timescales in the range between 0.1 and 1.0 Gyr, which place the z-GAL sources between the main sequence' of star formation and the locus of starbursts. Finally, we derived a first estimate of stellar masses "modulo possible gravitational magnification "by inverting known gas scaling relations: the z-GAL sample is confirmed to be mostly composed by starbursts, whereas ∼25% of its members lie on the main sequence of star-forming galaxies (within ±0.5 dex).
Published: 2023

3. The hidden side of cosmic star formation at z > 3 Bridging optically dark and Lyman-break galaxies with GOODS-ALMA

Author: Xiao, M.-y., Elbaz, D., Gómez-guijarro, C., Leroy, L., Bing, L.-j., Daddi, E., Magnelli, B., Franco, M., Zhou, L., Dickinson, M., Wang, T., Rujopakarn, W., Magdis, G. E., Treister, E., Inami, H., Demarco, R., Sargent, M. T., Shu, X., Kartaltepe, J. S., Alexander, D. M., Béthermin, M., Bournaud, F., Ciesla, L., Ferguson, H. C., Finkelstein, S. L., Giavalisco, M., Gu, Q.-s., Iono, D., Juneau, S., Lagache, G., Leiton, R., Messias, H., Motohara, K., Mullaney, J., Nagar, N., Pannella, M., Papovich, C., Pope, A., Schreiber, C., Silverman, J., Xiao, M.-y., Elbaz, D., Gómez-guijarro, C., Leroy, L., Bing, L.-j., Daddi, E., Magnelli, B., Franco, M., Zhou, L., Dickinson, M., Wang, T., Rujopakarn, W., Magdis, G. E., Treister, E., Inami, H., Demarco, R., Sargent, M. T., Shu, X., Kartaltepe, J. S., Alexander, D. M., Béthermin, M., Bournaud, F., Ciesla, L., Ferguson, H. C., Finkelstein, S. L., Giavalisco, M., Gu, Q.-s., Iono, D., Juneau, S., Lagache, G., Leiton, R., Messias, H., Motohara, K., Mullaney, J., Nagar, N., Pannella, M., Papovich, C., Pope, A., Schreiber, C., and Silverman, J.
Published: 2023

4. The hidden side of cosmic star formation at z > 3:Bridging optically dark and Lyman-break galaxies with GOODS-ALMA

Author: Xiao, M. Y., Elbaz, D., Gómez-Guijarro, C., Leroy, L., Bing, L. J., Daddi, E., Magnelli, B., Franco, M., Zhou, L., Dickinson, M., Wang, T., Rujopakarn, W., Magdis, G. E., Treister, E., Inami, H., Demarco, R., Sargent, M. T., Shu, X., Kartaltepe, J. S., Alexander, D. M., Béthermin, M., Bournaud, F., Ciesla, L., Ferguson, H. C., Finkelstein, S. L., Giavalisco, M., Gu, Q. S., Iono, D., Juneau, S., Lagache, G., Leiton, R., Messias, H., Motohara, K., Mullaney, J., Nagar, N., Pannella, M., Papovich, C., Pope, A., Schreiber, C., Silverman, J., Xiao, M. Y., Elbaz, D., Gómez-Guijarro, C., Leroy, L., Bing, L. J., Daddi, E., Magnelli, B., Franco, M., Zhou, L., Dickinson, M., Wang, T., Rujopakarn, W., Magdis, G. E., Treister, E., Inami, H., Demarco, R., Sargent, M. T., Shu, X., Kartaltepe, J. S., Alexander, D. M., Béthermin, M., Bournaud, F., Ciesla, L., Ferguson, H. C., Finkelstein, S. L., Giavalisco, M., Gu, Q. S., Iono, D., Juneau, S., Lagache, G., Leiton, R., Messias, H., Motohara, K., Mullaney, J., Nagar, N., Pannella, M., Papovich, C., Pope, A., Schreiber, C., and Silverman, J.
Abstract: Our current understanding of the cosmic star formation history at z > 3 is primarily based on UV-selected galaxies (Lyman-break galaxies, i.e., LBGs). Recent studies of H-dropouts (HST-dark galaxies) have revealed that we may be missing a large proportion of star formation that is taking place in massive galaxies at z > 3. In this work, we extend the H-dropout criterion to lower masses to select optically dark or faint galaxies (OFGs) at high redshifts in order to complete the census between LBGs and H-dropouts. Our criterion (H > 26.5 mag & [4.5] < 25 mag) combined with a de-blending technique is designed to select not only extremely dust-obscured massive galaxies but also normal star-forming galaxies (typically E(B − V) > 0.4) with lower stellar masses at high redshifts. In addition, with this criterion, our sample is not contaminated by massive passive or old galaxies. In total, we identified 27 OFGs at zphot > 3 (with a median of zmed = 4.1) in the GOODS-ALMA field, covering a wide distribution of stellar masses with log(M⋆/M⊙) = 9.4 − 11.1 (with a median of log(M⋆med/M⊙) = 10.3). We find that up to 75% of the OFGs with log(M⋆/M⊙) = 9.5 − 10.5 were neglected by previous LBGs and H-dropout selection techniques. After performing an optical-to-millimeter stacking analysis of the OFGs, we find that rather than being limited to a rare population of extreme starbursts, these OFGs represent a normal population of dusty star-forming galaxies at z > 3. The OFGs exhibit shorter gas depletion timescales, slightly lower gas fractions, and lower dust temperatures than the scaling relation of typical star-forming galaxies. Additionally, the total star formation rate (SFRtot = SFRIR + SFRUV) of the stac
Published: 2023

5. Selection of powerful radio galaxies with machine learning

Author: Carvajal, R., Matute, I., Afonso, J., Norris, R. P., Luken, K. J., Sánchez-Sáez, P., Cunha, P. A. C., Humphrey, A., Messias, H., Amarantidis, S., Barbosa, D., Cruz, H. A., Miranda, H., Paulino-Afonso, A., Pappalardo, C., Carvajal, R., Matute, I., Afonso, J., Norris, R. P., Luken, K. J., Sánchez-Sáez, P., Cunha, P. A. C., Humphrey, A., Messias, H., Amarantidis, S., Barbosa, D., Cruz, H. A., Miranda, H., Paulino-Afonso, A., and Pappalardo, C.
Abstract: We developed and trained a pipeline of three machine learning (ML) models than can predict which sources are more likely to be an AGN and to be detected in specific radio surveys. Also, it can estimate redshift values for predicted radio-detectable AGNs. These models, which combine predictions from tree-based and gradient-boosting algorithms, have been trained with multi-wavelength data from near-infrared-selected sources in the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Spring field. Training, testing, calibration, and validation were carried out in the HETDEX field. Further validation was performed on near-infrared-selected sources in the Stripe 82 field. In the HETDEX validation subset, our pipeline recovers 96% of the initially labelled AGNs and, from AGNs candidates, we recover 50% of previously detected radio sources. For Stripe 82, these numbers are 94% and 55%. Compared to random selection, these rates are two and four times better for HETDEX, and 1.2 and 12 times better for Stripe 82. The pipeline can also recover the redshift distribution of these sources with $\sigma_{\mathrm{NMAD}}$ = 0.07 for HETDEX ($\sigma_{\mathrm{NMAD}}$ = 0.09 for Stripe 82) and an outlier fraction of 19% (25% for Stripe 82), compatible with previous results based on broad-band photometry. Feature importance analysis stresses the relevance of near- and mid-infrared colours to select AGNs and identify their radio and redshift nature. Combining different algorithms in ML models shows an improvement in the prediction power of our pipeline over a random selection of sources. Tree-based ML models (in contrast to deep learning techniques) facilitate the analysis of the impact that features have on the predictions. This prediction can give insight into the potential physical interplay between the properties of radio AGNs (e.g. mass of black hole and accretion rate)., Comment: Accepted for publication in A&A, 24 pages and 21 figures. Updated to include information on retrieval of data and models, which can be obtained from https://zenodo.org/doi/10.5281/zenodo.10220008
Published: 2023
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6. z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [III] Physical properties

Author: Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J., Beelen, A., Weiss, A., Nanni, A., Omont, A., van der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C., Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J., Beelen, A., Weiss, A., Nanni, A., Omont, A., van der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., and Vlahakis, C.
Abstract: The z-GAL survey observed 137 bright Herschel-selected targets with the IRAM NOrthern Extended Millimeter Array, with the aim to measure their redshift and study their properties. Several of them have been resolved into multiple sources. Consequently, robust spectroscopic redshifts have been measured for 165 individual galaxies in the range 0.8
Published: 2023
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7. z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [II] Dust properties

Author: Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., van der Werf, P., Vlahakis, C., Weiss, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Krips, B. M. Jones M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Urquhart, S., Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., van der Werf, P., Vlahakis, C., Weiss, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Krips, B. M. Jones M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., and Urquhart, S.
Abstract: (Abridged) We present the dust properties of 125 bright Herschel galaxies selected from the z-GAL survey. The large instantaneous bandwidth of NOEMA provides an exquisite sampling of the underlying dust continuum emission at 2 and 3 mm in the observed frame, with flux densities in at least four side bands for each source. Together with the available Herschel 250, 350, and 500 micron and SCUBA-2 850 micron flux densities, the spectral energy distribution of each source can be analyzed from the far-infrared to the millimeter, with a fine sampling of the Rayleigh-Jeans tail. This wealth of data provides a solid basis to derive robust dust properties, in particular the dust emissivity index, beta, and the dust temperature, T(dust). In order to demonstrate our ability to constrain the dust properties, we used a flux-generated mock catalog and analyzed the results under the assumption of an optically thin and optically thick modified black body emission. For the z-GAL sources, we report a range of dust emissivities with beta ~ 1.5 - 3 estimated up to high precision with relative uncertainties that vary in the range 7% - 15%, and an average of 2.2 +/- 0.3. We find dust temperatures varying from 20 to 50 K with an average of T(dust) ~ 30 K for the optically thin case and ~38 K in the optically thick case. For all the sources, we estimate the dust masses and apparent infrared luminosities (based on the optically thin approach). An inverse correlation is found between T(dust) and beta, which is similar to what is seen in the local Universe. Finally, we report an increasing trend in the dust temperature as a function of redshift at a rate of 6.5 +/- 0.5 K/z for this 500 micron-selected sample. Based on this study, future prospects are outlined to further explore the evolution of dust temperature across cosmic time., Comment: Accepted for publication on A&A; 32 pages; 26 figures
Published: 2023
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8. z-GAL -- A NOEMA spectroscopic redshift survey of bright Herschel galaxies: [I] Overview

Author: Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-Fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiss, A., van der Werf, P., Yang, C., Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-Fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiss, A., van der Werf, P., and Yang, C.
Abstract: (Abridged) Using the IRAM NOEMA interferometer, we measures the redshifts of 126 bright galaxies detected in the Herschel H-ATLAS, HeLMS, and HerS surveys. We report reliable spectroscopic redshifts for a total of 124 of the Herschel-selected galaxies. The redshifts are estimated from scans of the 3 and 2-mm bands (and, in one case, the 1-mm band) and are based on the detection of at least two emission lines. Together with the Pilot Programme (Neri et al. 2020), including spectroscopic redshifts of 11 sources, our survey has derived precise redshifts for 135 bright Herschel-selected galaxies, making it the largest sample of high-z galaxies with robust redshifts to date. Most emission lines detected are from 12CO (mainly from J=2-1 to 5-4), with some sources seen in [CI] and H2O emission lines. The spectroscopic redshifts are in the range 0.8
Published: 2023
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9. ALMA High-Level Data Products: Submillimetre counterparts of SDSS quasars in the ALMA footprint

Author: Wong, A., Hatziminaoglou, E., Borkar, A., Popping, G., Pérez-Fournon, I., Poidevin, F., Stoehr, F., Messias, H., Wong, A., Hatziminaoglou, E., Borkar, A., Popping, G., Pérez-Fournon, I., Poidevin, F., Stoehr, F., and Messias, H.
Abstract: The Atacama Large Millimetre/submillimetre Array (ALMA) is the world's most advanced radio interferometric facility, producing science data with an average rate of about 1 TB per day. After a process of calibration, imaging and quality assurance, the scientific data are stored in the ALMA Science Archive (ASA), along with the corresponding raw data, making the ASA an invaluable resource for original astronomical research. Due to their complexity, each ALMA data set has the potential for scientific results that go well beyond the ideas behind the original proposal that led to each observation. For this reason, the European ALMA Regional Centre initiated the High-Level Data Products initiative to develop science-oriented data products derived from data sets publicly available in the ASA, that go beyond the formal ALMA deliverables. The first instance of this initiative is the creation of a catalogue of submillimetre (submm) detections of Sloan Digital Sky Survey (SDSS) quasars from the SDSS Data Release 14 that lie in the aggregate ALMA footprint observed since ALMA Cycle 0. The ALMA fluxes are extracted in an automatic fashion, using the ALMA Data Mining Toolkit. All extractions above a signal-to-noise cut of 3.5 are considered, they have been visually inspected and the reliable detections are presented in a catalogue of 376 entries, corresponding to 275 unique quasars. Interesting targets found in the process, i.e. lensed or jetted quasars as well as quasars with nearby submm counterparts are highlighted, to facilitate further studies or potential follow up observations.
Published: 2023
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10. Bright Extragalactic ALMA Redshift Survey (BEARS) III: Detailed study of emission lines from 71 Herschel targets

Author: Hagimoto, M., Bakx, T. J. L. C., Serjeant, S., Bendo, G. J., Urquhart, S. A., Eales, S., Harrington, K. C., Tamura, Y., Umehata, H., Berta, S., Cooray, A. R., Cox, P., De Zotti, G., Lehnert, M. D., Riechers, D. A., Scott, D., Temi, P., van der Werf, P. P., Yang, C., Amvrosiadis, A., Andreani, P. M., Baker, A. J., Beelen, A., Borsato, E., Buat, V., Butler, K. M., Dannerbauer, H., Dunne, L., Dye, S., Enia, A. F. M., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Ivison, R. J., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Neri, R., Omont, A., Perez-Fournon, I., Sedgwick, C., Smith, M. W. L., Stanley, F., Verma, A., Vlahakis, C., Ward, B., Weiner, C., Weiss, A., Young, A. J., Hagimoto, M., Bakx, T. J. L. C., Serjeant, S., Bendo, G. J., Urquhart, S. A., Eales, S., Harrington, K. C., Tamura, Y., Umehata, H., Berta, S., Cooray, A. R., Cox, P., De Zotti, G., Lehnert, M. D., Riechers, D. A., Scott, D., Temi, P., van der Werf, P. P., Yang, C., Amvrosiadis, A., Andreani, P. M., Baker, A. J., Beelen, A., Borsato, E., Buat, V., Butler, K. M., Dannerbauer, H., Dunne, L., Dye, S., Enia, A. F. M., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Ivison, R. J., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Neri, R., Omont, A., Perez-Fournon, I., Sedgwick, C., Smith, M. W. L., Stanley, F., Verma, A., Vlahakis, C., Ward, B., Weiner, C., Weiss, A., and Young, A. J.
Abstract: We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies between redshifts 1.4 to 4.6 detected by the Atacama Large Millimetre/submillimetre Array. These lines include a total of 156 CO, [C I], and H2O emission lines. For 46 galaxies, we detect two transitions of CO lines, and for these galaxies we find gas properties similar to those of other dusty star-forming galaxy (DSFG) samples. A comparison to photo-dissociation models suggests that most of Herschel-selected galaxies have similar interstellar medium conditions as local infrared-luminous galaxies and high-redshift DSFGs, although with denser gas and more intense far-ultraviolet radiation fields than normal star-forming galaxies. The line luminosities agree with the luminosity scaling relations across five orders of magnitude, although the star-formation and gas surface density distributions (i.e., Schmidt-Kennicutt relation) suggest a different star-formation phase in our galaxies (and other DSFGs) compared to local and low-redshift gas-rich, normal star-forming systems. The gas-to-dust ratios of these galaxies are similar to Milky Way values, with no apparent redshift evolution. Four of 46 sources appear to have CO line ratios in excess of the expected maximum (thermalized) profile, suggesting a rare phase in the evolution of DSFGs. Finally, we create a deep stacked spectrum over a wide rest-frame frequency (220-890 GHz) that reveals faint transitions from HCN and CH, in line with previous stacking experiments., Comment: 30 pages, 17 figures, accepted for publication in Monthly Notices of the Royal Astronomical Society Main Journal. Comments are warmly welcomed
Published: 2023
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11. The Bright Extragalactic ALMA Redshift Survey (BEARS) II: Millimetre photometry of gravitational lens candidates

Author: Bendo, G. J., Urquhart, S. A., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M. D., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., González-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Jones, B. M., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Pérez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., van der Werf, P., Verma, A., Vlahakis, C., Weiß, A., Yang, C., Young, A. J., Bendo, G. J., Urquhart, S. A., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M. D., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., González-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D. H., Ismail, D., Jones, B. M., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Pérez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., van der Werf, P., Verma, A., Vlahakis, C., Weiß, A., Yang, C., and Young, A. J.
Abstract: We present 101 and 151 GHz ALMA continuum images for 85 fields selected from Herschel observations that have 500 micron flux densities >80 mJy and 250-500 micron colours consistent with z > 2, most of which are expected to be gravitationally lensed or hyperluminous infrared galaxies. Approximately half of the Herschel 500 micron sources were resolved into multiple ALMA sources, but 11 of the 15 brightest 500 micron Herschel sources correspond to individual ALMA sources. For the 37 fields containing either a single source with a spectroscopic redshift or two sources with the same spectroscopic redshift, we examined the colour temperatures and dust emissivity indices. The colour temperatures only vary weakly with redshift and are statistically consistent with no redshift-dependent temperature variations, which generally corresponds to results from other samples selected in far-infrared, submillimetre, or millimetre bands but not to results from samples selected in optical or near-infrared bands. The dust emissivity indices, with very few exceptions, are largely consistent with a value of 2. We also compared spectroscopic redshifts to photometric redshifts based on spectral energy distribution templates designed for infrared-bright high-redshift galaxies. While the templates systematically underestimate the redshifts by ~15%, the inclusion of ALMA data decreases the scatter in the predicted redshifts by a factor of ~2, illustrating the potential usefulness of these millimetre data for estimating photometric redshifts., Comment: Accepted for publication in Monthly Notices of the Royal Astronomical Society
Published: 2023
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12. z-GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies: I.Overview

Author: Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiß, A., Van Der Werf, P., Yang, C., Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiß, A., Van Der Werf, P., and Yang, C.
Published: 2023

13. z -GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies II. Dust properties

Author: Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., Van Der Werf, P., Vlahakis, C., Weiß, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Krips, M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., Urquhart, S., Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., Van Der Werf, P., Vlahakis, C., Weiß, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Krips, M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., and Urquhart, S.
Published: 2023

14. z-GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies III. Physical properties

Author: Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J. L. C., Beelen, A., Weiß, A., Nanni, A., Omont, A., Van Der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C., Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J. L. C., Beelen, A., Weiß, A., Nanni, A., Omont, A., Van Der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., and Vlahakis, C.
Published: 2023

15. The hidden side of cosmic star formation at z > 3 Bridging optically dark and Lyman-break galaxies with GOODS-ALMA

Author: Xiao, M.-y., Elbaz, D., Gómez-guijarro, C., Leroy, L., Bing, L.-j., Daddi, E., Magnelli, B., Franco, M., Zhou, L., Dickinson, M., Wang, T., Rujopakarn, W., Magdis, G. E., Treister, E., Inami, H., Demarco, R., Sargent, M. T., Shu, X., Kartaltepe, J. S., Alexander, D. M., Béthermin, M., Bournaud, F., Ciesla, L., Ferguson, H. C., Finkelstein, S. L., Giavalisco, M., Gu, Q.-s., Iono, D., Juneau, S., Lagache, G., Leiton, R., Messias, H., Motohara, K., Mullaney, J., Nagar, N., Pannella, M., Papovich, C., Pope, A., Schreiber, C., Silverman, J., Xiao, M.-y., Elbaz, D., Gómez-guijarro, C., Leroy, L., Bing, L.-j., Daddi, E., Magnelli, B., Franco, M., Zhou, L., Dickinson, M., Wang, T., Rujopakarn, W., Magdis, G. E., Treister, E., Inami, H., Demarco, R., Sargent, M. T., Shu, X., Kartaltepe, J. S., Alexander, D. M., Béthermin, M., Bournaud, F., Ciesla, L., Ferguson, H. C., Finkelstein, S. L., Giavalisco, M., Gu, Q.-s., Iono, D., Juneau, S., Lagache, G., Leiton, R., Messias, H., Motohara, K., Mullaney, J., Nagar, N., Pannella, M., Papovich, C., Pope, A., Schreiber, C., and Silverman, J.
Published: 2023

16. z-GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies: I.Overview

Author: Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiß, A., Van Der Werf, P., Yang, C., Cox, P., Neri, R., Berta, S., Ismail, D., Stanley, F., Young, A., Jin, S., Bakx, T., Beelen, A., Dannerbauer, H., Krips, M., Lehnert, M., Omont, A., Riechers, D. A., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Marchetti, L., Messias, H., Nanni, A., Negrello, M., Perez-fournon, I., Serjeant, S., Urquhart, S., Vlahakis, C., Weiß, A., Van Der Werf, P., and Yang, C.
Published: 2023

17. z-GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies III. Physical properties

Author: Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J. L. C., Beelen, A., Weiß, A., Nanni, A., Omont, A., Van Der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C., Berta, S., Stanley, F., Ismail, D., Cox, P., Neri, R., Yang, C., Young, A. J., Jin, S., Dannerbauer, H., Bakx, T. J. L. C., Beelen, A., Weiß, A., Nanni, A., Omont, A., Van Der Werf, P., Krips, M., Baker, A. J., Bendo, G., Borsato, E., Buat, V., Butler, K. M., Chartab, N., Cooray, A., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R. J., Jones, B. M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., and Vlahakis, C.
Published: 2023

18. z -GAL:A NOEMA spectroscopic redshift survey of bright Herschel galaxies II. Dust properties

Author: Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., Van Der Werf, P., Vlahakis, C., Weiß, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Krips, M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., Urquhart, S., Ismail, D., Beelen, A., Buat, V., Berta, S., Cox, P., Stanley, F., Young, A., Jin, S., Neri, R., Bakx, T., Dannerbauer, H., Butler, K., Cooray, A., Nanni, A., Omont, A., Serjeant, S., Van Der Werf, P., Vlahakis, C., Weiß, A., Yang, C., Baker, A. J., Bendo, G., Borsato, E., Chartab, N., Dye, S., Eales, S., Gavazzi, R., Hughes, D., Ivison, R., Jones, B. M., Krips, M., Lehnert, M., Marchetti, L., Messias, H., Negrello, M., Perez-fournon, I., Riechers, D. A., and Urquhart, S.
Published: 2023

19. BJS commission on surgery and perioperative care post-COVID-19

Author: Abahuje, E, Abbas, A, Abd El Aziz Abd El Maksoud, M, Abdelhady, A, Abdelhamid, S, Abdelkarem Ahmed Faraj, H, Abdelqader, B, Abdelrahman, T, Abdou, H, Abdullah, A, Abedua Harrison, M, Abem Owusu, E, Aboalazayem, A, Aboulhosn, R, Abu Oda, S, Abubakar, A, Abutaka, A, Acevedo Fontalvo, D, Acuna, S, Adefemi, A, Adegbola, S, Adenuga, T, Adeyeye, A, Adil Hilmi, A, Adisa, A, Aditya, K, Adjeso, T, Aftab, R, Afzal, A, Aggarwal, V, Aggarwal, A, Aguilera, R, Aguilera-Arevalo, M, Aguirre Salamanca, E, Aguirre-Allende, I, Ahari, D, Ahmad, H, Ahmad Rauf, F, Ahmad Zartasht Khan, A, Ahmed, S, Ahmed Fieturi, N, Ahmed Mohamed, S, Ahmed-Bakhsh, Z, Ahsan Javed, M, Akano, L, Akbar, A, Akhbari, M, Akhmedov, P, Aksit, G, Akula, Y, Alagaratnam, A, Al Majid, S, Al Mukhtar, O, Al Omran, H, Alasali, N, Al-Azzawi, M, Al-Habsi, R, Al-Iraqi, H, Al-Naggar, H, Alameer, E, Albirnawi, H, Alderson, D, Aldulaijan, F, Alejandro Miranda Ojeda, R, Alhasan, A, Ali, S, Ali, A, Ali Khan, M, Alimova, Y, Aljanadi, F, Aljubure, R, Allopi, N, Almedbal, H, Almubarak, M, Alqaidoom, Z, Alselaim, N, Alshaar, M, Alshammari, R, Altaf, K, Altiner, S, Altunpak, B, Alvarez Lozada, L, Amal Nahal, E, Amer, A, Amin, K, Aminu, U, Amisi Numbi, N, Amjad, T, Amoah, R, An, Y, Anastasopoulos, N, Andres Urrutia, J, Angarita, F, Angarita, K, Angel Freiria Eiras, M, Antypas, A, Anwar, M, Anwar, H, Apampa, T, Apostolou, K, Aquina, C, Arachchige Adithi Himika Randeni, R, Archila Godinez, M, Arez, O, Arezzo, A, Armonis, P, Arshad, S, Arshad Salman, M, Arshid, A, Arteaga Asensio, P, Arthur, T, Arumuga Jothi, A, Aryo Damara, F, Asensio Gomez, L, Ashcroft, J, Ashraf, S, Asif, A, Atif, M, Attaullah Khan, M, Avellaneda, N, Awad, S, Awadh, M, Axiaq, A, Ayad Mohammed Shuwayyah, A, Ayalew, D, Aytac, E, Azam, F, Azevedo, J, Azhar, B, Aziz, J, Aziz, A, Azzam, A, Baba Ndajiwo, A, Baig, M, Baker, D, Bakko, F, Balachandran, R, Balachandran, G, Balagizi Mudekereza, J, Balai, E, Balci, B, Balduzzi, A, Balhareth, A, Bandyopadhyay, S, Banerjee, D, Bangalore Mahalinga, D, Bankhead-Kendall, B, Bankole, N, Banwell, V, Baris Bengur, F, Baris Ozmen, B, Barnard, M, Barnett, R, Barreras Espinoza, J, Barrios, A, Bass, G, Bass, M, Bausys, A, Bavikatte, A, Bayram, J, Belousov, M, Berardi, A, Beamish, A, Beattie, C, Belia, F, Bellato, V, Bellikatti, S, Benjamens, S, Benlice, C, Bennedsgaard, S, Bennett, S, Bentounsi, Z, Bergenfeldt, H, Bergenfelz, A, Besselink, M, Bhandoria, G, Bhangu, E, Bhatia, M, Bhatti, M, Bilgili, Z, Bislenghi, G, Bisset, C, Biswas, S, Blake, J, Blanco, R, Boccalatte, L, Boden, R, Bojanic, C, Boland, M, Boland, P, Bollen, E, Bonci, E, Boni, L, Booth, A, Booth, R, Borakati, A, Borunda Escudero, G, Bosco, S, Bostrom, P, Botelho De Alencar Ferreira Cruz, P, Bouchagier, K, Bouhuwaish, A, Boutros, M, Boyce, K, Boyle, C, Bradshaw, L, Brandl, A, Brar, A, Brat, G, Brenkman, H, Brennan, C, Brines, C, Brookmyre, A, Brosnan, C, Brouwers, L, Brown, A, Brown, L, Brown, C, Brown, J, Bs, V, Buksh, M, Bunani Emmanuel, M, Burbano, D, Burelli, A, Burke, A, Burke, J, Burlov, N, Burns, A, Burton, O, Butt, A, Buzra Ozkan, B, Cabrera Silva, L, Caicedo, E, Calderbank, T, Cambridge, W, Campelo, G, Can Tatar, O, Carbone, F, Carrano, F, Casallas, D, Casanova Portoles, D, Casciani, F, Cassimjee, I, Castaneda Ramirez, O, Catalan, V, Caviedes, J, Cayetano, L, Ceresoli, M, Chan, M, Chan, V, Chandrasinghe, P, Chapman, S, Chaturvedi, A, Chaudhry, D, Chaudry, H, Chen, H, Cheng, A, Chernykh, M, Cherrie, A, Cheruiyot, I, Cheung, J, Chia, C, Chica, J, Chinai, N, Chirwa, A, Chiwaligo, J, Choi, A, Choi, J, Chowdhury, M, Christopher, E, Christou, N, Chu, T, Chua, D, Chua, H, Chung, C, Cihat Yildirim, A, Cillo, M, Cioffi, S, Claireaux, H, Clermonts, S, Clifford, R, Climent, M, Clynch, A, Coelen, R, Colas-Ruiz, E, Collar, A, Collard, M, Conlon, K, Connelly, T, Connor, K, Cook, J, Correia De Sa, T, Cosgun Acar, N, Costa, T, Couch, D, Cowper, S, Creavin, B, Crook, B, Curell, A, D'Alessio, R, Dale, J, Damgaard Eriksen, J, Dario Martin Gonzalez, I, Darwish, A, Das, M, Das, R, Das, K, Dave, R, David, S, Davies, T, Davis, C, Davison, S, Davletshina, V, Dawidziuk, A, Dawson, A, De Andres Crespo, M, De Berker, H, De Dieu Ngo, P, Dekker, E, De La Caridad Espinosa Luis, R, De Lacy, B, Demartines, N, De Montserrat Medina Sifuentes, A, De Silva, S, Del Rio, C, Delaune, V, Dell, A, Demirbas, I, Demirli Atici, S, Deniz Tepe, M, Derebey, M, Desai, G, Desai, M, Devarakonda, S, Deveras, N, Di Franco, G, Di Martino, M, Di Marzo, F, Diaz, A, Diaz Del Gobbo, G, Diazcastrillon, C, Dick, L, Dickinson, K, Diego, E, Dimasi, I, Ding, A, Dingemans, S, Dixon, L, Dixon, B, Doherty, W, Dooreemeah, D, Donohue, C, Dornseifer, M, Dossa, F, Dossou, W, Drake, T, Drami, I, Drevin, G, Du Plessis, M, Dudi-Venkata, N, Dudley, R, Duffy, S, Duklas, D, Dumbrava, B, Duygu Avlar, F, Dworzynska, A, Ebrahim, W, Ebrahim, A, Efren Lozada Hernandez, E, Ehigie, N, El Boghdady, M, El Hasnaoui, C, El Sheikh, M, El-Hussuna, A, Eldurssi, O, Elfeki, H, Elhadi, M, Elhassan, M, Elhissi, A, Elliot, B, Elsenbroek, C, Elsolh, B, Elson, N, Eltyeb, H, Emerson, H, Emile, S, Endalle, G, English, W, Ercisli, C, Espinosa, G, Essam Abdelraheem, M, Essangri, H, Etienne, P, Evans, M, Evans, T, Ezeme, C, Ezzahraa, F, Fadalla, T, Fagan, J, Fahmy, M, Fairfield, C, Falade, O, Famularo, S, Faqar-Uz-Zaman, F, Farid, Y, Farooq, A, Farooq, H, Farooqui, F, Farquharson, B, Faruqi, A, Faulder, R, Faut, M, Fechner, K, Feenstra, T, Fehervari, M, Fernandez, L, Fernandez Alberti, J, Ferrario, L, Field, D, Fiore, L, Fingerhut, S, Finlayson, S, Fleming, N, Fleming, C, Florial, E, Fok, M, Fokin, D, Foley, M, Forero, M, Forgan, T, Fornasiero, M, Fowler, H, Fowler, G, Franchi, E, Franklin, L, Fredriksson, A, Fruhling, P, Fuentes Navarrette, G, Fulop, A, Furtado, M, Gaarder, T, Galbraith, N, Gallagher, I, Gallo, G, Gana, T, Gaskin, E, Gasparini, M, Gatan, R, Geary, E, Gelaye Wudineh, K, Gemenetzis, G, Georgi, M, Ghalige, H, Ghareeb, W, Ghatwary Tantawy, T, Ghomsi, C, 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Hite, M, Hoh, S, Holmberg, C, Holmich, E, Holst, F, Hossam, A, Hossam Elfallal, A, Howard, P, Huaman, E, Huang, Y, Huang, L, Huang, D, Huber, T, Hugh, J, Hughes, J, Huttner, F, Huynh, R, Hylands, A, Iannuzzi, J, Ielpo, B, Iftikhar Talib, A, Ignacio, J, Ignatavicius, P, Ike, S, Ikwu, C, Inama, M, Ing, A, Ingels, A, Isik, A, Islam, N, Ives, I, Al-Hasan, A, Perez Rivera, C, Jacome, F, Jaffer, T, Jagiella-Lodise, O, Jain, M, Jain, K, Jakubauskas, M, Jalal, M, James, H, Jang, Y, Janssen, B, Jansson, H, Jariod-Ferrer, U, Javanmard, H, Javed, S, Jayarajah, U, Jayasuriya, I, Je, J, Jessop, Z, Jia Lin Tang, E, Jiang, H, Jiayan, Y, Jih Huei, T, Jimenez-Rodriguez, R, Joh, D, Johnson, A, Jones, N, Jones, C, Jordan, C, Jose Nunez Ju, J, Jose Pizarro, M, Jose Salazar, C, Joseph, J, Justiniano, C, Kabir, T, Kadhum, M, Kalfountzos, C, Kalogiannaki, E, Kalyanasundaram, K, Kamarajah, S, Kamil Quraishi, M, Kanemitsu, Y, Kapila, A, Kapila, V, Karagiannidis, G, Kashif, M, Kathiravelupillai, S, 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Abbas A., Abd El Aziz Abd El Maksoud M., Abdelhady A., Abdelhamid S., Abdelkarem Ahmed Faraj H., Abdelqader B., Abdelrahman T., Abdou H., Abdullah A., Abedua Harrison M., Abem Owusu E., Aboalazayem A., Aboulhosn R., Abu Oda S., Abubakar A., Abutaka A., Acevedo Fontalvo D., Acuna S., Adefemi A., Adegbola S., Adenuga T., Adeyeye A., Adil Hilmi A., Adisa A., Aditya K., Adjeso T., Aftab R., Afzal A., Aggarwal V., Aggarwal A., Aguilera R., Aguilera-Arevalo M. -L., Aguirre Salamanca E. 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A., Armonis P., Arshad S., Arshad Salman M., Arshid A., Arteaga Asensio P. C., Arthur T., Arumuga Jothi A., Aryo Damara F., Asensio Gomez L., Ashcroft J., Ashraf S., Asif A., Atif M., Attaullah Khan M., Avellaneda N., Awad S., Awadh M., Axiaq A., Ayad Mohammed Shuwayyah A., Ayalew D., Aytac E., Azam F., Azevedo J., Azhar B., Aziz J., Aziz A., Azzam A., Baba Ndajiwo A., Baig M., Baker D., Bakko F., Balachandran R., Balachandran G., Balagizi Mudekereza J., Balai E., Balci B., Balduzzi A., Balhareth A., Bandyopadhyay S., Banerjee D., Bangalore Mahalinga D., Bankhead-Kendall B., Bankole N. D. A., Banwell V., Baris Bengur F., Baris Ozmen B., Barnard M., Barnett R., Barreras Espinoza J. A., Barrios A., Bass G., Bass M., Bausys A., Bavikatte A., Bayram J., Belousov M., Berardi A. 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P., Forgan T., Fornasiero M., Fowler H., Fowler G., Franchi E., Franklin L., Fredriksson A., Fruhling P., Fuentes Navarrette G., Fulop A., Furtado M., Gaarder T., Galbraith N., Gallagher I. T. K., Gallo G., Gana T., Gaskin E., Gasparini M., Gatan R. G., Geary E., Gelaye Wudineh K., Gemenetzis G., Georgi M., Ghalige H., Ghareeb W., Ghatwary Tantawy T., Ghomsi C., Ghuman A., Giannakis P., Giron F., Gjengedal K., Gkotsis E., Glasbey J., Godahewa S., Godula D., Goffredo P., Goh S., Golriz M., Gomez L., Gomez Gomez D., Gonzalez R., Gonzalez D., Gonzalez Gutierrez E., Gopar D., Gordini L., Gori A., Gortazar S., Gousy N., Gowda R., Gowda M., Gqada J., Grechenig M., Greer J., Gregorio L., Grigorova A., Grimes H., Groot V., Grossman R. C., Gruber R., Gruter A., Guest R., Gujjuri R., Gulcek E., Gulcu B., Gull K., Gulmez M., Gupta V., Gutlic A., Guven T., Gwatirisa T., Gwini G., Gwodog P., Gysling S., Habib M., Hafeez Bhatti A. B., Hallesmith J., Halloran S., Hamza Sadiq M., Haney C., Hanna N., Hanna L., Hannington M., Harbjerg J., Haribaskaran D., Harran N., Harrington B., Harrison E., Hasan R., Hashmi S., Hassan M., Hassan A., Haverkamp L., Hazen S., Heer B., Heil J., Helliwell J., Henriksen N., Henshall D., Hermanson M., Hermena S., Hettiarachchi D., Hextall C., Hidalgo M., Hidayat H., Hider A., Higgins P., Hinchliffe R., Hirani D., Hirpara D., Hisham I., Hite M., Hoh S. M., Holmberg C., Holmich E., Holst F., Hossam A., Hossam Elfallal A., Howard P., Huaman E., Huang Y., Huang L., Huang D., Huber T., Hugh J., Hughes J., Huttner F., Huynh R., Hylands A., Iannuzzi J., Ielpo B., Iftikhar Talib A., Ignacio J., Ignatavicius P., Ike S., Ikwu C., Inama M., Ing A., Ingels A., Isik A., Islam N., Ives I. J., Al-Hasan A. J. M. S., Perez Rivera C. 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F., Khan S., Khan M., Khan D., Khan H., Khatkar H., Khatkov E., Khaw R., Kim B., Kishore Siddiraju K., Kitua D., Kirimtay B., Kmezic S., Knight S., Koeter T., Koh A., Koh Hong Xiang F., Kojo Anyomih T., Kok A. I. N., Kokelaar R., Koliarakis I., Kolli S., Kong J., Konig D., Koshy M., Kotze P., Kourdouli A., Kowal M., Kraima A., Kramer F., Kryzauskas M., Kuchynskyi I., Kuemmerli C., Kuiper S., Kumar S., Kumar A., Kumar L., Kumar H., Kumar N., Kumar Bandyopadhyay S., Kumar Garg P., Kumar Venkatappa S., Kung J., Kural S., Kushairi A., Kuuzie E., Kvietkauskas M., Kwek I., La J., Lai L., Lakpriya S., Lam K., Lami M., Lansdorp-Vogelaar I., Lapolla P., Larsen H., Latif J., Laudari U., Laurnezi A., Lawal A., Lawday S., Lederhuber H., Lednev A., Lee R., Van Leerdam M. E., Lefevbre G., Lesmus M., Leyva Moraga F. A., Leyva Moraga E., Leyva Moraga F., Li H. L., Li A., Li Z., Licardie E., Light A., Lightner A. L., Lin A., Lincango E., Litta F., Liu H., Lofthouse B., Londono M. A., Lopes R., Lopes De Freitas R., Lopez L., Lopez A. I., Lopez-Gomez J., Lopez-Pena G., Lowe R., Lowe D., Lowey M., Loy G., Lozanovski V., Luzon J., Lynn P., MacCabe T., MacHielsen A., Mafla Herreria C. A., Maggino L., Mahawar K., Mahmood D., Mahmoud M., Mahtani K., Maitra I., Maji S., Majiet I., Mal L., Malherbe J., Malhotra K., Malkomes P., Man E., Manan Sheikh A., Manjunath S., Manzano Nunez R., Manzoor S., Maqsood R., Marchegiani G., Marchegiani F., Marin D., Marin A., Marks I., Marson E., Martensen A., Martin D., Martin Martin G., Martin-Perez B., Martinez P., Marwaha P., Mashauri C., Mashbari H., Masior L., Masri R., Masud L., Masudi S., Mateu Calabuig G., Math S., Matrachisia A., Mayol J., Mazingi D., Mazzotta A., McAlinden J., McCabe G., McColm L., McElvaney H., McGivern K., McGovern J., McGuinness E., McInerney N., McKay S., McKee C., McKenna M., McKenna N., McLean K., Mediratta S., Medkova Y., Medzhidov O., Mehraj A., Mekhael M., Mekinde O., Mellenthin C., Melucci A., Mentor K., Merchant J., Messias H., Messeha M., Meza C., Mhango P., Miladinov M., Milagros Niquen Jimenez M., Miller P., Mills E., Milton A., Minayeva O. 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O., Davies T., Davis C., Davison S., Davletshina V., Dawidziuk A., Dawson A., De Andres Crespo M., De Berker H., De Dieu Ngo P., Dekker E., De La Caridad Espinosa Luis R., De Lacy B., Demartines N., De Montserrat Medina Sifuentes A., De Silva S., Del Rio C., Delaune V., Dell A., Demirbas I., Demirli Atici S., Deniz Tepe M., Derebey M., Desai G., Desai M., Devarakonda S., Deveras N., Di Franco G., Di Martino M., Di Marzo F., Diaz A., Diaz Del Gobbo G., DiazCastrillon C., Dick L., Dickinson K., Diego E., Dimasi I., Ding A., Dingemans S., Dixon L., Dixon B., Doherty W., Dooreemeah D., Donohue C., Dornseifer M., Dossa F., Dossou W., Drake T., Drami I., Drevin G., Du Plessis M. C., Dudi-Venkata N., Dudley R., Duffy S., Duklas D., Dumbrava B. -D., Duygu Avlar F., Dworzynska A., Ebrahim W., Ebrahim A., Efren Lozada Hernandez E., Ehigie N., El Boghdady M., El Hasnaoui C., El Sheikh M., El-Hussuna A., Eldurssi O., Elfeki H., Elhadi M., Elhassan M., Elhissi A., Elliot B., Elsenbroek C., Elsolh B., Elson N., Eltyeb H., Emerson H., Emile S. H., Endalle G., English W., Ercisli C., Espinosa G., Essam Abdelraheem M., Essangri H., Etienne P., Evans M. D., Evans T., Ezeme C., Ezzahraa F., Fadalla T., Fagan J., Fahmy M., Fairfield C., Falade O., Famularo S., Faqar-Uz-Zaman F., Farid Y., Farooq A., Farooq H., Farooqui F., Farquharson B., Faruqi A., Faulder R., Faut M., Fechner K., Feenstra T., Fehervari M., Fernandez L., Fernandez Alberti J., Ferrario L., Field D., Fiore L., Fingerhut S., Finlayson S., Fleming N., Fleming C., Florial E., Fok M., Fokin D., Foley M., Forero M. P., Forgan T., Fornasiero M., Fowler H., Fowler G., Franchi E., Franklin L., Fredriksson A., Fruhling P., Fuentes Navarrette G., Fulop A., Furtado M., Gaarder T., Galbraith N., Gallagher I. T. K., Gallo G., Gana T., Gaskin E., Gasparini M., Gatan R. G., Geary E., Gelaye Wudineh K., Gemenetzis G., Georgi M., Ghalige H., Ghareeb W., Ghatwary Tantawy T., Ghomsi C., Ghuman A., Giannakis P., Giron F., Gjengedal K., Gkotsis E., Glasbey J., Godahewa S., Godula D., Goffredo P., Goh S., Golriz M., Gomez L., Gomez Gomez D., Gonzalez R., Gonzalez D., Gonzalez Gutierrez E., Gopar D., Gordini L., Gori A., Gortazar S., Gousy N., Gowda R., Gowda M., Gqada J., Grechenig M., Greer J., Gregorio L., Grigorova A., Grimes H., Groot V., Grossman R. C., Gruber R., Gruter A., Guest R., Gujjuri R., Gulcek E., Gulcu B., Gull K., Gulmez M., Gupta V., Gutlic A., Guven T., Gwatirisa T., Gwini G., Gwodog P., Gysling S., Habib M., Hafeez Bhatti A. B., Hallesmith J., Halloran S., Hamza Sadiq M., Haney C., Hanna N., Hanna L., Hannington M., Harbjerg J., Haribaskaran D., Harran N., Harrington B., Harrison E., Hasan R., Hashmi S., Hassan M., Hassan A., Haverkamp L., Hazen S., Heer B., Heil J., Helliwell J., Henriksen N., Henshall D., Hermanson M., Hermena S., Hettiarachchi D., Hextall C., Hidalgo M., Hidayat H., Hider A., Higgins P., Hinchliffe R., Hirani D., Hirpara D., Hisham I., Hite M., Hoh S. M., Holmberg C., Holmich E., Holst F., Hossam A., Hossam Elfallal A., Howard P., Huaman E., Huang Y., Huang L., Huang D., Huber T., Hugh J., Hughes J., Huttner F., Huynh R., Hylands A., Iannuzzi J., Ielpo B., Iftikhar Talib A., Ignacio J., Ignatavicius P., Ike S., Ikwu C., Inama M., Ing A., Ingels A., Isik A., Islam N., Ives I. J., Al-Hasan A. J. M. S., Perez Rivera C. J., Jacome F., Jaffer T., Jagiella-Lodise O., Jain M., Jain K., Jakubauskas M., Jalal M., James H., Jang Y., Janssen B., Jansson H., Jariod-Ferrer U., Javanmard H., Javed S., Jayarajah U., Jayasuriya I., Je J., Jessop Z., Jia Lin Tang E., Jiang H., Jiayan Y., Jih Huei T., Jimenez-Rodriguez R., Joh D., Johnson A., Jones N., Jones C., Jordan C., Jose Nunez Ju J., Jose Pizarro M., Jose Salazar C., Joseph J., Justiniano C., Kabir T., Kadhum M., Kalfountzos C., Kalogiannaki E., Kalyanasundaram K., Kamarajah S., Kamil Quraishi M., Kanemitsu Y., Kapila A., Kapila V., Karagiannidis G., Kashif M., Kathiravelupillai S., Kathiravelupillai A., Katsogridakis E., Kaur K., Kaur Sekhon Inderjit Singh H., Kausur N., Kawka M., Keehan G., Kehlet Watt S., Kelly M., Kelly M. E., Kelvin Egbuchulem I., Kembuan G., Khajeh E., Khaled Elfaitur A., Khan M. F., Khan S., Khan M., Khan D., Khan H., Khatkar H., Khatkov E., Khaw R., Kim B., Kishore Siddiraju K., Kitua D., Kirimtay B., Kmezic S., Knight S., Koeter T., Koh A., Koh Hong Xiang F., Kojo Anyomih T., Kok A. I. N., Kokelaar R., Koliarakis I., Kolli S., Kong J., Konig D., Koshy M., Kotze P., Kourdouli A., Kowal M., Kraima A., Kramer F., Kryzauskas M., Kuchynskyi I., Kuemmerli C., Kuiper S., Kumar S., Kumar A., Kumar L., Kumar H., Kumar N., Kumar Bandyopadhyay S., Kumar Garg P., Kumar Venkatappa S., Kung J., Kural S., Kushairi A., Kuuzie E., Kvietkauskas M., Kwek I., La J., Lai L., Lakpriya S., Lam K., Lami M., Lansdorp-Vogelaar I., Lapolla P., Larsen H., Latif J., Laudari U., Laurnezi A., Lawal A., Lawday S., Lederhuber H., Lednev A., Lee R., Van Leerdam M. E., Lefevbre G., Lesmus M., Leyva Moraga F. A., Leyva Moraga E., Leyva Moraga F., Li H. L., Li A., Li Z., Licardie E., Light A., Lightner A. L., Lin A., Lincango E., Litta F., Liu H., Lofthouse B., Londono M. A., Lopes R., Lopes De Freitas R., Lopez L., Lopez A. I., Lopez-Gomez J., Lopez-Pena G., Lowe R., Lowe D., Lowey M., Loy G., Lozanovski V., Luzon J., Lynn P., MacCabe T., MacHielsen A., Mafla Herreria C. A., Maggino L., Mahawar K., Mahmood D., Mahmoud M., Mahtani K., Maitra I., Maji S., Majiet I., Mal L., Malherbe J., Malhotra K., Malkomes P., Man E., Manan Sheikh A., Manjunath S., Manzano Nunez R., Manzoor S., Maqsood R., Marchegiani G., Marchegiani F., Marin D., Marin A., Marks I., Marson E., Martensen A., Martin D., Martin Martin G., Martin-Perez B., Martinez P., Marwaha P., Mashauri C., Mashbari H., Masior L., Masri R., Masud L., Masudi S., Mateu Calabuig G., Math S., Matrachisia A., Mayol J., Mazingi D., Mazzotta A., McAlinden J., McCabe G., McColm L., McElvaney H., McGivern K., McGovern J., McGuinness E., McInerney N., McKay S., McKee C., McKenna M., McKenna N., McLean K., Mediratta S., Medkova Y., Medzhidov O., Mehraj A., Mekhael M., Mekinde O., Mellenthin C., Melucci A., Mentor K., Merchant J., Messias H., Messeha M., Meza C., Mhango P., Miladinov M., Milagros Niquen Jimenez M., Miller P., Mills E., Milton A., Minayeva O. A., MinHua Zheng Z., Mischlinger H., Mockli B., Modi R., Mohamed H. M., Mohamed M., Mohamed Abulghasm T., Mohammad S. A., Mohammed T. O., Mohammed A., Mohan H., Mohan M., Moin I., Mok V., Molina G., Moloney J., Moneim J., Monfort Mira M., Montcusi Ventura B., Montouri M., Moossdorff M., Mora-Guzman I., Moran B., Moran R. A. R., Moreno-Ordaz S., Morera A., Morgan R., Morley R., Moro-Valdezate D., Moros S., Moss J. -L., Morven A., Morton D., Moynihan A., Moyon M., Muduli N., Mugla N., Mugla W., Muller P., Mun G., Mundhada R., Munir I., Munoz F., Munoz E., Munoz A., Munoz Balderas D. C., Murgitroyd E., Murray V., Murthy S., Mushiwokufa W., Mustafa H., Mustakimov B., Mutambanengwe P., Myint P., Nadkarni S., Naess P. A., Nahar S., Naidoo P., Nam R., Nandhra S., Nanjappa N., Narasimhan V., Nardi W., Nasir M., Naughton A., Naumann D., Navarro S., Nawaaz Karimbocus M., Nazir A., Ndereya S., Ndong A., Negoi I., Nel D., Nelson D., Nepal S., Nugent T., Nepogodiev D., Neufeld J., Ng J., Ng D., Ng C. E., Ngaserin S., Ngu L., Ngwenya E., Fhearaigh R. N., Nikolousakis T. -K., Ninkovic M., Nita G., Nitschke C., Noren E., Noton T., Novikova A., Nowinka Z., Nyakunengwa T., Nyalundja A., Nzenwa I., Kristensen H. O., O'Brien C., O'Brien L., O'Brien S., O'Reilly J., O'Rourke S., O'Sullivan M., O'Dwyer M., Ochieng L., Oderoha E., Oh K. E., Ohlberger L., Olcum M., Olkina A., Omkumar M., Omnitel B., Oncel Yakar D., Ong K., Ong Wei Lin L., Ooi R., Ooi S., Oomman A., Oon Tyjet D., Opiyo S., Oscullo Yepez J. J., Osei-Kuffour N., Osunronbi T., Ottlakan A., Oussama Kacimi S., Ovaere S., Ozair A., Pachler F., Pai Oo S., Paiella S., Panaiotti L., Panda N., Pandarinath S., Pandey D., Pandrowala S., Papa Mamadou F., Paranathala M., Park J., Parmar C., Parvez A., Pasovic L., Pasquer A., Pasumarthy N., Pata F., Patel T., Patel P., Patel N., Patel M., Patron Uriburu N., Patrone R., Paul A., Pavan Kumar O. M., Pavithran A., Pedraza Ciro M., Pellino G., Peloso A., Pena Gallardo M. T., Pena Velazquez A., Perea J., Perez-Sanchez L. E., Perra T., Perrotta G., Petersson P., Petra G., Petrucciani N., Pickin C., Pino V., Pinotti E., Pinto F., Plum P., Podesta F., Pollini T., Pompeu Sa M., Ponce Leon F., Ponniah H. S., Ponte De Sousa X., Ponton J., Pontula A., Popa M., Portilla A. L., Posner F., Post S., Potolicchio A., Pouwels S., Povo A., Prasad P., Preciado S., Preece R., Proud D., Pulido Segura J. A., Puliyath N., Qui M., Quimbaya Rodriguez A. S., Raby-Smith W., Racovita A., Rad A., Radwan R., Rafaih Iqbal M., Rafik A., Raguan B., Rahi M., Rahiri J. -L., Rahme J., Rai L., Raj A., Raj Saksena A., Raja M., Ramirez J., Ramzi J., Ranstam J., Rao C., Rashid A., Ratnayake B., Rattanasirivilai K., Raubenheimer K., Ravikumar N., Ravn S., Razoz N., Rea W., Regan A., Rela M., Remme A., Rey Chaves C. E., Reyes A., Riad A., Rice D., Rios Quintana K., Ritter A., Roalso M., Robinson D., Rodriguez J., Rodriguez F., Rodriguez M. C., Rogers A., Rohila J., Romanyuc D., Romic I., Rommaneh M., Rompianesi G., Rosa F., Roscio F., Rose A., Rotimi T., Ruiz H., Ruiz Yucuma J., Ruiz-Ucar E., Ruslan M., Rutegard M., Ryan Harper E., Ryckx A., Rydbeck D., Sa-Marta E., Sadien I., Safari Nteranya D., Sagoo K., Sakata S., Saladino E., Saleem A., Saleem S., Salehi M., Salih S., Sallinen V., Salvans S., Sam Z. H., Samadov E., Sampaio Alves M., Sanad A., Sanchez Fonseca S., Sanchez Teran A., Sanchez Ussa S., Sandli O., Sanfey H., Sanghera J., Sani I., Santafe Guerrero M., Sante Fornasiero M., Santes Jasso O., Santos Pereira I., Santos Sousa H., Saratzis A., Sarmiento Alarcon A., Saumtally T., Sayyed R., Schettino M., Schleimer L., Schmidt T., Schondffelt K., Schwab M., Scott A., Searle H., Sebopelo L., Seeglier B., Seishima R., Semenvov D., Senent-Boza A., Sepulveda J., Serenari M., Serrano Navidad M., Sert I., Sewart E., Sgro A., Shadrina V., Shah K., Shahid F., Shalaby M., Shankar B., Shapiro J., Sharma L., Sheel A., Shenfine A., Shenoy S., Sherif A., Shetty N., Shetty R., Sia T. C., Sichimba D., Siddique H., Siddiqui I., Simkens G., Simoe J., Simon H., Sinan L., Singh T., Singh K., Singh Y., Sinha L., Siragusa L., Sluckin T., Smart Y. W., Smith H., Smith K., Smits L., Sneep-Van Kessel C., Sohrabi C., Solorzano Pineda O., Soma A., Sooriyapiragasam L., Soreide K., Sparavigna M., Spence R., Spencer N., Spiers H., Spinelli A., Sprakel J., Sravanam S., Srinivasan M., Srinivasan R., Staniszewska A., Stanworth S. J., Stasinos K., Steele R. J. C., Steinholt I., Steinruecke M., Stephen B. -J., Stijns J., Still M., Stupalkowska W., Subba S., Subbotin V. V., Sucharitkul P., Sudarsanam A., Sudhamsh Reddy D., Suhardja T., Suliman M., Sund M., Sunilkumar A., Suresh N., Sussmes S., Sutton P., Syltern J., Taha A., Takamizawa Y., Takoutsing Dongmo A. B., Tamas T., Tan L., Tan J. L., Tan K., Tan E., Tan Yong Hui A., Tanase A., Tariverdiev A., Tasnem A., Tatar C., Tay E., Tejedor P., Tesfaye G., Tetinou F., Thorpe C., Thyo A., Tlelo Amastal D., Tolani M., Tolga Saracoglu K., Tolgyes T., Tong J., Torrent Jansa L., Toscano Igartua S., Tovani Palone M. R., Traff H., Trevis J., Tummers W., Tur A., Turchenko I., Uche V., Uddin A., Udonsak N., Ullah M., Urbonas T., Uwins C., Uy Magadia E., Uzair Qureshi A., Uzun K., Vadim P., Valarche G., Valdez Gonzalez R. A., Vallee M., Van Beek D. -J., Van Dalen A. S., Van Den Hondel D., Van Der Stok E., Van Dorp M., Van Oostendorp S., Van Praag E., Van Rees J., Van Silfhout L., Varga Z., Varghese S., Varghese C., Varghese J., Vasilica A. -M., Vasquez Ojeda X., Vega E., Vehler S., Venchiarutti R., Vengatesan S., Venn M., Verma D., Vianey Partida Nava G., Victoria D., Vieira P., Vilar Alvarez M. E., Vinci D., Viscasillas Pallas G., Viswanath M., Vivanco J., Vizcaya Rodriguez V., Vo J., Volchanski D., Voron T., Voronovskyi Y., Vu J., Wadhwa M., Wadhwa S., Wagner G., Wallace M., Wang Y. Y., Wang J., Wani A., Wanigasooriya K., Wanjara S., Wanjiku N., Warner C., Wei Leow T., Weiser T., Weisters M., Wellington M. J., Wells C., Wenzelberg C., Wettstein D., Wezel A., Wheldon L., Widmer L., Wilson M., Wigmore S., Wijayaratne T., Wijeyaratne M., Wijnhoven B. P. L., Wilkin R., Williams E., Willis F., Winter D., Wirsik M. M., Wishah B., Wong G., Wong W. J., Wong K., Wong K. -Y., Worku D., Wright E., Wright J., Wroe Wright O., Xenacki S., Xia W., Xu W., Xu Z., Yalcinkaya A., Yang W., Yang P. -C., Yanishev A., Yanzon De La Torre A., Yao H., Yaqoob E., Yen Ling Quake S., Yeo D., Yeom B., Yershov D., Yiasemidou M., Yildiz A., Yiu A., Yoav M., Yong E., Yoshimura R., Younis M. U., Younis Ringshawl Z., Youssef M., Yue Y., Yuen S., Yuldashev R., Yurttas C., Yves B., Zaborowski A., Zackeri R., Zafar A., Zahra W., Zaidi A., Zainudin S., Zakeri R., Zamora I., Zamora A. T., Zawistowski M., Zbikowska G., Zegers W., Zehra S., Zeyra A., Zhagniyev Z., Zhukova L. G., Zivanovic M., Zmuc J., Zope M., Zubayraeva A., and Zucker B.
Abstract: Background: Coronavirus disease 2019 (COVID-19) was declared a pandemic by the WHO on 11 March 2020 and global surgical practice was compromised. This Commission aimed to document and reflect on the changes seen in the surgical environment during the pandemic, by reviewing colleagues experiences and published evidence. Methods: In late 2020, BJS contacted colleagues across the global surgical community and asked them to describe how severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2) had affected their practice. In addition to this, the Commission undertook a literature review on the impact of COVID-19 on surgery and perioperative care. A thematic analysis was performed to identify the issues most frequently encountered by the correspondents, as well as the solutions and ideas suggested to address them. Results: BJS received communications for this Commission from leading clinicians and academics across a variety of surgical specialties in every inhabited continent. The responses from all over the world provided insights into multiple facets of surgical practice from a governmental level to individual clinical practice and training. Conclusion: The COVID-19 pandemic has uncovered a variety of problems in healthcare systems, including negative impacts on surgical practice. Global surgical multidisciplinary teams are working collaboratively to address research questions about the future of surgery in the post-COVID-19 era. The COVID-19 pandemic is severely damaging surgical training. The establishment of a multidisciplinary ethics committee should be encouraged at all surgical oncology centres. Innovative leadership and collaboration is vital in the post-COVID-19 era.
Published: 2021

20. The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS

Author: Urquhart, S. A., Bendo, G. J., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M., Sedgwick, C., Weiner, C., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D., Ismail, D., Ivison, R., Jin, S., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Perez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., Vlahakis, C., Weiss, A., van der Werf, P., Verma, A., Yang, C., Young, A. J., Urquhart, S. A., Bendo, G. J., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M., Sedgwick, C., Weiner, C., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D., Ismail, D., Ivison, R., Jin, S., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Perez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., Vlahakis, C., Weiss, A., van der Werf, P., Verma, A., Yang, C., and Young, A. J.
Abstract: We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimeter sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources which resolved into 142. We have obtained robust redshift measurements for all sources using the 12-m Array and an efficient tuning of ALMA to optimise its use as a redshift hunter, with 73 per cent of the sources having a robust redshift identification. Nine of these redshift identifications also rely on observations from the Atacama Compact Array. The spectroscopic redshifts span a range $1.41
Published: 2022
Full Text: View/download PDF

21. The bright extragalactic ALMA redshift survey (BEARS) I: Redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS

Author: Urquhart, SA, Bendo, GJ, Serjeant, S, Bakx, T, Hagimoto, M, Cox, P, Neri, R, Lehnert, M, Sedgwick, C, Weiner, C, Dannerbauer, H, Amvrosiadis, A, Andreani, P, Baker, AJ, Beelen, A, Berta, S, Borsato, E, Buat, V, Butler, KM, Cooray, A, De Zotti, G, Dunne, L, Dye, S, Eales, S, Enia, A, Fan, L, Gavazzi, R, González-Nuevo, J, Harris, AI, Herrera, CN, Hughes, D, Ismail, D, Ivison, R, Jin, S, Jones, B, Kohno, K, Krips, M, Lagache, G, Marchetti, L, Massardi, M, Messias, H, Negrello, M, Omont, A, Perez-Fournon, I, Riechers, DA, Scott, D, Smith, MWL, Stanley, F, Tamura, Y, Temi, P, Vlahakis, C, Weiß, A, Van Der Werf, P, Verma, A, Yang, C, Young, AJ, Urquhart, SA, Bendo, GJ, Serjeant, S, Bakx, T, Hagimoto, M, Cox, P, Neri, R, Lehnert, M, Sedgwick, C, Weiner, C, Dannerbauer, H, Amvrosiadis, A, Andreani, P, Baker, AJ, Beelen, A, Berta, S, Borsato, E, Buat, V, Butler, KM, Cooray, A, De Zotti, G, Dunne, L, Dye, S, Eales, S, Enia, A, Fan, L, Gavazzi, R, González-Nuevo, J, Harris, AI, Herrera, CN, Hughes, D, Ismail, D, Ivison, R, Jin, S, Jones, B, Kohno, K, Krips, M, Lagache, G, Marchetti, L, Massardi, M, Messias, H, Negrello, M, Omont, A, Perez-Fournon, I, Riechers, DA, Scott, D, Smith, MWL, Stanley, F, Tamura, Y, Temi, P, Vlahakis, C, Weiß, A, Van Der Werf, P, Verma, A, Yang, C, and Young, AJ
Abstract: We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimetre sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources which resolved into 142. We have obtained robust redshift measurements for all sources using the 12-m Array and an efficient tuning of ALMA to optimize its use as a redshift hunter, with 73 per cent of the sources having a robust redshift identification. Nine of these redshift identifications also rely on observations from the Atacama Compact Array. The spectroscopic redshifts span a range 1.41 < z < 4.53 with a mean value of 2.75, and the CO emission line full-width at half-maxima range between $\rm 110\, km\, s^{-1} \lt FWHM \lt 1290\, km\, s^{-1}$ with a mean value of ∼500 km s−1, in line with other high-z samples. The derived CO(1-0) luminosity is significantly elevated relative to line-width to CO(1-0) luminosity scaling relation, which is suggestive of lensing magnification across our sources. In fact, the distribution of magnification factors inferred from the CO equivalent widths is consistent with expectations from galaxy–galaxy lensing models, though there is a hint of an excess at large magnifications that may be attributable to the additional lensing optical depth from galaxy groups or clusters.
Published: 2022

22. Orbital motion near Sagittarius A*: Constraints from polarimetric ALMA observations

Author: Wielgus, M., Moscibrodzka, M.A., Vos, J., Gelles, Z., Marti-Vidal, I, Farah, J., Goddi, C., Messias, H., Wielgus, M., Moscibrodzka, M.A., Vos, J., Gelles, Z., Marti-Vidal, I, Farah, J., Goddi, C., and Messias, H.
Abstract: Contains fulltext : 281840.pdf (Publisher’s version ) (Open Access)
Published: 2022

23. Orbital motion near Sagittarius A*: Constraints from polarimetric ALMA observations

Author: Wielgus, M., Moscibrodzka, M.A., Vos, J., Gelles, Z., Marti-Vidal, I, Farah, J., Goddi, C., Messias, H., Wielgus, M., Moscibrodzka, M.A., Vos, J., Gelles, Z., Marti-Vidal, I, Farah, J., Goddi, C., and Messias, H.
Abstract: Contains fulltext : 281840.pdf (Publisher’s version ) (Open Access)
Published: 2022

24. The bright extragalactic ALMA redshift survey (BEARS) I: redshifts of bright gravitationally lensed galaxies from the Herschel ATLAS

Author: Urquhart, S. A., Bendo, G. J., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M., Sedgwick, C., Weiner, C., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V, Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A., I, Herrera, C. N., Hughes, D., Ismail, D., Ivison, R., Jin, S., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Perez-Fournon, I, Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., Vlahakis, C., Weiss, A., van der Werf, P., Verma, A., Yang, C., Young, A. J., Urquhart, S. A., Bendo, G. J., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M., Sedgwick, C., Weiner, C., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V, Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A., I, Herrera, C. N., Hughes, D., Ismail, D., Ivison, R., Jin, S., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Perez-Fournon, I, Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., Vlahakis, C., Weiss, A., van der Werf, P., Verma, A., Yang, C., and Young, A. J.
Abstract: We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimetre sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources which resolved into 142. We have obtained robust redshift measurements for all sources using the 12-m Array and an efficient tuning of ALMA to optimize its use as a redshift hunter, with 73 per cent of the sources having a robust redshift identification. Nine of these redshift identifications also rely on observations from the Atacama Compact Array. The spectroscopic redshifts span a range 1.41 < z < 4.53 with a mean value of 2.75, and the CO emission line full-width at half-maxima range between 110 km s(-1) < FWHM < 1290 km s(-1) with a mean value of similar to 500 km s(-1), in line with other high-z samples. The derived CO(1-0) luminosity is significantly elevated relative to line-width to CO(1-0) luminosity scaling relation, which is suggestive of lensing magnification across our sources. In fact, the distribution of magnification factors inferred from the CO equivalent widths is consistent with expectations from galaxy-galaxy lensing models, though there is a hint of an excess at large magnifications that may be attributable to the additional lensing optical depth from galaxy groups or clusters.
Published: 2022

25. The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS

Author: Urquhart, S. A., Bendo, G. J., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M., Sedgwick, C., Weiner, C., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D., Ismail, D., Ivison, R., Jin, S., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Perez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., Vlahakis, C., Weiss, A., van der Werf, P., Verma, A., Yang, C., Young, A. J., Urquhart, S. A., Bendo, G. J., Serjeant, S., Bakx, T., Hagimoto, M., Cox, P., Neri, R., Lehnert, M., Sedgwick, C., Weiner, C., Dannerbauer, H., Amvrosiadis, A., Andreani, P., Baker, A. J., Beelen, A., Berta, S., Borsato, E., Buat, V., Butler, K. M., Cooray, A., De Zotti, G., Dunne, L., Dye, S., Eales, S., Enia, A., Fan, L., Gavazzi, R., Gonzalez-Nuevo, J., Harris, A. I., Herrera, C. N., Hughes, D., Ismail, D., Ivison, R., Jin, S., Jones, B., Kohno, K., Krips, M., Lagache, G., Marchetti, L., Massardi, M., Messias, H., Negrello, M., Omont, A., Perez-Fournon, I., Riechers, D. A., Scott, D., Smith, M. W. L., Stanley, F., Tamura, Y., Temi, P., Vlahakis, C., Weiss, A., van der Werf, P., Verma, A., Yang, C., and Young, A. J.
Abstract: We present spectroscopic measurements for 71 galaxies associated with 62 of the brightest high-redshift submillimeter sources from the Southern fields of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), while targeting 85 sources which resolved into 142. We have obtained robust redshift measurements for all sources using the 12-m Array and an efficient tuning of ALMA to optimise its use as a redshift hunter, with 73 per cent of the sources having a robust redshift identification. Nine of these redshift identifications also rely on observations from the Atacama Compact Array. The spectroscopic redshifts span a range $1.41
Published: 2022
Full Text: View/download PDF

26. Polarimetric Properties of Event Horizon Telescope Targets from ALMA

Author: Goddi, C., Martí-Vidal, I., Messias, H., Moscibrodzka, M.A., Brinkerink, C.D., Bronzwaer, T.J.W., Davelaar, J.R.J., Falcke, H., Fraga-Encinas, R., Issaoun, S., Müller, C., Olivares, H., Roelofs, F.J., Tilanus, R.P.J., Rossum, D.R. van, Rösch, F., Valtonen, M., Goddi, C., Martí-Vidal, I., Messias, H., Moscibrodzka, M.A., Brinkerink, C.D., Bronzwaer, T.J.W., Davelaar, J.R.J., Falcke, H., Fraga-Encinas, R., Issaoun, S., Müller, C., Olivares, H., Roelofs, F.J., Tilanus, R.P.J., Rossum, D.R. van, Rösch, F., and Valtonen, M.
Abstract: Contains fulltext : 231617.pdf (publisher's version ) (Open Access)
Published: 2021

27. Polarimetric Properties of Event Horizon Telescope Targets from ALMA

Author: Goddi, C., Martí-Vidal, I., Messias, H., Moscibrodzka, M.A., Brinkerink, C.D., Bronzwaer, T.J.W., Davelaar, J.R.J., Falcke, H., Fraga-Encinas, R., Issaoun, S., Müller, C., Olivares, H., Roelofs, F.J., Tilanus, R.P.J., Rossum, D.R. van, Rösch, F., Valtonen, M., Goddi, C., Martí-Vidal, I., Messias, H., Moscibrodzka, M.A., Brinkerink, C.D., Bronzwaer, T.J.W., Davelaar, J.R.J., Falcke, H., Fraga-Encinas, R., Issaoun, S., Müller, C., Olivares, H., Roelofs, F.J., Tilanus, R.P.J., Rossum, D.R. van, Rösch, F., and Valtonen, M.
Abstract: Contains fulltext : 231617.pdf (publisher's version ) (Open Access)
Published: 2021

28. Polarimetric Properties of Event Horizon Telescope Targets from ALMA

Author: Goddi, C., Martí-Vidal, I., Messias, H., Moscibrodzka, M.A., Brinkerink, C.D., Bronzwaer, T.J.W., Davelaar, J.R.J., Falcke, H., Fraga-Encinas, R., Issaoun, S., Müller, C., Olivares, H., Roelofs, F.J., Tilanus, R.P.J., Rossum, D.R. van, Rösch, F., Valtonen, M., Goddi, C., Martí-Vidal, I., Messias, H., Moscibrodzka, M.A., Brinkerink, C.D., Bronzwaer, T.J.W., Davelaar, J.R.J., Falcke, H., Fraga-Encinas, R., Issaoun, S., Müller, C., Olivares, H., Roelofs, F.J., Tilanus, R.P.J., Rossum, D.R. van, Rösch, F., and Valtonen, M.
Abstract: Contains fulltext : 231617.pdf (publisher's version ) (Open Access)
Published: 2021

29. A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time

Author: Lacy, M., Surace, J. A., Farrah, D., Nyland, K., Afonso, J., Brandt, W. N., Clements, D. L., Lagos, C. D. P., Maraston, C., Pforr, J., Sajina, A., Sako, M., Vaccari, M., Wilson, G., Ballantyne, D. R., Barkhouse, W. A., Brunner, R., Cane, R., Clarke, T. E., Cooper, M., Cooray, A., Covone, G., D'Andrea, C., Evrard, A. E., Ferguson, H. C., Frieman, J., Gonzalez-Perez, Abel, Gupta, R., Hatziminaoglou, E., Huang, J., Jagannathan, P., Jarvis, M. J., Jones, K. M., Kimball, A., Lidman, C., Lubin, L., Marchetti, L., Martini, P., McMahon, R. G., Mei, S., Messias, H., Murphy, E. J., Newman, J. A., Nichol, R., Norris, R. P., Oliver, S., Perez-Fournon, I., Peters, W. M., Pierre, M., Polisensky, E., Richards, G. T., Ridgway, S. E., Rottgering, H. J. A., Seymour, N., Shirley, R., Somerville, R., Strauss, M. A., Suntzeff, N., Thorman, P. A., van Kampen, E., Verma, A., Wechsler, R., Wood-Vasey, W. M., Lacy, M., Surace, J. A., Farrah, D., Nyland, K., Afonso, J., Brandt, W. N., Clements, D. L., Lagos, C. D. P., Maraston, C., Pforr, J., Sajina, A., Sako, M., Vaccari, M., Wilson, G., Ballantyne, D. R., Barkhouse, W. A., Brunner, R., Cane, R., Clarke, T. E., Cooper, M., Cooray, A., Covone, G., D'Andrea, C., Evrard, A. E., Ferguson, H. C., Frieman, J., Gonzalez-Perez, Abel, Gupta, R., Hatziminaoglou, E., Huang, J., Jagannathan, P., Jarvis, M. J., Jones, K. M., Kimball, A., Lidman, C., Lubin, L., Marchetti, L., Martini, P., McMahon, R. G., Mei, S., Messias, H., Murphy, E. J., Newman, J. A., Nichol, R., Norris, R. P., Oliver, S., Perez-Fournon, I., Peters, W. M., Pierre, M., Polisensky, E., Richards, G. T., Ridgway, S. E., Rottgering, H. J. A., Seymour, N., Shirley, R., Somerville, R., Strauss, M. A., Suntzeff, N., Thorman, P. A., van Kampen, E., Verma, A., Wechsler, R., and Wood-Vasey, W. M.
Abstract: The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main survey. In this paper, we describe the 'DeepDrill' survey, which used the Spitzer Space Telescope Infrared Array Camera (IRAC) to observe three of the four currently defined DDFs in two bands, centred on 3.6 and 4.5 mu m. These observations expand the area that was covered by an earlier set of observations in these three fields by the Spitzer Extragalactic Representative Volume Survey (SERVS). The combined DeepDrill and SERVS data cover the footprints of the LSST DDFs in the Extended Chandra Deep Field-South (ECDFS) field, the ELAIS-S1 field (ES1), and the XMM-Large-Scale Structure Survey field (XMM-LSS). The observations reach an approximate 5s point-source depth of 2 mu Jy (corresponding to an AB magnitude of 23.1; sufficient to detect a 10(11) M-circle dot galaxy out to z approximate to 5) in each of the two bands over a total area of approximate to 29 deg(2). The dual-band catalogues contain a total of 2.35 million sources. In this paper, we describe the observations and data products from the survey, and an overview of the properties of galaxies in the survey. We compare the source counts to predictions from the SHARK semi-analytic model of galaxy formation. We also identify a population of sources with extremely red ([3.6]-[4.5] >1.2) colours which we show mostly consists of highly obscured active galactic nuclei.
Published: 2021

30. A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time

Author: Lacy, M., Surace, J. A., Farrah, D., Nyland, K., Afonso, J., Brandt, W. N., Clements, D. L., Lagos, C. D. P., Maraston, C., Pforr, J., Sajina, A., Sako, M., Vaccari, M., Wilson, G., Ballantyne, D. R., Barkhouse, W. A., Brunner, R., Cane, R., Clarke, T. E., Cooper, M., Cooray, A., Covone, G., D'Andrea, C., Evrard, A. E., Ferguson, H. C., Frieman, J., Gonzalez-Perez, Abel, Gupta, R., Hatziminaoglou, E., Huang, J., Jagannathan, P., Jarvis, M. J., Jones, K. M., Kimball, A., Lidman, C., Lubin, L., Marchetti, L., Martini, P., McMahon, R. G., Mei, S., Messias, H., Murphy, E. J., Newman, J. A., Nichol, R., Norris, R. P., Oliver, S., Perez-Fournon, I., Peters, W. M., Pierre, M., Polisensky, E., Richards, G. T., Ridgway, S. E., Rottgering, H. J. A., Seymour, N., Shirley, R., Somerville, R., Strauss, M. A., Suntzeff, N., Thorman, P. A., van Kampen, E., Verma, A., Wechsler, R., Wood-Vasey, W. M., Lacy, M., Surace, J. A., Farrah, D., Nyland, K., Afonso, J., Brandt, W. N., Clements, D. L., Lagos, C. D. P., Maraston, C., Pforr, J., Sajina, A., Sako, M., Vaccari, M., Wilson, G., Ballantyne, D. R., Barkhouse, W. A., Brunner, R., Cane, R., Clarke, T. E., Cooper, M., Cooray, A., Covone, G., D'Andrea, C., Evrard, A. E., Ferguson, H. C., Frieman, J., Gonzalez-Perez, Abel, Gupta, R., Hatziminaoglou, E., Huang, J., Jagannathan, P., Jarvis, M. J., Jones, K. M., Kimball, A., Lidman, C., Lubin, L., Marchetti, L., Martini, P., McMahon, R. G., Mei, S., Messias, H., Murphy, E. J., Newman, J. A., Nichol, R., Norris, R. P., Oliver, S., Perez-Fournon, I., Peters, W. M., Pierre, M., Polisensky, E., Richards, G. T., Ridgway, S. E., Rottgering, H. J. A., Seymour, N., Shirley, R., Somerville, R., Strauss, M. A., Suntzeff, N., Thorman, P. A., van Kampen, E., Verma, A., Wechsler, R., and Wood-Vasey, W. M.
Abstract: The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main survey. In this paper, we describe the 'DeepDrill' survey, which used the Spitzer Space Telescope Infrared Array Camera (IRAC) to observe three of the four currently defined DDFs in two bands, centred on 3.6 and 4.5 mu m. These observations expand the area that was covered by an earlier set of observations in these three fields by the Spitzer Extragalactic Representative Volume Survey (SERVS). The combined DeepDrill and SERVS data cover the footprints of the LSST DDFs in the Extended Chandra Deep Field-South (ECDFS) field, the ELAIS-S1 field (ES1), and the XMM-Large-Scale Structure Survey field (XMM-LSS). The observations reach an approximate 5s point-source depth of 2 mu Jy (corresponding to an AB magnitude of 23.1; sufficient to detect a 10(11) M-circle dot galaxy out to z approximate to 5) in each of the two bands over a total area of approximate to 29 deg(2). The dual-band catalogues contain a total of 2.35 million sources. In this paper, we describe the observations and data products from the survey, and an overview of the properties of galaxies in the survey. We compare the source counts to predictions from the SHARK semi-analytic model of galaxy formation. We also identify a population of sources with extremely red ([3.6]-[4.5] >1.2) colours which we show mostly consists of highly obscured active galactic nuclei.
Published: 2021

31. Cosmic evolution of molecular gas mass density from an empirical relation between $\rm L_{1.4GHz}$ and $\rm L^{\prime}_{CO}$

Author: Orellana-González, G., Ibar, E., Leiton, R., Thomson, A. P., Cheng, C., Ivison, R. J., Herrera-Camus, R., Messias, H., Calderón-Castillo, P., Hughes, T. M., Leeuw, L., Orellana-González, G., Ibar, E., Leiton, R., Thomson, A. P., Cheng, C., Ivison, R. J., Herrera-Camus, R., Messias, H., Calderón-Castillo, P., Hughes, T. M., and Leeuw, L.
Abstract: Historically, GHz radio emission has been used extensively to characterize the star-formation activity in galaxies. In this work, we look for empirical relations amongst the radio luminosity, the infrared luminosity, and the CO-based molecular gas mass. We assemble a sample of 278 nearby galaxies with measurements of radio continuum and total infrared emission, and the $^{12}$CO (J = 1-0) emission line. We find a correlation between the radio continuum and the CO emission line (with a scatter of 0.36 dex), in a large sample of different kind of galaxies. Making use of this correlation, we explore the evolution of the molecular gas mass function and the cosmological molecular gas mass density in six redshift bins up to $z = 1.5$. These results agree with previous semi-analytic predictions and direct measurements: the cosmic molecular gas density increases up to $z=1.5$. In addition, we find a single plane across five orders of magnitude for the explored luminosities, with a scatter of 0.27 dex. These correlations are sufficiently robust to be used for samples where no CO measurements exist., Comment: 11 Pages, 5 figures
Published: 2020
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32. The Molecular Gas in the NGC 6240 Merging Galaxy System at the Highest Spatial Resolution

Author: Treister, E., Messias, H., Privon, G. C., Nagar, N., Medling, A. M., U., V., Bauer, F. E., Cicone, C., Munoz, L. Barcos, Evans, A. S., Muller-Sanchez, F., Comerford, J. M., Armus, L., Chang, C., Koss, M., Venturi, G., Schawinski, K., Casey, C., Urry, C. M., Sanders, D. B., Scoville, N., Sheth, K., Treister, E., Messias, H., Privon, G. C., Nagar, N., Medling, A. M., U., V., Bauer, F. E., Cicone, C., Munoz, L. Barcos, Evans, A. S., Muller-Sanchez, F., Comerford, J. M., Armus, L., Chang, C., Koss, M., Venturi, G., Schawinski, K., Casey, C., Urry, C. M., Sanders, D. B., Scoville, N., and Sheth, K.
Abstract: We present the highest resolution --- 15 pc (0.03'') --- ALMA $^{12}$CO(2-1) line emission and 1.3mm continuum maps, tracers of the molecular gas and dust, respectively, in the nearby merging galaxy system NGC 6240, that hosts two supermassive black holes growing simultaneously. These observations provide an excellent spatial match to existing Hubble optical and near-infrared observations of this system. A significant molecular gas mass, $\sim$9$\times$10$^9$M$_\odot$, is located in between the two nuclei, forming a clumpy stream kinematically dominated by turbulence, rather than a smooth rotating disk as previously assumed from lower resolution data. Evidence for rotation is seen in the gas surrounding the southern nucleus, but not in the northern one. Dynamical shells can be seen, likely associated with nuclear supernovae remnants. We further detect the presence of significant high velocity outflows, some of them reaching velocities $>$500 km/s, affecting a significant fraction, $\sim$11\% of the molecular gas in the nuclear region. Inside the spheres of influence of the northern and southern supermassive black holes we find molecular masses of 7.4$\times$10$^8$M$_\odot$ and 3.3$\times$10$^9$M$_\odot$, respectively. We are thus directly imaging the reservoir of gas that can accrete onto each supermassive black hole. These new ALMA maps highlight the critical need for high resolution observations of molecular gas in order to understand the feeding of supermassive black holes and its connection to galaxy evolution in the context of a major galaxy merger., Comment: 27 pages, 13 figures, accepted for publication by The Astrophysical Journal
Published: 2020
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33. A Spitzer survey of Deep Drilling Fields to be targeted by the Vera C. Rubin Observatory Legacy Survey of Space and Time

Author: Lacy, M., Surace, J. A., Farrah, D., Nyland, K., Afonso, J., Brandt, W. N., Clements, D. L., Lagos, C. D. P., Maraston, C., Pforr, J., Sajina, A., Sako, M., Vaccari, M., Wilson, G., Ballantyne, D. R., Barkhouse, W. A., Brunner, R., Cane, R., Clarke, T. E., Cooper, M., Cooray, A., Covone, G., D'Andrea, C., Evrard, A. E., Ferguson, H. C., Frieman, J., Gonzalez-Perez, V., Gupta, R., Hatziminaoglou, E., Huang, J., Jagannathan, P., Jarvis, M. J., Jones, K. M., Kimball, A., Lidman, C., Lubin, L., Marchetti, L., Martini, P., McMahon, R. G., Mei, S., Messias, H., Murphy, E. J., Newman, J. A., Nichol, R., Norris, R. P., Oliver, S., Perez-Fournon, I., Peters, W. M., Pierre, M., Polisensky, E., Richards, G. T., Ridgway, S. E., Röttgering, H. J. A., Seymour, N., Shirley, R., Somerville, R., Strauss, M. A., Suntzeff, N., Thorman, P. A., van Kampen, E., Verma, A., Wechsler, R., Wood-Vasey, W. M., Lacy, M., Surace, J. A., Farrah, D., Nyland, K., Afonso, J., Brandt, W. N., Clements, D. L., Lagos, C. D. P., Maraston, C., Pforr, J., Sajina, A., Sako, M., Vaccari, M., Wilson, G., Ballantyne, D. R., Barkhouse, W. A., Brunner, R., Cane, R., Clarke, T. E., Cooper, M., Cooray, A., Covone, G., D'Andrea, C., Evrard, A. E., Ferguson, H. C., Frieman, J., Gonzalez-Perez, V., Gupta, R., Hatziminaoglou, E., Huang, J., Jagannathan, P., Jarvis, M. J., Jones, K. M., Kimball, A., Lidman, C., Lubin, L., Marchetti, L., Martini, P., McMahon, R. G., Mei, S., Messias, H., Murphy, E. J., Newman, J. A., Nichol, R., Norris, R. P., Oliver, S., Perez-Fournon, I., Peters, W. M., Pierre, M., Polisensky, E., Richards, G. T., Ridgway, S. E., Röttgering, H. J. A., Seymour, N., Shirley, R., Somerville, R., Strauss, M. A., Suntzeff, N., Thorman, P. A., van Kampen, E., Verma, A., Wechsler, R., and Wood-Vasey, W. M.
Abstract: The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will observe several Deep Drilling Fields (DDFs) to a greater depth and with a more rapid cadence than the main survey. In this paper, we describe the ``DeepDrill'' survey, which used the Spitzer Space Telescope Infrared Array Camera (IRAC) to observe three of the four currently defined DDFs in two bands, centered on 3.6 $\mu$m and 4.5 $\mu$m. These observations expand the area which was covered by an earlier set of observations in these three fields by the Spitzer Extragalactic Representative Volume Survey (SERVS). The combined DeepDrill and SERVS data cover the footprints of the LSST DDFs in the Extended Chandra Deep Field-South field (ECDFS), the ELAIS-S1 field (ES1), and the XMM Large-Scale Structure Survey field (XMM-LSS). The observations reach an approximate $5\sigma$ point-source depth of 2 $\mu$Jy (corresponding to an AB magnitude of 23.1; sufficient to detect a 10$^{11} M_{\odot}$ galaxy out to $z\approx 5$) in each of the two bands over a total area of $\approx 29\,$deg$^2$. The dual-band catalogues contain a total of 2.35 million sources. In this paper we describe the observations and data products from the survey, and an overview of the properties of galaxies in the survey. We compare the source counts to predictions from the SHARK semi-analytic model of galaxy formation. We also identify a population of sources with extremely red ([3.6]$-$[4.5] $>1.2$) colours which we show mostly consists of highly-obscured active galactic nuclei., Comment: 20 pages, 9 figures; MNRAS in press
Published: 2020
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34. Close-up view of a luminous star-forming galaxy at z=2.95

Author: Berta, S., Young, A. J., Cox, P., Neri, R., Jones, B. M., Baker, A. J., Omont, A., Dunne, L., Rosell, A. Carnero, Marchetti, L., Negrello, M., Yang, C., Riechers, D. A., Dannerbauer, H., Perez-Fournon, I., van der Werf, P., Bakx, T., Ivison, R. J., Beelen, A., Buat, V., Cooray, A., Cortzen, I., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Herrera, C. N., Hughes, D., Jin, S., Krips, M., Lagache, G., Lehnert, M., Messias, H., Serjeant, S., Stanley, F., Urquhart, S., Vlahakis, C., Weiss, A., Berta, S., Young, A. J., Cox, P., Neri, R., Jones, B. M., Baker, A. J., Omont, A., Dunne, L., Rosell, A. Carnero, Marchetti, L., Negrello, M., Yang, C., Riechers, D. A., Dannerbauer, H., Perez-Fournon, I., van der Werf, P., Bakx, T., Ivison, R. J., Beelen, A., Buat, V., Cooray, A., Cortzen, I., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Herrera, C. N., Hughes, D., Jin, S., Krips, M., Lagache, G., Lehnert, M., Messias, H., Serjeant, S., Stanley, F., Urquhart, S., Vlahakis, C., and Weiss, A.
Abstract: (Abridged) Exploiting the sensitivity and broad band width of NOEMA, we have studied the molecular gas and dust in the galaxy HerBS-89a, at z=2.95. High angular resolution images reveal a partial 1.0" diameter Einstein ring in the dust continuum emission and the molecular emission lines of 12CO(9-8) and H2O(2_02-1_11). We report the detection of the three fundamental transitions of the molecular ion OH+, seen in absorption; the molecular ion CH+(1-0) seen in absorption (and tentatively in emission); two transitions of amidogen (NH2), seen in emission; and HCN(11-10) and/or NH(1_2-0_1) seen in absorption. The NOEMA data are complemented with VLA data tracing the 12CO(1-0) emission line, which provides a measurement of the total mass of molecular gas and an anchor for a CO excitation analysis. In addition, we present HST imaging that reveals the foreground lensing galaxy in the near-infrared. Together with data from the GTC, we derive a photometric redshift of z(phot)~0.9 for the foreground lensing galaxy. Modelling the lensing of HerBS-89a, we reconstruct the dust continuum and molecular emission lines (magnified by a factor ~4-5) in the source plane. The 12CO(9-8) and H2O emission lines have comparable spatial and kinematic distributions; the source-plane reconstructions do not clearly distinguish between a one-component and a two-component scenario, but the latter accounts for the observed broad line widths. HerBS-89a is a powerful star forming galaxy with a dust-to-gas ratio delta(GDR)~80, a SFR = 614 +/- 59 Msun/yr and a depletion timescale tau(depl) = (3.4 +/- 1.0) 1e8 years. The OH+ and CH+ absorption lines, all have their main velocity component red-shifted by \Delta(V)~100 km/s relative to the global CO reservoir. We argue that these absorption lines trace a rare example of gas inflow towards the center of the galaxy., Comment: 33 pages, Accepted for publication on A&A
Published: 2020
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35. Turbulent Gas in Lensed Planck-selected Starbursts at redshifts 1-3.5

Author: Harrington, Kevin C., Weiss, Axel, Yun, Min S., Magnelli, Benjamin, Sharon, C. E., Leung, T. K. D., Vishwas, A., Wang, Q. D., Jimenez-Andrade, E. F., Frayer, D. T., Liu, D., Garcia, P., Romano-Diaz, E., Frye, B. L., Jarugula, S., Badescu, T., Berman, D., Dannerbauer, H., Diaz-Sanchez, A., Grassitelli, L., Kamieneski, P., Kim, W. J., Kirkpatrick, A., Lowenthal, J. D., Messias, H., Puschnig, J., Stacey, G. J., Torne, P., Bertoldi, F., Harrington, Kevin C., Weiss, Axel, Yun, Min S., Magnelli, Benjamin, Sharon, C. E., Leung, T. K. D., Vishwas, A., Wang, Q. D., Jimenez-Andrade, E. F., Frayer, D. T., Liu, D., Garcia, P., Romano-Diaz, E., Frye, B. L., Jarugula, S., Badescu, T., Berman, D., Dannerbauer, H., Diaz-Sanchez, A., Grassitelli, L., Kamieneski, P., Kim, W. J., Kirkpatrick, A., Lowenthal, J. D., Messias, H., Puschnig, J., Stacey, G. J., Torne, P., and Bertoldi, F.
Abstract: Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the Universe. Key aspects to these processes are the gas heating and cooling mechanisms. Although it is well known that these galaxies are gas-rich, little is known about the gas excitation conditions. Here we examine these processes in a sample of 24 strongly lensed star-forming galaxies identified by the \textit{Planck} satellite (LPs) at z ~ 1.1 - 3.5. We analyze 162 CO rotational transitions (ranging from Jupper = 1 - 12) and 37 atomic carbon fine-structure lines ([CI]) in order to characterize the physical conditions of the gas in sample of LPs. We simultaneously fit the CO and [CI] lines, and the dust continuum emission, using two different non-LTE, radiative transfer models. The first model represents a two component gas density, while the second assumes a turbulence driven log-normal gas density distribution. These LPs are among the most gas-rich, infrared (IR) luminous galaxies ever observed ($\mu_{\rm L}$L$_{\rm IR(8-1000\mu m) } \sim 10^{13-14.6} $\Lsun; $< \mu_{\rm L}$M$_{\rm ISM}> = 2.7 \pm 1.2 \times 10^{12}$ \Msun, with $\mu_{\rm L} \sim 10-30$ the average lens magnification factor). Our results suggest that the turbulent ISM present in the LPs can be well-characterized by a high turbulent velocity dispersion ($<\Delta V_{\rm turb}> \sim 100 $ \kms) and gas kinetic temperature to dust temperature ratios $ \sim 2.5$, sustained on scales larger than a few kpc. We speculate that the average surface density of the molecular gas mass and IR luminosity $\Sigma_{\rm M_{\rm ISM}}$ $\sim 10^{3 - 4}$ \Msun pc$^{-2}$ and $\Sigma_{\rm L_{\rm IR}}$ $\sim 10^{11 - 12}$ \Lsun kpc$^{-2}$, arise from both stellar mechanical feedback and a steady momentum injection from the accretion of intergalactic gas., Comment: 54 pages, 18 figures. Accepted for publication in The Astrophysical Journal (as of Oct. 30, 2020). Please feel free to view the supplementary figures here (which can later be found online in the ApJ after the full publication procedure): https://drive.google.com/drive/folders/1CN3rqlUDcNi5JSDH2GhFk_SLSlo10han?usp=sharing
Published: 2020
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36. GOODS-ALMA: Optically dark ALMA galaxies shed light on a cluster in formation at z = 3.5

Author: Zhou, L., Elbaz, D., Franco, M., Magnelli, B., Schreiber, C., Wang, T., Ciesla, L., Daddi, E., Dickinson, M., Nagar, N., Magdis, G., Alexander, D. M., Béthermin, M., Demarco, R., Mullaney, J., Bournaud, F., Ferguson, H., Finkelstein, S. L., Giavalisco, M., Inami, H., Iono, D., Juneau, S., Lagache, G., Messias, H., Motohara, K., Okumura, K., Pannella, M., Papovich, C., Pope, A., Rujopakarn, W., Shi, Y., Shu, X., Silverman, J., Zhou, L., Elbaz, D., Franco, M., Magnelli, B., Schreiber, C., Wang, T., Ciesla, L., Daddi, E., Dickinson, M., Nagar, N., Magdis, G., Alexander, D. M., Béthermin, M., Demarco, R., Mullaney, J., Bournaud, F., Ferguson, H., Finkelstein, S. L., Giavalisco, M., Inami, H., Iono, D., Juneau, S., Lagache, G., Messias, H., Motohara, K., Okumura, K., Pannella, M., Papovich, C., Pope, A., Rujopakarn, W., Shi, Y., Shu, X., and Silverman, J.
Abstract: In this paper we study the properties of the six optically dark galaxies detected in the 69 arcmin^2 GOODS-ALMA 1.1mm continuum survey. While none of them are listed in the deepest H-band based CANDELS catalog in the GOODS-South field down to H=28.16AB, we were able to de-blend two of them from their bright neighbor and measure an $H$-band flux for them. We note that AGS4 and AGS15 have H=25.23, 27.11AB respectively. Their extreme proximity (0.50", 0.27") to a bright optical source and their extreme faintness prevented them from being included in the H-band catalog. We present the spectroscopic scan follow-up of five of the six sources with ALMA band 4. All are detected in the 2mm continuum with signal-to-noise ratios higher than eight. One emission line is detected in AGS4 (\nu_{obs} =151.44GHz with a S/N=8.58) and AGS17 (\nu_{obs} =154.78GHz with a S/N=10.23), which we interpret in both cases as being due to the CO(6-5) line at z^{AGS4}_{spec}=3.556 and z^{AGS4}_{spec}=3.467, respectively. These redshifts match both the probability distribution of the photometric redshifts derived from the UV to near-infrared spectral energy distributions (SEDs) and the far-infrared SEDs for typical dust temperatures of galaxies at these redshifts. We present evidence that nearly 70% (4/6 of galaxies) of the optically dark galaxies belong to the same overdensity of galaxies at z~3.5. overdensity The most massive one, AGS24 (M_{\star} = 10^{11.32^{+0.02}_{-0.19}} M_{\odot}), is the most massive galaxy without an active galactic nucleus (AGN) at $z$\,>\,3 in the GOODS-ALMA field. It falls in the very center of the peak of the galaxy surface density, which suggests that the surrounding overdensity is a proto-cluster in the process of virialization and that AGS24 is the candidate progenitor of the future brightest cluster galaxy (BCG)., Comment: 17 pages, 13 figures, 3 tables, accepted by A&A
Published: 2020
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37. Cosmic evolution of molecular gas mass density from an empirical relation between $\rm L_{1.4GHz}$ and $\rm L^{\prime}_{CO}$

Author: Orellana-González, G., Ibar, E., Leiton, R., Thomson, A. P., Cheng, C., Ivison, R. J., Herrera-Camus, R., Messias, H., Calderón-Castillo, P., Hughes, T. M., Leeuw, L., Orellana-González, G., Ibar, E., Leiton, R., Thomson, A. P., Cheng, C., Ivison, R. J., Herrera-Camus, R., Messias, H., Calderón-Castillo, P., Hughes, T. M., and Leeuw, L.
Abstract: Historically, GHz radio emission has been used extensively to characterize the star-formation activity in galaxies. In this work, we look for empirical relations amongst the radio luminosity, the infrared luminosity, and the CO-based molecular gas mass. We assemble a sample of 278 nearby galaxies with measurements of radio continuum and total infrared emission, and the $^{12}$CO (J = 1-0) emission line. We find a correlation between the radio continuum and the CO emission line (with a scatter of 0.36 dex), in a large sample of different kind of galaxies. Making use of this correlation, we explore the evolution of the molecular gas mass function and the cosmological molecular gas mass density in six redshift bins up to $z = 1.5$. These results agree with previous semi-analytic predictions and direct measurements: the cosmic molecular gas density increases up to $z=1.5$. In addition, we find a single plane across five orders of magnitude for the explored luminosities, with a scatter of 0.27 dex. These correlations are sufficiently robust to be used for samples where no CO measurements exist., Comment: 11 Pages, 5 figures
Published: 2020
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38. The Molecular Gas in the NGC 6240 Merging Galaxy System at the Highest Spatial Resolution

Author: Treister, E., Messias, H., Privon, G. C., Nagar, N., Medling, A. M., U., V., Bauer, F. E., Cicone, C., Munoz, L. Barcos, Evans, A. S., Muller-Sanchez, F., Comerford, J. M., Armus, L., Chang, C., Koss, M., Venturi, G., Schawinski, K., Casey, C., Urry, C. M., Sanders, D. B., Scoville, N., Sheth, K., Treister, E., Messias, H., Privon, G. C., Nagar, N., Medling, A. M., U., V., Bauer, F. E., Cicone, C., Munoz, L. Barcos, Evans, A. S., Muller-Sanchez, F., Comerford, J. M., Armus, L., Chang, C., Koss, M., Venturi, G., Schawinski, K., Casey, C., Urry, C. M., Sanders, D. B., Scoville, N., and Sheth, K.
Abstract: We present the highest resolution --- 15 pc (0.03'') --- ALMA $^{12}$CO(2-1) line emission and 1.3mm continuum maps, tracers of the molecular gas and dust, respectively, in the nearby merging galaxy system NGC 6240, that hosts two supermassive black holes growing simultaneously. These observations provide an excellent spatial match to existing Hubble optical and near-infrared observations of this system. A significant molecular gas mass, $\sim$9$\times$10$^9$M$_\odot$, is located in between the two nuclei, forming a clumpy stream kinematically dominated by turbulence, rather than a smooth rotating disk as previously assumed from lower resolution data. Evidence for rotation is seen in the gas surrounding the southern nucleus, but not in the northern one. Dynamical shells can be seen, likely associated with nuclear supernovae remnants. We further detect the presence of significant high velocity outflows, some of them reaching velocities $>$500 km/s, affecting a significant fraction, $\sim$11\% of the molecular gas in the nuclear region. Inside the spheres of influence of the northern and southern supermassive black holes we find molecular masses of 7.4$\times$10$^8$M$_\odot$ and 3.3$\times$10$^9$M$_\odot$, respectively. We are thus directly imaging the reservoir of gas that can accrete onto each supermassive black hole. These new ALMA maps highlight the critical need for high resolution observations of molecular gas in order to understand the feeding of supermassive black holes and its connection to galaxy evolution in the context of a major galaxy merger., Comment: 27 pages, 13 figures, accepted for publication by The Astrophysical Journal
Published: 2020
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39. GOODS-ALMA:Optically dark ALMA galaxies shed light on a cluster in formation at z=3.5

Author: Zhou, L., Elbaz, D., Franco, M., Magnelli, B., Schreiber, C., Wang, T., Ciesla, L., Daddi, E., Dickinson, M., Nagar, N., Magdis, G., Alexander, D. M., Bethermin, M., Demarco, R., Mullaney, J., Bournaud, F., Ferguson, H., Finkelstein, S. L., Giavalisco, M., Inami, H., Iono, D., Juneau, S., Lagache, G., Messias, H., Motohara, K., Okumura, K., Pannella, M., Papovich, C., Pope, A., Rujopakarn, W., Shi, Y., Shu, X., Silverman, J., Zhou, L., Elbaz, D., Franco, M., Magnelli, B., Schreiber, C., Wang, T., Ciesla, L., Daddi, E., Dickinson, M., Nagar, N., Magdis, G., Alexander, D. M., Bethermin, M., Demarco, R., Mullaney, J., Bournaud, F., Ferguson, H., Finkelstein, S. L., Giavalisco, M., Inami, H., Iono, D., Juneau, S., Lagache, G., Messias, H., Motohara, K., Okumura, K., Pannella, M., Papovich, C., Pope, A., Rujopakarn, W., Shi, Y., Shu, X., and Silverman, J.
Abstract: Thanks to its outstanding angular resolution, the Atacama Large Millimeter /submillimeter Array (ALMA) has recently unambiguously identified a population of optically dark galaxies with redshifts greater than z = 3, which play an important role in the cosmic star formation in massive galaxies. In this paper we study the properties of the six optically dark galaxies detected in the 69 arcmin(2) GOODS-ALMA 1.1mm continuum survey. While none of them are listed in the deepest H-band based CANDELS catalog in the GOODS-South field down to H = 28.16 AB, we were able to de-blend two of them from their bright neighbor and measure an H-band flux for them. We present the spectroscopic scan follow-up of five of the six sources with ALMA band 4. All are detected in the 2mm continuum with signal-to-noise ratios higher than eight. One emission line is detected in AGS4 (nu(obs) = 151.44 GHz with an S/N = 8.58) and AGS17 (nu(obs) = 154.78 GHz with an S/N = 10.23), which we interpret in both cases as being due to the CO(6-5) line at z(spec)(-AGS4) = 3.556 and z(spec)(AGS17) = 3.467, respectively. These redshifts match both the probability distribution of the photometric redshifts derived from the UV to near-infrared spectral energy distributions (SEDs) and the far-infrared SEDs for typical dust temperatures of galaxies at these redshifts. We present evidence that nearly 70% (4 /6 of galaxies) of the optically dark galaxies belong to the same overdensity of galaxies at z similar to 3.5. overdensity The most massive one, AGS24 (M-star = 10(-0.19)(11.32)(+0.02) M-circle dot), is the most massive galaxy without an active galactic nucleus at z > 3 in the GOODS-ALMA field. It falls in the very center of the peak of the galaxy surface density, which suggests that the surrounding overdensity is a proto-cluster in the process of virialization and that AGS24 is the candidate progenitor of the future brightest cluster galaxy.
Published: 2020

40. GOODS-ALMA:Optically dark ALMA galaxies shed light on a cluster in formation at z=3.5

Author: Zhou, L., Elbaz, D., Franco, M., Magnelli, B., Schreiber, C., Wang, T., Ciesla, L., Daddi, E., Dickinson, M., Nagar, N., Magdis, G., Alexander, D. M., Bethermin, M., Demarco, R., Mullaney, J., Bournaud, F., Ferguson, H., Finkelstein, S. L., Giavalisco, M., Inami, H., Iono, D., Juneau, S., Lagache, G., Messias, H., Motohara, K., Okumura, K., Pannella, M., Papovich, C., Pope, A., Rujopakarn, W., Shi, Y., Shu, X., Silverman, J., Zhou, L., Elbaz, D., Franco, M., Magnelli, B., Schreiber, C., Wang, T., Ciesla, L., Daddi, E., Dickinson, M., Nagar, N., Magdis, G., Alexander, D. M., Bethermin, M., Demarco, R., Mullaney, J., Bournaud, F., Ferguson, H., Finkelstein, S. L., Giavalisco, M., Inami, H., Iono, D., Juneau, S., Lagache, G., Messias, H., Motohara, K., Okumura, K., Pannella, M., Papovich, C., Pope, A., Rujopakarn, W., Shi, Y., Shu, X., and Silverman, J.
Abstract: Thanks to its outstanding angular resolution, the Atacama Large Millimeter /submillimeter Array (ALMA) has recently unambiguously identified a population of optically dark galaxies with redshifts greater than z = 3, which play an important role in the cosmic star formation in massive galaxies. In this paper we study the properties of the six optically dark galaxies detected in the 69 arcmin(2) GOODS-ALMA 1.1mm continuum survey. While none of them are listed in the deepest H-band based CANDELS catalog in the GOODS-South field down to H = 28.16 AB, we were able to de-blend two of them from their bright neighbor and measure an H-band flux for them. We present the spectroscopic scan follow-up of five of the six sources with ALMA band 4. All are detected in the 2mm continuum with signal-to-noise ratios higher than eight. One emission line is detected in AGS4 (nu(obs) = 151.44 GHz with an S/N = 8.58) and AGS17 (nu(obs) = 154.78 GHz with an S/N = 10.23), which we interpret in both cases as being due to the CO(6-5) line at z(spec)(-AGS4) = 3.556 and z(spec)(AGS17) = 3.467, respectively. These redshifts match both the probability distribution of the photometric redshifts derived from the UV to near-infrared spectral energy distributions (SEDs) and the far-infrared SEDs for typical dust temperatures of galaxies at these redshifts. We present evidence that nearly 70% (4 /6 of galaxies) of the optically dark galaxies belong to the same overdensity of galaxies at z similar to 3.5. overdensity The most massive one, AGS24 (M-star = 10(-0.19)(11.32)(+0.02) M-circle dot), is the most massive galaxy without an active galactic nucleus at z > 3 in the GOODS-ALMA field. It falls in the very center of the peak of the galaxy surface density, which suggests that the surrounding overdensity is a proto-cluster in the process of virialization and that AGS24 is the candidate progenitor of the future brightest cluster galaxy.
Published: 2020

41. Calibration of ALMA as a Phased Array. ALMA Observations During the 2017 VLBI Campaign

Author: Goddi, C., Marti-Vidal, I., Messias, H., Crew, G.B., Herrero-Illana, R., Impellizzeri, V., Janssen, M., Wielgus, M., Goddi, C., Marti-Vidal, I., Messias, H., Crew, G.B., Herrero-Illana, R., Impellizzeri, V., Janssen, M., and Wielgus, M.
Abstract: Contains fulltext : 204197.pdf (preprint version ) (Open Access)
Published: 2019

42. The ALMA Frontier Fields survey V: ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223

Author: Carvajal, R., Bauer, F. E., Bouwens, R. J., Oesch, P. A., González-López, J., Anguita, T., Aravena, M., Demarco, R., Guaita, L., Infante, L., Kim, S., Kneissl, R., Koekemoer, A. M., Messias, H., Treister, E., Villard, E., Zitrin, A., Troncoso, P., Carvajal, R., Bauer, F. E., Bouwens, R. J., Oesch, P. A., González-López, J., Anguita, T., Aravena, M., Demarco, R., Guaita, L., Infante, L., Kim, S., Kneissl, R., Koekemoer, A. M., Messias, H., Treister, E., Villard, E., Zitrin, A., and Troncoso, P.
Abstract: The Hubble Frontier Fields offer an exceptionally deep window into the high-redshift universe, covering a substantially larger area than the Hubble Ultra-Deep field at low magnification and probing 1--2 mags deeper in exceptional high-magnification regions. We aim to leverage Atacama Large Millimetre Array (ALMA) band 6 ($\approx$263\,GHz) mosaics in the central portions of five Frontier Fields to characterize the infrared (IR) properties of $1582$ ultraviolet (UV)-selected Lyman-Break Galaxies (LBGs) at redshifts of $z {\sim}$2--8. We investigated individual and stacked fluxes and IR excess (IRX) values of the LBG sample as functions of stellar mass ($\mathrm{M}_{\bigstar}$), redshift, UV luminosity and slope $\beta$, and lensing magnification. Two (2) LBG candidates were individually detected above a significance of $4.1{-}\sigma$, while stacked samples of the remaining LBG candidates yielded no significant detections. We investigated our detections and upper limits in the context of the IRX-$\mathrm{M}_{\bigstar}$ and IRX-$\beta$ relations, probing at least one dex lower in stellar mass than past studies have done. Our upper limits exclude substantial portions of parameter space and they are sufficiently deep in a handful of cases to create mild tension with the typically assumed attenuation and consensus relations. We observe a clear and smooth trend between $\mathrm{M}_{\bigstar}$ and $\beta$, which extends to low masses and blue (low) $\beta$ values, consistent with expectations from previous works., Comment: Accepted for publication in A&A, 28 pages and 20 figures. Full versions of Tables C.1, C.2, C.3, C.4, and C.5 are available for download at http://astro.puc.cl/~rcarvaja/docs/tables_ALMA_FF_V_RCP.tar.gz
Published: 2019
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43. NOEMA redshift measurements of bright Herschel galaxies

Author: Neri, R., Cox, P., Omont, A., Beelen, A., Berta, S., Bakx, T., Lehnert, M., Baker, A. J., Buat, V., Cooray, A., Dannerbauer, H., Dunne, L., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Herrera, C. N., Hughes, D., Ivison, R., Jin, S., Krips, M., Lagache, G., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C., Weiss, A., van der Werf, P., Yang, C., Young, A. J., Neri, R., Cox, P., Omont, A., Beelen, A., Berta, S., Bakx, T., Lehnert, M., Baker, A. J., Buat, V., Cooray, A., Dannerbauer, H., Dunne, L., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Herrera, C. N., Hughes, D., Ivison, R., Jin, S., Krips, M., Lagache, G., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C., Weiss, A., van der Werf, P., Yang, C., and Young, A. J.
Abstract: Using the IRAM NOrthern Extended Millimeter Array (NOEMA), we conducted a program to measure redshifts for 13 bright galaxies detected in the Herschel Astrophysical Large Area Survey (H-ATLAS) with $S_{500{\mu}\rm m}\ge$80 mJy. We report reliable spectroscopic redshifts for 12 individual sources, which are derived from scans of the 3 and 2 mm bands, covering up to 31 GHz in each band, and are based on the detection of at least two emission lines. The spectroscopic redshifts are in the range $2.08 10^{13}\,L_\odot$ galaxies. We also present a reanalysis of the spectral energy distributions including the continuum flux densities measured at 3 and 2 mm to derive the overall properties of the sources. Future prospects based on these efficient measurements of redshifts of high-z galaxies using NOEMA are outlined, including a comprehensive survey of all the brightest Herschel galaxies., Comment: 18 pages, 21 figures
Published: 2019
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44. A SCUBA-2 Selected Herschel-SPIRE Dropout and the Nature of this Population

Author: Greenslade, J., Aguilar, E., Clements, D. L., Dannerbauer, H., Cheng, T., Petitpas, G., Yang, C., Messias, H., Oteo, I., Farrah, D., Michalowski, M. J., Fournon, I. Perez, Aretxaga, I., Yun, M. S., Eales, S., Dunne, L., Cooray, A., Andreani, P., Hughes, D. H., Velazquez, M., Sanchez-Arguelles, D., Ponthieu, N., Greenslade, J., Aguilar, E., Clements, D. L., Dannerbauer, H., Cheng, T., Petitpas, G., Yang, C., Messias, H., Oteo, I., Farrah, D., Michalowski, M. J., Fournon, I. Perez, Aretxaga, I., Yun, M. S., Eales, S., Dunne, L., Cooray, A., Andreani, P., Hughes, D. H., Velazquez, M., Sanchez-Arguelles, D., and Ponthieu, N.
Abstract: Dusty star-forming galaxies (DSFGs) detected at $z > 4$ provide important examples of the first generations of massive galaxies. However, few examples with spectroscopic confirmation are currently known, with Hershel struggling to detect significant numbers of $z > 6$ DSFGs. NGP6_D1 is a bright 850 $\mu m$ source (12.3 $\pm$ 2.5 mJy) with no counterparts at shorter wavelengths (a SPIRE dropout). Interferometric observations confirm it is a single source, with no evidence for any optical or NIR emission, or nearby likely foreground lensing sources. No $>3\sigma$ detected lines are seen in both LMT RSR and IRAM 30m EMIR spectra of NGP6_D1 across 32 $GHz$ of bandwidth despite reaching detection limits of $\sim 1 mJy/500 km~s^{-1}$, so the redshift remains unknown. Template fitting suggests that NGP6_D1 is most likely between $z = 5.8$ and 8.3. SED analysis finds that NGP6_D1 is a ULIRG, with a dust mass $\sim 10^8$ - $10^9$ $M_{\odot}$ and a SFR of $\sim$ 500 $M_{\odot}~yr^{-1}$. We place upper limits on the gas mass of NGP6_D1 of $M_{H2}$ $ < (1.1~\pm~3.5) \times 10^{11}$ $M_{\odot}$, consistent with a gas-to-dust ratio of $\sim$ 100 - 1000. We discuss the nature of NGP6_D1 in the context of the broader submm population, and find that comparable SPIRE dropouts account for $\sim$ 20% of all SCUBA-2 detected sources, but with a similar flux density distribution to the general population., Comment: Accepoted for publication in MNRAS
Published: 2019
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45. Calibration of ALMA as a Phased Array. ALMA Observations During the 2017 VLBI Campaign

Author: Goddi, C., Marti-Vidal, I., Messias, H., Crew, G.B., Herrero-Illana, R., Impellizzeri, V., Janssen, M., Wielgus, M., Goddi, C., Marti-Vidal, I., Messias, H., Crew, G.B., Herrero-Illana, R., Impellizzeri, V., Janssen, M., and Wielgus, M.
Abstract: Contains fulltext : 204197.pdf (preprint version ) (Open Access)
Published: 2019

46. NOEMA redshift measurements of bright Herschel galaxies

Author: Neri, R., Cox, P., Omont, A., Beelen, A., Berta, S., Bakx, T., Lehnert, M., Baker, A. J., Buat, V., Cooray, A., Dannerbauer, H., Dunne, L., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Herrera, C. N., Hughes, D., Ivison, R., Jin, S., Krips, M., Lagache, G., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C., Weiss, A., van der Werf, P., Yang, C., Young, A. J., Neri, R., Cox, P., Omont, A., Beelen, A., Berta, S., Bakx, T., Lehnert, M., Baker, A. J., Buat, V., Cooray, A., Dannerbauer, H., Dunne, L., Dye, S., Eales, S., Gavazzi, R., Harris, A. I., Herrera, C. N., Hughes, D., Ivison, R., Jin, S., Krips, M., Lagache, G., Marchetti, L., Messias, H., Negrello, M., Perez-Fournon, I., Riechers, D. A., Serjeant, S., Urquhart, S., Vlahakis, C., Weiss, A., van der Werf, P., Yang, C., and Young, A. J.
Abstract: Using the IRAM NOrthern Extended Millimeter Array (NOEMA), we conducted a program to measure redshifts for 13 bright galaxies detected in the Herschel Astrophysical Large Area Survey (H-ATLAS) with $S_{500{\mu}\rm m}\ge$80 mJy. We report reliable spectroscopic redshifts for 12 individual sources, which are derived from scans of the 3 and 2 mm bands, covering up to 31 GHz in each band, and are based on the detection of at least two emission lines. The spectroscopic redshifts are in the range $2.08 10^{13}\,L_\odot$ galaxies. We also present a reanalysis of the spectral energy distributions including the continuum flux densities measured at 3 and 2 mm to derive the overall properties of the sources. Future prospects based on these efficient measurements of redshifts of high-z galaxies using NOEMA are outlined, including a comprehensive survey of all the brightest Herschel galaxies., Comment: 18 pages, 21 figures
Published: 2019
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47. The ALMA Frontier Fields survey V: ALMA Stacking of Lyman-Break Galaxies in Abell 2744, Abell 370, Abell S1063, MACSJ0416.1-2403 and MACSJ1149.5+2223

Author: Carvajal, R., Bauer, F. E., Bouwens, R. J., Oesch, P. A., González-López, J., Anguita, T., Aravena, M., Demarco, R., Guaita, L., Infante, L., Kim, S., Kneissl, R., Koekemoer, A. M., Messias, H., Treister, E., Villard, E., Zitrin, A., Troncoso, P., Carvajal, R., Bauer, F. E., Bouwens, R. J., Oesch, P. A., González-López, J., Anguita, T., Aravena, M., Demarco, R., Guaita, L., Infante, L., Kim, S., Kneissl, R., Koekemoer, A. M., Messias, H., Treister, E., Villard, E., Zitrin, A., and Troncoso, P.
Abstract: The Hubble Frontier Fields offer an exceptionally deep window into the high-redshift universe, covering a substantially larger area than the Hubble Ultra-Deep field at low magnification and probing 1--2 mags deeper in exceptional high-magnification regions. We aim to leverage Atacama Large Millimetre Array (ALMA) band 6 ($\approx$263\,GHz) mosaics in the central portions of five Frontier Fields to characterize the infrared (IR) properties of $1582$ ultraviolet (UV)-selected Lyman-Break Galaxies (LBGs) at redshifts of $z {\sim}$2--8. We investigated individual and stacked fluxes and IR excess (IRX) values of the LBG sample as functions of stellar mass ($\mathrm{M}_{\bigstar}$), redshift, UV luminosity and slope $\beta$, and lensing magnification. Two (2) LBG candidates were individually detected above a significance of $4.1{-}\sigma$, while stacked samples of the remaining LBG candidates yielded no significant detections. We investigated our detections and upper limits in the context of the IRX-$\mathrm{M}_{\bigstar}$ and IRX-$\beta$ relations, probing at least one dex lower in stellar mass than past studies have done. Our upper limits exclude substantial portions of parameter space and they are sufficiently deep in a handful of cases to create mild tension with the typically assumed attenuation and consensus relations. We observe a clear and smooth trend between $\mathrm{M}_{\bigstar}$ and $\beta$, which extends to low masses and blue (low) $\beta$ values, consistent with expectations from previous works., Comment: Accepted for publication in A&A, 28 pages and 20 figures. Full versions of Tables C.1, C.2, C.3, C.4, and C.5 are available for download at http://astro.puc.cl/~rcarvaja/docs/tables_ALMA_FF_V_RCP.tar.gz
Published: 2019
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48. A SCUBA-2 Selected Herschel-SPIRE Dropout and the Nature of this Population

Author: Greenslade, J., Aguilar, E., Clements, D. L., Dannerbauer, H., Cheng, T., Petitpas, G., Yang, C., Messias, H., Oteo, I., Farrah, D., Michalowski, M. J., Fournon, I. Perez, Aretxaga, I., Yun, M. S., Eales, S., Dunne, L., Cooray, A., Andreani, P., Hughes, D. H., Velazquez, M., Sanchez-Arguelles, D., Ponthieu, N., Greenslade, J., Aguilar, E., Clements, D. L., Dannerbauer, H., Cheng, T., Petitpas, G., Yang, C., Messias, H., Oteo, I., Farrah, D., Michalowski, M. J., Fournon, I. Perez, Aretxaga, I., Yun, M. S., Eales, S., Dunne, L., Cooray, A., Andreani, P., Hughes, D. H., Velazquez, M., Sanchez-Arguelles, D., and Ponthieu, N.
Abstract: Dusty star-forming galaxies (DSFGs) detected at $z > 4$ provide important examples of the first generations of massive galaxies. However, few examples with spectroscopic confirmation are currently known, with Hershel struggling to detect significant numbers of $z > 6$ DSFGs. NGP6_D1 is a bright 850 $\mu m$ source (12.3 $\pm$ 2.5 mJy) with no counterparts at shorter wavelengths (a SPIRE dropout). Interferometric observations confirm it is a single source, with no evidence for any optical or NIR emission, or nearby likely foreground lensing sources. No $>3\sigma$ detected lines are seen in both LMT RSR and IRAM 30m EMIR spectra of NGP6_D1 across 32 $GHz$ of bandwidth despite reaching detection limits of $\sim 1 mJy/500 km~s^{-1}$, so the redshift remains unknown. Template fitting suggests that NGP6_D1 is most likely between $z = 5.8$ and 8.3. SED analysis finds that NGP6_D1 is a ULIRG, with a dust mass $\sim 10^8$ - $10^9$ $M_{\odot}$ and a SFR of $\sim$ 500 $M_{\odot}~yr^{-1}$. We place upper limits on the gas mass of NGP6_D1 of $M_{H2}$ $ < (1.1~\pm~3.5) \times 10^{11}$ $M_{\odot}$, consistent with a gas-to-dust ratio of $\sim$ 100 - 1000. We discuss the nature of NGP6_D1 in the context of the broader submm population, and find that comparable SPIRE dropouts account for $\sim$ 20% of all SCUBA-2 detected sources, but with a similar flux density distribution to the general population., Comment: Accepoted for publication in MNRAS
Published: 2019
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49. VALES V:a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z similar to 0.03-0.35 using ALMA

Author: Molina, J., Ibar, Edo, Villanueva, V., Escala, A., Cheng, C., Baes, M., Messias, H., Yang, C., Bauer, F. E., van der Werf, Leiton, R., Aravena, M., Swinbank, A. M., Michalowski, M. J., Munoz-Arancibia, A. M., Orellana, G., Hughes, T. M., Farrah, D., De Zotti, G., Lara-Lopez, M. A., Eales, S., Dunne, L., Molina, J., Ibar, Edo, Villanueva, V., Escala, A., Cheng, C., Baes, M., Messias, H., Yang, C., Bauer, F. E., van der Werf, Leiton, R., Aravena, M., Swinbank, A. M., Michalowski, M. J., Munoz-Arancibia, A. M., Orellana, G., Hughes, T. M., Farrah, D., De Zotti, G., Lara-Lopez, M. A., Eales, S., and Dunne, L.
Published: 2019

50. VALES V:a kinematic analysis of the molecular gas content in H-ATLAS galaxies at z similar to 0.03-0.35 using ALMA

Author: Molina, J., Ibar, Edo, Villanueva, V., Escala, A., Cheng, C., Baes, M., Messias, H., Yang, C., Bauer, F. E., van der Werf, Leiton, R., Aravena, M., Swinbank, A. M., Michalowski, M. J., Munoz-Arancibia, A. M., Orellana, G., Hughes, T. M., Farrah, D., De Zotti, G., Lara-Lopez, M. A., Eales, S., Dunne, L., Molina, J., Ibar, Edo, Villanueva, V., Escala, A., Cheng, C., Baes, M., Messias, H., Yang, C., Bauer, F. E., van der Werf, Leiton, R., Aravena, M., Swinbank, A. M., Michalowski, M. J., Munoz-Arancibia, A. M., Orellana, G., Hughes, T. M., Farrah, D., De Zotti, G., Lara-Lopez, M. A., Eales, S., and Dunne, L.
Published: 2019

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