adsabs/AstroCLIMB huggingface dataset:
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Top and right: images of continuum and Hα velocity, velocity dispersion, and their residuals in Q2346_BX482 (z = 2.26). Bottom left: 1D Hα intensity, velocity, and velocity dispersion cuts along PAmajor, as well as the best-fit DYSMAL model (red line).
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Top and right: images of continuum and Hα velocity, velocity dispersion, and their residuals in K20_ID7 (z = 2.23). Bottom left: 1D Hα intensity, velocity, and velocity dispersion cuts along PAmajor, as well as the best-fit DYSMAL model (red line).
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Top and right: images of continuum and Hα velocity, velocity dispersion, and their residuals in zC_405226 (z = 2.29). Bottom left: 1D Hα intensity, velocity, and velocity dispersion cuts along PAmajor, as well as the best-fit DYSMAL model (red line).
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Kinemetry of Hα velocity maps in zC_403741.
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Kinemetry of Hα velocity maps in GS4_43501.
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Kinemetry of Hα velocity maps in Q2346_BX482.
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Kinemetry of Hα velocity maps in K20_ID7.
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Kinemetry of Hα velocity maps in zC_405226.
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Top and right: images of continuum and Hα velocity, velocity dispersion, and their residuals in D3a_15504 (z = 2.38). Bottom left: 1D Hα intensity, velocity, and velocity dispersion cuts along PAmajor, as well as the best-fit DYSMAL model (red line).
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Top and right: images of continuum and Hα velocity, velocity dispersion, and their residuals in D3a_6004 (z = 2.39). Bottom left: 1D Hα intensity, velocity, and velocity dispersion cuts along PAmajor, as well as the best-fit DYSMAL model (red line).
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: (Top) Velocity maps of the mock data sets without inflows, for each of the three cases (cases 1–3, from left to right) and (bottom) corresponding velocity residuals.
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Kinemetry of Hα velocity maps in D3a_6004.
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Kinemetry of Hα velocity maps in D3a_15504.
Paper: Evidence for Large-scale, Rapid Gas Inflows in z ∼ 2 Star-forming Disks
Authors: R. Genzel, J.-B. Jolly, D. Liu, S. H. Price, L. L. Lee, N. M. Förster Schreiber, L. J. Tacconi, R. Herrera-Camus, C. Barfety, A. Burkert, Y. Cao, R. I. Davies, A. Dekel, M. M. Lee, D. Lutz, T. Naab, R. Neri, A. Nestor Shachar, S. Pastras, C. Pulsoni, A. Renzini, K. Schuster, T. T. Shimizu, F. Stanley, A. Sternberg, H. Übler
Figure caption: Kinemetry analysis of case 1.
Paper: Illuminating the Dark Side of Cosmic Star Formation. II. A Second Date with RS-NIRdark Galaxies in COSMOS
Authors: Meriem Behiri, Margherita Talia, Andrea Cimatti, Andrea Lapi, Marcella Massardi, Andrea Enia, Cristian Vignali, Matthieu Bethermin, Andreas Faisst, Fabrizio Gentile, Marika Giulietti, Carlotta Gruppioni, Francesca Pozzi, Vernesa Smolçić, Gianni Zamorani
Figure caption: Top: median SED of Types 0 + 1 + 2 galaxies. Crimson and empty teal points and arrows represent, respectively, this work and T21 detections and 1σ upper limits. The best-fit model derived for our stack is the dark gray line for this work, while for T21 it is represented by the light gray dashed line. The SED fitting is performed on the median stacked photometry from the UV to the mid-IR bands and on the median fluxes from the Super-Deblended catalog (Jin et al. 2018) in the FIR regime, as explained in the text. The table shows some of the properties from the SED fitting, i.e., photometric redshift, stellar mass, dust luminosity, and extinction, for both T21 and this work. The errors are computed as the semi-interval between the 16th and the 84th percentiles of the probability distribution functions of each parameter. The quoted error on the redshift includes also a component from bootstrap analysis on the stacked photometry. Bottom: median stacking of the Types 0 + 1 + 2 subsamples in the u* to MIPS 24 μm bands.
Paper: Illuminating the Dark Side of Cosmic Star Formation. II. A Second Date with RS-NIRdark Galaxies in COSMOS
Authors: Meriem Behiri, Margherita Talia, Andrea Cimatti, Andrea Lapi, Marcella Massardi, Andrea Enia, Cristian Vignali, Matthieu Bethermin, Andreas Faisst, Fabrizio Gentile, Marika Giulietti, Carlotta Gruppioni, Francesca Pozzi, Vernesa Smolçić, Gianni Zamorani
Figure caption: Star formation rate density as a function of redshift. The crimson patterned and the violet rectangles show the confidence intervals for the results of this work and T21, where the lower boundary is the value obtained for Case 3 and the upper boundary the value obtained for Case 1. We indicate with green, pink, and turquoise the values found by Gruppioni et al. (2020) HST-dark, Gruppioni et al. (2020) HST-bright ALMA Band-7 ALPINE detections, and Yamaguchi et al. (2019) respectively. The violet arrow is the result of Enia et al. (2022) for H-dark galaxies. Red crosses are the results of Novak et al. (2017) for VLA-COSMOS 3 GHz Large Project sources with an optical/NIR counterpart, while light green diamonds are the results of Williams et al. (2019), purple diamonds are from Wang et al. (2019), blue diamonds from Fudamoto et al. (2021), and gray circles from Barrufet et al. (2023). The best-fit curve of Madau & Dickinson (2014), scaled to a Chabrier (2003) IMF, is displayed as a dashed black line.
Paper: Illuminating the Dark Side of Cosmic Star Formation. II. A Second Date with RS-NIRdark Galaxies in COSMOS
Authors: Meriem Behiri, Margherita Talia, Andrea Cimatti, Andrea Lapi, Marcella Massardi, Andrea Enia, Cristian Vignali, Matthieu Bethermin, Andreas Faisst, Fabrizio Gentile, Marika Giulietti, Carlotta Gruppioni, Francesca Pozzi, Vernesa Smolçić, Gianni Zamorani
Figure caption: SPIRE color–color diagram of our 500 μm risers, overlaid with redshift tracks of Arp 220 (Rangwala et al. 2011) and Cosmic Eyelash (Swinbank et al. 2010) and other samples of DSFGs as a reference (Oteo et al. 2017). The color scale indicates the photometric redshifts as computed by MAGPHYS.
Paper: Illuminating the Dark Side of Cosmic Star Formation. II. A Second Date with RS-NIRdark Galaxies in COSMOS
Authors: Meriem Behiri, Margherita Talia, Andrea Cimatti, Andrea Lapi, Marcella Massardi, Andrea Enia, Cristian Vignali, Matthieu Bethermin, Andreas Faisst, Fabrizio Gentile, Marika Giulietti, Carlotta Gruppioni, Francesca Pozzi, Vernesa Smolçić, Gianni Zamorani
Figure caption: Example of the deblending procedure on an IRAC-1 map. The first image is the input map, with the input positions (white circles). The second image is the model produced by TRACTOR, where the white crosses indicate the best-fit positions. The last image is the residual map.
Paper: Illuminating the Dark Side of Cosmic Star Formation. II. A Second Date with RS-NIRdark Galaxies in COSMOS
Authors: Meriem Behiri, Margherita Talia, Andrea Cimatti, Andrea Lapi, Marcella Massardi, Andrea Enia, Cristian Vignali, Matthieu Bethermin, Andreas Faisst, Fabrizio Gentile, Marika Giulietti, Carlotta Gruppioni, Francesca Pozzi, Vernesa Smolçić, Gianni Zamorani
Figure caption: Histogram showing the percentage of galaxies in our primary sample in a given S 500/F 530 bin. The dashed line indicates the median value.