adsabs/AstroCLIMB huggingface dataset:
Paper: COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs
Authors: J. R. Weaver, O. B. Kauffmann, O. Ilbert, H. J. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. C. Hsieh, C. Laigle, A. Anastasiou, C. K. Jespersen, J. Vinther, P. Capak, C. M. Casey, C. J. R. McPartland, B. Milvang-Jensen, B. Mobasher, D. B. Sanders, L. Zalesky, S. Arnouts, H. Aussel, J. S. Dunlop, A. Faisst, M. Franx, L. J. Furtak, J. P. U. Fynbo, K. M. L. Gould, T. R. Greve, S. Gwyn, J. S. Kartaltepe, D. Kashino, A. M. Koekemoer, V. Kokorev, O. Le Fèvre, S. Lilly, D. Masters, G. Magdis, V. Mehta, Y. Peng, D. A. Riechers, M. Salvato, M. Sawicki, C. Scarlata, N. Scoville, R. Shirley, A. Sneppen, V. Smolc̆ić, C. Steinhardt, D. Stern, M. Tanaka, Y. Taniguchi, H. I. Teplitz, M. Vaccari, W.-H. Wang, and G. Zamorani
Figure caption: Coordinate offset between sources in the Gaia DR1 catalog and sources extracted in the combined detection image as measured in the aperture-based CLASSIC catalog (see Section 3.1.1) The spacing between the dashed lines corresponds to the linear dimension of a pixel in the resampled images. Light and dark shaded regions are ellipses containing 68% and 99% of all sources respectively. For clarity, only 1 in 10 sources are plotted.
Paper: COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs
Authors: J. R. Weaver, O. B. Kauffmann, O. Ilbert, H. J. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. C. Hsieh, C. Laigle, A. Anastasiou, C. K. Jespersen, J. Vinther, P. Capak, C. M. Casey, C. J. R. McPartland, B. Milvang-Jensen, B. Mobasher, D. B. Sanders, L. Zalesky, S. Arnouts, H. Aussel, J. S. Dunlop, A. Faisst, M. Franx, L. J. Furtak, J. P. U. Fynbo, K. M. L. Gould, T. R. Greve, S. Gwyn, J. S. Kartaltepe, D. Kashino, A. M. Koekemoer, V. Kokorev, O. Le Fèvre, S. Lilly, D. Masters, G. Magdis, V. Mehta, Y. Peng, D. A. Riechers, M. Salvato, M. Sawicki, C. Scarlata, N. Scoville, R. Shirley, A. Sneppen, V. Smolc̆ić, C. Steinhardt, D. Stern, M. Tanaka, Y. Taniguchi, H. I. Teplitz, M. Vaccari, W.-H. Wang, and G. Zamorani
Figure caption: Best-fitting Moffat profile PSF integrated in circular apertures, ﹩{{ \mathcal F }}_{i}﹩, normalized to the target PSF ﹩{{ \mathcal F }}_{T}﹩, as a function of the aperture radius for all bands. Top: before PSF homogenization, for all bands except Suprime-Cam. Middle: after PSF homogenization, for all bands except Suprime-Cam. Bottom: after PSF homogenization, for Suprime-Cam bands. The horizontal dashed lines indicate a ±5% relative offset. The color map reflects the PSF FWHM before homogenization for all bands and after homogenization for the Suprime-Cam bands.
Paper: COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs
Authors: J. R. Weaver, O. B. Kauffmann, O. Ilbert, H. J. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. C. Hsieh, C. Laigle, A. Anastasiou, C. K. Jespersen, J. Vinther, P. Capak, C. M. Casey, C. J. R. McPartland, B. Milvang-Jensen, B. Mobasher, D. B. Sanders, L. Zalesky, S. Arnouts, H. Aussel, J. S. Dunlop, A. Faisst, M. Franx, L. J. Furtak, J. P. U. Fynbo, K. M. L. Gould, T. R. Greve, S. Gwyn, J. S. Kartaltepe, D. Kashino, A. M. Koekemoer, V. Kokorev, O. Le Fèvre, S. Lilly, D. Masters, G. Magdis, V. Mehta, Y. Peng, D. A. Riechers, M. Salvato, M. Sawicki, C. Scarlata, N. Scoville, R. Shirley, A. Sneppen, V. Smolc̆ić, C. Steinhardt, D. Stern, M. Tanaka, Y. Taniguchi, H. I. Teplitz, M. Vaccari, W.-H. Wang, and G. Zamorani
Figure caption: Distribution of the difference between the local and the global median half-light radius for the selected stars in the IB464 band, as a function of position, before (top) and after (bottom) PSF homogenization.
Paper: COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs
Authors: J. R. Weaver, O. B. Kauffmann, O. Ilbert, H. J. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. C. Hsieh, C. Laigle, A. Anastasiou, C. K. Jespersen, J. Vinther, P. Capak, C. M. Casey, C. J. R. McPartland, B. Milvang-Jensen, B. Mobasher, D. B. Sanders, L. Zalesky, S. Arnouts, H. Aussel, J. S. Dunlop, A. Faisst, M. Franx, L. J. Furtak, J. P. U. Fynbo, K. M. L. Gould, T. R. Greve, S. Gwyn, J. S. Kartaltepe, D. Kashino, A. M. Koekemoer, V. Kokorev, O. Le Fèvre, S. Lilly, D. Masters, G. Magdis, V. Mehta, Y. Peng, D. A. Riechers, M. Salvato, M. Sawicki, C. Scarlata, N. Scoville, R. Shirley, A. Sneppen, V. Smolc̆ić, C. Steinhardt, D. Stern, M. Tanaka, Y. Taniguchi, H. I. Teplitz, M. Vaccari, W.-H. Wang, and G. Zamorani
Figure caption: Demonstration of the model-fitting method from The Tractor. A pair of detected but overlapping sources is shown in the HSC i band (top). They are jointly modeled using THE FARMER with constraints from each of the izYJHKs images in order to provide a parameterized solution that is suitably optimized and from which the total flux is measured. The same pair of sources is shown in the less resolved IRAC channel 1 (bottom), where the two models are convolved with the channel 1 PSF and reoptimized using the channel 1 image to measure the flux contributed by each source. The extremely blended nature of this pair is underscored by the overlapping 2″  apertures, consistent with the methodology of the CLASSIC catalog. Pixel values are logarithmically scaled between the rms level and 95% of the peak flux per pixel.
Paper: COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs
Authors: J. R. Weaver, O. B. Kauffmann, O. Ilbert, H. J. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. C. Hsieh, C. Laigle, A. Anastasiou, C. K. Jespersen, J. Vinther, P. Capak, C. M. Casey, C. J. R. McPartland, B. Milvang-Jensen, B. Mobasher, D. B. Sanders, L. Zalesky, S. Arnouts, H. Aussel, J. S. Dunlop, A. Faisst, M. Franx, L. J. Furtak, J. P. U. Fynbo, K. M. L. Gould, T. R. Greve, S. Gwyn, J. S. Kartaltepe, D. Kashino, A. M. Koekemoer, V. Kokorev, O. Le Fèvre, S. Lilly, D. Masters, G. Magdis, V. Mehta, Y. Peng, D. A. Riechers, M. Salvato, M. Sawicki, C. Scarlata, N. Scoville, R. Shirley, A. Sneppen, V. Smolc̆ić, C. Steinhardt, D. Stern, M. Tanaka, Y. Taniguchi, H. I. Teplitz, M. Vaccari, W.-H. Wang, and G. Zamorani
Figure caption: Summary of the difference between broadband magnitudes measured by THE FARMER and CLASSIC catalogs, ΔMag. Magnitudes for CLASSIC are the rescaled 2″ total magnitudes. For UltraVISTA, sources in both the ultradeep and deep regions are shown. Agreement for individual sources is shown by the underlying density histogram, which is described by the overlaid median binned by 0.2 AB with an envelope containing 68% of points per bin (solid line and shaded area). 1σ and 3σ photometric uncertainty estimates on ΔMag are indicated by the gray dotted curves. The 3σ depths measured with 3″ diameter apertures as reported in Table 1 are shown by vertical dashed lines. The median Δmagnitudes for sources brighter than the depth limit are reported in each panel.
Paper: COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs
Authors: J. R. Weaver, O. B. Kauffmann, O. Ilbert, H. J. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. C. Hsieh, C. Laigle, A. Anastasiou, C. K. Jespersen, J. Vinther, P. Capak, C. M. Casey, C. J. R. McPartland, B. Milvang-Jensen, B. Mobasher, D. B. Sanders, L. Zalesky, S. Arnouts, H. Aussel, J. S. Dunlop, A. Faisst, M. Franx, L. J. Furtak, J. P. U. Fynbo, K. M. L. Gould, T. R. Greve, S. Gwyn, J. S. Kartaltepe, D. Kashino, A. M. Koekemoer, V. Kokorev, O. Le Fèvre, S. Lilly, D. Masters, G. Magdis, V. Mehta, Y. Peng, D. A. Riechers, M. Salvato, M. Sawicki, C. Scarlata, N. Scoville, R. Shirley, A. Sneppen, V. Smolc̆ić, C. Steinhardt, D. Stern, M. Tanaka, Y. Taniguchi, H. I. Teplitz, M. Vaccari, W.-H. Wang, and G. Zamorani
Figure caption: Comparison of broadband colors between the THE FARMER and CLASSIC catalogs, Δcolor. THE FARMER magnitudes of the first color term in each panel are shown on the x-axis. Colors for individual sources are shown by the underlying density histogram, which is described by the overlaid median binned by 0.2 AB with a 68% confidence interval. 1σ and 3σ photometric uncertainty estimates on the colors are indicated by the gray dotted curves, and the mean 3σ depth computed from both bands of interest and measured with 3″ diameter apertures as reported in Table 1 are shown by vertical dashed lines; brighter than the median Δ are reported.
Paper: COSMOS2020: A Panchromatic View of the Universe to z ∼ 10 from Two Complementary Catalogs
Authors: J. R. Weaver, O. B. Kauffmann, O. Ilbert, H. J. McCracken, A. Moneti, S. Toft, G. Brammer, M. Shuntov, I. Davidzon, B. C. Hsieh, C. Laigle, A. Anastasiou, C. K. Jespersen, J. Vinther, P. Capak, C. M. Casey, C. J. R. McPartland, B. Milvang-Jensen, B. Mobasher, D. B. Sanders, L. Zalesky, S. Arnouts, H. Aussel, J. S. Dunlop, A. Faisst, M. Franx, L. J. Furtak, J. P. U. Fynbo, K. M. L. Gould, T. R. Greve, S. Gwyn, J. S. Kartaltepe, D. Kashino, A. M. Koekemoer, V. Kokorev, O. Le Fèvre, S. Lilly, D. Masters, G. Magdis, V. Mehta, Y. Peng, D. A. Riechers, M. Salvato, M. Sawicki, C. Scarlata, N. Scoville, R. Shirley, A. Sneppen, V. Smolc̆ić, C. Steinhardt, D. Stern, M. Tanaka, Y. Taniguchi, H. I. Teplitz, M. Vaccari, W.-H. Wang, and G. Zamorani
Figure caption: Growth of photometric uncertainties as a function of magnitude. The colored curves indicate the distributions for individual sources in THE FARMER catalog, described by the running median and a tight envelope containing 68% of sources. The gray curves represent the median growth of uncertainty for the total magnitudes in the CLASSIC catalog derived from 2″ aperture photometry, shown by the dashed and dotted curves for the uncorrected and corrected uncertainties, respectively. The 3σ depths measured with 3″ diameter apertures as reported in Table 1 are shown by vertical dashed lines. The two curves shown for each band in YJHKs are due to different depths of the deep and ultradeep regions.