adsabs/AstroCLIMB huggingface dataset:
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20181204v030-9900010004. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190504v019-9900150006. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190316v023-9900090004. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190325v015-9900150001. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190630v013-9900030001. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190306v014-9900010001. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20170923v017-9900050003. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20191029v020-9900140002. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20191217v011-9900060004. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20180411v012-9900160001. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190429v016-9900140004. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190901v019-9900190001. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20180913v018-9900100003. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20180516v009-9900100002. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20181108v021-9900080002. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20171120v006-9900050002. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20180912v018-9900070002. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190403v022-9900000002. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20181115v016-9900070005. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20200129v020-9900060001. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20181205v014-9900080003. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: A Search for Lensed Lyα Emitters within the Early HETDEX Data Set
Authors: Isaac H. Laseter, Steven L. Finkelstein, Micaela J. Bagley, Dustin M. Davis, Karl Gebhardt, Caryl Gronwall, Robin Ciardullo, Gregory R. Zeimann, Erin Mentuch Cooper, Daniel Farrow
Figure caption: 20190808v018-9900040003. Top Left: Two best VIRUS fibers, pixel flats, smoothed VIRUS fibers, and weighted sum of fibers. Top Middle: Gaussian fit to emission line. Top Right: Best available imaging on location of lensed LAE candidate. Bottom: Full spectrum of lensed LAE candidate. The yellow box with a dashed line denotes the location of Lyα.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: (a) Schematic 3D geometry inferred for the central region (reproduced from Figure 8(b) in Miyauchi & Kishimoto 2020). (b) 2D cut of the 3D geometry shown in panel (a) (reproduced from Figure 8(d) in Miyauchi & Kishimoto 2020 with additional annotations). (c) The same geometry as in panel (a), but rotated in 3D to match the possible configuration in NGC 4151 as seen from our perspective, where the central dotted square schematically corresponds to the region mapped by the CHARA Array and KI as indicated in panel (e), which is the same as Figure 3. (d) The same 3D geometry, but further rotated to a side view, perpendicular to our line of sight to the object. Approximate 3D locations inferred for the VLBI components (15 GHz; Ulvestad et al. 2005) are schematically shown in red circles. (e) See the description for panel (c). (f) Reconstructed 3D distribution shown in Figure 4(c), but with approximate 3D positions inferred for knots A–H of the radio jet (Mundell et al. 2003). The molecular hydrogen distribution as inferred by Fernandez et al. (1999) is shown as a red transparent ring in 3D with inner and outer radii of 0.″5 and 1.″5.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: (a) The same ring radii as in Figure 3 but with the fitted thin-ring model shown in dotted line. The inner dashed–solid line indicates the polar axis as probed by the optical polarization, and the outer dashed–solid line segments show the PA of the radio jet, exactly the same as in Figure 3. (b) HST/WFPC2 archival image of the narrow-line region in [O III]5007 line, with the two sets of dashed–solid line segments corresponding to those in panel (a). (c) Three-dimensional distribution of [O III]-emitting clouds reconstructed from HST/STIS multi-slit data, which cover the volume indicated by gray lines. For reference, the HST image from panel (b) in green is also shown at the back of the 3D cube, as the 2D flux distribution projected on to the sky plane. This is as seen almost perpendicular to our line of sight. An approximate axis of this 100 pc scale conical structure is indicated in a dashed–solid line.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: Details of the fringe track for NGC 4151 on 2020 February 15. (a) Fringe envelopes of the scans are shown in grayscale, with each scan in the horizontal direction, forming a waterfall plot along the vertical direction. (b) Power spectrum of each scan is shown in grayscale along the horizontal direction, again forming a waterfall plot of power spectra. (c) Dotted lines show the raw V 2 obtained from integrating each power spectrum, and the blue dots indicate its 10-scan average. (d) Averaged power spectrum is shown as a red dotted line, with its smoothed version indicated by a red solid line. The blue spectrum is before the subtraction of the noise bias, which is shown in gray, with the scale axis shown on the right side in the same shade blue color.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: Observed raw visibilities in the night of 2020 February 15 at CHARA. Light dotted lines show the raw visibilities averaged over 10 scans (∼15 s) in each track of objects. Blue filled circles show the raw visibilities integrated over each track of calibrators with uncertainties. Blue open circles are the system visibilities estimated from the calibrator observations. The green filled circle is the raw visibility of the science target from the integration over the track.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: Observed raw visibilities in the night of 2020 February 16 at CHARA. The notations are the same as in Figure 6.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: Observed raw visibilities in the night of 2021 April 30 at CHARA. The notations are the same as in Figure 6.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: Observed raw visibilities in the night of 2021 March 19 at CHARA. The notations are the same as in Figure 6.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: Details of the fringe track for NGC 4151 on 2020 February 16, in the same format as in Figure 7.
Paper: The Dust Sublimation Region of the Type 1 AGN NGC 4151 at a Hundred Microarcsecond Scale as Resolved by the CHARA Array Interferometer
Authors: Makoto Kishimoto, Matthew Anderson, Theo ten Brummelaar, Christopher Farrington, Robert Antonucci, Sebastian Hönig, Florentin Millour, Konrad R. W. Tristram, Gerd Weigelt, Laszlo Sturmann, Judit Sturmann, Gail Schaefer, Nic Scott
Figure caption: Details of the fringe track for NGC 4151 on 2021 March 19, in the same format as in Figure 7.
Paper: A Radio-selected Population of Dark, Long Gamma-Ray Bursts: Comparison to the Long Gamma-Ray Burst Population and Implications for Host Dust Distributions
Authors: Genevieve Schroeder, Tanmoy Laskar, Wen-fai Fong, Anya E. Nugent, Edo Berger, Ryan Chornock, Kate D. Alexander, Jennifer Andrews, R. Shane Bussmann, Alberto J. Castro-Tirado, Armaan V. Goyal, Charles D. Kilpatrick, Maura Lally, Adam A. Miller, Peter Milne, Kerry Paterson, Alicia Rouco Escorial, Michael C. Stroh, Giacomo Terreran, Bevin Ashley Zauderer
Figure caption: Median host extinction (A  V,Host) vs. GRB line-of-sight extinction (A  V,GRB) for the dark (light red squares) and typical, optically bright (blue circles) long GRB populations, with A  V,GRB from Kann et al. (2006, 2010), Zafar et al. (2011), Greiner et al. (2011), Krühler et al. (2011), and Perley et al. (2013), and A  V,Host from Savaglio et al. (2009), Perley et al. (2013), Krühler et al. (2015), Japelj et al. (2016), Krühler et al. (2011), and Perley et al. (2013). Our sample of six dark GRBs with A  V,Host and A  V,GRB measurements are represented by red squares with dark outlines. When necessary, we convert E  B−V  values to A  V,Host using the convention R = E  B−V /A  V  = 3.14 (Schultz & Wiemer 1975). To be consistent with Figure 15 from Perley et al. (2013), for host galaxies with upper limits on their median host extinction, we plot the upper limit at the upper bound (+ 1 σ) of the allowed A  V,Host range. Additionally, we choose the A  V,GRB derived from the SMC dust fit from Table 1 of Kann et al. (2006) and Table 3 of Kann et al. (2010), both to be consistent with Figure 15 from Perley et al. (2013) and to be consistent with our sample, for which we also use an SMC dust extinction law. For clarity, for GRBs with A  V,Host or A  V,GRB ≈ 0.0 mag, we plot their upper bounds at 0.05 mag. The dotted line denotes a 1:1 relation between median host extinction and GRB line-of-sight extinction. The dashed line denotes the correlation found between A  V,Host-A  V,GRB pairs, with a slope of ≈0.05 (see Section 5.2). These lines are meant to guide the reader’s eye.