adsabs/AstroCLIMB huggingface dataset:
Paper: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
Authors: Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos, Maximilien Franco, Santosh Harish, Louise Paquereau, Olivier Ilbert, Caitlin Rose, Isabella G. Cox, James W. Nightingale, Brant E. Robertson, John D. Silverman, Anton M. Koekemoer, Richard Massey, Henry Joy McCracken, Jason Rhodes, Hollis B. Akins, Natalie Allen, Aristeidis Amvrosiadis, Rafael C. Arango-Toro, Micaela B. Bagley, Angela Bongiorno, Peter L. Capak, Jaclyn B. Champagne, Nima Chartab, Óscar A. Chávez Ortiz, Katherine Chworowsky, Kevin C. Cooke, Olivia R. Cooper, Behnam Darvish, Xuheng Ding, Andreas L. Faisst, Steven L. Finkelstein, Seiji Fujimoto, Fabrizio Gentile, Steven Gillman, Katriona M. L. Gould, Ghassem Gozaliasl, Christopher C. Hayward, Qiuhan He, Shoubaneh Hemmati, Michaela Hirschmann, Knud Jahnke, Shuowen Jin, Ali Ahmad Khostovan, Vasily Kokorev, Erini Lambrides, Clotilde Laigle, Rebecca L. Larson, Gene C. K. Leung, Daizhong Liu, Tobias Liaudat, Arianna S. Long, Georgios Magdis, Guillaume Mahler, Vincenzo Mainieri, Sinclaire M. Manning, Claudia Maraston, Crystal L. Martin, Jacqueline E. McCleary, Jed McKinney, Conor J. R. McPartland, Bahram Mobasher, Rohan Pattnaik, Alvio Renzini, R. Michael Rich, David B. Sanders, Zahra Sattari, Diana Scognamiglio, Nick Scoville, Kartik Sheth, Marko Shuntov, Martin Sparre, Tomoko L. Suzuki, Margherita Talia, Sune Toft, Benny Trakhtenbrot, C. Megan Urry, Francesco Valentino, Brittany N. Vanderhoof, Eleni Vardoulaki, John R. Weaver, Katherine E. Whitaker, Stephen M. Wilkins, Lilan Yang, Jorge A. Zavala
Figure caption: The COSMOS-Web NIRCam (left) and MIRI (right) coverage shown together with the PRIMER NIRCam and MIRI coverage in a joint exposure map in grayscale. The two instruments’ coverage are shown separately for clarity. We overlay maps of a number of multiwavelength data sets for context. The JWST coverage from COSMOS-Web and PRIMER are shown in shades of blue. The Hubble CANDELS survey (Grogin et al. 2011; Koekemoer et al. 2011) area is shown in dashed black, the Atacama Large Millimeter/submillimeter Array (ALMA) extended MORA survey (Casey et al. 2021; Zavala et al. 2021; A. Long et al. 2023, in preparation) is shown in burnt orange and the deep SCUBA-2 450 μm +850 μm coverage area of the eS2-COSMOS survey and STUDIES survey (Wang et al. 2017) is shown in light orange (note that the entire COSMOS field is covered with 850 μm SCUBA-2 coverage from the S2COSMOS Survey; Simpson et al. 2019). In the radio, we highlight the deep continuum coverage at 3 GHz and 10 GHz in dark and light green, respectively, from the COSMOS-XS survey (van der Vlugt et al. 2021), which complements the full-field 3 GHz VLA COSMOS Survey of Smolčić et al. (2017). In the X-ray, we show the area covered by the Chandra C-COSMOS Deep survey (dashed magenta) as well as the medium-depth survey (solid magenta), both summarized by Elvis et al. (2009), with full COSMOS field coverage extended by Civano et al. (2016). Finally, we note that the full COSMOS field has coverage with Subaru’s Hyper Suprime-Cam (Aihara et al. 2022).
Paper: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
Authors: Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos, Maximilien Franco, Santosh Harish, Louise Paquereau, Olivier Ilbert, Caitlin Rose, Isabella G. Cox, James W. Nightingale, Brant E. Robertson, John D. Silverman, Anton M. Koekemoer, Richard Massey, Henry Joy McCracken, Jason Rhodes, Hollis B. Akins, Natalie Allen, Aristeidis Amvrosiadis, Rafael C. Arango-Toro, Micaela B. Bagley, Angela Bongiorno, Peter L. Capak, Jaclyn B. Champagne, Nima Chartab, Óscar A. Chávez Ortiz, Katherine Chworowsky, Kevin C. Cooke, Olivia R. Cooper, Behnam Darvish, Xuheng Ding, Andreas L. Faisst, Steven L. Finkelstein, Seiji Fujimoto, Fabrizio Gentile, Steven Gillman, Katriona M. L. Gould, Ghassem Gozaliasl, Christopher C. Hayward, Qiuhan He, Shoubaneh Hemmati, Michaela Hirschmann, Knud Jahnke, Shuowen Jin, Ali Ahmad Khostovan, Vasily Kokorev, Erini Lambrides, Clotilde Laigle, Rebecca L. Larson, Gene C. K. Leung, Daizhong Liu, Tobias Liaudat, Arianna S. Long, Georgios Magdis, Guillaume Mahler, Vincenzo Mainieri, Sinclaire M. Manning, Claudia Maraston, Crystal L. Martin, Jacqueline E. McCleary, Jed McKinney, Conor J. R. McPartland, Bahram Mobasher, Rohan Pattnaik, Alvio Renzini, R. Michael Rich, David B. Sanders, Zahra Sattari, Diana Scognamiglio, Nick Scoville, Kartik Sheth, Marko Shuntov, Martin Sparre, Tomoko L. Suzuki, Margherita Talia, Sune Toft, Benny Trakhtenbrot, C. Megan Urry, Francesco Valentino, Brittany N. Vanderhoof, Eleni Vardoulaki, John R. Weaver, Katherine E. Whitaker, Stephen M. Wilkins, Lilan Yang, Jorge A. Zavala
Figure caption: Literature rest-frame UV luminosity functions from 6 < z < 13; both data points and functional fits are drawn directly from the literature to illustrate the range of predictions made to-date at each epoch. Data and fits are specifically drawn from McLure et al. (2013), Oesch et al. (2013), Bouwens et al. (2015, 2021), Finkelstein et al. (2015), Finkelstein (2016), McLeod et al. (2016), Stefanon et al. (2019), Bowler et al. (2020), Kauffmann et al. (2022), Naidu et al. (2022b), Donnan et al. (2023), and Harikane et al. (2023). Gray regions mask out rest-frame UV magnitudes where COSMOS-Web will not be sensitive; the light gray region marks the limit corresponding to our two image depth while the dark gray region corresponds to four image depth. The horizontal dashed line marks the rarity of galaxies at which we would expect only to see one in all of COSMOS-Web. The blue and green corners mark the sensitivity limits (in depth and source rarity) of all of the Cycle 1 medium-depth surveys combined and deep-depth surveys combined, respectively.
Paper: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
Authors: Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos, Maximilien Franco, Santosh Harish, Louise Paquereau, Olivier Ilbert, Caitlin Rose, Isabella G. Cox, James W. Nightingale, Brant E. Robertson, John D. Silverman, Anton M. Koekemoer, Richard Massey, Henry Joy McCracken, Jason Rhodes, Hollis B. Akins, Natalie Allen, Aristeidis Amvrosiadis, Rafael C. Arango-Toro, Micaela B. Bagley, Angela Bongiorno, Peter L. Capak, Jaclyn B. Champagne, Nima Chartab, Óscar A. Chávez Ortiz, Katherine Chworowsky, Kevin C. Cooke, Olivia R. Cooper, Behnam Darvish, Xuheng Ding, Andreas L. Faisst, Steven L. Finkelstein, Seiji Fujimoto, Fabrizio Gentile, Steven Gillman, Katriona M. L. Gould, Ghassem Gozaliasl, Christopher C. Hayward, Qiuhan He, Shoubaneh Hemmati, Michaela Hirschmann, Knud Jahnke, Shuowen Jin, Ali Ahmad Khostovan, Vasily Kokorev, Erini Lambrides, Clotilde Laigle, Rebecca L. Larson, Gene C. K. Leung, Daizhong Liu, Tobias Liaudat, Arianna S. Long, Georgios Magdis, Guillaume Mahler, Vincenzo Mainieri, Sinclaire M. Manning, Claudia Maraston, Crystal L. Martin, Jacqueline E. McCleary, Jed McKinney, Conor J. R. McPartland, Bahram Mobasher, Rohan Pattnaik, Alvio Renzini, R. Michael Rich, David B. Sanders, Zahra Sattari, Diana Scognamiglio, Nick Scoville, Kartik Sheth, Marko Shuntov, Martin Sparre, Tomoko L. Suzuki, Margherita Talia, Sune Toft, Benny Trakhtenbrot, C. Megan Urry, Francesco Valentino, Brittany N. Vanderhoof, Eleni Vardoulaki, John R. Weaver, Katherine E. Whitaker, Stephen M. Wilkins, Lilan Yang, Jorge A. Zavala
Figure caption: A comparison of several of the JWST Cycle 1 extragalactic survey programs in depth and area for NIRCam imaging (left) and MIRI imaging (right). The vertical bars bracket the survey depths across all filters. In the case of MIRI, the dynamic range of depths is large due to substantial depth differences by filter; the depths at F770W are marked with stars for each survey. In the case of COSMOS-Web that has a large dither, the vertical bars also capture the range of depths across the mosaic. Note that for MIRI we show the exposure time calculator (ETC)-predicted depths, while the measured 7.7 μm depths for COSMOS-Web, CEERS, and PRIMER are shown with circles. We expect the depth of all programs to be similarly offset between ETC estimates and actual depth achieved. Depths have been converted to approximate 5σ point-source depths as detailed in Tables 3 and 4.
Paper: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
Authors: Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos, Maximilien Franco, Santosh Harish, Louise Paquereau, Olivier Ilbert, Caitlin Rose, Isabella G. Cox, James W. Nightingale, Brant E. Robertson, John D. Silverman, Anton M. Koekemoer, Richard Massey, Henry Joy McCracken, Jason Rhodes, Hollis B. Akins, Natalie Allen, Aristeidis Amvrosiadis, Rafael C. Arango-Toro, Micaela B. Bagley, Angela Bongiorno, Peter L. Capak, Jaclyn B. Champagne, Nima Chartab, Óscar A. Chávez Ortiz, Katherine Chworowsky, Kevin C. Cooke, Olivia R. Cooper, Behnam Darvish, Xuheng Ding, Andreas L. Faisst, Steven L. Finkelstein, Seiji Fujimoto, Fabrizio Gentile, Steven Gillman, Katriona M. L. Gould, Ghassem Gozaliasl, Christopher C. Hayward, Qiuhan He, Shoubaneh Hemmati, Michaela Hirschmann, Knud Jahnke, Shuowen Jin, Ali Ahmad Khostovan, Vasily Kokorev, Erini Lambrides, Clotilde Laigle, Rebecca L. Larson, Gene C. K. Leung, Daizhong Liu, Tobias Liaudat, Arianna S. Long, Georgios Magdis, Guillaume Mahler, Vincenzo Mainieri, Sinclaire M. Manning, Claudia Maraston, Crystal L. Martin, Jacqueline E. McCleary, Jed McKinney, Conor J. R. McPartland, Bahram Mobasher, Rohan Pattnaik, Alvio Renzini, R. Michael Rich, David B. Sanders, Zahra Sattari, Diana Scognamiglio, Nick Scoville, Kartik Sheth, Marko Shuntov, Martin Sparre, Tomoko L. Suzuki, Margherita Talia, Sune Toft, Benny Trakhtenbrot, C. Megan Urry, Francesco Valentino, Brittany N. Vanderhoof, Eleni Vardoulaki, John R. Weaver, Katherine E. Whitaker, Stephen M. Wilkins, Lilan Yang, Jorge A. Zavala
Figure caption: Color–color diagrams of mock galaxies drawn from a semianalytic model illustrating the selection of z ∼ 6–7 (top panel) and z ∼ 8–9 galaxies (bottom panel) using the COSMOS-Web filter-set. In the z ∼ 6–7 panel, green points and contours illustrate the distribution of mock galaxies at all redshifts relative to those at 6 < z < 7.5, shown in purple points and contours. A strong drop in the [F814W]–[F115W] color and a blue [F115W]–[F150W] correlates strongly with galaxies at z ∼ 6–7; z ∼ 1 sources serve as the major contaminant due to degeneracy with the Balmer break. In the z ∼ 8–9 panel, green points and contours show galaxies with photometric redshift solutions above z = 5 and purple points highlight sources with known redshifts 8 < z < 9.5. At these redshifts, we expect the drop to migrate to the [F115W]–[F150W] color, yet sources are still expected to be relatively blue in [F150W]–[F277W].
Paper: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
Authors: Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos, Maximilien Franco, Santosh Harish, Louise Paquereau, Olivier Ilbert, Caitlin Rose, Isabella G. Cox, James W. Nightingale, Brant E. Robertson, John D. Silverman, Anton M. Koekemoer, Richard Massey, Henry Joy McCracken, Jason Rhodes, Hollis B. Akins, Natalie Allen, Aristeidis Amvrosiadis, Rafael C. Arango-Toro, Micaela B. Bagley, Angela Bongiorno, Peter L. Capak, Jaclyn B. Champagne, Nima Chartab, Óscar A. Chávez Ortiz, Katherine Chworowsky, Kevin C. Cooke, Olivia R. Cooper, Behnam Darvish, Xuheng Ding, Andreas L. Faisst, Steven L. Finkelstein, Seiji Fujimoto, Fabrizio Gentile, Steven Gillman, Katriona M. L. Gould, Ghassem Gozaliasl, Christopher C. Hayward, Qiuhan He, Shoubaneh Hemmati, Michaela Hirschmann, Knud Jahnke, Shuowen Jin, Ali Ahmad Khostovan, Vasily Kokorev, Erini Lambrides, Clotilde Laigle, Rebecca L. Larson, Gene C. K. Leung, Daizhong Liu, Tobias Liaudat, Arianna S. Long, Georgios Magdis, Guillaume Mahler, Vincenzo Mainieri, Sinclaire M. Manning, Claudia Maraston, Crystal L. Martin, Jacqueline E. McCleary, Jed McKinney, Conor J. R. McPartland, Bahram Mobasher, Rohan Pattnaik, Alvio Renzini, R. Michael Rich, David B. Sanders, Zahra Sattari, Diana Scognamiglio, Nick Scoville, Kartik Sheth, Marko Shuntov, Martin Sparre, Tomoko L. Suzuki, Margherita Talia, Sune Toft, Benny Trakhtenbrot, C. Megan Urry, Francesco Valentino, Brittany N. Vanderhoof, Eleni Vardoulaki, John R. Weaver, Katherine E. Whitaker, Stephen M. Wilkins, Lilan Yang, Jorge A. Zavala
Figure caption: The first epoch of COSMOS-Web MIRI observations obtained on 2023 January 5–6. Covering six visits, the MIRI data are distributed in six nonoverlapping tiles and include data from both the MIRI imager and Lyot Coronograph field of view. At left is a comparison between Spitzer IRAC channel 4 (8 μm) data and MIRI 7.7 μm data in a 40″ × 40″ zoomed-in panel, highlighting the increased sensitivity and resolution of MIRI observations over those previously obtained with IRAC.
Paper: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
Authors: Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos, Maximilien Franco, Santosh Harish, Louise Paquereau, Olivier Ilbert, Caitlin Rose, Isabella G. Cox, James W. Nightingale, Brant E. Robertson, John D. Silverman, Anton M. Koekemoer, Richard Massey, Henry Joy McCracken, Jason Rhodes, Hollis B. Akins, Natalie Allen, Aristeidis Amvrosiadis, Rafael C. Arango-Toro, Micaela B. Bagley, Angela Bongiorno, Peter L. Capak, Jaclyn B. Champagne, Nima Chartab, Óscar A. Chávez Ortiz, Katherine Chworowsky, Kevin C. Cooke, Olivia R. Cooper, Behnam Darvish, Xuheng Ding, Andreas L. Faisst, Steven L. Finkelstein, Seiji Fujimoto, Fabrizio Gentile, Steven Gillman, Katriona M. L. Gould, Ghassem Gozaliasl, Christopher C. Hayward, Qiuhan He, Shoubaneh Hemmati, Michaela Hirschmann, Knud Jahnke, Shuowen Jin, Ali Ahmad Khostovan, Vasily Kokorev, Erini Lambrides, Clotilde Laigle, Rebecca L. Larson, Gene C. K. Leung, Daizhong Liu, Tobias Liaudat, Arianna S. Long, Georgios Magdis, Guillaume Mahler, Vincenzo Mainieri, Sinclaire M. Manning, Claudia Maraston, Crystal L. Martin, Jacqueline E. McCleary, Jed McKinney, Conor J. R. McPartland, Bahram Mobasher, Rohan Pattnaik, Alvio Renzini, R. Michael Rich, David B. Sanders, Zahra Sattari, Diana Scognamiglio, Nick Scoville, Kartik Sheth, Marko Shuntov, Martin Sparre, Tomoko L. Suzuki, Margherita Talia, Sune Toft, Benny Trakhtenbrot, C. Megan Urry, Francesco Valentino, Brittany N. Vanderhoof, Eleni Vardoulaki, John R. Weaver, Katherine E. Whitaker, Stephen M. Wilkins, Lilan Yang, Jorge A. Zavala
Figure caption: The first epoch of COSMOS-Web NIRCam observations obtained on 2023 January 5–6. These data cover six visits (or pointings) out of a total of 152. The total area covered by NIRCam here is ∼77 arcmin2. The relative position of this mosaic in the survey is shown at upper left. At lower left are several zoomed-in 10″ × 10″ cutouts (and one 16″ × 16″ cutout) of a handful of interesting objects, highlighting the level of detail revealed by these first data.
Paper: Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs
Authors: Ashraf Ayubinia, Jong-Hak Woo, Suvendu Rakshit, Donghoon Son
Figure caption: The fractional distribution of the non-normalized ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ line width (top) and ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ line width normalized by either stellar velocity dispersion (middle) or stellar mass (bottom) for radio-luminous (red) and radio-weak (blue) AGNs as well as our full sample (black). Left: flux-weighted average FWHM and right: velocity dispersion.
Paper: Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs
Authors: Ashraf Ayubinia, Jong-Hak Woo, Suvendu Rakshit, Donghoon Son
Figure caption: The ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ velocity dispersion with and without normalization by stellar velocity dispersion and stellar mass, as a function of ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ luminosity (left) and the bolometric-Eddington ratio (hereafter, Eddington ratio, right) for the high radio-Eddington (red) and low radio-Eddington AGNs (blue). The mean value of ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ velocity dispersion in each bin is denoted with triangles. The contours enclose 30%, 70%, and 90% of targets in each subsample. The error bars indicate 1σ dispersion.
Paper: Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs
Authors: Ashraf Ayubinia, Jong-Hak Woo, Suvendu Rakshit, Donghoon Son
Figure caption:                       ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ velocity–velocity dispersion diagram, with and without normalization by stellar velocity dispersion and stellar mass, as a function of radio-Eddington ratio. Compact and extended sources are represented by red and blue dots, respectively.
Paper: Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs
Authors: Ashraf Ayubinia, Jong-Hak Woo, Suvendu Rakshit, Donghoon Son
Figure caption: The ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ velocity dispersion with and without normalization by stellar velocity dispersion and stellar mass, as a function of radio luminosity (left) and radio-Eddington ratio (right) for the high Eddington (red) and low Eddington AGNs (blue). The mean value of the ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ velocity dispersion in each bin is denoted with triangles. The contours enclose 30%, 70%, and 90% of targets in each subsample. The error bars indicate 1σ dispersion.
Paper: Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs
Authors: Ashraf Ayubinia, Jong-Hak Woo, Suvendu Rakshit, Donghoon Son
Figure caption: The normalized ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ velocity dispersion as a function of ﹩\left[{\rm{O}}\,{\rm\small{III}}\right]﹩ luminosity for radio-luminous (red) and radio-weak AGNs (blue). The mean value of ﹩{\sigma }_{\left[{\rm{O}}\,{\rm\small{III}}\right]}﹩/σ * in each ﹩{L}_{\left[{\rm{O}}\,{\rm\small{III}}\right]}﹩ bin (with Δ log ﹩{L}_{\left[{\rm{O}}\,{\rm\small{III}}\right]}﹩ =1 dex) is denoted by triangles. The contours enclose 30%, 70%, and 90% of targets in each subsample. The error bars indicate 1σ dispersion.
Paper: Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs
Authors: Ashraf Ayubinia, Jong-Hak Woo, Suvendu Rakshit, Donghoon Son
Figure caption: Same as in Figure 6, but for compact (red) and extended (blue) radio sources.
Paper: Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs
Authors: Ashraf Ayubinia, Jong-Hak Woo, Suvendu Rakshit, Donghoon Son
Figure caption: Same as in Figure 6, but for RL (red) and RQ AGNs (blue).
Paper: Investigating the Correlation of Outflow Kinematics with Radio Activity. VII. Gas Outflows in AGNs
Authors: Ashraf Ayubinia, Jong-Hak Woo, Suvendu Rakshit, Donghoon Son
Figure caption: Same as in Figure 6, but for AGN-dominated (red) and SF-contaminated AGNs (blue).
Paper: Domain Adaptation for Simulation-based Dark Matter Searches with Strong Gravitational Lensing
Authors: Stephon Alexander, Sergei Gleyzer, Hanna Parul, Pranath Reddy, Marcos Tidball, Michael W. Toomey
Figure caption: Confusion matrices for the detection of lensing images on real data. The top row represents the naive application on the target data set, and the bottom row shows after training with ADDA. The left and right columns represent training with balanced and unbalanced data sets, respectively.
Paper: Domain Adaptation for Simulation-based Dark Matter Searches with Strong Gravitational Lensing
Authors: Stephon Alexander, Sergei Gleyzer, Hanna Parul, Pranath Reddy, Marcos Tidball, Michael W. Toomey
Figure caption: Evolution of loss during training with ADDA for models aimed at lens identification.
Paper: COSMOS-Web: An Overview of the JWST Cosmic Origins Survey
Authors: Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos, Maximilien Franco, Santosh Harish, Louise Paquereau, Olivier Ilbert, Caitlin Rose, Isabella G. Cox, James W. Nightingale, Brant E. Robertson, John D. Silverman, Anton M. Koekemoer, Richard Massey, Henry Joy McCracken, Jason Rhodes, Hollis B. Akins, Natalie Allen, Aristeidis Amvrosiadis, Rafael C. Arango-Toro, Micaela B. Bagley, Angela Bongiorno, Peter L. Capak, Jaclyn B. Champagne, Nima Chartab, Óscar A. Chávez Ortiz, Katherine Chworowsky, Kevin C. Cooke, Olivia R. Cooper, Behnam Darvish, Xuheng Ding, Andreas L. Faisst, Steven L. Finkelstein, Seiji Fujimoto, Fabrizio Gentile, Steven Gillman, Katriona M. L. Gould, Ghassem Gozaliasl, Christopher C. Hayward, Qiuhan He, Shoubaneh Hemmati, Michaela Hirschmann, Knud Jahnke, Shuowen Jin, Ali Ahmad Khostovan, Vasily Kokorev, Erini Lambrides, Clotilde Laigle, Rebecca L. Larson, Gene C. K. Leung, Daizhong Liu, Tobias Liaudat, Arianna S. Long, Georgios Magdis, Guillaume Mahler, Vincenzo Mainieri, Sinclaire M. Manning, Claudia Maraston, Crystal L. Martin, Jacqueline E. McCleary, Jed McKinney, Conor J. R. McPartland, Bahram Mobasher, Rohan Pattnaik, Alvio Renzini, R. Michael Rich, David B. Sanders, Zahra Sattari, Diana Scognamiglio, Nick Scoville, Kartik Sheth, Marko Shuntov, Martin Sparre, Tomoko L. Suzuki, Margherita Talia, Sune Toft, Benny Trakhtenbrot, C. Megan Urry, Francesco Valentino, Brittany N. Vanderhoof, Eleni Vardoulaki, John R. Weaver, Katherine E. Whitaker, Stephen M. Wilkins, Lilan Yang, Jorge A. Zavala
Figure caption: A map of the COSMOS-Web tiling pattern embedded within the Hubble ACS F814W mosaic of the COSMOS field (Koekemoer et al. 2007; Scoville et al. 2007). The mosaic consists of 152 visits where NIRCam serves as the primary instrument (long-wavelength detector coverage shown in blue) with MIRI in parallel (shown in orange). The entire NIRCam mosaic is centered on the position α = 10:00:27.9, δ = +02:12:03.5 and is 41.′5 (in the east–west direction) × 46.′6 (in the north–south direction) in size. The entire mosaic has an average position angle of 110°, with individual visit PAs equal to 293° in the northern half and 107° in the southern half. Three visits required slightly different position angles due to availability of guide stars; this includes the lone northern-most MIRI tile. The detailed coordinates and position angles of each visit are provided in the Appendix.