CaltechAUTHORS
  A Caltech Library Service

Seeing-sorted Visible Multi-Object Spectrograph U-band Imaging of the GOODS-south Field

Otteson, Lillian and McCabe, Tyler and Ashcraft, Teresa A. and Windhorst, Rogier A. and Jansen, Rolf A. and Cohen, Seth H. and Nonino, Mario and Paris, Diego and Grazian, Andrea and Fontana, Adriano and Giallongo, Emanuele and Speziali, Roberto and Testa, Vincenzo and Boutsia, Konstantina and Koekemoer, Anton and O’Connell, Robert W. and Rutkowski, Michael J. and Ryan, Russell E. and Scarlata, Claudia and Teplitz, Harry I. (2021) Seeing-sorted Visible Multi-Object Spectrograph U-band Imaging of the GOODS-south Field. Research Notes of the AAS, 5 (8). Art. No. 190. ISSN 2515-5172. https://resolver.caltech.edu/CaltechAUTHORS:20210820-231113645

[img] PDF - Published Version
Creative Commons Attribution.

3MB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20210820-231113645

Abstract

We present the optimal resolution and optimal depth U-filter mosaics using the seeing-sorted method of Ashcraft et al. on deep, ground-based U-bandimaging of the Great Observatories Origins Deep Survey South field as part of the near-UV imaging program UVCANDELS. We use the U-bandimages obtained with the VIsible Multi-Object Spectrograph on the European Southern Observatory Very Large Telescope by Nonino et al. Our best resolution mosaic includes images with a seeing full-width half maximum (FWHM) ≤ 0.”8, and encompasses 50% of the data. Our best depth mosaic includes images with FWHM ≤ 1.”5, corresponding to 100% of the data. Prior to being combined, the source fluxes in each individual background-subtracted image are corrected to match a 3D-HST photometric catalog of the same field to correct variations in the U-band zero-points. These mosaics provide deep U-banddata complementary to the UVCANDELS HST WFC3 F275W and ACS F435W images. We assess the depth of both U-bandmosaics.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/2515-5172/ac1db6DOIArticle
ORCID:
AuthorORCID
Otteson, Lillian0000-0001-9665-3003
McCabe, Tyler0000-0002-5506-3880
Windhorst, Rogier A.0000-0001-8156-6281
Jansen, Rolf A.0000-0003-1268-5230
Cohen, Seth H.0000-0003-3329-1337
Nonino, Mario0000-0001-6342-9662
Paris, Diego0000-0002-7409-8114
Grazian, Andrea0000-0002-5688-0663
Fontana, Adriano0000-0003-3820-2823
Giallongo, Emanuele0000-0003-0734-1273
Speziali, Roberto0000-0003-3754-387X
Testa, Vincenzo0000-0003-1033-1340
Boutsia, Konstantina0000-0003-4432-5037
Koekemoer, Anton0000-0002-6610-2048
O’Connell, Robert W.0000-0002-8190-7573
Rutkowski, Michael J.0000-0001-7016-5220
Ryan, Russell E.0000-0003-0894-1588
Scarlata, Claudia0000-0002-9136-8876
Teplitz, Harry I.0000-0002-7064-5424
Additional Information:© 2021. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received August 2021; Revised August 2021; Accepted August 2021; Published August 2021. Based on data acquired using the Very Large Telescope (VLT) of the European Southern Observatory (ESO). This work used data from the 3D-HST Treasury Program (HST-GO-12177 and 12328). We also acknowledge support from UVCANDELS grant HST-GO-15647 provided by NASA through the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. We acknowledge support from NASA JWST Interdisciplinary Scientist grants NAG5-12460, NNX14AN10G and 80NSSC18K0200 from GSFC. M.N. acknowledges INAF 1.05.01.86.20.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASAHST-GO-12177
NASAHST-GO-12328
NASAHST-GO-15647
NASANAS 5-26555
NASANAG5-12460
NASANNX14AN10G
NASA80NSSC18K0200
Istituto Nazionale di Astrofisica (INAF)1.05.01.86.20
Subject Keywords:Ultraviolet astronomy; Astronomical seeing; Astronomy data analysis
Issue or Number:8
Record Number:CaltechAUTHORS:20210820-231113645
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210820-231113645
Official Citation:Lillian Otteson et al 2021 Res. Notes AAS 5 190
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:110336
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:21 Aug 2021 18:18
Last Modified:21 Aug 2021 18:18

Repository Staff Only: item control page