PEARS emission-line galaxies spectroscopy Virtual Observatory Resource

Authors

1. Xia L.
2. Malhotra S.
3. Rhoads J.
4. Pirzkal N.
5. Zheng Z.
6. Meurer G.,Straughn A.
7. Grogin N.
8. Floyd D.

Published by

CDS

Abstract

We present spectroscopy of 76 emission-line galaxies (ELGs) in Chandra Deep Field South taken with the LDSS3 spectrograph on the Magellan Telescope. These galaxies are selected because they have emission lines with the Advanced Camera for Surveys (ACS) grism data in the Hubble Space Telescope Probing Evolution and Reionization Spectroscopically (PEARS) grism Survey. The ACS grism spectra cover the wavelength range 6000-9700{AA} and most PEARS grism redshifts are based on a single emission line + photometric redshifts from broadband colors; the Magellan spectra cover a wavelength range from 4000{AA} to 9000{AA} and provide a check on redshifts derived from PEARS data.

Keywords

1. Galaxies
2. Spectroscopy
3. Optical astronomy
4. Sloan photometry
5. Redshifted

Bibliographic source Bibcode

2011AJ....141...64X

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/141/64

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AJ/141/64

Document Object Identifer DOI

doi:10.26093/cds/vizier.51410064

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/141/64
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/141/64
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/141/64

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/141/64/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/141/64/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/141/64/table1?