Other Targets
Constraints:
- Observable from the SOAR-4m on the nights of September 28 - October 2, 2018.
- Targets in the RA range of 20h00m->05h00m and DEC < 0 would be ideal.
- Targets in the RA range of 15h00m->10h00m may be do-able, depending on the DEC (e.g., a field at 10h00m, -60d00m is do-able).
- Preferably brighter than r=18; definitely brighter than r=20.
- Program that can make use of the main program's setup (Goodman spectrgraph, 400l/mm grating, 2x2 pixel binning, wavelength coverage of about 3700-7200A with a (binned) dispersion of about 2A/pixel.
Combined Target Lists for Secondary Programs (Version: v20180929):
Detailed Instructions from Target Contributors:
Quasar Candidates
Contact(s): Paul Martini, Zhefu Yu
Purpose: Obtain spectra sufficient to classify the candidate as a QSO (or not), and, if so, its redshift and line widths (the latter for estimating the mass of the central black hole).
Instructions:
Here is some basic information about each target, as well as priorities:
Pri ObjID r-band RA DEC
1 520 17.2 325.3 -0.8
2 268 20.6 15.8 -0.2
3 204 19.1 15.2 -0.9
Note the last object is almost certainly a blazar, as there is an SDSS
spectrum. It shows a fairly convincing continuum lag, but no broad lines
(just continuum). We're curious about it, but it is definitely our lowest
priority as we don't have a good way to estimate the BH mass.
Targets: QSOcandidates.csv
Finding Charts: QSO Candidate Finding Chart Page
Tarball: QSOcandidates.tgz
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Last updated: 29 September 2018