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A spectroscopic survey of faint compact objects

Colless, Matthew and Ellis, Richard S. and Taylor, Keith and Shaw, Graham (1991) A spectroscopic survey of faint compact objects. Monthly Notices of the Royal Astronomical Society, 253 (4). pp. 686-702. ISSN 0035-8711. doi:10.1093/mnras/253.4.686. https://resolver.caltech.edu/CaltechAUTHORS:20210130-165032906

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Abstract

We present results from a low-resolution (73 Å) spectroscopic survey of faint compact objects conducted with the Low Dispersion Survey Spectrograph at the Anglo-Australian Telescope. The sample is a random subset of all compact sources with 22.5⩽ bⱼ ⩽23.5 in three high-latitude fields. Additional data on compact sources with 21⩽bⱼ⩽22.5 have been selected from the higher resolution (13 Å) survey previously published by Colless et al. ( 1990 ), and a subset of these brighter objects has been studied at both dispersions. The new fainter survey was motivated by the possibility of discovering rare, but potentially important, populations of hitherto unidentified compact sources and establishing limits on their contributions to the source counts. Low-dispersion spectra have been secured for 117 new sources, of which spectroscopic identifications are possible for 67. Incompleteness arises primarily because only certain types of object have spectral features recognizable at this low dispersion. The bulk of the identified sources are intermediate- and late-type stars but a few galaxies and QSOs are also found. Completeness is a strong function of optical colour however, permitting us to derive important new constraints on the abundance of three populations at faint magnitudes as follows. (1) We demonstrate that our survey is sensitive to the presence of typical QSOs with broad emission features, and obtain limits on the surface density of QSOs at fainter magnitudes than previously possible. Our estimates support a flattening of the count-magnitude relation beyond bⱼ = 20, as indicated by earlier work at brighter magnitudes. This result is especially significant since our sample is selected only by apparent magnitude, and is thus more inclusive than previous studies which have relied on additional selection criteria such as colour or variability. (2) For faint Galactic stars, we find a colour-magnitude distribution that is consistent with models invoking an intermediate population II thick disc. More complete and extensive data would provide numerical constraints on such models. (3) Finally, we investigate whether locally rare populations may make significant contributions to the very faint (B ~ 27) source counts. The paucity of very blue compact sources in the LDSS survey suggests the abundance of such objects at fainter limits arises via a gradual increase in the star formation rates in the galaxy population, rather than via a Euclidean increase due to a compact local population or a sudden onset with apparent magnitude of very distant sources. The absence of red objects in the very faint colour distribution, together with the dominant population of Galactic stars in the LDSS sample, limits any significant contribution from dwarf stellar systems such as intergalactic globular clusters and dE galaxies.


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URLURL TypeDescription
https://doi.org/10.1093/mnras/253.4.686DOIArticle
http://adsabs.harvard.edu/doi/10.1093/mnras/253.4.686ADSArticle
ORCID:
AuthorORCID
Colless, Matthew0000-0001-9552-8075
Ellis, Richard S.0000-0001-7782-7071
Additional Information:© 1991 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. Accepted 1991 July 31. Received 1991 July 31: in original form 1991 May 9. We acknowledge the generous allocations of time on the Anglo-Australian Telescope which made this work possible. The photographic photometry was performed on the COSMOS machine at the Royal Observatory, Edinburg, and calibrated with CCD Data kindly supplied by Laurence Jones and Karl Glazebrook, Lance Miller and Chris Collins. We thank Raja Guhathakurta for supplying data in machine-readable form. The computing and data reduction was carried out on STARLINK, which is funded by SERC. MCC acknowledges the support of SERC PDRA and a Fellowship at King's College, Cambridge. RSE and GDS acknowledge financial support from SERC.
Funders:
Funding AgencyGrant Number
Science and Engineering Research Council (SERC)UNSPECIFIED
King's College, CambridgeUNSPECIFIED
Issue or Number:4
DOI:10.1093/mnras/253.4.686
Record Number:CaltechAUTHORS:20210130-165032906
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210130-165032906
Official Citation:Matthew Colless, Richard S. Ellis, Keith Taylor, Graham Shaw, A spectroscopic survey of faint compact objects, Monthly Notices of the Royal Astronomical Society, Volume 253, Issue 4, December 1991, Pages 686–702, https://doi.org/10.1093/mnras/253.4.686
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:107830
Collection:CaltechAUTHORS
Deposited By: Rebecca Minjarez
Deposited On:11 Feb 2021 17:44
Last Modified:16 Nov 2021 19:06

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