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MILLIQUAS - Million Quasars Catalog, Version 7.10 (15 April 2023) |
HEASARC Archive |
Overview
This table contains the Million Quasars (MILLIQUAS) Catalog, Version 7.10 (15 April 2023). It is a compendium of 845,286 type-I QSOs and AGN, largely complete from the literature to 15 April 2023. 553,966 QSO candidates are also included, which are those calculated (via radio/X-ray association including double radio lobes) to be 50%-100% likely to be quasars. Blazars and type-II objects are also included, bringing the total count to 1,447,613. About 73% of all objects show Gaia-EDR3 or Pan-STARRS astrometry.Low-confidence/quality or questionable objects (so deemed by their researchers) are not included in Milliquas. Additional quality cuts can be applied as detailed in the HMQ paper (Flesch 2015,PASA,32,10). Full QSO/AGN classification is accomplished via spectral lines, yielding a reliable spectroscopic redshift. Two spectral lines are required, or one spectral line refining a compatible photometric redshift. Obscured AGN with redshifts from the hosts only are taken to be type-II objects. Some legacy quasars with neither good spectra nor radio/X-ray association were flagged by Gaia-EDR3 as 5-sigma moving (i.e., stars), and so were removed from Milliquas. All objects are de-duplicated across source catalogs. The author's aim here is to present one unique reliable object per each data row. Two NIQs offset < 2 arcsec can be reported as a single object if within the same host. Lenses are reported as single objects onto the brightest source, although some extra images are identified (as type L) if they carry radio/X-ray associations. Milliquas is not a catalog of lenses.
This version has the following changes from the previous edition:
(1) Quasars added from publications to 15 April 2023.
(2) Gaia-DR3 quasar candidates' redshifts are henceforth rounded to the 0.01z
instead of 0.1z because their performance is being seen (by the
astronomical community) to be that good.
(3) The method of Cristiani+ 2023 (cite='QUBzs') approaches full spectroscopy
and is used to classify selected Gaia-DR3 candidates as quasars. That
subset of their output which show radio/X-ray association are accepted as
quasars here.
(4) ~15,000 candidates with only single-band photometry and only one
radio/X-ray detection were dropped because ~half of those are not
optically seen at all.
Note: The author readied Gaia-DR3 astrometry to replace DR2 in Milliquas, but testing found that DR2 has better completeness of desired objects in crowded sky. Examples are J121450.06-055228.1 and SDSS J222942.84+002954.0, both of which are close Red-blue doublets for which VLASS gives a radio detection onto the blue object; Gaia-DR2 presents those blue objects but Gaia-DR3 gives only the red. The author suggests that maybe a Gaia on-spacecraft software change has prioritized red/yellow sources over blue, but whatever the cause, the author has decided that Gaia-DR2 seems better suited.
The contents are relatively simple; each object is shown as one entry with the sky coordinates (of whatever epoch), its original name, object class, red and blue optical magnitudes, PSF class, redshift, the citations for the name and redshift, and up to four radio/X-ray identifiers where applicable.
Questions/comments/praise/complaints may be directed to Eric Flesch at eric@flesch.org. If you use this catalog in published research, the author requests that you please cite it. The paper for Milliquas is at https://arxiv.org/abs/2105.12985. Please cite as Milliquas v7.10 (2023) update, Flesch, E.W. 2021,arXiv:2105.12985 or as the refereed citation, Milliquas v7.10 (2022) update, Flesch, E.W. 2015,PASA,32,10.
The confirmed quasars of this catalog (to Jan 2015) were published as the Half Million Quasars (HMQ) catalog: Flesch E., 2015,PASA,32,10. Note however that Milliquas uses optical sky data from ASP (2017,PASA,34,25) whereas the HMQ used optical sky data from QORG (2004,A&A,427,387) Appendix A.
This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
This research has made use of the SIMBAD database and cross-match service (to obtain Gaia and Pan-STARRS data) provided by CDS, Strasbourg, France. https://simbad.cds.unistra.fr/simbad
References
Flesch, E.
The Million Quasars (MILLIQUAS) Catalog, Version 7.10 (15 April 2023)
https://quasars.org/milliquas.htm
See also:
APM Catalog http://www.ast.cam.ac.uk/~mike/apmcat USNO-A/B Catalogs http://tdc-www.harvard.edu/catalogs/ub1.html NVSS Catalog http://www.cv.nrao.edu/nvss FIRST Catalog http://sundog.stsci.edu SUMSS Catalog http://www.astrop.physics.usyd.edu.au/sumsscat/ MGPS Catalog http://www.astrop.physics.usyd.edu.au/mgpscat/ https://www.sydney.edu.au/science/our-research/research-centres/sydney-institute-for-astronomy/astronomy-surveys.html ROSAT Catalogs http://www2011.mpe.mpg.de/xray/wave/rosat/catalogue/index.php 1WGA Catalog https://heasarc.gsfc.nasa.gov/wgacat/ Chandra Source Catalog http://cxc.cfa.harvard.edu/csc/ XAssist Home Page https://asd.gsfc.nasa.gov/xassist/ XMM-Newton Catalog http://xmmssc.irap.omp.eu/ XMM-Newton Slew Survey http://www.star.le.ac.uk/~amr30/Slew
Provenance
This table was updated by the HEASARC in February 2023 based on a machine-readable catalog obtained from the author's MILLIQUAS website at https://quasars.org/milliquas.htm.Version Log
0.1 22Apr09
0.3 6May09 Added a radio identifier and an X-ray identifier.
0.5 11May09 Added 30816 objects from newly calculated associations to
XMM, Chandra and SUMSS detections, plus some tweaks.
Also added QSO probability % for non-confirmed QSOs.
0.8 22Jun09 Added Chandra Source Catalog 1.0 (2009).
1.0 3Aug09 Extensive de-duplication. XMM Slew Catalog data added.
1.4 20Aug09 Misc fixes in the de-duplications.
1.5 29Aug09 Used XMM Slew Catalog v1.3
2.0 14Jun10 Used XMM Slew Catalog v1.4, XMM3, and XAssist4.
2.1 17Aug10 Removed 8627 NELGs masquerading as AGNe.
2.2 7Jan11 About 10,000 AGNe from the previous edition are now
presented as QSOs. 796 AGNe mistakenly expunged in 2.1
have been restored.
2.3 5Mar11 SDSS DR-8 and BOSS targets have been included and the
threshold for inclusions of candidates has been raised
from 60% to 70%.
2.4 5Jun11 Improved QSO-likelihood calculation for the BOSS targets,
so 17% of previously included BOSS targets drop out.
Newly included data from several sources (see above).
2.5 20Jul11 Some de-duplication of quasars which were discovered prior
to 1990, 200 recent NED quasars added, some radio/X-ray
associations to USNO-B optical data added.
2.6 10Sep11 The USNO-B catalog has been added and hard-deduplicated
against APM and SDSS data to make a background pool of
1.04 billion optical objects. Also, about 12 million
orphaned one-color APM objects have been removed. There
are consequently improvements in this catalog's optical
selections and astrometry without changing the net totals
much. XMM Slew 1.5 catalog added. Some further astrometric
fixes and de-duplications of early quasars.
2.7 5Nov11 New quasar publications to 4 November 2011 were added,
and a few fixes on individual objects incorporated.
2.8 29Jan12 Completed the fixes of non-astrometric relic data from the
Veron-Cetty & Veron 13th edition. About 150 other fixes.
Quasars compilation updated through 27 January 2012.
2.9 2Apr12 Data brought up to publications as of 31 March 2012,
about 50 astrometric fixes done, and the new FIRST radio
catalog, 12Feb16 version, incorporated.
2.10 6Aug12 Data brought up to publications as of 31 July 2012, including
the SDSS-DR9 release, XAssist XMM-Newton and Chandra X-ray
data updated to 30 June 2012; as this is a catalog for
type I (broad-line) objects, 1870 Seyfert-2s, 532 LINERs,
and 6 NELGs were removed, but BL Lacs were retained as
unconstrained emission objects.
3.0 9Sep12 Data brought up to publications as of 31 August 2012.
Redshifts are calculated for the XDQSO photometric quasar
candidates. Fixed issues with 30 DEEP2 object. Separated
out 15 SDSS-DR9 object that had been conflated with others.
QSO-AGN separator restored to that used through v2.9, thus
~5000 QSOs were re-classified as AGNe. AGNe historic names
sourced from the Principal Galaxy Catalogue.
3.1 22Oct12 Quasar data brought up to publications as of 20 Oct. 2012,
including the new DR9 Quasar catalog (Paris I., 2012,
arXiv:1210.5166).
3.2 10Feb13 Quasar data brought up to publications as of 9 Feb. 2013.
MMT quasar positions fixed, and made a few small
miscellaneous fixes.
3.3 7Apr13 Quasar data brought up to publications as at 6 April 2013.
Added 713 new quasars from Palanque-Delabrouille et al.
(2013, A&A, 551, A29). Included SWIRE data, consisting of
117 confirmed quasars and >20K photometric quasars from
Rowan-Robinson et al. (2013, MNRAS, 428, 1958).
Located 8 QSOs that were previously uncertainly located
and removed 1 that had no credible candidates. Removed 26
SDSS-DR9 quasars after inspection showed they were only
artifacts. Removed 144 questionable quasars from Iovino
et al. (1996, A&AS, 119, 265). Removed 8 blazars classified
as white dwarfs by the SDSS DR7 WD Cat (2013,ApJS,204,5).
Miscellaneous: 4 moves, 2 de-dups, and 4 deletions found
after extensive trawling.
3.4 11Jul13 Quasar data brought up to publications as at 11 July 2013.
The author's paper (2013, PASA, 30, 4) marked 9 QSOs as
uncertainly located. Of those:
(a) Q 0112-27 is finally sited at J011517.2-271223,
courtesy Cyril Hazard.
(b) Q 0752+617 is moved to J075646.6+613639, r=16.9, b=17.4,
as a better fit with its co-published quasar (NOTNI 16,
r=16.7, b=17.2).
Added 92 new quasars from Cyril Hazard. Q 1409+732 was found
to be sited on a plate flaw, and is now moved one arcmin
due East to perfect optical fit at J141003.2+725939,
r=19.3, b>22. XAssist v4 XMM-Newton & Chandra X-ray data
updated to 30-June-2013.
3.5 11Aug13 Quasar data brought up to publications as at 10 August 2013,
including SDSS-DR10. Note that the DR10 is an automated
catalog, so its object classifications are not as
trustworthy as manual classifications. Thus, earlier
manual classifications are retained over DR10
classifications. XMM-Newton X-ray data updated to 3XMM-DR4
version (24-July-2013). FIRST radio data updated to
13Jun05 version (05-June-2013).
3.6 23Oct13 Quasar data brought up to publications as at 22 October
2013. Two additional columns of radio/X-ray detections
were added. This is so that any radio lobes will always be
fully displayed, and extra detections from other source
catalogs give a sense of fuller coverage. 158 additional
quasars were added from SDSS-DR10. These were flagged as
bad astrometry, but they are confirmed by the author's
optical background database. Photometric quasar candidates
from surveys other than NBCKDE and XDQSO, e.g., SWIRE,
have been dropped because much of their yield are type 2.
This includes Palanque-Delabrouille et al.
(2011,A&A,530,122), which has been well investigated
spectroscopically and its residue thus less likely to be
QSOs. X-ray detections from the Champ2 catalog, Kim M. et
al., 2007,ApJS,169,401 have been removed. It's a small
catalog which, unlike others, does not present its raw
astrometry needed for calculating optical solutions. The
Veron quasar catalog v13 (2010 A&A,518A,10) included some
objects denoted as non-quasars by their discovery papers,
and the following have been removed as a result:
(a) 484 emission-line galaxies (ELGs) of z<0.46 from
Schneider/Schmidt/Gunn 1994,AJ,107,1245, incorporated
as QSOs by VCV13;
(b) 55 ELGs of Schneider/Schmidt/Gunn 1999,AJ,117,40;
(c) 58 galaxies from 2dF-GRS (Colless M. et al.,
astro-ph/0306581); and
(d) 41 galaxies from La Franca F. et al.,
1999,A&AS,140,351.
A few positional fixes, de-duplications, and removals of
type-2s.
3.7 26Nov13 Quasar data brought up to publications as at 26 November
2013, including the SDSS DR10Q release by Isabelle Paris
et al., 2013 arXiv:1311.4870. 318 SDSS "quasars" of
auto-redshift>4 which were not subsequently confirmed by
visual inspection are removed as bogus (communication Adam
Myers). The Veron quasar catalog v13 (2010 A&A,518A,10)
flagged some objects as questionable in their "spec"
field. These have unclear spectra or are described as
"possible" by their discovery papers. 178 of these are
removed, and 52 such BL Lacs with redshift>0.5 are
re-classed to AGNs. Some positional fixes and
de-duplications of individual objects.
3.8 16Feb14 Quasar data brought up to publications as at 15 February
2014. NBCKDE and BOSS quasar likelihoods have been
calibrated against the DR10Q (Paris I. et al., 2013
arXiv:1311.4870) classifications. The Swift X-ray Point
Source catalog (Evans P.A. et al., 2014,ApJS,210,8) is added
to the background data, resulting in 12604 associations.
110 SDSS-DR10 automated survey objects are removed as
artifacts. De-duplication of radio/X-ray detections
improved.
3.9 30Jun14 Quasar data brought up to publications as at 30 June 2014.
The XMM-Newton Slew Survey source catalog release 1.6 was
added to X-ray data. The 1SXPS X-ray detections were being
dropped; this was fixed and 21268 were included as a
result. The Veron-Cetty & Veron Quasar Catalog (VCV) 13th
edition (2010,A&A,518,10) was fully mapped into optical;
corrections from this were incorporated.
4.0 05Aug14 Quasar data brought up to publications as at 5 August 2014.
The threshold for inclusion of QSO candidates was raised
to 80% confidence. This resulted in the loss of ~240,000
objects from v3.9, but it improved the confidence of use.
XAssist v4 XMM-Newton and Chandra X-ray data was updated
to 21-July-2014. 98 entries were found to be type II or
not quasars, and so removed. The catalog layout was
changed to conform better to the NED guide "Best Practices
for Data Publication" by Marion Schmitz et al. (v1.2, 2013)
in these ways: (a) all citations were changed to original
discovery papers and no longer to VCV 13th edition or to
NED and discovery citations are now indexed in a separate
file; (b) quasar and radio/X-ray names which used to run
together have been corrected to adhere to naming standards.
4.1 20Oct14 Quasar data brought up to publications as at 5 October 2014.
The input values of RA and DEC used for this table were
given in degrees rather than sexagesimal. Type 2 objects
were included for the convenience of the users, but
completeness of these is only about 95%. The type I
objects are believed to be 100% complete from the
literature. About 3000 SDSS "quasars" were removed as not
quasars. These were auto-objects which were not taken up
by the manual Paris files, and which were not given a
subclass by the SDSS pipeline -- thus, the lowest quality
objects. Another 2000 were reclassified as AGN or type 2
in this catalog. VCV mis-copied the redshifts from 2008
A&A,488,417 -- now fixed. QSOs & AGN re-partitioned by psf
class and modified luminosity equation. Miscellaneous
tweaks and fixes done when revealed by publication-related
analysis.
4.2 06Dec14 Quasar data brought up to publications as at 6 December
2014. SDSS DR10/DR10Q and DR7/DR7Q data were reprocessed,
yielding a few more quasars and using the DR10Q redshifts
more as the current standard. Further adjustments were
made to the luminosity equation separating QSOs from AGN,
resulting in about 2000 AGN reclassified as QSOs. 18 new
quasars from Dan Weedman, based on his re-analysis of the
Weedman 1985 spectra in combination with NBCKDE
photometric redshifts for those objects.
4.3 11Jan15 Quasar data brought up to publications as at 10 January
2015, including the newly-released SDSS-DR12 and
SDSS-DR12Q (www.sdss.org). Approximately, 800 quasars
sourced from the AGES catalog, Kochanek et al. (2012,
ApJS, 200, 8). Approximately, 200 extra quasars added in a
full round-up from NED and SIMBAD.
4.4 06Feb15 Quasar data brought up to publications as at 25 January
2015. Some reprocessing of the SDSS-DR12 and SDSS-DR12Q
data. About 1000 type-1 objects reclassified to type-2.
Photometric candidate likelihoods and redshifts were
recalibrated using the SDSS-DR12Q quasars as the benchmark.
4.5 10May15 780 new quasars from LAMOST-DR1 (Luo et al. 2015,
arXiv:1505.01570) were added. LAMOST-DR1 is a pipeline
catalog with much provisional data, so the author selected
the best-eligible objects only. LAMOST plans a manual
(reliable) QSO catalog later this year. Also, NED/SIMBAD
quasar data is included up to 9 May 2015. Citations were
greatly simplified, referencing the recently published
Half Million Quasars catalog (HMQ: Flesch E., 2015
PASA, 32, 10, arXiv:1502.06303) for smaller legacy citations
while still citing large surveys like SDSS and 2QZ. A
legend for the citations is given below, and the separate
citations file is no longer needed as a result of this.
3XMM-DR5 (Rosen et al., 2015, arXiv:1504.07051) included
in X-ray data. Also, high-confidence data from 2XMMi-DR3
is included, as acknowledged in section 8.2 of the Rosen
paper (dropped 2XMMi-DR3 data recognized as valid). Minor
fixes to optical data resulted in a few more radio/X-ray
associations.
4.6 30Nov15 Additional QSO candidates were sourced from the new
NBCKDE v3 catalog (Richards G.T. et al., 2015-ApJS-219-39)
and a variability and refraction sourced catalog (Peters
C.M. et al., 2015-ApJ-811-95). These added about 300,000
new candidates to Milliquas. Note that the NBCKDE v3
catalog uses different selection criteria from its
predecessor, and so augments it rather than superseding
it. The threshold for inclusion of QSO candidates was
raised from 80% QSO-likelihood to 90%, so the catalog
should be reliable even for spot checks. NED and SIMBAD
listed quasars were included through 30-Nov-2015.
4.7 02Mar16 527 new QSOs were added from recent publications, including
33 new QSOs with z>5 of which 4 have z>6. The UV-Bright
Quasar Survey (UVQS, T.R. Monroe et al., arXiv:1602.06255)
was included with two mag-14 and 43 mag-15 QSOs plus many
brighter AGN.
4.8 22Jun16 The Chandra ACIS source catalog (Wang S. et al., 2016,ApJS,
224,40) was added and new X-ray associations calculated.
The 2nd RASS source catalog 2RXS (Boller Th. et al., 2016,
A&A,588,103) replaced 1RXS for the most part, with
significant differences in places. Radio/X-ray processing
was tightened and data recalibrated to improve likelihood
reliability, as part of a new radio/X-ray catalog in
preparation. 23,727 radio/X-ray associated objects, recently
dropped, were restored on the criterion that they are each
80%+ likely to be true quasars. This was done because this
information is not found elsewhere.
4.8b 30Jul16 The 3XMM-DR6 X-ray source catalog was added and new X-ray
associations calculated. The radio/X-ray data have been
reprocessed in line with that of the Million Optical
Radio/X-ray (MORX) Associations Catalog (Flesch 2016,
PASA, 33, 52).
5.0 19Jun17 The J2000 coordinates now have 1/10th arcsecond precision,
and the magnitudes have 1/100th mag precision, either from
the original surveys or from the All-Sky Portable (ASP)
optical catalog (arXiv:1705.05434). 5414 net QSOs/AGNs were
added from recent surveys (listed below), notably AAOz,
OzDES, LAMOST DR2, and a reload of AGES. The 3XMM-DR7 and
XMMSL2-2.0 Slew X-ray source catalogs were added and new
X-ray associations calculated. A few duplicates were
removed. Notably, SDSS J131715.46+601533.1 was found to be
a duplicate of SBS 1315+605.
5.1 30Jun17 Included full coverage of the Subaru-XMM Deep Field from
multiple authors, LAMOST DR3, and other miscellaneous
papers.
5.2 05Aug17 SDSS-DR14 and SDSS-DR14Q were added, using the processing
rules from the Half Million Quasars catalog (HMQ: Flesch
2015, PASA, 32, 10). WISE quasar candidates were added
from Secrest et al. 2015, ApJS, 221, 12. These are
~430,000 candidates over the whole sky for which 2-color
optical objects were found within a 2-arcsec radius. They
were processed into pQSOs from calibration against the
SDSS-DR12Q multi-class superset, and photometric redshifts
obtained using the four-color based method from the HMQ
Appendix 2. The four colors used were B-R, R-W1, W1-W2,
and W2-W3. Type-II narrow emission-line galaxies (NELGs,
class='N') were added as the luminosity class
corresponding to the type-I AGN galaxies. High-luminosity
type-II NLAGN (class='K') correspond to the type-I
quasars. The NLAGN/NELG divider is the same luminosity/psf
function which separates QSOs from AGNs. Type-II NELGs
include unquantified contamination by LINERs and probably
a few starbursts which eluded removal, so it serves as a
catch-all category presented for completeness, rather than
as a strict type-II class. Small publications through 5
August 2017 were added. Positional fixes (of about 2
arcsec) were applied to ~150 objects.
5.3 12Sep18 Radio/X-ray association likelihoods calculated to a
granularity of 1/10th of an arcsecond for Chandra,
XMM-Newton, and Swift X-ray source catalogs and the FIRST
radio source catalog. All associations have been
recalculated onto the APM/USNO-B optical background of
Flesch 2017,PASA,34,25 (Figure 3). Radio/X-ray association
likelihoods to faint SDSS sources not in the optical
background were previously halved, based on the
approximately doubled sky density of SDSS. This deduction
was changed to be classed by PSF and red-blue color,
consequentially most SDSS likelihoods were reduced more,
often by 60%-90%. Associations to other faint objects were
also reduced. The overall effect was that ~20,000
candidates fell below the 80% likelihood threshold for
inclusion in Milliquas, and so were removed. Visually
inspected quasars from the LAMOST DR3Q (Dong et al.,
2018,AJ,155,189) and auto-quasars from the LAMOST DR4
(https://dr4.lamost.org/) were quality checked and a total
of 10,624 quasars/AGN added to Milliquas.
5.4 17Oct18 Quasars from individual papers from August 2017 forward to
15 October 2018 have been added, plus some from a couple
older papers. Quasar doublets are more carefully processed
to show 2 quasars instead of 1. A few gravitationally
lensed images are added as type='L', in addition to the
already-catalogued brightest one. These are added only
where the optical data shows them in order to account for
any radio/X-ray associations to them. The 3XMM-DR8 X-ray
source catalog has been added and new X-ray associations
calculated. A bug in v5.3 dropped radio/X-ray associations
to some high-z quasars was fixed.
5.5 19Nov18 Quasars from publications to 14 November 2018 were added.
The SDSS data were reprocessed to ensure DR14 data is used
where available. Close quasar pairs and lens images
processing was completed. 631 "unknown class" (type=U)
objects (SDSS pipeline QSOs without subclass) were added.
There are not usually accepted into Milliquas but they had
probable radio/X-ray associations of p>80% which thus
qualify them for inclusion. The SDSS pipeline redshift for
these were included provisionally. The J2000 decimal
round-up was increased to avert truncation.
5.6 17Dec18 Quasars from publications to 15 December 2018 were added.
The 3rd release of SDSS-DR14Q (v4.4) was incorporated,
adding ~300 quasars which had no astrometry in their
earlier releases. All SDSS data was reprocessed to get rid
of artifacts which had crept in. In preparation for LAMOST
DR5Q (Yao et al 2018,arXiv:1811.01570), the LAMOST DR4
auto-quasars were demoted to quasar-candidates. LAMOST
pipeline quasars were processed using the same rules as
with SDSS pipeline. Removed 223 objects from
Iovino/Clowes/Shaver,1996,A&AS,119,265 which had no quasar
profile nor radio/X-ray/WISE associations, leaving 917 in
Milliquas, resolving the cautionary note from
HMQ (2015,PASA,32,10) section 2.B.4 end.
5.7 07Jan19 Quasars were added from publications to 7 January 2019,
including LAMOST QSO DR5. The logic was tightened up for
using SDSS SUBCLASS and ZWARNING fields to decide
classifications for SDSS objects, including pipeline-only
candidates. Milliquas was previously classifying all
QSOs/AGN of z<0.1 as AGN. This boundary was moved to
z=0.05 because of many core-dominated QSOs between z=0.05
and 0.1, e.g., IRAS 01267-2157 (SDSS J012910.99-214156.8)
at z=0.93. HMQ (2015,PASA,32,10), section 5, discusses
these luminosity-based boundaries. 22 objects from Boyle
et al., 1990,MNRAS,243,18, classified by them as "possible"
QSOs with "uncertain" redshifts, were removed from
Milliquas. Positional fixes were done on ~90 legacy
objects, mostly moves of <5 arcsec.
6.0 15Mar19 Quasars were added from publications to 15 March 2019.
For ease of use, the "HMQ" citation (necessitating
consultation of the HMQ catalog 2015-PASA-32-10 to
identify the discovery article) was replaced by the
HMQ-given 4-digit citation number. 30512 entries were
changed, and the HMQ references file can be directly
consulted for any numeric citation, making Milliquas into
a stand-alone catalog. Positional fixes were made to 9
legacy objects. Where SDSS had a different redshift for a
LAMOST-discovered quasar, if the difference is >0.1z, the
name and discovery credit were transferred to SDSS. This
was done for 6 objects. 42 AGN are dropped because their
discovery paper Mauch & Sadler 2007,MNRAS,375,931 flagged
those classifications as "not certain" and they had
neither stellar psfs nor secure (80%+) radio/X-ray
associations. The unseen Soviet BAL quasar "SBS 1401+566"
was dropped. The quasar "Q 1409+732" was moved to the
coordinates stated by its discovery paper Anderson &
Margon 1987,Nature,327,125, where a suitable object
resides. Confusion came from that paper's discrepant
finding chart onto a plate flaw.
6.1 12May19 Quasars were added from publications to 12 May 2019.
Gaia-DR2 astrometry was used and flagged for 63% of
Milliquas (MQ) objects. Gaia sources were matched 1-to-1
with MQ objects on the criterion that the Gaia source is
that nearest to the MQ object and that the MQ object is
that nearest optical (out of a 1.163G optical DB) to the
Gaia source. Care was taken to avoid false matches. 99%
of all matches are within an arcsec offset, but to find
valid farther matches, all matches were binned by object
class and offset distance in 0.1 arcsec bins, with
hundreds of targeted spot checks done to refine offset
limits and to check objects with anomalous Gaia BP-RP
color suggestive of a false match. SDSS quasar candidates
could not be matched beyond 1 arcsec offset because they
are often optically faint and/or in close groups for which
Gaia had a different object only. AGN cores match to 1.5
arcsec beyond which Gaia often shows nearby stars only.
QSOs/Bl-Lacs match well out to within 4 arcsec; for these
I spot-checked all matches beyond 2 arcsec and all with
off-colors beyond 1 arcsec offset and removed 14 false
matches. However, for Gaia sources without BP and RP
colors, QSOs match reliably only within 2 arcsec and
Bl-Lacs within 1.5 arcsec. X-ray/radio-only candidates
(unique to MQ) match reliably out to within 2.5 arcsec
offset. In all cases it was paramount to avoid false
matches, thus very many true matches were lost beyond
the offset cutoffs. Reclassifications were done for
Milliquas objects deemed by the SDSS-DR14 pipeline to be
plain galaxies -- these were heavily spot-checked to
confirm. 16 QSOs, 172 AGN and 2343 type-II objects were
found to be just galaxies and so are dropped, and 433
host-dominated QSOs were reclassified to AGN.
6.2 22May19 About 50 fixes were done on Gaia-DR2 opticals selected in
crowded places. Quasars were added from publications to 22
May 2019, including the PS-ELQS. 3LAC was reprocessed to
fix a few selections and improve completeness. The z=2.136
QSO "SDSS J101012.77+560520.0", overlooked by SDSS, was
added.
6.3 16Jun19 Quasars were added from publications to 15 June 2019,
including 4LAC. 3,581 galaxies with double radio lobes
were added as type=G because the lobes show that they have
active nuclei of some kind, even if well hidden.
Positional fixes of a few arcsec were done for ~50 legacy
objects. Blazar candidates with neither redshift nor
radio/X-ray association, about 30 objects, were dropped.
Most were stated to be low confidence in legacy papers.
6.4 11Dec19 Quasars were added from publications to 11 December 2019.
The SDSS-DR16 pipeline release was added. The author
processed it using the standard HMQ rules which yield QSO
classifications that accord well to the follow-up manual
SDSS classifications. A new rule for Milliquas
classification was added such that STARFORMING and
STARBURST subclasses, or GALAXY classification by the
DR12Q superset, are now taken to indicate optical host
domination, e.g., classed as AGN instead of QSO. More
candidates with double radio lobes were added, active
nuclei being indicated. A photometric threshold guards
against starforming interlopers. The pQSOs of SDSS
candidates which are eBOSS targets were lowered due to
anti-selection, i.e., possibly DR16Q-classified as a
non-quasar. Candidates which consequently fell below
pQSO=80% (~57K) were dropped. The Chandra Source Catalog
v2 was added, but only as a supplement to the CSC v1.1
because v2 provides only stacked data for which the
optical solution used by Milliquas cannot be calculated.
6.4b 19Dec19 Some extra processing of the new SDSS-DR16 data yielded 534
more type-I objects and fixed the astrometry of 381
objects which had been offset by up to 3 arcseconds. About
800 QSOs were flagged as host-dominated and so were
reclassified to AGN.
6.4c 31Dec19 Quasars were added from publications to 31 December 2019.
The 4XMM-DR9 XMM-Newton catalog was added and X-ray
associations calculated, replacing 3XMM-DR8. The 2SXPS
Swift XRT catalog was added and X-ray associations
calculated, replacing 1SXPS. Gaia astrometry was removed
from 18 quasars and 66 candidates which were in doublets
(on the sky) for which Gaia had astrometry only for the
other object. SDSS-DR16 redshifts more fully replaced
earlier SDSS pipeline data.
6.5 14Jun20 Quasars were added from publications to 14 June 2020.
Gaia-sourced parallaxes and proper motions were analyzed
to see if they could identify false quasars. Legacy quasar
publications were then group tested such that those with a
high flag rate (>20% compared with 2% overall, signaling
the presence of low-quality data) had their flagged
objects dropped, provided, as a confirmation, that those
objects also had no radio/X-ray associations. The counts
of dropped objects were:
-- 28 out of 40 (70%) from Zhan & Chen, 1987 & 1989 ChA&A
-- 400 out of 916 (44%) from Iovino/Clowes/Shaver,
1996,A&AS,119,265
-- 50 out of 194 (26%) from Savage/Trew/Chen/Weston,
1984,MNRAS,207,393
-- 111 out of 517 (21%) from Drinkwater 1987.
In total, 589 "quasars" were dropped for having
parallaxes/proper motions. 136 SDSS-DR14 objects which
were dropped by SDSS-DR16 were removed. About 1500 objects
had their photometry supplemented from Pan-STARRS data.
6.6 30Aug20 Quasars were added from publications to 30 August 2020.
The SDSS-DR16Q data (Lyke+ 2020) were incorporated.
Combined with the DR16 pipeline data, these contributed
~200K new quasars beyond DR14 plus many valuable
reclassifications of the SDSS-IV data. In processing this
vast data pool, the author identified 37 new quasars not
classified by DR16/DR16Q. These were added in Milliquas
with ref_name="MQ" and ref_redshift="DR16QN"/"DR16". Data
selection of DR16 pipeline data was by HMQ (Flesch 2015)
rules, including choice of spectra. Data flagged with
ZWARNING=256 (bad astrometry) were validated by testing
and are included. Details of usage of the SDSS-DR16/DR16Q
data will be included in a Milliquas paper in preparation
(Flesch 2021).
7.0 30Sep20 Quasars were added from publications to 30 September 2020.
SDSS-DR16 represented the conclusion of the eBOSS and BOSS
quasar surveys, and that conclusion somewhat orphaned the
leftover candidates from the SDSS-based photometric
catalogs. Said candidates without any radio/X-ray/WISE
associations were unlikely to be targeted in this decade,
and so were dropped from Milliquas, 574,538 of them. Said
candidates which did have WISE associations, numbering
35,086, were changed to display AllWISE names. These
significant changes prompted this release to be numbered
v7.0.Clean-ups were done on the uptake of SDSS-DR16Q/DR16
by Milliquas v6.6, notably 4,506 DR16Q quasars previous
presented as candidates, were designated to be QSOs. Also,
404 low-quality pipeline objects which were presented as
QSOs were dropped. WISEA photometric redshifts were
recalculated using the DR16-augmented training set, and
Pan-STARRS-based photometric redshifts were calculated for
radio/X-ray associated candidates on the PS1 footprint
(all-sky N of decl. S30) using the four-color method of
2015,PASA,32,10, Appendix 2. 222 candidates in a solid
degree centered on J2033+412 in Cygnus were dropped. They
are obvious stars, albeit near to background Galactic
X-ray sources.
7.1 14Feb21 Quasars were added from publications to 14 February 2021.
For quasar candidates, the pQSO (likelihood that the
candidate is a quasar) threshold for inclusion into
Milliquas was lowered to 60%. This was done to present
more radio/X-ray associated candidates which were not
available elsewhere. Audits on the inclusion of DR16Q into
Milliquas led to tweaks of the selection of DR16Q objects.
Other SDSS data were also audited. Also, all galaxy data
are removed in order to focus exclusively on quasars.
LAMOST-DR6 was added -- being pipeline-only data, its
quasar classifications were accepted into Milliquas only
when supported by radio/X-ray/WISEA pQSOs. 4XMM-DR10 X-ray
sources were added, replacing DR9.
7.2 02May21 Quasars were added from publications to 30 April 2021.
The VLASS Quick Look radio catalog was included, which
added 34189 new radio core associations and 6793 probable
double radio lobe associations. Ongoing audits of SDSS and
LAMOST quasars resulted in a few additions and drops. Some
WISEA-supported SDSS/LAMOST pipeline quasars were accepted
which were otherwise marginal. Also, some likely galaxies
were removed.
7.3 31Oct21 Quasars were added from publications to 31 October 2021.
17 classified quasars were dropped as moving stars
(Gaia-DR2 flagged and confirmed on legacy DSS charts), 4
as galaxies, and 1 line poacher. 42,637 quasar candidates
for which Gaia-DR2 shows proper motion or parallax, have
been dropped for efficiency. 1365 quasars and ~100K
candidates without Gaia-DR2 J2000 were reconciled to
Pan-STARRS or SDSS J2000 with an average positional shift
of ~0.1 arcsec. About 400 very faint (r>22) legacy quasars
were positionally tweaked by comparing to DES and
Pan-STARRS images, usually ~1 arcsec, some more. Selection
and processing tweaks done on candidates, adding a net 93.
AGES (Kochanek+ 2012) was reloaded using the CDWFS X-ray
survey (Masini+ 2020,ApJS,251,2) to support object
selection. AGES did not publish their spectra; 368 of
their objects were switched to cite DR16Q which shows
spectra. RACS (Hale+ 2021, arXiv:2109.00956) radio
associations were added. RASS (ROSAT All-Sky Survey) X-ray
data was dropped, as it has become clear over time that
its resolution is too coarse to confidently identify
sources. OzDES1 (Tie+ 2017,AJ,153,107) were fully replaced
by OzDES2. 4XMM-DR11 X-ray sources were added, replacing
4XMM-DR10.
7.4 12Dec21 Quasars were added from publications to 12 December 2021.
SDSS-DR17 was processed, with 1003 new quasars and 266 new
MaNGA AGN added. The eFEDS AGN catalog was processed, with
532 new quasars added. Only the best-quality data were
used (5029#); of which, 1139 were new objects.
Redshift/photometry cut-offs were used on those to avoid
galaxy contamination. WISEA-only candidates were removed
to avoid repeating candidates from other catalogs, which
resulted in 448,009 candidates removed. The only
candidates presented are those with radio/X-ray
associations calculated by this work. More Pan-STARRS
astrometry was added. 1219 RACS associations with bad RACS
names (wrong hemisphere) were fixed.
7.5 30Apr22 Quasars were added from publications to 30 April 2022.
The LAMOST DR7 pipeline added 646 QSOs supported by
radio/X-ray/WISEA association. A search revealed six
earlier (2011-2021) papers missed due to not being on
ArXiv, paywalled data, or otherwise overlooked. The were
added (yielding 156 new objects) and indexed below as
AT20G, ICRFz, GB6hiz, Hdots1, Hdots2, and 4FGL3.
Candidates selection was tweaked for efficiency with a net
total of ~800 fewer objects. The citations 2MAGN
(Zaw+,2019) and 6dAGN (Chen+,2022) classify faint nuclear
emission. Their type-I & Kewley-criterion type-II objects
were accepted into the catalog. HETDEX AGN of 2+ spectral
lines were added into Milliquas after deduplication.
7.6 15Sep22 Quasars were added from publications to 31 August 2022.
All objects/candidates calculated as having 80-100%
likelihood of radio/X-ray association (RXpct) were
included, including classified galaxies. This increased
the Milliquas row count by ~50%. The threshold was
increased to 80% to increase reliability. RXpct and Qpct
(pQSO) were split into separate columns clarify the
distinction for users. Gaia-DR3 QSO candidates (indexed as
"GAIA3" below) with redshifts were matched to radio/X-ray
detections, and those with calculated associations of 80%+
likelihood were added as candidates. Their redshifts were
rounded to 0.1z to show that they are only approximate;
because of the lack of spectral redshift, they could not
be fully classified as QSOs in Milliquas. The
classification of "q" (quasar candidate) was added to
denote candidates which are 99% likely to be true QSOs, as
per the method of Flesch 2015,PASA,32,10 Section 8.
4XMM-DR12 X-ray sources were added, replacing DR11.
MIGHTEE spectral AGN (indexed as "MIGHTE" below) were
added, but with cuts to avoid galaxy contamination: 2/5
MIGHTEE "True" tests required, and z>0.7.
7.7 15Oct22 Quasars were added from publications to 15 October 2022.
Some quasar candidates of pQSO 60%-79% were missing; now
added. Positional fixes done on ~6000 candidates which had
"epoch 2000" astrometry from USNO-B. Where USNO-B adjudged
the object to be moving, the epoch 2000 projection could
be discrepant by many arcsec. Pan-STARRS astrometry has
been obtained for these objects where available, i.e.,
those of decl>-30. Those remaining have been flagged as
questionably located.
7.8 04Dec22 Quasars were added from publications to 4 December 2022.
LoTSS (2022,A&A,659,A1) radio associations were included,
adding about 272K candidates. VLASS was reprocessed to
include only Gaussian detections, and more of them. This
added a net 14,734 more quasar candidates. Association
likelihoods were calculated in 0.1-arcsec offset bins for
all radio/X-ray input surveys. Galaxies and low-likelihood
QSO candidates were removed.
7.9 05Feb23 Quasars were added from publications to 5 February 2023,
including SDSS-DR18 and LAMOST QSO DR6-DR9. Gaia-EDR3
proper motion data were used to select objects to audit,
especially those of unclear classification from legacy
surveys. The net outcome was the addition of ~500 quasars,
mostly from LAMOST QSO DR1-DR5. Also notable were 12 (out
of 91) Hazard objects dropped due to proper motion
detected, and with no redshift confirmation from SDSS nor
radio/X-ray. DES DR2 astrometry and/or photometry were
supplied to ~15K objects.
7.10 15Apr23 See list of changes above.
Parameters
Name
The designation of the source as taken from the literature.
Nameless radio/X-ray associated objects here utilize the J2000 position in
"HHMMSS.SS+DDMMSS.S" for the convenience of the user. If needing a name for it,
just prefix this value with "MQ ", e.g., MQ J000001.89+443053.8.
RA
The Right Ascension of the quasar candidate in the selected equinox. This was
given in J2000.0 decimal degrees to a precision of 10-7 degrees in the
original table. That suits objects with Gaia-DR2 astrometry and accommodates a
minuscule round-up to avoid truncation in use, but it is too precise for
other objects, although it prevents inadvertent truncation when converting to
sexagesimal.
Dec
The Declination of the quasar candidate in the selected equinox. This was
given in J2000.0 decimal degrees to a precision of 10-7 degrees in the
original table. That suits objects with Gaia-DR2 astrometry and accommodates a
minuscule round-up to avoid truncation in use, but it is too precise for
other objects, although it prevents inadvertent truncation when converting to
sexagesimal.
LII
The Galactic Longitude of the quasar candidate. This parameter has been added
by the HEASARC and is converted from the provided equatorial position.
BII
The Galactic Latitude of the quasar candidate. This parameter has been added
by the HEASARC and is converted from the provided equatorial position.
Broad_Type
The classification of the object, where the following abbreviations are used:
Q = QSO, type-I broad-line core-dominated, 802340 of these.
A = AGN, type-I Seyferts/host-dominated, 42946 of these.
B = BL Lac type object, 2814 of these. (FSRQs are typed as QSOs here.)
L = lensed quasar extra image with radio/X-ray, only 17 of these.
K = NLQSO, type-II narrow-line core-dominated, 5999 of these.
N = NLAGN, type-II Seyferts/host-dominated, 39531 of these. Incomplete,
and includes an unquantified residue of legacy NELGs/ELGs/LINERs,
plus some unclear AGN. This is the catch-all category.
S = star classified but showing quasar-like properties, 1183 of these.
q = best quasar candidates, 99% likely to be true QSOs, as per the method
of Flesch 2015,PASA,32,10 Section 8. 69054 of these.
R = radio association displayed.
X = X-ray association displayed.
2 = double radio lobes displayed (declared by data-driven algorithm).
Rmag
The red optical magnitude of the object. The type and source of this
magnitude is specified in the optical_flag parameter value. Optical data are
mostly from the ASP optical catalog (2017,PASA,34,25) which presents data
from the APM (http://www.ast.cam.ac.uk/~mike/apmcat/), USNO-A and USNO-B
(http://tdc-www.harvard.edu/catalogs/ub1.html), and the SDSS
(https://sdss.org/). APM/USNO-A magnitudes were recalibrated from the
original values as documented in 2004,A&A,427,387. As a result, these
recalibrated USNO-A magnitudes are often used in preference to USNO-B. APM
galaxies brighter than 17th magnitude are usually represented as far too
bright due to PSF modeling. Integer magnitudes (e.g., 22.00) are estimates if
both bands are integers or one band is empty. If the optical_flag parameter
value contains r/b/g/i/v/u/z, then the magnitudes are from the object's
source catalog, e.g., SDSS, 2QZ, etc. Note that many SDSS magnitudes are
extinction-"corrected" ~0.3 mag brighter than observed.
Bmag
The blue optical magnitude of the object. The type and source of this
magnitude is specified in the optical_flag parameter value. Optical data are
mostly from the ASP optical catalog (2017,PASA,34,25) which presents data
from the APM (http://www.ast.cam.ac.uk/~mike/apmcat/), USNO-A and USNO-B
(https://web.archive.org/web/20180529212008/http://www.nofs.navy.mil/), and
the SDSS (https://sdss.org/). APM/USNO-A magnitudes were recalibrated from
the original values as documented in 2004,A&A,427,387). As a result, these
calibrated USNO-A magnitudes are often used in preference to USNO-B. APM
galaxies brighter than 17th magnitude are usually represented as far too
bright due to PSF modeling. Integer magnitudes (e.g., 22.00) can be estimates
if both bands are integer or one band empty. If the optical_flag parameter
value contains r/b/g/i/v/u/z, then the magnitudes are from the object's
source catalog, e.g., SDSS, 2QZ, etc. Note that many SDSS magnitudes are
extinction-"corrected" ~0.3 mag brighter than photometry.
Optical_Flag
This field contains coded information on the optical source properties, as
follows:
p = optical magnitudes are POSS-I O (violet 4050A) and E (red 6400A).
These are preferred because O is well-offset from E, and those plates
were always taken on the same night, thus the red-blue color is
correct even for variable objects. The epochs for these are 1950s.
j = optical magnitudes are SERC J (Bj 4850A) and R (red 6400A) from the
POSS-II or UKST surveys. Red-blue color is less reliable because the
red and blue plates were taken in different epochs, i.e., years apart.
b = blue magnitude is Vega 4400A (Johnson), red is 6400A (Cousins).
g = blue magnitude is SDSS-type green 4900A, red is r 6200A.
n = blue magnitude is Pan-STARRS green 4900A, red is r 6200A.
d = magnitudes are DES DR2 AB r & g.
u = blue magnitude is SDSS ultraviolet 3850A.
v = red magnitude is visual 5500A, or estimated from a sky chart/viewer.
i = red magnitude is infrared 7500A.
z = red magnitude is infrared z 8600A.
r = red magnitude is r 6200A.
(blank) = red alone is 6400A (Cousins); if both magnitudes are present,
then estimates.
G = Gaia-DR2 astrometry shown, precessed to J2000 by CDS. If 'G' is alone
then the magnitudes are Gaia RP & BP, or Gaia G if red band only.
N = Pan-STARRS astrometry shown. If 'N' is alone, PS photometry also.
D = DES DR2 astrometry shown. If 'D' is alone, DES photometry also.
+ = variability nominally detected in both red/blue over multi-epoch data.
m = proper motion detected. If from Gaia-DR2/3 ('G' also present in this
field), then this is proper motion or parallax which usually signifies
a star, but optical centroids can deflect within the optical gradient
of a near moving neighbor or if either object is variable; some will
be quasars. If not Gaia, it is from USNO-B which is nominal only.
e = USNO-B1.0 "epoch 2000" projected location based on nominal proper
motion, can miss true location by many arcsec.
% = swap of two "unplugged" SDSS spectra which crossed wires (7 of these).
a = object is host-dominated with faint nuclear activity, such as an SDSS
pipeline galaxy with an AGN subclass or AGN-classed elsewhere, see
its citation. Milliquas class is 'A' if BROADLINE, else 'N'. (See
broad_type.)
Red_PSF_Flag
A coded representation for the point spread function (PSF) of
the optical source in the red. The APM, USNO-B, and SDSS provide PSF class,
albeit using different criteria. The codes are as follows:
- = point source / stellar PSF (APM notation: -1, here truncated)
1 = fuzzy / galaxy shape (APM notation: 1 and some 2)
n = no PSF available, whether borderline or too faint to tell, etc.
x = unseen / unclear in this band (fainter than plate depth, confused, etc.)
Blue_PSF_Flag
A coded representation for the point spread function (PSF) of
the optical source in the blue. The APM, USNO-B, and SDSS provide PSF class,
albeit using different criteria. The codes are as follows:
- = point source / stellar PSF (APM notation: -1, here truncated)
1 = fuzzy / galaxy shape (APM notation: 1 and some 2)
n = no PSF available, whether borderline or too faint to tell, etc.
x = unseen / unclear in this band (fainter than plate depth, confused, etc.)
Redshift
The redshift of the object, taken from the literature as specified in the
ref_redshift parameter. Spectroscopic/grism redshifts are required for
objects classified as Q/A/K/N/L and is optional for B (BL Lac type).
Photometric redshifts are rounded to 0.1z (and can be identified by that
rounding) and are either taken from the cited catalog or calculated here
using the four-color method of Flesch 2015,PASA,32,10, Appendix 2, using 4
colors from SDSS ugriz, Pan-STARRS grizy (or ogriz with calibrated POSS-I O),
or WISEA colors B-R, R-W1, W1-W2, and W2-W3. Photometric redshifts apply onto
a quasar template mostly and not so well to galaxies. GAIA3 candidates show the
"QSOC" estimated redshift provided by Gaia-DR3, rounded here to 0.01z.
Ref_Name
A character code for the literature reference from which the name was taken
is indicated below. The meaning of any 4-digit numerical code can be found in
the "HMQ-references.txt" file of the author's Half Million Quasars Catalog
(HMQ: Flesch 2015,PASA,32,10) at
http://cdsarc.cds.unistra.fr/ftp/pub/cats/VII/273/refs.dat. The 4-digit
reference codes for galaxies and stars are indexed in the file
"MORX-references.txt" from Flesch 2016,PASA,33,52.
Code (No. of names, No. of redshifts): Reference
2dF (382,212): 2dF galaxy survey, Colless M. et al., 2001,MNRAS,328,1039
2MAGN (7,4552): 2MASS AGN, Zaw/Chen/Farrar, 2019,ApJ,872,134
2MRS (244,3): Huchra J.P. et al., 2012,ApJS,199,26, http://tdc-www.harvard.edu/2mrs/
2QZ (27535,24169): Croom S.M. et al., 2004,MNRAS,349,1397
2SLAQ (10367,8689): Croom S.M. et al., 2009,MNRAS,392,19
3FGL (16,11): Fermi cleanups, Paiano S. et al., 2017,ApJ,851,135
3FGL2 (20,19): Fermi cleanups II, Paiano S. et al., 2019,ApJ,871,162
3HSP (812,981): 3HSP blazars, Chang Y.-L. et al., 2019,A&A,632A,77
3XLSS (24,24): The XXL Survey, Pierre M. et al., 2016,A&A,592A,1P
4FGL1 (15,3): Fermi cleanups, de Menezes R. et al., 2019,A&A,630A,55
4FGL2 (19,23): Fermi cleanups X, de Menezes R. et al., 2020,Ap&SS,365,12
4FGL3 (18,31): Gamma-ray blazars, Peña-Herazo H.A. et al., 2021,AJ,162,177
4FGL4 (23,21): Fermi spectra, Olmo-García A. et al., 2022,MNRAS,516,5702
4LAC (437,379): Fermi AGN v4 DR3, Fermi-LAT collab., 2022,ApJS,263,24
6dF (1752,234): 6dF galaxy survey, Jones D.H. et al., 2009,MNRAS 399,683
6dAGN (0,4433): 6dF AGN, Chen/Zaw/Farrar/Elgamal, 2022,ApJS,258,29
AAOz (1491,1498): AAOmega XXL-South, Lidman C. et al., 2016,PASA,33,1
ABQ (148,155): AllBRICQS bright, Onken C.A. et al., 2022,arXiv:2209.09342v3
AGEL (60,60): Strongly lensed QSOs, Tran K.H. et al., 2022,AJ,164,148
AGES (1774,1774): AGES survey, Kochanek C.S. et al., 2012,ApJS,200,8
AGNEL2 (13,13): VST-Gaia QSO pairs, Agnello A. et al., 2018,MNRAS,475,2086
AGNELA (1,1): SDSS J1433+6007 4-lens, Agnello A. et al., 2018,MNRAS,474,3391
AGNELL (2,3): DES lenses, Agnello A. et al., 2015,MNRAS,454,1260
AKARI (1,1): overlooked luminous quasar, Aoki K. et al., 2011,PASJ,63,457
ALCS (2,2): ALMA lensing clusters, Uematsu R. et al., 2023,arXiv:2301.09275
ALMA (4,2): ALMA hi-z, Decarli R. et al., 2018,ApJ,854,97
ANDIKA (2,2): Hi-z starbursts, Andika I.T. et al., 2020,ApJ,903,34
ANGUIT (1,1): COSMOS lens, Anguita T. et al., 2009,A&A,507,35
ASDA2 (3,10): Dual AGN II, Zhang Y.-W. et al., 2021,AJ,162,289
ASDA3 (0,13): Dual AGN III, Zhang Y.-W. et al., 2021,AJ,162,276
AT20G (59,65): radio quasars, Mahony E.K. et al., 2011,MNRAS,417,2651
ATel (5,6): Astronomers Telegraph posts, http://www.astronomerstelegram.org
ATHENS (86,108): VIPERS AGN SEDs, Pouliasis E. et al., 2020,MNRAS,495,1853
ATLAS (229,269): Mao M.Y. et al., 2012,MNRAS,426,3334
BAHM (24,24): dust-reddened QSOs, Banerji M. et al., 2015,MNRAS,447,3368
BASS2 (53,164): Swift-BAT AGN DR2 catalog, Koss M. et al., 2022,ApJS,261,2
BERGHE (1,1): Pan-STARRS lens, Berghea C.T. et al., 2017,ApJ,844,90
BGGFC (4,4): COSMOS hi-z, Boutsia K. et al., 2018,ApJ,869,20
BLAZZ (0,8): Blazar redshifts, Goldoni P. et al., 2021,A&A,650,A106
BLAZZ2 (5,9): Blazar redshifts, Kasai E. et al., 2023,MNRAS,518,2675
BMCGCS (1,1): Belladitta S. et al., 2019,A&A,629A,68
BMCS (1,1): Blazar at z>6, Belladitta S. et al., 2020,A&A,635L,7
BQLS (11,11): BOSS QSO lenses & pairs, More A. et al., 2016,MNRAS,456,1595
BULLET (16,16): Bullet cluster, Puccetti S. et al., 2020,A&A,634,A137
BZCAT (4,2): BZCAT, Massaro+, 2015, http://cdsarc.cds.unistra.fr/ftp/cats/VII/274
C-COSM (180,180): Chandra COSMOS IDs, Marchesi S. et al., 2016,ApJ,817,34
COOLL (1,1): 25.9" lensed QSO, Martinez M. et al., 2022,arXiv:2209.03972v1
ChaMP (190,186): Trichas M. et al., 2012,ApJS,200,17
DABAST (1,1): Diaz-Santos T. et al., 2018,Sci,362,1034
Dart (26,25): Heavily Obscured QSOs, Hviding R. et al., 2018,MNRAS,474,1955
DDC2 (14,14): variable AGN, De Cicco D. et al., 2019,A&A,627A,33
DEShiz (441,442): DESI z>=5 Quasars, Yang J. et al., 2023,arXiv:2302.01777v1
DESz (1,1): Dark Energy hi-z, Reed S.L. et al., 2015,MNRAS,454,3952
DESQQ (26,26): STRIDES lenses, Anguita T. et al., 2018,MNRAS,480,5017
DESQQ2 (12,12): STRIDES lenses, Treu T. et al., 2018,MNRAS,481,1041
DESQQ3 (2,2): QSO Pair at z=5.66, Yue/Fan/Yang/Wang, 2021,ApJ,921,27
DESQQ4 (4,4): double/quad DESI QSOs, Dawes C. et al., 2022,arXiv:2208.06356
DPeake (683,656): Double-peaked NELGs, Ge J.-Q. et al., 2012,ApJS,201,31
DR7 (6,29): SDSS-DR7 pipeline, Abazajian K.N. et al., 2009,ApJS,182,543
DR7Q (1968,200): SDSS-DR7Q visual, Schneider D. et al., 2010,AJ,139,2360,
data on SDSS, with Table 5 available at journal (AJ) page.
DR12 (10,9): SDSS-DR12 pipeline, Alam S. et al., 2015,ApJS,219,12
DR12Q (252,19): SDSS-DR12Q visual, Paris I. et al., 2017,A&A,597,79
DR14 (23,50): SDSS-DR14 pipeline, Abolfathi B. et al., 2018,ApJS,235,42
DR14Q (1529,1537): SDSS-DR14Q visual, Paris I. et al., 2018,A&A,613A,51
data at https://data.sdss.org/sas/dr14/eboss/qso/DR14Q
DR16 (43243,377608): SDSS-DR16 pipeline, Ahumada R. et al., 2020,ApJS,249,3
data at https://data.sdss.org/sas/dr16/sdss/spectro/redux
DR16Q (717405,395230): SDSS-DR16Q visual, Lyke B. et al., 2020,ApJS,250,8
2 files, data at https://data.sdss.org/sas/dr16/eboss/qso/DR16Q
DR16QN (0,2334): same as DR16Q, using the QuasarNET redshift supplied.
DR17 (1066,1334): SDSS-DR17, Abdurro'uf et al., 2022,ApJS,259,35,
pipeline, includes MaNGA AGN, data in https://data.sdss.org/sas/dr17
DR18 (7,7): SDSS-DR18 pipeline, Almeida A. et al., 2023,arXiv:2301.07688,
data at https://dr18.sdss.org/sas/dr18/spectro/boss/redux/eFEDS
DR18Q (4731,4733): SDSS-DR18Q visual VAC, Merloni A. et al in preparation,
data at https://data.sdss.org/sas/dr18/vac/bhm/efeds_speccomp/v1.4.3
DUALQ (1,1): Dual QSOs HSC, Silverman J.D. et al., 2020,ApJ,899,154
DUHIZ (2,2): DECaLS-UKIRT hi-z, Wang F. et al., 2017,ApJ,839,27
Dusty (11,11): Dusty Starbursts, Rodighiero G. et al., 2019,ApJ,877L,38R
DUz6 (19,19): DESI & UKIRT hi-z, Wang F. et al., 2019,ApJ,884,30
eFEDS (529,530): eFEDS AGN, Liu T. et al., 2022,A&A,661A,5
eHAQ (82,80): Extended High AV, Krogager J.-K., 2016,ApJ,832,49
ELQ-PS (216,215): ELQS on PS1, Schindler J.-T. et al., 2019,ApJS,243,5
ELQS-N (38,38): ELQS in NGC, Schindler J.-T. et al., 2018,ApJ,863,144
ELQS-S (125,125): ELQS in SGC, Schindler J.-T. et al., 2019,ApJ,871,258
ENEAR (4,0): Wegner G. et al., 2003,AJ,126,2268
FISCBA (1,1): HST lens, Fischer/Schade/Barrientos, 1998,ApJ,503,L127
FLES40 (40,0): Salvaged QSOs, Flesch E.W., 2021,MNRAS,504,621
FYNBO (1,1): LiBAL QSO, Fynbo J.P.U. et al., 2020,A&A,634A,111
GAIA1 (21,0): Gaia DR1, Gaia Collaboration et al., 2016,A&A,595A,1
GAIA2 (226,222): Gaia DR2, Gaia Collaboration et al., 2018,A&A,616,A1,
(GAIA data as presented by SIMBAD, http://simbad.cds.unistra.fr/simbad)
GAIA3 (23580,26892): Gaia DR3 QSO candidates, Gaia Collaboration et al.,
2022,arXiv:2206.05681, https://gea.esac.esa.int/archive
GAMA (64,64): Low-mass AGN, Salehirad/Reines/Molina, 2022,ApJ,937,7
GB6hiz (7,6): z>4 blazars, Caccianiga A. et al., 2019,MNRAS,484,204
GEIER (1,1): Geier S.J. et al., 2019,A&A,625L,9
GGLS (3,4): Gaia GraL, Krone-Martins A. et al., 2019,arXiv:1912.08977
GL2hiz (2,2): Two lensed hi-z, Desira C. et al., 2022,MNRAS,509,738
GLDD (1,1): Lensed QSO data-driven, Ostrovski F. et al., 2017,MNRAS,465,4325
GLIKMA (28,28): red WISE QSOs, Glikman E. et al., 2018,ApJ,861,37
GLOH (1,1): Grav Lensed Objs HSC, Jaelani A.T. et al., 2021,MNRAS,502,1487
GLRED (1,1): lensed red QSO, Glikman E. et al., 2018,arXiv:1807.05434
GMM1 (1,1): Gaussian Mixture QSO, Wagenveld J.D. et al., 2022,A&A,660A,22
GPQ (199,198): Galactic plane, Fu Y. et al., 2022,ApJS,261,32
GQ (2,2): serendipitous binary, Altamura E. et al., 2020,AJ,159,122
GRAL4 (9,9): Gaia GraL quads, Stern D. et al., 2021,AJ,921,42
GSAC (478,480): GOODS-S AGN, Lyu J. et al., 2022,ApJ,941,191
GUTI (1,1): not a ULX, Gutiérrez C.M., 2013,A&A,549,A81
GZPM (23,23): Gaia zero pm, Heintz K.E. et al., 2020,A&A,644A,17
H-DOGs (16,16): Herschel DOGs, Riguccini L.A. et al., 2019,AJ,157,233
HAQ (2,2): High AV serendipitous, Heintz K.E. et al., 2016,AJ,152,13
HAQC (1,1): High AV in COSMOS, Heintz K.E. et al., 2016,A&A,595,13
Hdots1 (8,5): H-alpha dots, Kellar J.A. et al., 2012,AJ,143,145
Hdots2 (17,18): H-alpha dots II, Salzer J.J. et al., 2020,AJ,160,242
HE2QS (103,103): HeII quasar survey, Schmidt T.M. et al., 2017,ApJ,847,81
HE2QS2 (5,5): HeII HST/COS quasars, Worseck G. et al., 2019,ApJ,875,111
HEINTZ (1,1): dusty absorbed QSO, Heintz K.E. et al., 2018,A&A,615A,43
HETDEX (1144,1169): HETDEX AGN, Liu C. et al., 2022,ApJS,261,24
HIZ7.5 (1,1): QSO z=7.5, Bañados E. et al., 2018,Natur,553,473
HSC (3,3): Low-luminosity QSOs, Niida M. et al., 2020,ApJ,904,89
HSDQ (4,4): z~5 quasars, Shin/Im/Kim/Jiang, 2022,JKAS,55,131
HSTvar (40,40): variable AGN, Pouliasis E. et al., 2019,MNRAS,487,4285
HzQCA (3,3): hi-z QSO cands archive, Yang D.-M. et al.,2022,arXiv:2211.16996
ICECUB (9,11): IceCube spectra, Paiano S. et al., 2021,MNRAS,504,3338
ICRFz (91,113): ICRF quasars, Titov O. et al., 2017,AJ,153,157
IGMCP (10,10): IGM close pairs, Rorai A. et al., 2017,Sci,356,418
IKEDA (1,1): Ikeda H. et al., 2017,ApJ,846,57
ILT1 (20,19): LoTSS quasars, Gloudemans A.J. et al., 2022,A&A,668A,27
IMDS (3,3): IR medium-deep hi-z VII, Shin S. et al., 2020,ApJ,893,45
IMS (1,1): IR medium-deep hi-z, Kim Y. et al., 2015,ApJ,813,35
IMS2 (10,11): IR medium-deep hi-z, Kim Y. et al., 2019,ApJ,870,86
IMS3 (2,2): IR medium-deep hi-z, Kim Y. et al., 2022,AJ,164,114
INAF (1,1): UV bright hi-z, Grazian A. et al., 2020,ApJ,897,94
INAF2 (1,1): radio-loud hi-z, Belladitta S. et al., 2023,A&A,669A,134
INTGRL (9,13): INTEGRAL/IBIS update, Malizia A. et al., arXiv:2301.09999
J1030 (49,49): AGN in J1030 field, Marchesi S. et al., 2021,A&A,656,A117
JERAM (1,1): extremely bright, Jeram S. et al., 2020,ApJ,899,76
JPLUS (24,24): luminous Ly, Spinoso D. et al., 2020,A&A,643A,149
K4K (2,2): K4000 bz, Uwitonze/Nkundabakura/Mutabazi, 2021,IAUS,356,355
KHOR1 (7,6): 3XMM hi-z, Khorunzhev G.A. et al., 2017,AstL,43,135
KHOR2 (11,11): 3XMM hi-z, Khorunzhev G.A. et al., 2019,AstL,45,411
KHOR3 (1,1): X-ray luminous, Khorunzhev G.A. et al., 2021,AstL,47,123
KODQ3 (4,4): KODIAQ DR3, O'Meara J.M. et al., 2021,AJ,161,45
KOVACS (1,1): bright QSO behind Milky Way, Kovács T. et al., 2019,RNAAS,3,3
LAMDR6 (729,761): LAMOST-DR6, pipeline, http://dr6.lamost.org
LAMDR7 (72,74): LAMOST-DR7, pipeline, http://dr7.lamost.org
LAMQ1 (727,666): LAMOST Quasar DR1, Ai Y.L. et al., 2016,AJ,151,24
LAMQ3 (7190,7051): LAMOST Quasar DR3/DR2, Dong X.Y. et al., 2018,AJ,155,189
LAMQ5 (8132,8125): LAMOST Quasar DR5/DR4, Yao S. et al., 2019,ApJS,240,6
LAMQ9 (4882,4892): LAMOST Quasar DR6-DR9, Jin J.J. et al., 2023,ApJS,265,25
LEMON (32,32): 24 Gaia lenses, Lemon C. et al., 2018,MNRAS,479,5060
LEMON2 (25,25): 22 Gaia lenses, Lemon/Auger/McMahon, 2019,MNRAS,483,4242
LEMON3 (52,51): STRIDES lenses etc, Lemon C. et al., 2020,MNRAS,494,3491
LEMON4 (152,152): Gaia lenses etc, Lemon C. et al., 2023,MNRAS,520,3305
LGGS (11,11): M31/M33 area, Massey/Neugent/Levesque, 2019,AJ,157,227
LIDMAN (1,1): SN Host Galaxy redshifts, Lidman C. et al., 2013,PASA,30,1
LIN (1,1): DES lens, Lin H. et al., 2017,ApJ,838,15
LIRAS (169,154): LoCuSS IR AGNs, Xu, L. et al., 2015,ApJS,219,18
LOZAGN (37,10992): Low-redshift AGN, Liu H.-Y. et al., 2019,ApJS,243,21
LSSA (2,1): 2 lenses, Lucey/Schechter/Smith/Anguita, 2018,MNRAS,476,927
LUMIz5 (66,66): Luminous hi-z, Yang J. et al., 2019,ApJ,871,199
LUMQ (1,1): Most luminous quasar, Onken C. et al., 2022,PASA,39,37
M31UV (1,1): UV flare QSO on M31, Meusinger H. et al., 2010,A&A,512,A1
MAGN1 (1,7): MaNGA type-1 AGN, Cortes-Suárez et al., 2022,MNRAS,514,3626
MALS-N (68,67): MALS-NOT QSOs, Krogager J.-K. et al., 2018,ApJS,235,10
MALS-S (150,152): MALS-SALT QSOs, Gupta N. et al., 2022,ApJ,929,108
MC1988 (1,1): Serendipitous hi-z, McCarthy P.J. et al., 1988,ApJL,328,L29
MFJC (52,51): McGreer I.D., Fan X., Jiang L. & Cai Z., 2018,AJ,155,131
MIGHTE (81,81): MIGHTEE faint AGN, Whittam I.H. et al., 2022,MNRAS,516,245
MQ (444049,263199): MILLIQUAS,original data in this catalog,Flesch E.,2023
NBCKDE (3454,3143): Richards G.T. et al., 2009,ApJS,180,67
NBCKv3 (26577,22769): NBCKDE v3, Richards G.T. et al., 2015,ApJS,219,39
NED (8,8): NASA/IPAC Extragalactic Database, https://ned.ipac.caltech.edu
NIRhiz (5,5): Near-IR hi-z, Yang J. et al., 2021,ApJ,923,262
NLTT (1,0): Luyton moving stars, Salim S. & Gould A., 2003,ApJ,582,1011
OBHIZ (1,1): obscured hi-z, Endsley D. et al., 2022,arXiv:2206.00018v2
OBVLA (61,61): obscured VLA-imaged, Patil P. et al., 2020,AJ,896,18
OGLE2 (2,2): OGLE quasars, Kozlowski S. et al., 2019,ApJ,878,115
OVRLAP (5,5): SDSS overlap hi-z QSOs, Jiang L. et al., 2015,AJ,149,188
OzDES2 (1215,1241): OzDES-DR2 QSOs, Lidman C. et al., 2020,MNRAS,496,19
P352-1 (1,1): P352-15, Bañados E. et al., 2018,ApJ,861L,14
PETERS (235,233): photo special, Peters C.M. et al., 2015,ApJ,811,95
PFTS (2,11): blazar spectroscopy, Paiano S. et al., 2020,MNRAS,497,94
PGC (20308,8): Principal Galaxy Catalog, Paturel G. et al., 2003,A&A,412,45
PHILLI (1,0): MERLIN lens, Phillips P.M. et al., 2000,MNRAS,319,L7
PRFhiz (39,39): PR Forests hi-z, Guarneri F. et al., 2021,MNRAS,506,2471
PS1hz (63,63): PAN-STARRS1 hi-z, Bañados E. et al., 2016,ApJS,227,11
PS1hz2 (46,49): PAN-STARRS1 hi-z II, Bañados E. et al., 2023,ApJS,265,29
PS1MAZ (6,6): Mazzucchelli C. et al., 2017,ApJ,849,91M
PS1z66 (1,1): Tang, Ji-Jia et al., 2017,MNRAS,466,4568
PSO (3,3): PAN-STARRS z-dropouts, Venemans B.P. et al., 2015,ApJ,801L,11V
QLSV (23,21): QUEST-La Silla, Sánchez-Sáez P. et al., 2019,ApJS,242,10
QPQ10 (70,70): Quasar pair DB, Findlay J.R. et al., 2018,ApJS,236,44
QQhiz (17,17): hi-z lenses etc, Yue/Fan/Yang/Wang, 2023,arXiv:2303.04357
QUBNIR (16,17): QUBRICS NIR spectra, Cupani G. et al., 2022,MNRAS,510,2509
QUBRF (187,187): QUBRICS PRF, Guarneri F. et al., 2022,MNRAS,517,2436
QUBRIC (91,91): QUBRICS I, Calderone G. et al., 2019,ApJ,887,268
QUBRIX (249,251): QUBRICS II, Boutsia K. et al., 2020,ApJS,250,26
QUBzs (199,217): QUBRICS z many, Cristiani S. et al., 2023,arXiv:2304.00362
RBS (3,3): Laporte N. et al., 2017,ApJ,851,40
Redden (25,25): Reddened QSOs, Temple M.J. et al., 2019,MNRAS,487,2594
REQ4 (6,6): Reionization-Era quasars, Yang J. et al., 2019,AJ,157,236
REQ7 (1,1): Reionization-Era QSO z=7.5, Yang J. et al., 2020,ApJ,897,14
RFhiz (17,17): Random Forests, Wenzl L. et al., 2021,AJ,162,72
RLQ (4,3): Tuccillo D./Gonzalez-Serrano J.I./Benn C.R., 2015,MNRAS,449,2818
RLQhiz (2,2): hi-z RL QSOs, Ighina L. et al., 2023,MNRAS,519,2060
RSG (1,1): Dorn-Wallenstein T.Z. & Levesque E., 2017,IAUS,329,376
S82X (71,75): Stripe 82 AGN, LaMassa S.M. et al., 2019,ApJ,876,50
S82XRQ (8,8): Red Quasars, LaMassa S.M. et al., 2017,ApJ,847,100
SAGE1 (1,1): SAGE IR AGN, Hony S. et al., 2011,A&A,531A,137
SCULPT (2,3): Sculptor X-ray, Arnason R. M. et al., 2019,MNRAS,485,2259
SDLENS (2,2): SDSS Lenses, Williams P.R. et al., 2018,MNRAS,477L,70
SDSSHI (6,6): SDSS hi-z, Jiang L. et al., 2016,ApJ,833,222
SELMAN (1,1): serendipitous, Selman F.J. et al., 2020,AN,341,26
SFM201 (1,1): Schulze S. et al., 2012,A&A,546,20
SHELLQ (33,33): Subaru hi-z, Matsuoka Y. et al., 2018,PASJ,70S,35
SHELQ3 (28,28): Subaru hi-z, Matsuoka Y. et al., 2019,ApJ,883,183
SHELQ4 (69,69): Subaru hi-z, Matsuoka Y. et al., 2022,ApJS,259,18
SHELQS (31,31): SHELLQS hi-z, Matsuoka Y. et al., 2018,ApJS,237,5
SHELz7 (1,1): SHELLQS z=7, Matsuoka Y. et al., 2019,ApJ,872L,2
SMhiz (140,140): Luminous SkyMapper, Onken C.A.+, 2022,MNRAS,511,572
SOLARZ (13,13): AllWISE anomalies, Solarz A. et al., 2020,A&A,642A,103
SPIN18 (1,1): KiDS-SQuaD lens, Spiniello C. et al., 2018,MNRAS,480,1163
SPIN19 (2,2): 2 lensed quasars, Spiniello C. et al., 2019,MNRAS,485,5086
SPIR (23,23): Spitzer IRAC, Ishikawa Y. et al., 2023,arXiv:2304.02085
SQLS (39,32): SDSS DR7 QSO Lens Search, Inada N. et al., 2012,AJ,143,119
SQUAD (13,13): UVES DB DR1, Murphy M.T. et al., 2019,MNRAS,482,3458
SRG1 (2,2): SRG Orbital Observatory 1st, Khorunzhev G.A. et al., 2020,AstL,46,149
SRG2 (4,4): SRG/eROSITA, Dodin A.V. et al., 2020,AstL,46,429
SRG3 (7,7): SRG RTT-150, Bikmaev I.F. et al., 2020,AstL,46,645
SRG4 (4,8): SRG ART-XC AGN, Zaznobin I.A. et al., 2021,AstL,47,71
SRGA (3,8): SRG ART-XC/eROSITA AGN, Uskov G.S. et al., 2022,AstL,48,87
SRGQQ (1,1): SRG/eROSITA lens, Tubín-Arenas D. et al., 2023,arXiv:2304.02499
SSLENS (3,3): South sky lenses, Spiniello C. et al., 2019,MNRAS,483,3888
SUV (22,22): SDSS-ULAS/VHS QSOs, Yang J. et al., 2017,AJ,153,184
SXDF (39,39): Subaru-XMMDF redshifts, Simpson C. et al., 2012,MNRAS,421,3060
SXDS (307,306): Subaru-XMMDF spectra, Akiyama M. et al., 2015,PASJ,67,82
UGC (10,0): UGC Galaxies, Cotton W.D. and Condon J.J., 1999,ApJS,125,409
ULTRA (1,1): Ultraluminous hi-z, Wu, X.-B. et al., 2015,Nature,518,512
UNIONS (14,14): UV-NIR QSO lens, Chan J.H.H. et al., 2022,A&A,659,140
UVQS (435,502): UV QSOs, Monroe T.R. et al., 2016,AJ,152,25
VAHIZ (2,2): VST ATLAS hi-z, Carnall A.C. et al., 2015,MNRAS,451,L16
VAHIZ2 (1,1): bright z>6 QSOs, Chehade B. et al., 2018,MNRAS,478,1649
VAHIZ3 (1,1): VST-ATLAS lens, Schechter P.L. et al., 2018,RNAAS,2b,21
VAQL (11,11): VST-ATLAS QSO systems, Schechter P.L. et al., 2017,AJ,153,219
VARAGN (5,4): GALEX var, Wasleske/Baldassare/Carroll, 2022,arXiv:2205.00547
VCRF (2,4): VLBI ICRF blazars, Jovanovic M. et al., 2023,arXiv:2304.03664
VDES (8,8): VISTA Dark Energy QSOs, Reed S.L. et al., 2017,MNRAS,468,4702
VDES2 (2,2): more VHS-DES quasars, Reed S.L. et al., 2019,MNRAS,487,1874
VIKING (4,4): VIKING IR, Venemans G.A. et al., 2015,MNRAS,453,2259
VIPERS (241,284): VIPERS PDR-2, Scodeggio M. et al., 2018,A&A,609A,84
VMC (34,34): Magellanic IR QSOs, Ivanov V.D. et al., 2016,A&A,588,A93
VMC2 (10,10): Magellanic dusty, Pennock C.M. et al., 2022,MNRAS,515,6046
W2M2 (27,25): WISE-2MASS red QSOs, Glikman E. et al., 2022,ApJ,934,119
WARSAW (3,3): OGLE lens, Kostrzewa-Rutkowska Z. et al.,2018,MNRAS,476,663
WERTZ (1,1): Gaia GraL lens, Wertz O. et al., 2019,A&A,628A,17
WGD (2,2): DES/Gaia lenses, Agnello A. et al., 2018,MNRAS,479,4345
WILLIG (1,1): Williger, G., 2020, p comm., data on LJMU Robotic Telescope
WISEA (31364,0): AllWISE QSO candidates, Secrest N. et al.,2015,ApJS,221,12
WISEHI (72,70): Hi-z QSOs from WISE, Wang F. et al., 2016,ApJ,819,24
WOLF1 (1,0): most ultraluminous QSO, Wolf C. et al., 2018,PASA,35,24
WOLF2 (18,18): hi-z ultraluminous QSOs, Wolf C. et al., 2020,MNRAS,491,1970
WYFH (1,1): z=7.642 quasar, Wang F. et al., 2021,ApJ,907,1
XDQSO (20999,0): SDSS-XDQSO, Bovy J. et al., 2011,ApJ,729,141
XLSS (306,118): Stalin C.S. et al., 2010,MNRAS,401,294
XMM2 (10,10): 2XMM-Newton cross-search, Combi J.A. et al., 2011,Ap&SS,331,53
XMMSMC (6,6): SMC quasars, Maitral C. et al., 2019,A&A,622A,29
XMSS (183,148): Barcons X. et al., 2007,A&A,476,1191
XWAS (489,448): Esquej P. et al., 2013,A&A,557,A123
XXL (57,57): bright X-ray stellar, Fotopoulou S. et al., 2016,A&A,592A,5
YQLF (25,25): deep CFHT QSOs, Yang J. et al., 2018,AJ,155,110
YSZ (0,414): Type 2 QSOs IDd, Yuan/Strauss/Zakamska, 2016,MNRAS,462,1603
z6.51 (1,1): lensed quasar z=6.51, Fan X. et al., 2019,ApJ,870L,11
z6.82 (1,1): radio-loud z=6.82, Bañados E. et al., 2021,ApJ,909,80
z7.02 (1,1): lensed quasar z=7.02, Wang F. et al., 2018,ApJ,869L,9
The citation for the classification (e.g., that the object is a quasar) can
be from either the name or redshift citation. Four-digit numeric citations
can be found in the HMQ (2015,PASA,32,10) references list.
Ref_Redshift
A character code for the literature reference from which the redshift was
taken, using the same rubric as used for the ref_name parameter (q.v.).
RX_Assoc_Prob
This field contains the calculated percent likelihood that the shown
radio/X-ray detection(s) is (are) truly associated with the object. These
values are calculated as described in Flesch & Hardcastle, 2004,A&A,427,387.
QSO_Prob
This field contains the pQSO, the calculated likelihood that this optical
object is a QSO, in percent, based on radio/X-ray association and optical
photometry, plus WISEA analysis where applicable. This is not relevant for
published quasars, but it shows the outcome of the algorithm's calculation.
Any original authors' estimation is not included in this pQSO.
Radio_Name
The identification of the best core radio detection associated with the
quasar candidate, if any.
Xray_Name
This is the identification of the best X-ray detection (i.e., the highest
probability X-ray source associated with the quasar candidate, if any), but
it can also be the identification of a radio lobe, if the radio_name
parameter for the object itself contains the name of a radio lobe.
Radio/X-ray detections come from the following catalogs (and their respective home pages):
FIRST: VLA FIRST survey, 13Jun05 version, https://sundog.stsci.edu
VLA (abbrev. of VLASS1QLCIR): VLASS Quick Look, https://cirada.ca/catalogues
RACS: Rapid ASKAP Continuum Survey, 2021,PASA,38,58, main source file.
RACD: RACS as above, but from their main detection ("Gaussian") file.
ILT: LoTSS (LOFAR Two-metre Sky Survey), 2022,A&A,659,A1, main source file
ILD: LoTSS as above, but from their main detection ("Gaussian") file.
NVSS: NRAO VLA sky survey, https://www.cv.nrao.edu/nvss
SUMSS: Sydney U. Molonglo, http://www.astrop.physics.usyd.edu.au/sumsscat/
MGPS: Molonglo galactic plane, http://www.astrop.physics.usyd.edu.au/mgpscat/
ROSAT catalogs available from http://cdsarc.cds.unistra.fr/cats/IX.htx are:
- IX/28A is 1RXH: ROSAT HRI (high resolution imager)
- IX/30 is 2RXP: ROSAT PSPC (position sensitive proportional counter)
2RXF: https://heasarc.gsfc.nasa.gov/W3Browse/rosat/rospspcftot.html
1WGA: White, Giommi & Angelini, https://heasarc.gsfc.nasa.gov/wgacat/
CXOG: Chandra ACIS source catalog, Wang S. et al., 2016,ApJS,224,40
CXO: Chandra Source Catalog v1.1, https://cxc.harvard.edu/csc
2CXO: Chandra Source Catalog v2, https://cxc.harvard.edu/csc
CXOX: XAssist Chandra source list, https://asd.gsfc.nasa.gov/xassist/
2XMM/2XMMi: XMM-Newton DR3, http://cdsarc.cds.unistra.fr/cat/?IX/41
4XMM: XMM-Newton DR12, https://www.cosmos.esa.int/web/xmm-newton/xsa
XMMSL: XMM-Newton Slew Survey Release 2.0, same attribution as 4XMM
XMMX: XAssist XMM-Newton source list, https://asd.gsfc.nasa.gov/xassist/
2SXPS: Swift X-ray Point Source catalog, https://www.swift.ac.uk/2SXPS
Optical field solutions are calculated from the raw source positions of all
these catalogs (except 2CXO) as described in the author's MORX paper
(2016,PASA,33,52).
Alt_Name_1
The identification of the radio lobe (as indicated by a "2" in the broad_type
parameter) or an additional radio or X-ray identification associated with the
quasar candidate, if any.
Alt_Name_2
An additional identification of the radio lobe (as indicated by a "2" in the
broad_type parameter) or an extra X-ray identification associated with the
quasar candidate, if any.
Class
The HEASARC Browse object classification, based on the information given in
the broad_type parameter.
Contact Person
Questions regarding the MILLIQUAS database table can be addressed to the HEASARC Help Desk.Page Author: Browse Software Development Team
Last Modified: Tuesday, 18-Apr-2023 17:27:44 EDT
- HEASARC Director: Dr. Alan P. Smale
- NASA Official: Phil Newman
- Web Curator: J.D. Myers
- Last Modified: 18-Apr-2023