YZ UMi

varchive ID10000000117710ASAS-SN ID8590393236VSX OID142131Gaia DR31727329331262393472

DSCTδ ScuticlassifierHADS✓value-added

Report a problem

α 15ʰ35ᵐ30.4ˢδ +85°37′39.0″l 119.61 · b +30.39BP−RP 0.55

2.2k116————light curves from 2 of 6 surveys · detections in 2

Adopted period

0.09661d

GLS · ASAS-SN g · confidence 1.00

Amplitude

0.501mag

ASAS-SN g · 2% of the light from neighbors

Magnitude

12.24

median · ASAS-SN g

Distance

966pc

Bailer-Jones+21 · 954–978 pc

E(B−V)

0.108

± 0.006 · 3D map (Edenhofer+2024) · 2D map 0.113

Phase-folded light curve

light curve

Period d· adopted

More fold options

zero phase φ₀ fixed zero point

binned median P and 2P side by side odd / even cycles

fold data table

5 more periods

About the periods

Each period's tag gives its relation to the period on screen: same, 2P, P/2, a sidereal or yearly alias, or × and the ratio when unrelated. Click a period to fold at it.

Classification

δ Scuticlassified

99.2%

predicted class

HADShigh-amplitude δ Scuti

broad · δ Scuti · 99.3%

behavior · pulsating · 100.0%

✓ agrees with VSX

VSX · DSCT

probabilities, likely classes, anomaly scores

likely classes (90 % set)

HADSDSCT2 classes · all of them δ Scuti

statusclassifiedmodelclf-v2026.09.20

class probability

HADS

99.2%

In-class anomaly

0.74

typical

Novelty (out-of-distribution)

0.84

unusual — top 20%

Fold oddity

0.05

morphology, not significance

Classifier model card →

About the classifier

Fine class: 23 classes in 9 broad families (broad probability = sum of its fine classes). Behavior: what the light curve does, predicted separately, so a star can be both LPV and IRREGULAR.

The likely classes (a conformal set) contain the true class 90 % of the time and always include the top class. The model abstains when they span more than one broad family or more than four classes.

Light curves

ASAS-SN g
ASAS-SN V
Gaia G
Gaia BP
Gaia RP
Hue is the band family in wavelength order; the glyph is the survey.

error bars remove outliers

ASAS-SNSky Patrol v2g 1,669/2,117 · V 553/670queued

ASAS-SN data table

GaiaDR3G 38/38 · BP 39/39 · RP 39/39queued

Gaia data table

What is drawn

Filled glyph: detection. Open ▽: non-detection, drawn at the limit. Hollow glyph: excluded by the survey's quality flags. The overlay shifts each survey by its median, for display only. MASCARA's magnitudes are its catalog V plus its published differential, mag_delta.

Periodograms

ASAS-SN gstored spectrum

power	FAP	alias of
0.591	2×10⁻³¹⁷	—
0.253	9×10⁻¹⁰⁰	#6
0.235	4×10⁻⁹¹	#6
0.139	2×10⁻⁴⁸	#6
0.109	2×10⁻³⁶	#6

ASAS-SN Vstored peaks

power	FAP	alias of
0.777	3×10⁻¹⁷³	—
0.351	4×10⁻⁴⁶	#6
0.340	4×10⁻⁴⁴	#6
0.314	1×10⁻³⁹	#6
0.297	1×10⁻³⁶	#6

Gaia G+BP+RP (joint)stored peaks (joint fit)FAP is an upper bound

power	FAP	alias of
0.607	1×10⁻¹²	—
0.469	7×10⁻⁸	—
0.440	5×10⁻⁷	—
0.426	1×10⁻⁶	—
0.419	2×10⁻⁶	—

Reading the periodograms

The faint comb marks the survey's known aliases (sidereal day, year, lunar month; for Gaia, its scanning harmonics and known spurious periods): a peak on a comb line is likely an alias. Click a peak to refold.

Identity & links

Links are matched against this star's position, 15ʰ35ᵐ30.4ˢ +85°37′39.0″ (epoch J2016.0, from Gaia DR3).

ASAS-SNSky Patrol v2name only

by name — position not independently checked

ASAS-SN ID: 8590393236
separation: matched by ID, not position
blend probability: 32%
blend flux fraction: 2.2% of the light in a 16″ PSF
light curve: 2,222 detections of 2,787 epochs

GaiaDR3position only

by position — within the match radius, no name

Gaia ID: 1727329331262393472
separation: 0.179″
runner-up: 13.620″
candidates: 2
match radius: 0.30″
blend probability: 0.0%
blend flux fraction: 0.0% of the light in a 0.18″ PSF
light curve: 116 detections of 116 epochs

Not linked: OGLE, ZTF, ASAS-3, MASCARA (outside the footprint, too faint, or no match).

About links

Links come from a survey ID, the name VSX records, or position within a match radius measured per survey. Both catalogs are propagated to J2000.0 before matching.

Blend probability: chance another source is in the survey's PSF. Blend flux fraction: share of the light not from this star.

Full link tables (method, candidates, radii, magnitude checks) are published with each release; see the data guide.

Crossmatch & physical

Gaia DR3

Gaia DR3optical

source_id: 1727329331262393472
parallax: 1.002 ± 0.013 mas
proper motion: 3.03, 5.91 mas/yr
RUWE: 1.06
Teff: 7,083 [7,053, 7,116] K
log g: 3.87 [3.86, 3.88]
[M/H]: −0.82 [−0.86, −0.77]
radial velocity: −40.2 ± 4.4 km/s

G12.06BP12.25RP11.71

BP−RP0.55

nearest 0.179″ · runner-up 13.620″

Gaia's own verdictSOS

variable flag: VARIABLE
class: DSCT|GDOR|SXPHE · 0.89
classifier: nTransits:5+
SOS period: no SOS period

G cleanBP cleanRP clean

Spurious flags are per band: that band's photometry correlates with scan geometry. They do not mean the period is spurious.

Other catalogs · 5 of 8 matched

TIC v8TESS input

TIC 160120432

B12.59V11.96

B−V0.63

nearest 0.002″ · no runner-up

2MASSnear-IR

2MASS J15353035+8537389

J11.41H11.23Ks11.19

J−Ks0.22

nearest 0.031″ · no runner-up

CatWISE2020mid-IR

J153530.43+853739.0

W111.10W211.10

W1−W20.00

proper motion: 3, 9 mas/yr
W1 S/N: 96.3

nearest 0.020″ · no runner-up

AllWISEmid-IR

WISE J153530.40+853739.0

W111.10W211.10W311.12W49.58

W1−W20.00

nearest 0.035″ · no runner-up

Pan-STARRS1DR2optical

PS1 210752338764823825

g12.24r12.10i12.11z12.16y12.15

g−i0.13

detections: 68

nearest 0.039″ · no runner-up

SkyMapperoptical · south

no SkyMapper match (southern sky only).

GALEXultraviolet

not observed, or no UV source.

eROSITA eRASS1X-ray

outside the eRASS1 footprint.

Cluster membership · Hunt & Reffert 2023

Not in Hunt & Reffert (2023).

Interstellar reddening

E(B−V) 0.108 magA_V ≈ 3.1·E(B−V)_SFD = 0.33 magmoderately reddened

0 · cleardusty · 0.5+

3D map: 0.108 ± 0.006
2D total (CSFD): 0.113
source: Edenhofer+2024 3D map (to 1.25 kpc)
integrated to: 966 pc

VSX, as published

variability flag: 0
maximum: 12.15 (R1)
minimum: 12.53 (R1)
period: 0.096605 d
epoch: 2451511.6
spectral type: —
revised: 2026-08-23
status: active

Color–magnitudedereddened (BP−RP)₀ vs absolute G

backdrop: archive stars, dereddened

color–magnitude data table

Notes

Where a 3D dust map is reliable, E(B−V) is the 2D CSFD total scaled by the share of that map's dust in front of the star; elsewhere it is the 2D CSFD total. Both are on the SFD scale: A_V ≈ 3.1·E(B−V)_SFD (≈ 2.74·E(B−V)_SFDon the Schlafly & Finkbeiner 2011 recalibration).

The CMD marker is dereddened the way the backdrop is (A_G = 2.3895 E(B−V), E(BP−RP) = 1.3872 E(B−V)); a star outside the frame is clamped to its edge with an arrow.

Finder & sky

DSS2 color finder chart, 9 arcminutes across, centered on YZ UMi at right ascension 233.8768 degrees, declination 85.6275 degrees. North is up, east is left; the star is at the crosshair in the center. — DSS2 color · 9′ · N up, E left

Elsewhere

About the finder

The crosshair marks the catalog position; a high-proper-motion star may sit off it on the old plates.Explore in Aladin loads Aladin Lite (~1.9 MB).

CDS hips2fits (DSS2 color) · Aladin Lite

Observability

—

altitude

sun: —
transit: —
moon sep.: —

Observable months

JanDec

About observability

Observable: star above 20° and Sun below −18°. The site defaults to Siding Spring; change it with the site button above (your location, an observatory, or coordinates). It stays in your browser.

Observable months: share of each month's dark hours with the star above 20°. Months with no astronomical darkness read as unobservable.

Download the light curves

survey	bands	detections	download
ASAS-SNSky Patrol v2	g, V	2,222 / 2,787	CSV VOTable
GaiaDR3	G, BP, RP	116 / 116	CSV VOTable
All surveysone file, with a survey column	5 series	2,338 / 2,903	CSV VOTable

About the files

Per-survey files contain band, bjd_tdb, mag, mag_err, detected and the survey's own columns, including its native time column (every survey but Gaia). Non-detections and flagged epochs are included and marked.

All surveys stacks the per-survey rows, sorted by bjd_tdb. Filter on survey and band before analysis; magnitudes from different bands are not comparable.

→ TOPCAT / Aladin sends the file over SAMP and needs a running hub (TOPCAT or Aladin Desktop). If the browser blocks it, copy the URL instead.

Access in code

PythonOne star over HTTP

import requests

BASE = "https://api.varchive.app"
row = requests.get(f"{BASE}/star/10000000117710", params={"fields": "core,periods"}).json()
print(row["star"]["adopted_period"], row["star"]["period_source"], row["star"]["is_periodic"])

# one survey's epochs as JSON, or .csv / .vot for a file
lc = requests.get(f"{BASE}/star/10000000117710/lightcurve", params={"survey": "asassn"}).json()

# every survey's epochs in one table, with a survey column
csv = requests.get(f"{BASE}/star/10000000117710/lightcurve.csv", params={"survey": "all"}).text

PythonBulk access with LSDB

import json, lsdb
from upath import UPath

root = UPath("https://data.varchive.app")
ptr = json.loads((root / "catalogs/latest.json").read_text())

# the scalars collection: one row per star, every catalog column
scalars = lsdb.read_hats(root / ptr["collections"]["varchive_scalars"]["path"])
row = scalars.cone_search(233.876753, 85.627511, 1.0).compute()
print(row.iloc[0]["adopted_period"])

# light curves: a nested lc_asassn column, split by band: V in curves_static, g in curves_live
static = lsdb.read_hats(root / ptr["collections"]["curves_static"]["path"])
lc_static = static.cone_search(233.876753, 85.627511, 1.0).compute().iloc[0]["lc_asassn"]
live = lsdb.read_hats(root / ptr["collections"]["curves_live"]["path"])
lc_live = live.cone_search(233.876753, 85.627511, 1.0).compute().iloc[0]["lc_asassn"]
# never concatenate across bands or surveys — one trace per (survey, band)

How to cite

Download .bib22 entries

varchivev2026.09.25
this archive
YZ UMi · varchive_id 10000000117710 · varchive.app/star/10000000117710
AAVSO VSX
public, with attribution requestedsource archive ↗
- Watson et al. 2006, SASS 25, 47The International Variable Star Index (VSX)
This research has made use of the International Variable Star Index (VSX) database, operated at AAVSO, Cambridge, Massachusetts, USA.
GaiaDR3
CC BY-SA 3.0 IGO (ESA Gaia data)source archive ↗
- Gaia Collaboration et al. 2016, A&A 595, A1The Gaia mission
- Gaia Collaboration et al. 2023, A&A 674, A1Gaia Data Release 3. Summary of the content and survey properties
- Eyer et al. 2023, A&A 674, A13Gaia Data Release 3. Summary of the variability processing and analysis
- Riello et al. 2021, A&A 649, A3Gaia Early Data Release 3. Photometric content and validation
- Holl et al. 2023, A&A 674, A25Gaia Data Release 3. Gaia scan-angle-dependent signals and spurious periods
This work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
ASAS-SNSky Patrol v2
public, no registration required (ASAS-SN Sky Patrol)source archive ↗
- Shappee et al. 2014, ApJ 788, 48The Man behind the Curtain: X-Rays Drive the UV through NIR Variability in the 2013 Active Galactic Nucleus Outburst in NGC 2617
- Kochanek et al. 2017, PASP 129, 104502The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0
- Jayasinghe et al. 2018, MNRAS 477, 3145The ASAS-SN catalogue of variable stars I: The Serendipitous Survey
- Jayasinghe et al. 2019, MNRAS 486, 1907The ASAS-SN catalogue of variable stars - II. Uniform classification of 412 000 known variables
- Hart et al. 2023, arXiv:2304.03791ASAS-SN Sky Patrol V2.0
This work made use of data from the All-Sky Automated Survey for Supernovae (ASAS-SN), served through Sky Patrol v2.
2MASS
crossmatch catalogpublicsource archive ↗
- Skrutskie et al. 2006, AJ 131, 1163The Two Micron All Sky Survey (2MASS)
This publication makes use of data products from the Two Micron All Sky Survey.
AllWISE
crossmatch catalogpublicsource archive ↗
- Wright et al. 2010, AJ 140, 1868The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
This publication makes use of data products from the Wide-field Infrared Survey Explorer.
Bailer-Jones+2021 distances
crossmatch catalogCC BY 4.0source archive ↗
- Bailer-Jones et al. 2021, AJ 161, 147Estimating Distances from Parallaxes. V. Geometric and Photogeometric Distances to 1.47 Billion Stars in Gaia Early Data Release 3
TESS Input Catalog
crossmatch catalogpublicsource archive ↗
- Stassun et al. 2019, AJ 158, 138The Revised TESS Input Catalog and Candidate Target List
CatWISE2020
crossmatch catalogpublicsource archive ↗
- Marocco et al. 2021, ApJS 253, 8The CatWISE2020 Catalog
CatWISE uses data from the Wide-field Infrared Survey Explorer, which is a joint project of UCLA and JPL/Caltech.
Pan-STARRS1 DR2
crossmatch catalogpublicsource archive ↗
- Flewelling et al. 2020, ApJS 251, 7The Pan-STARRS1 Database and Data Products
- Chambers et al. 2016, arXiv:1612.05560The Pan-STARRS1 Surveys
The Pan-STARRS1 Surveys have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, and the Pan-STARRS Project Office.
CSFD dust map
dust mapCC BY 4.0source archive ↗
- Chiang 2023, ApJ 958, 118Corrected SFD: A More Accurate Galactic Dust Map with Minimal Extragalactic Contamination
- Schlegel et al. 1998, ApJ 500, 525Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds
Edenhofer+2024 3D dust map
dust mapCC BY 4.0source archive ↗
- Edenhofer et al. 2024, A&A 685, A82A parsec-scale Galactic 3D dust map out to 1.25 kpc from the Sun

BibTeX · 22 entries

@MISC{varchive_v2026_09_25,
  author       = {{varchive}},
  title        = {{varchive}: a multi-survey archive of light curves for {VSX} variable stars},
  year         = {2026},
  howpublished = {\url{https://varchive.app/star/10000000117710}},
  note         = {Catalog version v2026.09.25. Star YZ UMi (varchive_id 10000000117710), retrieved from https://varchive.app/star/10000000117710}
}

@ARTICLE{2006SASS...25...47W,
       author = {{Watson}, C.~L. and {Henden}, A.~A. and {Price}, A.},
        title = "{The International Variable Star Index (VSX)}",
      journal = {Society for Astronomical Sciences Annual Symposium},
         year = 2006,
        month = may,
       volume = {25},
        pages = {47},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2006SASS...25...47W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2016A&A...595A...1G,
       author = {{Gaia Collaboration} and {Prusti}, T. and {de Bruijne}, J.~H.~J. and {Brown}, A.~G.~A. and {Vallenari}, A. and {Babusiaux}, C. and {Bailer-Jones}, C.~A.~L. and {Bastian}, U. and {Biermann}, M. and {Evans}, D.~W. and {Eyer}, L. and {Jansen}, F. and {Jordi}, C. and {Klioner}, S.~A. and {Lammers}, U. and {Lindegren}, L. and {Luri}, X. and {Mignard}, F. and {Milligan}, D.~J. and {Panem}, C. and {Poinsignon}, V. and {Pourbaix}, D. and {Randich}, S. and {Sarri}, G. and {Sartoretti}, P. and {Siddiqui}, H.~I. and {Soubiran}, C. and {Valette}, V. and {van Leeuwen}, F. and {Walton}, N.~A. and {Aerts}, C. and {Arenou}, F. and {Cropper}, M. and {Drimmel}, R. and {H{\o}g}, E. and {Katz}, D. and {Lattanzi}, M.~G. and {O'Mullane}, W. and {Grebel}, E.~K. and {Holland}, A.~D. and {Huc}, C. and {Passot}, X. and {Bramante}, L. and {Cacciari}, C. and {Casta{\~n}eda}, J. and {Chaoul}, L. and {Cheek}, N. and {De Angeli}, F. and {Fabricius}, C. and {Guerra}, R. and {Hern{\'a}ndez}, J. and {Jean-Antoine-Piccolo}, A. and {Masana}, E. and {Messineo}, R. and {Mowlavi}, N. and {Nienartowicz}, K. and {Ord{\'o}{\~n}ez-Blanco}, D. and {Panuzzo}, P. and {Portell}, J. and {Richards}, P.~J. and {Riello}, M. and {Seabroke}, G.~M. and {Tanga}, P. and {Th{\'e}venin}, F. and {Torra}, J. and {Els}, S.~G. and {Gracia-Abril}, G. and {Comoretto}, G. and {Garcia-Reinaldos}, M. and {Lock}, T. and {Mercier}, E. and {Altmann}, M. and {Andrae}, R. and {Astraatmadja}, T.~L. and {Bellas-Velidis}, I. and {Benson}, K. and {Berthier}, J. and {Blomme}, R. and {Busso}, G. and {Carry}, B. and {Cellino}, A. and {Clementini}, G. and {Cowell}, S. and {Creevey}, O. and {Cuypers}, J. and {Davidson}, M. and {De Ridder}, J. and {de Torres}, A. and {Delchambre}, L. and {Dell'Oro}, A. and {Ducourant}, C. and {Fr{\'e}mat}, Y. and {Garc{\'\i}a-Torres}, M. and {Gosset}, E. and {Halbwachs}, J.-L. and {Hambly}, N.~C. and {Harrison}, D.~L. and {Hauser}, M. and {Hestroffer}, D. and {Hodgkin}, S.~T. and {Huckle}, H.~E. and {Hutton}, A. and {Jasniewicz}, G. and {Jordan}, S. and {Kontizas}, M. and {Korn}, A.~J. and {Lanzafame}, A.~C. and {Manteiga}, M. and {Moitinho}, A. and {Muinonen}, K. and {Osinde}, J. and {Pancino}, E. and {Pauwels}, T. and {Petit}, J.-M. and {Recio-Blanco}, A. and {Robin}, A.~C. and {Sarro}, L.~M. and {Siopis}, C. and {Smith}, M. and {Smith}, K.~W. and {Sozzetti}, A. and {Thuillot}, W. and {van Reeven}, W. and {Viala}, Y. and {Abbas}, U. and {Abreu Aramburu}, A. and {Accart}, S. and {Aguado}, J.~J. and {Allan}, P.~M. and {Allasia}, W. and {Altavilla}, G. and {{\'A}lvarez}, M.~A. and {Alves}, J. and {Anderson}, R.~I. and {Andrei}, A.~H. and {Anglada Varela}, E. and {Antiche}, E. and {Antoja}, T. and {Ant{\'o}n}, S. and {Arcay}, B. and {Atzei}, A. and {Ayache}, L. and {Bach}, N. and {Baker}, S.~G. and {Balaguer-N{\'u}{\~n}ez}, L. and {Barache}, C. and {Barata}, C. and {Barbier}, A. and {Barblan}, F. and {Baroni}, M. and {Barrado y Navascu{\'e}s}, D. and {Barros}, M. and {Barstow}, M.~A. and {Becciani}, U. and {Bellazzini}, M. and {Bellei}, G. and {Bello Garc{\'\i}a}, A. and {Belokurov}, V. and {Bendjoya}, P. and {Berihuete}, A. and {Bianchi}, L. and {Bienaym{\'e}}, O. and {Billebaud}, F. and {Blagorodnova}, N. and {Blanco-Cuaresma}, S. and {Boch}, T. and {Bombrun}, A. and {Borrachero}, R. and {Bouquillon}, S. and {Bourda}, G. and {Bouy}, H. and {Bragaglia}, A. and {Breddels}, M.~A. and {Brouillet}, N. and {Br{\"u}semeister}, T. and {Bucciarelli}, B. and {Budnik}, F. and {Burgess}, P. and {Burgon}, R. and {Burlacu}, A. and {Busonero}, D. and {Buzzi}, R. and {Caffau}, E. and {Cambras}, J. and {Campbell}, H. and {Cancelliere}, R. and {Cantat-Gaudin}, T. and {Carlucci}, T. and {Carrasco}, J.~M. and {Castellani}, M. and {Charlot}, P. and {Charnas}, J. and {Charvet}, P. and {Chassat}, F. and {Chiavassa}, A. and {Clotet}, M. and {Cocozza}, G. and {Collins}, R.~S. and {Collins}, P. and {Costigan}, G.},
        title = "{The Gaia mission}",
      journal = {\aap},
     keywords = {space vehicles: instruments, Galaxy: structure, astrometry, parallaxes, proper motions, telescopes, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2016,
        month = nov,
       volume = {595},
          eid = {A1},
        pages = {A1},
          doi = {10.1051/0004-6361/201629272},
archivePrefix = {arXiv},
       eprint = {1609.04153},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016A&A...595A...1G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2023A&A...674A...1G,
       author = {{Gaia Collaboration} and {Vallenari}, A. and {Brown}, A.~G.~A. and {Prusti}, T. and {de Bruijne}, J.~H.~J. and {Arenou}, F. and {Babusiaux}, C. and {Biermann}, M. and {Creevey}, O.~L. and {Ducourant}, C. and {Evans}, D.~W. and {Eyer}, L. and {Guerra}, R. and {Hutton}, A. and {Jordi}, C. and {Klioner}, S.~A. and {Lammers}, U.~L. and {Lindegren}, L. and {Luri}, X. and {Mignard}, F. and {Panem}, C. and {Pourbaix}, D. and {Randich}, S. and {Sartoretti}, P. and {Soubiran}, C. and {Tanga}, P. and {Walton}, N.~A. and {Bailer-Jones}, C.~A.~L. and {Bastian}, U. and {Drimmel}, R. and {Jansen}, F. and {Katz}, D. and {Lattanzi}, M.~G. and {van Leeuwen}, F. and {Bakker}, J. and {Cacciari}, C. and {Casta{\~n}eda}, J. and {De Angeli}, F. and {Fabricius}, C. and {Fouesneau}, M. and {Fr{\'e}mat}, Y. and {Galluccio}, L. and {Guerrier}, A. and {Heiter}, U. and {Masana}, E. and {Messineo}, R. and {Mowlavi}, N. and {Nicolas}, C. and {Nienartowicz}, K. and {Pailler}, F. and {Panuzzo}, P. and {Riclet}, F. and {Roux}, W. and {Seabroke}, G.~M. and {Sordo}, R. and {Th{\'e}venin}, F. and {Gracia-Abril}, G. and {Portell}, J. and {Teyssier}, D. and {Altmann}, M. and {Andrae}, R. and {Audard}, M. and {Bellas-Velidis}, I. and {Benson}, K. and {Berthier}, J. and {Blomme}, R. and {Burgess}, P.~W. and {Busonero}, D. and {Busso}, G. and {C{\'a}novas}, H. and {Carry}, B. and {Cellino}, A. and {Cheek}, N. and {Clementini}, G. and {Damerdji}, Y. and {Davidson}, M. and {de Teodoro}, P. and {Nu{\~n}ez Campos}, M. and {Delchambre}, L. and {Dell'Oro}, A. and {Esquej}, P. and {Fern{\'a}ndez-Hern{\'a}ndez}, J. and {Fraile}, E. and {Garabato}, D. and {Garc{\'\i}a-Lario}, P. and {Gosset}, E. and {Haigron}, R. and {Halbwachs}, J.-L. and {Hambly}, N.~C. and {Harrison}, D.~L. and {Hern{\'a}ndez}, J. and {Hestroffer}, D. and {Hodgkin}, S.~T. and {Holl}, B. and {Jan{\ss}en}, K. and {Jevardat de Fombelle}, G. and {Jordan}, S. and {Krone-Martins}, A. and {Lanzafame}, A.~C. and {L{\"o}ffler}, W. and {Marchal}, O. and {Marrese}, P.~M. and {Moitinho}, A. and {Muinonen}, K. and {Osborne}, P. and {Pancino}, E. and {Pauwels}, T. and {Recio-Blanco}, A. and {Reyl{\'e}}, C. and {Riello}, M. and {Rimoldini}, L. and {Roegiers}, T. and {Rybizki}, J. and {Sarro}, L.~M. and {Siopis}, C. and {Smith}, M. and {Sozzetti}, A. and {Utrilla}, E. and {van Leeuwen}, M. and {Abbas}, U. and {{\'A}brah{\'a}m}, P. and {Abreu Aramburu}, A. and {Aerts}, C. and {Aguado}, J.~J. and {Ajaj}, M. and {Aldea-Montero}, F. and {Altavilla}, G. and {{\'A}lvarez}, M.~A. and {Alves}, J. and {Anders}, F. and {Anderson}, R.~I. and {Anglada Varela}, E. and {Antoja}, T. and {Baines}, D. and {Baker}, S.~G. and {Balaguer-N{\'u}{\~n}ez}, L. and {Balbinot}, E. and {Balog}, Z. and {Barache}, C. and {Barbato}, D. and {Barros}, M. and {Barstow}, M.~A. and {Bartolom{\'e}}, S. and {Bassilana}, J.-L. and {Bauchet}, N. and {Becciani}, U. and {Bellazzini}, M. and {Berihuete}, A. and {Bernet}, M. and {Bertone}, S. and {Bianchi}, L. and {Binnenfeld}, A. and {Blanco-Cuaresma}, S. and {Blazere}, A. and {Boch}, T. and {Bombrun}, A. and {Bossini}, D. and {Bouquillon}, S. and {Bragaglia}, A. and {Bramante}, L. and {Breedt}, E. and {Bressan}, A. and {Brouillet}, N. and {Brugaletta}, E. and {Bucciarelli}, B. and {Burlacu}, A. and {Butkevich}, A.~G. and {Buzzi}, R. and {Caffau}, E. and {Cancelliere}, R. and {Cantat-Gaudin}, T. and {Carballo}, R. and {Carlucci}, T. and {Carnerero}, M.~I. and {Carrasco}, J.~M. and {Casamiquela}, L. and {Castellani}, M. and {Castro-Ginard}, A. and {Chaoul}, L. and {Charlot}, P. and {Chemin}, L. and {Chiaramida}, V. and {Chiavassa}, A. and {Chornay}, N. and {Comoretto}, G. and {Contursi}, G. and {Cooper}, W.~J. and {Cornez}, T. and {Cowell}, S. and {Crifo}, F. and {Cropper}, M. and {Crosta}, M. and {Crowley}, C. and {Dafonte}, C. and {Dapergolas}, A. and {David}, M. and {David}, P. and {de Laverny}, P. and {De Luise}, F. and {De March}, R.},
        title = "{Gaia Data Release 3. Summary of the content and survey properties}",
      journal = {\aap},
     keywords = {techniques: photometric, techniques: spectroscopic, techniques: radial velocities, catalogs, astrometry, parallaxes, Astrophysics - Astrophysics of Galaxies},
         year = 2023,
        month = jun,
       volume = {674},
          eid = {A1},
        pages = {A1},
          doi = {10.1051/0004-6361/202243940},
archivePrefix = {arXiv},
       eprint = {2208.00211},
 primaryClass = {astro-ph.GA},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2023A&A...674A...1G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2023A&A...674A..13E,
       author = {{Eyer}, L. and {Audard}, M. and {Holl}, B. and {Rimoldini}, L. and {Carnerero}, M.~I. and {Clementini}, G. and {De Ridder}, J. and {Distefano}, E. and {Evans}, D.~W. and {Gavras}, P. and {Gomel}, R. and {Lebzelter}, T. and {Marton}, G. and {Mowlavi}, N. and {Panahi}, A. and {Ripepi}, V. and {Wyrzykowski}, {\L}. and {Nienartowicz}, K. and {Jevardat de Fombelle}, G. and {Lecoeur-Taibi}, I. and {Rohrbasser}, L. and {Riello}, M. and {Garc{\'\i}a-Lario}, P. and {Lanzafame}, A.~C. and {Mazeh}, T. and {Raiteri}, C.~M. and {Zucker}, S. and {{\'A}brah{\'a}m}, P. and {Aerts}, C. and {Aguado}, J.~J. and {Anderson}, R.~I. and {Bashi}, D. and {Binnenfeld}, A. and {Faigler}, S. and {Garofalo}, A. and {Karbevska}, L. and {K{\'o}sp{\'a}l}, {\'A}. and {Kruszy{\'n}ska}, K. and {Kun}, M. and {Lanza}, A.~F. and {Leccia}, S. and {Marconi}, M. and {Messina}, S. and {Molinaro}, R. and {Moln{\'a}r}, L. and {Muraveva}, T. and {Musella}, I. and {Nagy}, Z. and {Pagano}, I. and {Palaversa}, L. and {Plachy}, E. and {Pr{\v{s}}a}, A. and {Rybicki}, K.~A. and {Shahaf}, S. and {Szabados}, L. and {Szegedi-Elek}, E. and {Trabucchi}, M. and {Barblan}, F. and {Grenon}, M. and {Roelens}, M. and {S{\"u}veges}, M.},
        title = "{Gaia Data Release 3. Summary of the variability processing and analysis}",
      journal = {\aap},
     keywords = {stars: variables: general, Galaxy: stellar content, catalogs, binaries: eclipsing, starspots, stars: oscillations, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2023,
        month = jun,
       volume = {674},
          eid = {A13},
        pages = {A13},
          doi = {10.1051/0004-6361/202244242},
archivePrefix = {arXiv},
       eprint = {2206.06416},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2023A&A...674A..13E},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...649A...3R,
       author = {{Riello}, M. and {De Angeli}, F. and {Evans}, D.~W. and {Montegriffo}, P. and {Carrasco}, J.~M. and {Busso}, G. and {Palaversa}, L. and {Burgess}, P.~W. and {Diener}, C. and {Davidson}, M. and {Rowell}, N. and {Fabricius}, C. and {Jordi}, C. and {Bellazzini}, M. and {Pancino}, E. and {Harrison}, D.~L. and {Cacciari}, C. and {van Leeuwen}, F. and {Hambly}, N.~C. and {Hodgkin}, S.~T. and {Osborne}, P.~J. and {Altavilla}, G. and {Barstow}, M.~A. and {Brown}, A.~G.~A. and {Castellani}, M. and {Cowell}, S. and {De Luise}, F. and {Gilmore}, G. and {Giuffrida}, G. and {Hidalgo}, S. and {Holland}, G. and {Marinoni}, S. and {Pagani}, C. and {Piersimoni}, A.~M. and {Pulone}, L. and {Ragaini}, S. and {Rainer}, M. and {Richards}, P.~J. and {Sanna}, N. and {Walton}, N.~A. and {Weiler}, M. and {Yoldas}, A.},
        title = "{Gaia Early Data Release 3. Photometric content and validation}",
      journal = {\aap},
     keywords = {catalogs, surveys, instrumentation: photometers, techniques: photometric, Galaxy: general, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2021,
        month = may,
       volume = {649},
          eid = {A3},
        pages = {A3},
          doi = {10.1051/0004-6361/202039587},
archivePrefix = {arXiv},
       eprint = {2012.01916},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...649A...3R},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2023A&A...674A..25H,
       author = {{Holl}, B. and {Fabricius}, C. and {Portell}, J. and {Lindegren}, L. and {Panuzzo}, P. and {Bernet}, M. and {Casta{\~n}eda}, J. and {Jevardat de Fombelle}, G. and {Audard}, M. and {Ducourant}, C. and {Harrison}, D.~L. and {Evans}, D.~W. and {Busso}, G. and {Sozzetti}, A. and {Gosset}, E. and {Arenou}, F. and {De Angeli}, F. and {Riello}, M. and {Eyer}, L. and {Rimoldini}, L. and {Gavras}, P. and {Mowlavi}, N. and {Nienartowicz}, K. and {Lecoeur-Ta{\"\i}bi}, I. and {Garc{\'\i}a-Lario}, P. and {Pourbaix}, D.},
        title = "{Gaia Data Release 3. Gaia scan-angle-dependent signals and spurious periods}",
      journal = {\aap},
     keywords = {methods: data analysis, techniques: photometric, methods: numerical, techniques: radial velocities, astrometry, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics},
         year = 2023,
        month = jun,
       volume = {674},
          eid = {A25},
        pages = {A25},
          doi = {10.1051/0004-6361/202245353},
archivePrefix = {arXiv},
       eprint = {2212.11971},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2023A&A...674A..25H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2014ApJ...788...48S,
       author = {{Shappee}, B.~J. and {Prieto}, J.~L. and {Grupe}, D. and {Kochanek}, C.~S. and {Stanek}, K.~Z. and {De Rosa}, G. and {Mathur}, S. and {Zu}, Y. and {Peterson}, B.~M. and {Pogge}, R.~W. and {Komossa}, S. and {Im}, M. and {Jencson}, J. and {Holoien}, T.~W.-S. and {Basu}, U. and {Beacom}, J.~F. and {Szczygie{\l}}, D.~M. and {Brimacombe}, J. and {Adams}, S. and {Campillay}, A. and {Choi}, C. and {Contreras}, C. and {Dietrich}, M. and {Dubberley}, M. and {Elphick}, M. and {Foale}, S. and {Giustini}, M. and {Gonzalez}, C. and {Hawkins}, E. and {Howell}, D.~A. and {Hsiao}, E.~Y. and {Koss}, M. and {Leighly}, K.~M. and {Morrell}, N. and {Mudd}, D. and {Mullins}, D. and {Nugent}, J.~M. and {Parrent}, J. and {Phillips}, M.~M. and {Pojmanski}, G. and {Rosing}, W. and {Ross}, R. and {Sand}, D. and {Terndrup}, D.~M. and {Valenti}, S. and {Walker}, Z. and {Yoon}, Y.},
        title = "{The Man behind the Curtain: X-Rays Drive the UV through NIR Variability in the 2013 Active Galactic Nucleus Outburst in NGC 2617}",
      journal = {\apj},
     keywords = {galaxies: active, galaxies: nuclei, galaxies: Seyfert, line: formation, line: profiles, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics},
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          doi = {10.1088/0004-637X/788/1/48},
archivePrefix = {arXiv},
       eprint = {1310.2241},
 primaryClass = {astro-ph.HE},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2014ApJ...788...48S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2017PASP..129j4502K,
       author = {{Kochanek}, C.~S. and {Shappee}, B.~J. and {Stanek}, K.~Z. and {Holoien}, T.~W.-S. and {Thompson}, Todd A. and {Prieto}, J.~L. and {Dong}, Subo and {Shields}, J.~V. and {Will}, D. and {Britt}, C. and {Perzanowski}, D. and {Pojma{\'n}ski}, G.},
        title = "{The All-Sky Automated Survey for Supernovae (ASAS-SN) Light Curve Server v1.0}",
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        pages = {104502},
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archivePrefix = {arXiv},
       eprint = {1706.07060},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2017PASP..129j4502K},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2018MNRAS.477.3145J,
       author = {{Jayasinghe}, T. and {Kochanek}, C.~S. and {Stanek}, K.~Z. and {Shappee}, B.~J. and {Holoien}, T.~W.-S. and {Thompson}, Todd A. and {Prieto}, J.~L. and {Dong}, Subo and {Pawlak}, M. and {Shields}, J.~V. and {Pojmanski}, G. and {Otero}, S. and {Britt}, C.~A. and {Will}, D.},
        title = "{The ASAS-SN catalogue of variable stars I: The Serendipitous Survey}",
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         year = 2018,
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       number = {3},
        pages = {3145-3163},
          doi = {10.1093/mnras/sty838},
archivePrefix = {arXiv},
       eprint = {1803.01001},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018MNRAS.477.3145J},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2019MNRAS.486.1907J,
       author = {{Jayasinghe}, T. and {Stanek}, K.~Z. and {Kochanek}, C.~S. and {Shappee}, B.~J. and {Holoien}, T.~W.-S. and {Thompson}, Todd A. and {Prieto}, J.~L. and {Dong}, Subo and {Pawlak}, M. and {Pejcha}, O. and {Shields}, J.~V. and {Pojmanski}, G. and {Otero}, S. and {Britt}, C.~A. and {Will}, D.},
        title = "{The ASAS-SN catalogue of variable stars - II. Uniform classification of 412 000 known variables}",
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        pages = {1907-1943},
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archivePrefix = {arXiv},
       eprint = {1809.07329},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.1907J},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2023arXiv230403791H,
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        title = "{ASAS-SN Sky Patrol V2.0}",
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        month = apr,
          eid = {arXiv:2304.03791},
        pages = {arXiv:2304.03791},
          doi = {10.48550/arXiv.2304.03791},
archivePrefix = {arXiv},
       eprint = {2304.03791},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2023arXiv230403791H},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2006AJ....131.1163S,
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}

@ARTICLE{2010AJ....140.1868W,
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        title = "{The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance}",
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 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2010AJ....140.1868W},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021AJ....161..147B,
       author = {{Bailer-Jones}, C.~A.~L. and {Rybizki}, J. and {Fouesneau}, M. and {Demleitner}, M. and {Andrae}, R.},
        title = "{Estimating Distances from Parallaxes. V. Geometric and Photogeometric Distances to 1.47 Billion Stars in Gaia Early Data Release 3}",
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     keywords = {Catalogs, Galaxy structure, Bayesian statistics, Parallax, Stellar parallax, Photometric parallax, Distance indicators, Astrometry, Markov chain Monte Carlo, Absolute magnitude, 205, 622, 1900, 1197, 1618, 1231, 394, 80, 1889, 10, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies},
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archivePrefix = {arXiv},
       eprint = {2012.05220},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021AJ....161..147B},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2019AJ....158..138S,
       author = {{Stassun}, Keivan G. and {Oelkers}, Ryan J. and {Paegert}, Martin and {Torres}, Guillermo and {Pepper}, Joshua and {De Lee}, Nathan and {Collins}, Kevin and {Latham}, David W. and {Muirhead}, Philip S. and {Chittidi}, Jay and {Rojas-Ayala}, B{\'a}rbara and {Fleming}, Scott W. and {Rose}, Mark E. and {Tenenbaum}, Peter and {Ting}, Eric B. and {Kane}, Stephen R. and {Barclay}, Thomas and {Bean}, Jacob L. and {Brassuer}, C.~E. and {Charbonneau}, David and {Ge}, Jian and {Lissauer}, Jack J. and {Mann}, Andrew W. and {McLean}, Brian and {Mullally}, Susan and {Narita}, Norio and {Plavchan}, Peter and {Ricker}, George R. and {Sasselov}, Dimitar and {Seager}, S. and {Sharma}, Sanjib and {Shiao}, Bernie and {Sozzetti}, Alessandro and {Stello}, Dennis and {Vanderspek}, Roland and {Wallace}, Geoff and {Winn}, Joshua N.},
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archivePrefix = {arXiv},
       eprint = {1905.10694},
 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2019AJ....158..138S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021ApJS..253....8M,
       author = {{Marocco}, Federico and {Eisenhardt}, Peter R.~M. and {Fowler}, John W. and {Kirkpatrick}, J. Davy and {Meisner}, Aaron M. and {Schlafly}, Edward F. and {Stanford}, S.~A. and {Garcia}, Nelson and {Caselden}, Dan and {Cushing}, Michael C. and {Cutri}, Roc M. and {Faherty}, Jacqueline K. and {Gelino}, Christopher R. and {Gonzalez}, Anthony H. and {Jarrett}, Thomas H. and {Koontz}, Renata and {Mainzer}, Amanda and {Marchese}, Elijah J. and {Mobasher}, Bahram and {Schlegel}, David J. and {Stern}, Daniel and {Teplitz}, Harry I. and {Wright}, Edward L.},
        title = "{The CatWISE2020 Catalog}",
      journal = {\apjs},
     keywords = {Astronomy databases, Infrared astronomy, Infrared photometry, Catalogs, 83, 786, 792, 205, Astrophysics - Instrumentation and Methods for Astrophysics},
         year = 2021,
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          eid = {8},
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          doi = {10.3847/1538-4365/abd805},
archivePrefix = {arXiv},
       eprint = {2012.13084},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJS..253....8M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2020ApJS..251....7F,
       author = {{Flewelling}, H.~A. and {Magnier}, E.~A. and {Chambers}, K.~C. and {Heasley}, J.~N. and {Holmberg}, C. and {Huber}, M.~E. and {Sweeney}, W. and {Waters}, C.~Z. and {Calamida}, A. and {Casertano}, S. and {Chen}, X. and {Farrow}, D. and {Hasinger}, G. and {Henderson}, R. and {Long}, K.~S. and {Metcalfe}, N. and {Narayan}, G. and {Nieto-Santisteban}, M.~A. and {Norberg}, P. and {Rest}, A. and {Saglia}, R.~P. and {Szalay}, A. and {Thakar}, A.~R. and {Tonry}, J.~L. and {Valenti}, J. and {Werner}, S. and {White}, R. and {Denneau}, L. and {Draper}, P.~W. and {Hodapp}, K.~W. and {Jedicke}, R. and {Kaiser}, N. and {Kudritzki}, R.~P. and {Price}, P.~A. and {Wainscoat}, R.~J. and {Chastel}, S. and {McLean}, B. and {Postman}, M. and {Shiao}, B.},
        title = "{The Pan-STARRS1 Database and Data Products}",
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       eprint = {1612.05243},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJS..251....7F},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2016arXiv161205560C,
       author = {{Chambers}, K.~C. and {Magnier}, E.~A. and {Metcalfe}, N. and {Flewelling}, H.~A. and {Huber}, M.~E. and {Waters}, C.~Z. and {Denneau}, L. and {Draper}, P.~W. and {Farrow}, D. and {Finkbeiner}, D.~P. and {Holmberg}, C. and {Koppenhoefer}, J. and {Price}, P.~A. and {Rest}, A. and {Saglia}, R.~P. and {Schlafly}, E.~F. and {Smartt}, S.~J. and {Sweeney}, W. and {Wainscoat}, R.~J. and {Burgett}, W.~S. and {Chastel}, S. and {Grav}, T. and {Heasley}, J.~N. and {Hodapp}, K.~W. and {Jedicke}, R. and {Kaiser}, N. and {Kudritzki}, R.-P. and {Luppino}, G.~A. and {Lupton}, R.~H. and {Monet}, D.~G. and {Morgan}, J.~S. and {Onaka}, P.~M. and {Shiao}, B. and {Stubbs}, C.~W. and {Tonry}, J.~L. and {White}, R. and {Ba{\~n}ados}, E. and {Bell}, E.~F. and {Bender}, R. and {Bernard}, E.~J. and {Boegner}, M. and {Boffi}, F. and {Botticella}, M.~T. and {Calamida}, A. and {Casertano}, S. and {Chen}, W.-P. and {Chen}, X. and {Cole}, S. and {Deacon}, N. and {Frenk}, C. and {Fitzsimmons}, A. and {Gezari}, S. and {Gibbs}, V. and {Goessl}, C. and {Goggia}, T. and {Gourgue}, R. and {Goldman}, B. and {Grant}, P. and {Grebel}, E.~K. and {Hambly}, N.~C. and {Hasinger}, G. and {Heavens}, A.~F. and {Heckman}, T.~M. and {Henderson}, R. and {Henning}, T. and {Holman}, M. and {Hopp}, U. and {Ip}, W.-H. and {Isani}, S. and {Jackson}, M. and {Keyes}, C.~D. and {Koekemoer}, A.~M. and {Kotak}, R. and {Le}, D. and {Liska}, D. and {Long}, K.~S. and {Lucey}, J.~R. and {Liu}, M. and {Martin}, N.~F. and {Masci}, G. and {McLean}, B. and {Mindel}, E. and {Misra}, P. and {Morganson}, E. and {Murphy}, D.~N.~A. and {Obaika}, A. and {Narayan}, G. and {Nieto-Santisteban}, M.~A. and {Norberg}, P. and {Peacock}, J.~A. and {Pier}, E.~A. and {Postman}, M. and {Primak}, N. and {Rae}, C. and {Rai}, A. and {Riess}, A. and {Riffeser}, A. and {Rix}, H.~W. and {R{\"o}ser}, S. and {Russel}, R. and {Rutz}, L. and {Schilbach}, E. and {Schultz}, A.~S.~B. and {Scolnic}, D. and {Strolger}, L. and {Szalay}, A. and {Seitz}, S. and {Small}, E. and {Smith}, K.~W. and {Soderblom}, D.~R. and {Taylor}, P. and {Thomson}, R. and {Taylor}, A.~N. and {Thakar}, A.~R. and {Thiel}, J. and {Thilker}, D. and {Unger}, D. and {Urata}, Y. and {Valenti}, J. and {Wagner}, J. and {Walder}, T. and {Walter}, F. and {Watters}, S.~P. and {Werner}, S. and {Wood-Vasey}, W.~M. and {Wyse}, R.},
        title = "{The Pan-STARRS1 Surveys}",
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        month = dec,
          eid = {arXiv:1612.05560},
        pages = {arXiv:1612.05560},
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archivePrefix = {arXiv},
       eprint = {1612.05560},
 primaryClass = {astro-ph.IM},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2016arXiv161205560C},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2023ApJ...958..118C,
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      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1998ApJ...500..525S,
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        title = "{Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds}",
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@ARTICLE{2024A&A...685A..82E,
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value-added catalog · 128,857 stars

SDSS-V DR19 ASTRA spectroscopic parameters

browse the catalog ↗

pipelineaspcapinstAPOGEETelescopeAPO 2.5 m1 visit with a good RV

Teff

6,865± 130 K

log g

3.30± 0.05

[Fe/H]

−0.66± 0.02

−50.79± 0 km/s

the catalog

Abundance pattern[X/H] by element · solar at zero

Metallicity [M/H]: −0.66 ± 0.03
α-element abundance [α/M]: 0.21 ± 0.03
Spectrum S/N: 51.3
Projected rotation v sin i: 16.1 ± 1.5 km/s
Microturbulence: 3.51 ± 1.14 km/s
Carbon [C/M]: 0.22
Nitrogen [N/M]: 0.03

matched on the star's Gaia DR3 source IDSDSS Collaboration et al. 2026, ApJS 285, 9 (DR19) ↗