ASAS J064727+0411.4

varchive ID10000000073069ASAS-SN ID188979201318VSX OID81052Gaia DR33127657036771783808

DCEPSCepheidsclassifierDCEPS✓value-added

Report a problem

α 6ʰ47ᵐ26.5ˢδ +4°11′27.3″l 208.75 · b +1.02BP−RP 1.32

1.3k78185—374—light curves from 4 of 6 surveys · detections in 4

Adopted period

2.3124d

GLS · ASAS-SN g · confidence 1.00

Amplitude

0.461mag

ASAS-SN g · 4% of the light from neighbors

Magnitude

11.93

median · ASAS-SN g

Distance

3,804pc

Bailer-Jones+21 · 3569–4007 pc

E(B−V)

0.772

2D map (CSFD)

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

10 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

Cepheidclassified

99.2%

predicted class

DCEPSCepheid (overtone)

broad · Cepheid · 99.4%

behavior · pulsating · 100.0%

✓ agrees with VSX

VSX · DCEPS

probabilities, likely classes, anomaly scores

likely classes (90 % set)

DCEPSDCEP2 classes · all of them Cepheid

statusclassifiedmodelclf-v2026.09.20

class probability

DCEPS

99.2%

In-class anomaly

0.59

typical

Novelty (out-of-distribution)

0.69

typical

Fold oddity

0.09

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
OGLE-II Iabsent
OGLE-II Vabsent
OGLE-III Iabsent
OGLE-III Vabsent
OGLE-IV I
OGLE-IV V
ASAS-3 V
Hue is the band family in wavelength order; the glyph is the survey.

error bars remove outliers

ASAS-SNSky Patrol v2g 950/1,138 · V 366/400queued

ASAS-SN data table

GaiaDR3G 28/28 · BP 25/25 · RP 25/25queued

Gaia data table

OGLEOCVSIV I 174/174 · IV V 11/11queued

OGLE data table

ASAS-3ACVSV 374/389queued

ASAS-3 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
0.921	0	—
0.222	4×10⁻⁴⁶	#6
0.203	4×10⁻⁴¹	#6
0.137	7×10⁻²⁵	#6
0.117	4×10⁻²⁰	#6

ASAS-SN Vstored peaks

power	FAP	alias of
0.947	1×10⁻²²⁵	—
0.530	6×10⁻⁵⁴	#6
0.490	1×10⁻⁴⁷	#6
0.454	3×10⁻⁴²	#6
0.405	2×10⁻³⁵	#6

OGLE-IV Istored peaks

power	FAP	alias of
0.885	2×10⁻⁷⁴	—
0.818	2×10⁻⁵⁷	#21
0.813	2×10⁻⁵⁶	#21
0.641	2×10⁻³²	#21
0.633	1×10⁻³¹	#21

OGLE-IV Vstored peaks

period d	power	FAP	alias of

ASAS-3 Vstored peaks

power	FAP	alias of
0.871	1×10⁻¹⁵⁸	—
0.716	1×10⁻⁹⁵	#1
0.688	5×10⁻⁸⁸	#1
0.631	1×10⁻⁷⁴	#1
0.618	9×10⁻⁷²	#1

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

power	FAP	alias of
0.725	1×10⁻¹¹	—
0.690	3×10⁻¹⁰	—
0.663	2×10⁻⁹	—
0.650	5×10⁻⁹	—
0.648	6×10⁻⁹	—

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, 6ʰ47ᵐ26.5ˢ +4°11′27.3″ (epoch J2016.0, from Gaia DR3).

ASAS-SNSky Patrol v2verified

verified — name and position agree, or confirmed by the publisher

ASAS-SN ID: 188979201318
separation: matched by ID, not position
blend probability: 97%
blend flux fraction: 3.8% of the light in a 16″ PSF
light curve: 1,316 detections of 1,538 epochs

GaiaDR3position only

by position — within the match radius, no name

Gaia ID: 3127657036771783808
separation: 0.048″
runner-up: 7.246″
candidates: 3
match radius: 0.30″
blend probability: 0.0%
blend flux fraction: 0.0% of the light in a 0.18″ PSF
light curve: 78 detections of 78 epochs

OGLEOCVSposition only

by position — within the match radius, no name

OGLE ID: OGLE-GD-CEP-0066
separation: 0.012″
blend probability: 1.9%
blend flux fraction: 0.0% of the light in a 1.2″ PSF
light curve: 185 detections of 185 epochs

ASAS-3ACVSverified

verified — name and position agree, or confirmed by the publisher

ASAS-3 ID: 064727+0411.4
separation: 3.144″
blend probability: 100%
blend flux fraction: 8.7% of the light in a 25″ PSF
light curve: 374 detections of 389 epochs

Not linked: ZTF, 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: 3127657036771783808
parallax: 0.234 ± 0.015 mas
proper motion: −0.28, −0.34 mas/yr
RUWE: 0.97
Teff: 6,075 [6,003, 6,091] K
log g: 2.35 [2.32, 2.37]
[M/H]: −0.16 [−0.16, −0.16]
radial velocity: 43.8 ± 2.3 km/s

G11.17BP11.72RP10.40

BP−RP1.32

nearest 0.048″ · runner-up 7.246″

Gaia's own verdictSOS

variable flag: VARIABLE
class: CEP · 0.55
classifier: nTransits:5+
SOS period: 2.3123 d · cepheid

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 · 6 of 8 matched

TIC v8TESS input

TIC 234218727

B12.40V11.42

B−V0.99

nearest 0.002″ · no runner-up

2MASSnear-IR

2MASS J06472645+0411272

J9.49H9.07Ks8.91

J−Ks0.58

nearest 0.085″ · no runner-up

CatWISE2020mid-IR

J064726.45+041127.2

W18.80W28.77

W1−W20.03

proper motion: 3, 0 mas/yr
W1 S/N: 88.6

nearest 0.013″ · no runner-up

AllWISEmid-IR

WISE J064726.45+041127.2

W18.76W28.74W38.73W48.18

W1−W20.02

nearest 0.021″ · no runner-up

SkyMapperDR4optical · south

SMSS 1091791535

u14.21v13.15g11.96r11.15i10.89z10.63

g−i1.07

star/galaxy score: 0.98

nearest 0.116″ · no runner-up

Pan-STARRS1DR2optical

PS1 113021018602989555

g11.98r11.26i10.89z10.66y10.56

g−i1.09

detections: 55

nearest 0.037″ · no runner-up

GALEXultraviolet

not observed, or no UV source.

eROSITA eRASS1X-ray

no X-ray source within 10″.

Cluster membership · Hunt & Reffert 2023

Not in Hunt & Reffert (2023).

Interstellar reddening

E(B−V) 0.772 magA_V ≈ 3.1·E(B−V)_SFD = 2.39 magheavily reddened

0 · cleardusty · 0.5+

3D map: not available
2D total (CSFD): 0.772
source: CSFD 2D total (no reliable 3D map)
integrated to: —

VSX, as published

variability flag: 0
maximum: 11.54 (V)
amplitude: 0.41 (V)
period: 2.312167 d
epoch: 2457001.931
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 ASAS J064727+0411.4 at right ascension 101.8602 degrees, declination 4.1909 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	1,316 / 1,538	CSV VOTable
GaiaDR3	G, BP, RP	78 / 78	CSV VOTable
OGLEOCVS	I, V, I, V, I, V	185 / 185	CSV VOTable
ASAS-3ACVS	V	374 / 389	CSV VOTable
All surveysone file, with a survey column	12 series	1,953 / 2,190	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/10000000073069", 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/10000000073069/lightcurve", params={"survey": "asassn"}).json()

# every survey's epochs in one table, with a survey column
csv = requests.get(f"{BASE}/star/10000000073069/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(101.860236, 4.190914, 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(101.860236, 4.190914, 1.0).compute().iloc[0]["lc_asassn"]
live = lsdb.read_hats(root / ptr["collections"]["curves_live"]["path"])
lc_live = live.cone_search(101.860236, 4.190914, 1.0).compute().iloc[0]["lc_asassn"]
# never concatenate across bands or surveys — one trace per (survey, band)

How to cite

Download .bib31 entries

varchivev2026.09.25
this archive
ASAS J064727+0411.4 · varchive_id 10000000073069 · varchive.app/star/10000000073069
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.
OGLEOCVS
public, with the per-class discovery paper requestedwith the OGLE papers for this star's collectionsource archive ↗
- Udalski et al. 2015, AcA 65, 1OGLE-IV: Fourth Phase of the Optical Gravitational Lensing Experiment
- Udalski et al. 2018, AcA 68, 315OGLE Collection of Galactic Cepheids
- Soszyński et al. 2020, AcA 70, 101Additional Galactic Cepheids from the OGLE Survey
This work uses data from the Optical Gravitational Lensing Experiment (OGLE) Collection of Variable Stars.
ASAS-3ACVS
publicsource archive ↗
- Pojmanski 1997, AcA 47, 467The All Sky Automated Survey
- Pojmanski 2002, AcA 52, 397The All Sky Automated Survey. Catalog of Variable Stars. I. 0 h - 6 hQuarter of the Southern Hemisphere
- Pojmanski 2003, AcA 53, 341The All Sky Automated Survey. The Catalog of Variable Stars. II. 6h-12h Quarter of the Southern Hemisphere
- Pojmanski & Maciejewski 2004, AcA 54, 153The All Sky Automated Survey. Catalog of Variable Stars. III. 12h-18h Quarter of the Southern Hemisphere
- Pojmanski & Maciejewski 2005, AcA 55, 97The All Sky Automated Survey. Catalog of Variable Stars. IV. 18h-24h Quarter of the Southern Hemisphere
- Pojmanski et al. 2005, AcA 55, 275The All Sky Automated Survey. Catalog of Variable Stars. V. Declinations 0° - +28° of the Northern Hemisphere
This work uses data from the All Sky Automated Survey (ASAS-3).
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
SkyMapper DR4
crossmatch catalogCC BY 4.0source archive ↗
- Onken et al. 2024, PASA 41, e061SkyMapper Southern Survey: Data release 4
SkyMapper research data are hosted by the Australian National University's data repository.
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

BibTeX · 31 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/10000000073069}},
  note         = {Catalog version v2026.09.25. Star ASAS J064727+0411.4 (varchive_id 10000000073069), retrieved from https://varchive.app/star/10000000073069}
}

@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,
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        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,
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        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},
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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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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,
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        title = "{The ASAS-SN catalogue of variable stars I: The Serendipitous Survey}",
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         year = 2018,
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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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         year = 2019,
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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,
       author = {{Hart}, K. and {Shappee}, B.~J. and {Hey}, D. and {Kochanek}, C.~S. and {Stanek}, K.~Z. and {Lim}, L. and {Dobbs}, S. and {Tucker}, M. and {Jayasinghe}, T. and {Beacom}, J.~F. and {Boright}, T. and {Holoien}, T. and {Ong}, J.~M. Joel and {Prieto}, J.~L. and {Thompson}, T.~A. and {Will}, D.},
        title = "{ASAS-SN Sky Patrol V2.0}",
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        month = apr,
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          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{2015AcA....65....1U,
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        title = "{OGLE-IV: Fourth Phase of the Optical Gravitational Lensing Experiment}",
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 primaryClass = {astro-ph.SR},
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      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2018AcA....68..315U,
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        title = "{OGLE Collection of Galactic Cepheids}",
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 primaryClass = {astro-ph.SR},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018AcA....68..315U},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2020AcA....70..101S,
       author = {{Soszy{\'n}ski}, I. and {Udalski}, A. and {Szyma{\'n}ski}, M.~K. and {Pietrukowicz}, P. and {Skowron}, J. and {Skowron}, D.~M. and {Poleski}, R. and {Koz{\l}owski}, S. and {Mr{\'o}z}, P. and {Ulaczyk}, K. and {Rybicki}, K. and {Iwanek}, P. and {Wrona}, M. and {Gromadzki}, M.},
        title = "{Additional Galactic Cepheids from the OGLE Survey}",
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       adsurl = {https://ui.adsabs.harvard.edu/abs/2020AcA....70..101S},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{1997AcA....47..467P,
       author = {{Pojmanski}, G.},
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       adsurl = {https://ui.adsabs.harvard.edu/abs/1997AcA....47..467P},
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}

@ARTICLE{2002AcA....52..397P,
       author = {{Pojmanski}, G.},
        title = "{The All Sky Automated Survey. Catalog of Variable Stars.  I. 0 h - 6 hQuarter of the Southern Hemisphere}",
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}

@ARTICLE{2003AcA....53..341P,
       author = {{Pojmanski}, G.},
        title = "{The All Sky Automated Survey. The Catalog of Variable Stars. II. 6\^h-12\^h Quarter of the Southern Hemisphere}",
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}

@ARTICLE{2004AcA....54..153P,
       author = {{Pojmanski}, G. and {Maciejewski}, G.},
        title = "{The All Sky Automated Survey. Catalog of Variable Stars. III. 12h-18h Quarter of the Southern Hemisphere}",
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}

@ARTICLE{2005AcA....55...97P,
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}

@ARTICLE{2005AcA....55..275P,
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}

@ARTICLE{2006AJ....131.1163S,
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@ARTICLE{2019AJ....158..138S,
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@ARTICLE{2024PASA...41...61O,
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}

@ARTICLE{2021ApJS..253....8M,
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@ARTICLE{2023ApJ...958..118C,
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}

value-added catalog · 364,427 stars

LAMOST DR11 spectroscopic parameters

browse the catalog ↗

classStartypeF01 LAMOST spectrum1 epoch with a LASP RV

Teff

6,617± 40 K

log g

2.92± 0.06

[Fe/H]

0.20± 0.03

48.57± 5.36 km/s

the catalog

α-element abundance [α/M]: 0.14 ± 0.05
Spectrum S/N (g): 57.3

matched on the star's Gaia DR3 source IDLuo et al. 2026, VizieR Online Data Catalog V/162 (LAMOST DR11) ↗