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— Viorica Hrincu
Having recently drawn a few skycharts (Superclusters & Voids, Sanctuary Project), I was frustrated by the lack of parsable resources for the Constellations. Not being able to find a plain-text parsable definition of the constellation figures proved impossible, I created my own.
Quotes on this page are from my conversation with the folks at Sky & Telescope and IAU.
The figures are based on the set drawn by Alan MacRobert for Sky and Telescope. These figures are used in Sky & Telescope's Pocket Sky Atlas by Roger Sinnott and appear in the Wikipedia entries for each constellation as well as on pages by the International Astronomical Union (IAU).
This file contains all the information you need to draw basic star maps (with name and designation labels) and constellation figures.
The file contains a long header that explains the contents. It has been formatted to be friendly to UNIX-style command-line tools — grep away!
This is the most complete (and self-contained) sky constellation dataset of its kind.
All stars in the Yale Bright Star Catalogue are reported (9,114 entries, see below). Each star has an entry like this
where the fields are
The Yale Bright Star Catalogue has 9,110 star entries. There are four additional entries in my file: HR 9602, HR 4796/4796A, HR 5727/5728 and HR 8799/8799A.
These entries are the consequence of SIMBAD records having more than one HR index value.
Each of the 88 constellations has its figure summarized in a line like this
The line reports the figure as a set of comma-delimited connections, each represented by a start and end point, which are identified by the corresponding star's HR index and its Bayer (or Flamsteed) designation. The thickness (which can be 1, 2 or 3) of the connection line is the middle digit.
For each constellation, each figure line is reported individually.
where the fields are
Piece-wise linear constellation boundaries are reported in conbound_pair lines. These boundaries are taken from https://vizier.cds.unistra.fr/viz-bin/VizieR-3?-source=VI/49/bound_18.
For example, the boundaries for Crux are
where each line reports a boundary line between two (ra,dec) points. The fields are
Each conbound_pair line is followed by a conbound_path line that reports the representation of the line segment along a great circle. This makes for nicer paths on maps using projections such as azimuthal equidistant.
+ added constellation boundaries + now all stars in Yale BSC are reported + records for line points that do not connect fully to a star (there's a gap between the end of the line and a star) are modified with ra/dec offsets + records for line points that are midpoints between two stars are annotated with the HR index of both stars + added shape for Microscopium, which is a wishbone analogous to Telescopium with the bonus that they point at each other + modified shape for Telescopium to be a wishbone by adding connection between alpha and midpoint between delta 1 and 2.
+ magnitude of alpha Com fixed to 4.32 from 5.08, which is the V magnitude reported in SIMBAD. + fixed midpointa 31-o3 (in Cygnus, which was a little off, as can be seen on this map old 3 20.25019 42.5288 31-o3Cyg 7735,7751 new 3.8 20.24253 42.7722 31-o3Cyg 7735,7751 The stars have Simbad V magnitude 3.8 (31 Omi, o1) and 3.98 (31 Cyg, omi2), so the brighter is used. + The second entry for delta Vela had a slightly different ra/de 1.95 8.74506 144.7083 dlt 2Vel ... 5.1 8.74469 144.7003 dlt 2Vel I could not find a reason for this -- tt may be that the second record refers to delta Vel B (delta Velorum is a triple star system: Aa Ab and B). These stars are extremely close to each other so I've changed the second record to point to delta Vel A (same as first record).
The data source for the constellation shapes was provided to be by Roger Sinnott in an in-house format used by Sky & Telescope's sky charting software.
I worked from this file to create edits and correction and provide an updated version of this file here. Unless you're working with the S&T software, you're likely to find the file linked to above more useful.
The shapes of all the constellations and the stars that define the asterisms shown in the image below. I also include all the 110 Messier objects with common names in this map (hollow circles).
The map also shows the galactic equator and the ecliptic. The vernal equinox, summer solstice, autumn equinox and winter solstice occur along the ecliptic at right ascension 0/360 (Pices), 270 (Sagittarius), 180 (Vigo) and 90 (Gemini/Taurus).
Whole-sky star charts are traditionally drawn with 360 right ascention on the left in decreasing order towards 0 on the right.
You can download this file as PNG, SVG or PDF.
If you're interested in more astronomical resources, check out my Universe Superclusters and Voids resource page.
It is not certain that everything is uncertain. —Blaise Pascal
We have already explored how we can mitigate bias caused by confounding variables in observational studies using propensity score (PS) matching (PSM) and propensity score weighting (PSW). However, any statistical model is only as good as its assumptions and, if it is specified incorrectly, it can itself produce biased estimates of the treatment effect.
This month, we explore double robustness, a powerful statistical concept that provides a valuable “safety net” against the risk of an incorrect model. It offers two opportunities, instead of just one, to obtain a valid estimate of the treatment effect — making it possible to draw credible causal inferences from observational data without having to depend on a single set of modeling assumptions.
Kurz, C.F., Krzywinski, M. & Altman, N. (2026) Points of significance: Double Robustness. Nat. Methods 23:868–869.
My cover design on the 7 April 2026 Nature Biotechnology issue shows the dendrogram that represents a cluster of uniquely expressed (or downregulated) genes in human naive stem cells induced from such cells. Within each dendrogram block, the genomic barcode sequence (sampled from Supplementary Table 1) is depicted with a Code 39 barcode. The highlighted barcode is one of those used for cell isolation.
Ishiguro S. et al. A multi-kingdom genetic barcoding system for precise clone isolation (2026) Nature Biotechnology 44:616–629.
Browse my gallery of cover designs.
Celebrate π Day (March 14th) and enjoy the art — but only if you're part of the 5%.
Go ahead, see what you can't see.
Authentic and accurate images of Ishihara's test plates photographed (and lovingly color-corrected) from the 38-plate Ishihara's Tests for Colour Deficiency.
I also provide the position, size, and color of each circle on each test plate.
What immortal hand or eye, could frame thy fearful symmetry? — William Blake, "The Tyger"
This month, we look at symmetric regression, which, unlike simple linear regression, it is reversible — remaining unaltered when the variables are swapped.
Simple linear regression can summarize the linear relationship between two variables `X` and `Y` — for example, when `Y` is considered the response (dependent) and `X` the predictor (independent) variable.
However, there are times when we are not interested (or able) to distinguish between dependent and independent variables — either because they have the same importance or the same role. This is where symmetric regression can help.
Luca Greco, George Luta, Martin Krzywinski & Naomi Altman (2025) Points of significance: Symmetric alternatives to the ordinary least squares regression. Nat. Methods 22:1610–1612.
Fuelled by philanthropy, findings into the workings of BRCA1 and BRCA2 genes have led to groundbreaking research and lifesaving innovations to care for families facing cancer.
This set of 100 one-of-a-kind prints explore the structure of these genes. Each artwork is unique — if you put them all together, you get the full sequence of the BRCA1 and BRCA2 proteins.