— GALLERY · MMXXVI

Pictures made
with 1snob AstroRoom.

Thirty-four photographs, each restacked from public archive data. Each one carries its band, its instrument, its integration time, and a recipe identifier. Every plate has a Merkle root on file — the picture is no longer just a picture.

— PORTRAITS · BARNARD 33

The Horsehead, twelve ways.

The same target — Barnard 33 — developed under twelve different recipes and band combinations. Same FITS source, same crop. Different decisions about colour, stretch, and which photons get the spotlight.

Horsehead — DSS H-α + Blue + 2MASS J composite
H-α + Blue + J
Horsehead — DSS Blue blues_r colormap
DSS · Blues_r
Horsehead — WISE 12µm + 2MASS K + DSS Blue
WISE12 + K + Blue
Horsehead — DSS pure greyscale photometric
DSS · Greyscale
Horsehead — 2MASS J viridis colormap
2MASS J · Viridis
Horsehead — IR + optical + J composite
IR + Optical + J
Horsehead — WISE 12µm hot colormap
WISE 12µm · Hot
Horsehead — WISE 3.4µm magma colormap
WISE 3.4µm · Magma
Horsehead — H-alpha pink stretch
H-α · Pink
Horsehead — DSS optical broadband
DSS · Optical
Horsehead — deep DSS exposure
DSS · Deep
Horsehead — DSS H-α pink stretch
H-α · Soft pink
— COMPOSITES · BARNARD 33

Four final renders.

Beyond the recipe matrix above, four masters that earned the wall — the Horsehead taken from study to publication.

Horsehead master stackB33 master
DSS H-α + Blue masterMaster stack

The published master.

The plate the room refers back to. Sixteen frames stacked, the dust lane reading red against the IC 434 emission.

Horsehead — deep DSS stackB33 deep
DSS · deep stackProcess

The deep DSS.

The same target driven harder on the stretch. The faint outer dust extends visibly past where the canonical crop ends.

Horsehead — false-colour compositeB33 false
3-band false colourRecipe

The false-colour.

Three bands run through one of the warm-edge palette family recipes. The silhouette is the same; the temperature reads differently.

Horsehead — ultimate compositeB33 ultimate
Multi-band ultimateRecipe

The ultimate composite.

The composite the team kept after argument — narrowband H-α driving the silhouette, near-IR underneath for the dust geometry, optical broadband as the whisper.

Sgr A* — Gabriela Mistral tribute compositeSgr A* · Mistral
Sgr A* · multi-bandTribute

For Gabriela Mistral.

A tribute composite of the galactic centre, dedicated to the Chilean poet who wrote about the night sky as if it were a familiar room. Same FITS sources as the standard Sgr A* master; different recipe.

— THIRTY OBJECTS

From the team
and the early community.

Thirty individual targets. Filter by band, scroll the grid, click any plate to open its provenance.

M31 — Andromeda multiband compositeM31
DSS · 2MASS · GALEX · WISEComposite

Andromeda, six ways.

The same galaxy in six wavelengths — optical red, optical blue, near-IR, ultraviolet, mid-IR, and a chosen RGB composite. Same dust, different witnesses.

M16 — Pillars of Creation, HSTM16
HST · WFC3Optical

Pillars of Creation.

The classic Hubble pillars, restacked from the public archive. The hottest star in the cluster is what's eating the columns from above; the youngest are still forming inside them.

M45 — The Pleiades, DSS + 2MASS compositeM45
DSS + 2MASSComposite

The Pleiades.

Reflection nebulosity in the seven sisters' bow shock. The cluster is moving, fast enough that the dust looks like wake.

The Crab — pulsar wind nebula radio synchrotronCrab
Radio · 1.4 GHzRadio

The pulsar's wind.

Synchrotron radiation from the supernova remnant of 1054. The yellow knot at the centre is the corpse of the star; it ticks every thirty-three milliseconds.

Carina Nebula — NGC 3372, HSTNGC 3372
HST · WFC3Optical

The Carina Nebula.

The luminous blue variable Eta Carinae lives inside the bright knot. It nearly went supernova in the 1840s and is still deciding whether to finish the job.

Centaurus A — NGC 5128 in X-rayCen A
Chandra · ACIS-IX-Ray

A galaxy eating itself.

NGC 5128 in X-ray. The dust lane is half a billion years old — a fossil of the merger that formed the present galaxy. The bright nucleus is the AGN feeding the central black hole.

M87 — Chandra X-ray jetM87
Chandra · ACIS-I · 593 ksX-Ray

The jet from a black hole.

Forty-seven Chandra obsids merged into one event file. The jet of M87's central engine, lit in photons that travelled fifty-five million years to reach the chip.

Stephan's Quintet — JWST megastackSQ
JWST · NIRCam + MIRIComposite

Five galaxies, one frame.

A megastack of public JWST exposures. Four of the five are gravitationally bound; one is a foreground impostor that just shares the line of sight.

Sgr A*
Chandra · ACIS-I · 1999 → 2025X-Ray · Time-resolved

Sgr A* across thirty years.

The galactic centre over three decades of Chandra observation, annotated. The flares are real. The orbital tracks are ours.

Cygnus X-1 — multi-band cinema, decade of state transitionsCyg X-1
Multi-band cinemaComposite · Time-resolved

Cygnus X-1, state transitions.

A stellar-mass black hole binary across a decade of state changes. Each frame is a different observation; the colour map is the spectral hardness ratio.

Black Hole top 9 — atlas excerptAtlas
9 recipes × 9 objectsAtlas excerpt

Black Hole top nine.

A condensed atlas. Nine of the most observable black holes in the sky, each in nine of the recipe library's families.

Horsehead Nebula — Barnard 33B33
DSS H-α + 2MASS JComposite

Barnard 33, developed.

Sixteen optical and infrared frames stacked into the iconic silhouette. The dust lane reads red against the IC 434 emission.

Southern Ring Nebula — NGC 3132NGC 3132
HST · WFC3 + JWST · NIRCamOptical + IR

The Southern Ring.

NGC 3132 — a planetary nebula caught in the act of expansion. Two stars at the centre, only one of which is the source of the shell.

Cat's Eye Nebula — NGC 6543NGC 6543
HST · WFPC2Optical

The Cat's Eye.

One of the most structurally complex planetary nebulae known. The concentric shells are episodic mass loss from the dying central star — one shell every fifteen hundred years.

Rosette Nebula — NGC 2237NGC 2237
DSS H-α + BlueOptical

The Rosette.

An H II region around the open cluster NGC 2244. The cluster carved the cavity. The rim glows because it is being ionised by the brightest stars at the centre.

Eagle Nebula — M16 wide fieldM16
HST · WFC3 + DSSOptical

The Eagle, wide.

The Pillars of Creation in their context. The full M16 H II region; the pillars themselves are a small dark feature near the centre.

M51 — Whirlpool GalaxyM51
HST · WFC3Composite

The Whirlpool.

M51 mid-merger with NGC 5195. The grand-design spiral structure is almost certainly enhanced by the gravitational disturbance from the smaller companion.

NGC 4565 — Needle GalaxyNGC 4565
SDSS + 2MASSOptical

The Needle.

An edge-on spiral with a dust lane drawn so straight it looks engraved. Forty million light-years away, in Coma Berenices.

M104 — Sombrero GalaxyM104
HST · ACSOptical

The Sombrero.

An almost edge-on spiral with a bulge so massive it dominates the silhouette. The dust ring is the disc, seen at six degrees of inclination.

M57 — Ring NebulaM57
HST · WFC3Optical

The Ring.

M57 in Lyra. A barrel-shaped shell of ionised gas seen end-on, which is why it reads as a ring. The white dwarf at the centre is what's left of the star.

M42 — Orion NebulaM42
HST · WFC3 + DSSOptical

Orion's nursery.

The closest large stellar nursery, and the first object most people learn to point at without a finder. The Trapezium cluster sits inside the brightest knot.

NGC 7293 — Helix NebulaNGC 7293
HST + Cerro TololoComposite

The Helix.

The closest planetary nebula to Earth. The "cometary knots" along the inner edge are aerodynamic features — the dying star's wind sculpting denser blobs of gas.

30 Doradus — Tarantula Nebula30 Dor
HST + JWST · NIRCamOptical + IR

The Tarantula.

The largest known stellar nursery in the Local Group, in the Large Magellanic Cloud. R136a1 — the most massive known star — sits inside the central cluster.

M33 — Triangulum GalaxyM33
DSS + GALEX + 2MASSComposite

Triangulum.

Third-largest galaxy in the Local Group, behind Andromeda and our own. The pinwheel structure is unusually clean; the H II regions trace the spiral arms.

Eta Carinae — Homunculus Nebulaη Car
HST · WFPC2Optical

Eta Carinae's Homunculus.

The bipolar shell ejected during the Great Eruption of the 1840s. The star at the centre is still alive, still a luminous blue variable, still on track to go supernova at some point.

NGC 6302 — Butterfly NebulaNGC 6302
HST · WFC3Optical

The Butterfly.

A bipolar planetary nebula with a central star at over 200,000 K — among the hottest known. The wings are gas at thousands of degrees, lit by stellar-wind shocks.

M8 — Lagoon NebulaM8
HST · WFC3 + DSSOptical

The Lagoon.

An H II region in Sagittarius with the cluster NGC 6530 at its core. The "hourglass" tornado of gas at the centre is being shaped by a single hot O-type star.

M20 — Trifid NebulaM20
HST + SpitzerComposite

The Trifid.

The "three-lobed" emission nebula, divided by dust lanes that read as silhouettes against the H-α background. The reflection-nebula component above gives the colour gradient.

Veil Nebula — Cygnus LoopVeil
HST · WFC3Optical

The Veil.

A small section of the Cygnus Loop, the fading shock front of a supernova that exploded around 5,000 BC. The filaments are gas being heated as it slams into the surrounding ISM.

M27 — Dumbbell NebulaM27
HST · WFC3Optical

The Dumbbell.

M27 in Vulpecula. A planetary nebula about 1,360 light-years away, expanding at thirty kilometres a second. The shell is more or less spherical; the apparent dumbbell shape is projection.

NGC 2024 — Flame NebulaNGC 2024
WISE · 12µm + 2MASSComposite · IR

The Flame Nebula.

A star-forming region in Orion, dust-obscured in optical but luminous in mid-IR. The young stars carving out the cavity at the centre would be hidden without the longer wavelengths.

Mz 3 — Ant NebulaMz 3
HST · WFPC2Optical

The Ant Nebula.

A bipolar planetary nebula with a structure so complex the central system is almost certainly a binary. The lobes look symmetric only because we are seeing them edge-on.

Lion Nebula — Sh2-132Sh2-132
Narrowband · H-α + O III + S IIComposite

The Lion.

An H II region in Cepheus shaped by the winds from two Wolf-Rayet stars. The narrowband filter set separates the ionisation states cleanly enough to read like a chemical map.

NGC 1300 — barred spiralNGC 1300
HST · ACSOptical

NGC 1300.

A barred spiral so well organised it became the textbook example. The bar is solid; the arms wind out from its endpoints. Fifty million light-years away, in Eridanus.

Cartwheel Galaxy — JWSTCartwheel
JWST · NIRCam + MIRIComposite

The Cartwheel.

A galaxy hit head-on by another, two hundred million years ago. The collision sent a ring-shaped wave outward; the wave is still expanding at over two hundred kilometres a second, igniting star formation as it goes.

Thirty-four objects plus a Horsehead portrait set is not the limit. The gallery grows with each edition. If you have a target you want to see in the next edition, the room takes requests in the monthly letter.