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#{ SLOANSPEC -- Query the SDSS Spectral Data (DR4) given an image footprint,
# object name, or equatorial position and search size.
procedure sloanspec (what)
string what { prompt = "Image or Object name" }
real ra = INDEF { prompt = "RA of Field (hours)" }
real dec = INDEF { prompt = "Dec of Field (degrees)" }
real sr = 0.25 { prompt = "Search size (degrees)" }
int maxrecords = 100 { prompt = "Max records to return" }
bool display = no { prompt = "Display result?" }
bool interactive = yes { prompt = "Interactive mode?" }
bool autosave = yes { prompt = "Auto-save downloaded data?" }
bool verbose = yes { prompt = "Verbose output?" }
bool ned = no { prompt = "Overlay NED objects?" }
bool grid = no { prompt = "Overlay coord grid?" }
bool download = no { prompt = "Automatically download data?" }
string spectype = "all" { prompt = "Spectra type (qso|galaxy|all)",
enum="qso|galaxy|all" }
real zlow = INDEF { prompt = "Low redshift filter" }
real zhigh = INDEF { prompt = "High redshift filter" }
real size = 15.0 { prompt = "Size of marker (pixels)" }
int color = 207 { prompt = "Marker color" }
int status = 0 { prompt = "Service status code" }
string *llist
begin
string this, img, obj, stab, ttab, mtab, coords, tvcoords, filter
string name, class, oclass, ch, cmd, tnames, imlist, sv_img, stype
bool verb, disp, do_grid, interact, saving, do_ned, found, getdata
int maxrec, mkcolor, n, wcs, siap, count
real szmark, d0, d1, xp, yp, z, x1, x2, y1, y2
real lra, ldec, lsr, sra, sdec, sz, sx, sy
real llx, lly, urx, ury, cx, cy, bsz, z1, z2
string sname, sid, sclass, mission
lra = ra
ldec = dec
this = ""
if (isindef(lra) && isindef(ldec))
this = what
lsr = sr
disp = display
maxrec = maxrecords
szmark = size
mkcolor = color
verb = verbose
interact = interactive
do_grid = grid
do_ned = ned
saving = autosave
stype = spectype
z1 = zlow
z2 = zhigh
getdata = download
sv_img = ""
# Set the environment.
set clobber = yes
set imclobber = yes
if (imaccess (this)) {
img = this
obj = ""
iferr { wcsinfo (this) } then {
error (0, "Cannot determine image coords for `"//this//"'")
} else {
ra = wcsinfo.midx
dec = wcsinfo.midy
size = max (wcsinfo.width, wcsinfo.height) / 60.0
}
} else {
# Assume it's an object name, resolve to coords.
sesame (this)
if (sesame.status < 0)
error (0, "Cannot resolve object `" // this // "'")
lra = sesame.ra
ldec = sesame.dec
lsr = sr
img = ""
obj = this
}
filter = ""
if (stype == "qso") {
filter = "Qso"
} else if (stype == "galaxy") {
filter = "Galaxy"
}
;
# Create temp files.
stab = mktemp ("tmp$stab")
ttab = mktemp ("tmp$ttab")
# Display an image early on so we have something to look at.
if (display) {
if (img == "" || imaccess(img) == no) {
# Display an image from the DSS.
img = mktemp ("tmp$sspec") // ".fits"
sv_img = img
# Get an image of the field if the user didn't supply one.
siap = dalSiapSvc(regResolver("ivo://nasa.heasarc/skyview/dss1","siap"), lra,ldec,lsr,lsr)
count = dalRecordCount(siap)
if (count <= 0)
error (0, "No optical images found")
s1 = dalGetData(siap, 0, osfn(img))
display (img//"[0]", 1, fill+, bpmask="", >& "dev$null")
img = ""
} else {
display (img, 1, fill+, bpmask="", >& "dev$null")
}
}
# Query for the spectra.
if (verb) {
printf ("#\n")
if (img != "")
printf ("# Search Params: Img='%s' RA=%.5f Dec=%.5f SR=%.2f\n",
img, lra, ldec, lsr)
else if (obj != "")
printf ("# Search Params: Obj='%s' RA=%.5f Dec=%.5f SR=%.2f\n",
obj, lra, ldec, lsr)
else
printf ("# Search Position: RA=%.5f Dec=%.5f SR=%.2f\n",
lra, ldec, lsr)
print ("#\n")
}
ssquery (image=img, object=obj, ra=lra, dec=ldec, sr=(lsr * 60.0),
zlow=z1, zhigh=z2, output="STDOUT", maxrec=maxrec, verb-) | \
match (filter, "STDIN", >& stab)
status = ssquery.status
if (ssquery.status < 0) {
error (0, "No results found.")
} else if (img != "") {
wcsinfo (img)
lra = wcsinfo.midx # decimal degrees
ldec = wcsinfo.midy
} else if (obj != "") {
sesame (obj)
lra = sesame.ra # decimal degrees
ldec = sesame.dec
}
#printf("img='%s' obj='%s' ra=%.4f dec=%.4f sr=%.2f\n",img,obj,lra,ldec,lsr)
# See whether we display the image or simply download a cutout of the
# field we want.
if (display) {
coords = mktemp ("tmp$coords")
tvcoords = mktemp ("tmp$coords")
if (img == "" || imaccess(img) == no) {
# # Display an image from the DSS.
# img = mktemp ("tmp$sspec") // ".fits"
img = sv_img
#
# # Get an image of the field if the user didn't supply one.
# siap = dalSiapSvc(regResolver("DSS2R","siap"), lra,ldec,lsr,lsr)
#
# count = dalRecordCount(siap)
# if (count <= 0)
# error (0, "No optical images found")
# s1 = dalGetData(siap, 0, osfn(img))
#
# display (img//"[0]", 1, fill+, bpmask="", >& "dev$null")
fields (stab, "2,3", >& coords)
wcsctran (coords, tvcoords, img//"[0]", "world", "logical",
units="h n", columns="1 2", verb-)
wcsinfo (img//"[0]")
sv_img = img
img = img // "[0]"
if (!interact && imaccess(sv_img//".fits"))
delete (sv_img//".fits", verify-, >& "dev$null")
} else {
# Display the image.
# display (img, 1, fill+, bpmask="", >& "dev$null")
fields (stab, "2,3", >& coords)
wcsctran (coords, tvcoords, img, "world", "logical",
units="h n", verb-)
sv_img = img
wcsinfo (img)
}
if (verb) {
printf ("#\n")
if (img != "")
printf ("# Image: %s\n", img)
else if (obj != "")
printf ("# Object %s\n", obj)
if (img == "" && obj == "")
printf ( "# Search Pos: (%H,%h) Size: %.2fx%.2f arcmin\n",
ra, dec, lsr, lsr)
else
printf ( "# Search Pos: (%H,%h) Size: %.2fx%.2f arcmin\n",
wcsinfo.midx, wcsinfo.midy, wcsinfo.width, wcsinfo.height)
printf ("#\n")
fields (stab, "1-5")
}
# Create local catalog of spectra.
joinlines (tvcoords//","//stab) | match ("-", "STDIN", stop+, >& ttab)
if (access(coords)) delete (coords, verify-, >& "dev$null")
if (access(tvcoords)) delete (tvcoords, verify-, >& "dev$null")
mtab = mktemp ("tmp$mtab")
fields (ttab, "1,2,3", >& mtab)
type (mtab)
tvmark (1, mtab, mark="circle", radii=szmark, col=mkcolor,
lab+, txsize=1)
if (access(mtab)) delete (mtab, verify-, >& "dev$null")
# Overlay the NED objects?
if (do_ned)
nedoverlay (img)
# Draw the coordinate overlay grid?
if (do_grid)
wcslab (img, 1, use-, fill+, overplot+, append+,
labout-, dev="imdy")
if (interact) {
# When verbose we printed the table above, otherwise we want some
# kind of summary visible here.
if (!verbose)
type (ttab)
print ("\n\nIMSSPEC Command Summary:")
print ("b Batch display w/in a box")
print ("d Download spectrum")
print ("i Print Info about spectrum")
print ("n NED Overlay")
print ("r Radio contour overlay")
print ("s Show spectrum")
print ("w WCS Overlay")
print ("q Quit")
printf ("\nCommand? ")
while (fscan (imcur, x, y, wcs, cmd) != EOF) {
# Find nearest point. All other commands will depend on the
# chosen spectrum.
d0 = 999999999.0
d1 = 0.0
found = no
llist = ttab
while (fscan(llist, xp,yp, name,ra,dec,z,class,line) != EOF) {
d1 = sqrt ((xp-x)*(xp-x) + (yp-y)*(yp-y))
if (d1 < d0) {
d0 = d1
sx = xp ; sy = yp
sra = lra ; sdec = ldec
sz = z
sname = name
sclass = class
found = yes
}
}
llist = ""
if (!found)
print ("Error: object not found")
print ("")
switch (cmd) {
case "i": # Show info on spectrum
{ printf ("%s %H %h %.5f %s\n",
sname, (sra*15.), sdec, sz, sclass)
}
case "b": # Get spectrum in the box
{ printf ("Again...")
x1 = x
y1 = y
n = fscan (imcur, x2, y2, wcs, ch)
tnames = mktemp ("tmp$tname")
imlist = mktemp ("tmp$imlist")
tabclip (ttab, "STDOUT", "c1","c2", x1,y1, x2,y2) | \
fields ("STDIN", "1,2,3,9", >& tnames)
# Draw a box around the selected region
printf ("%f %f 101 b\n%f %f 101 b\n", x1,y1,x2,y2) | \
tvmark (1, "", commands="STDIN", lab-, col=200)
print ("\nDownloading images ....")
llist = tnames
while (fscan (llist, x, y, sname, sid) != EOF) {
name = substr (sname, 1, 10) // ".fits"
print (name, >>& imlist)
printf ("%f %f %s\n", x, y, sname) | \
tvmark (1, "STDIN", mark="circle",
radii=szmark, col=205, lab+, txsize=1)
if (imaccess(name) == no)
ssget (sid, name, verbose+)
else
printf ("Image '%s' exists already...\n", name)
}
llist = ""
printf ("Running SPECLOT ....")
specplot ("@"//imlist, label="imname",cursor="dev$null")
if (!saving)
imdelete ("@"//imlist, >& "dev$null")
delete (imlist, verify-, >& "dev$null")
delete (tnames, verify-, >& "dev$null")
gflush
}
case "d": # Get spectrum
{
match (sname, stab) | scan (line)
print (line) | fields ("STDIN","1,7") | scan(sname,sid)
name = substr (sname, 1, 10) // ".fits"
printf ("%f %f %s\n", sx, sy, sname) | \
tvmark (1, "STDIN", mark="circle", radii=szmark,
col=205, lab+, txsize=1)
if (imaccess(name) == no)
ssget (sid, name, verbose+)
}
case "o": # Observation Overlay
{ while (yes) {
printf ("Mission (HST|XMM|Spitzer|Chandra|Rosat)? "
i = scan (mission)
if (i > 0)
break
}
obslogoverlay (img, mission)
}
case "r": # NVSS Radio contour overlay
{ radiooverlay (img)
}
case "n": # NED Overlay
{ nedoverlay (img)
}
case "w": # WCS Overlay
{ wcslab (img, 1, use-, fill+, overplot+, append+,
labout-, dev="imdy")
}
case "s": # SPLOT spectrum
{
match (sname, stab) | scan (line)
print (line) | fields ("STDIN","1,7") | scan(sname,sid)
name = substr (sname, 1, 10) // ".fits"
printf ("%f %f %s\n", sx, sy, sname) | \
tvmark (1, "STDIN", mark="circle", radii=szmark,
col=205, lab+, txsize=1)
if (imaccess(name) == no)
ssget (sid, name, verbose+)
if (imaccess(name) == yes) {
printf ("Running SPLOT on image '%s'....", name)
splot (name)
} else
printf ("Error loading image '%s'\n", name)
if (!saving)
imdelete (name, >& "dev$null")
gflush
}
case "q": # Quit
{ break
}
}
printf ("\nCommand? ")
}
}
} else {
type (stab)
if (getdata) {
spectab (stab, imroot="", verbose+)
}
}
# Clean up
if (access(stab)) delete (stab, verify-, >& "dev$null")
if (access(ttab)) delete (ttab, verify-, >& "dev$null")
ra = INDEF # reset params
dec = INDEF
if (interact && imaccess(sv_img//".fits"))
delete (sv_img//".fits", verify-, >& "dev$null")
end
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