#pipescript for UT April 7th, 2015 (~/mar15/38/)
#started by dewitt at summit

date= 15.0407
slitpa = 180.
fitsdir=archive

posfile=satscan2012.pos

######################
PI=Greathouse
PID=2015A048
######################

weather = variable over the night with light clouds coming and going
objtype=target

shift=false
weight=false
subsky=true
skyint= 1 3
sumscan=false

#slitrot=-0.05

longslit

#1246.452 right most line of the ch4 triplet on left
bounce=0.2
wno0 =   1247.5961
jup.7500
jup.7501
jup.7502

crossdisp
#jup.7503.hd:waveno0 = 1248
#1246.452, rtmost in 4th order
wno0 =   1247.029
hrr=9.801
jup.7503
jup.7504
bounce=0
jup.7505
bounce=0.2
jup.7506
jup.7507

#adjusted the echelle before jup.7508
#1246.452, rtmost in 3rd order
wno0 =   1247.692
hrr=9.801
jup.7508

longslit
#slitrot=-0.05
wno0 =   1247.535
jup.7509

#1938
# narrow line right of double blend in center is 1937.9480
wno0 =   1936.994
jup.7510
jup.7511

#1248
wno0 =   1247.515
jup.7512

crossdisp
#line 1246.452,4
wno0 = 1247.585
hrr=9.882
bounce=0.2
jup.7513
jup.7514
jup.7515
jup.7516
jup.7517

longslit
#slitrot=-0.05
#1246.452 right most line of the ch4 triplet on left
wno0 =   1247.484
jup.7518
jup.7519
jup.7520

#jup.7521.hd:instmode= hi-med
crossdisp
#line 1246.452,3
wno0 = 1247.585
hrr=9.8831
bounce=-0.2
jup.7521
jup.7522
jup.7523
jup.7524
jup.7525
jup.7526
jup.7527
jup.7528
jup.7529
jup.7530
jup.7531
jup.7532

longslit
#slitrot=-0.05
#1246.452 right most line of the ch4 triplet on left
wno0 =   1247.708
jup.7533

crossdisp
#line 1246.452 3
wno0 =   1247.587
hrr=9.881
jup.7534
jup.7535
jup.7536

longslit
#slitrot=-0.05
#1246.452 right most line of the ch4 triplet on left
wno0 =   1248.142
bounce=0.2
jup.7537
jup.7538
jup.7539
jup.7540

crossdisp
#line 1246.452 3
hrr=9.882
wno0 =   1247.585
jup.7541
jup.7542
jup.7543
jup.7544
jup.7545
jup.7546
jup.7547
jup.7548
jup.7549
jup.7550

longslit
#slitrot=-0.05
wno0=1247.690
jup.7551
jup.7552

crossdisp
wno0=1247.591
hrr=9.884
jup.7553

######################
PI=Guerlet
PID=2015A017
######################

objtype=target

#Saturn

longslit
#slitrot=-0.05
#1938 cm-1 med
#Used narrow line right of double blend in center is 1937.9480
wno0=1936.834
sat.7554

#539.5 cm-1 med
#Strong line on far right hand side is 539.577
wno0=539.330
sat.7555

#586.5 cm-1 med
#left hand line of the two middle weak lines is 586.2059
wno0=586.430
sat.7556

#730 cm-1 med
#used 730.5313
wno0=730.099
sat.7557

#818.5 cm-1 med
#3rd line from right is 818.7125
wno0=818.732
sat.7558

#773 cm-1 med
#
wno0=773.007
sat.7559
sat.7560

######################
PI=Hinkle
PID=2015A043
######################

##########################################################
##########moving on To Sak object and then Nova##########
########################################################
#

shift=true
weight=true
subsky = true
longslit

#slitrot=-0.06

#used 770.848 (03 on top of ozone)
wno0=772.9376

objtype=calibration

sumspec=pal.773
pal.7563
pal.7562
pal.7561
storesum

objtype=target

bounce=0.2
sumspec=sak.773
sak.7564
sak.7565
sak.7566
sak.7567
sak.7568
sak.7569
sak.7570
sak.7571
sak.7572
sak.7573
sak.7574
sak.7575
sak.7576
sak.7577
sak.7578
sak.7579
storesum

#After dividing by the first set of Palas specttra i think is see a fairly 
#broad C2H2 R(17) absorption feature doppler shifted about 0.31 to the blue.
#I might surmise that i see an HCN R(19) line emission with a doppler 
#shift of 90.2 to the blue.  And then I might go far as to suggest that we 
#don't see much at the other lines c2h2 R(18) and HCN R(19) because given 
#their spacing the emission from HCN is filling in the absorption from the
#c2h2 feature.  I'm guessing the ortho to para ratio should hold for c2h2
#and that we should expect a very weak R(18). 

#this was at avery low airmass so probably a bad match
#also we had a guider going, but realized in middle of file that non siderial
#rates weren't entered into the guider so we were drifting pretty bad.
#Pull what you can from this, but I think the division from the first set of
#files is really nice.
pal.7580    

########################
PI=Engineering
PID=2015A999
########################

objtype=target

#Okay, as a present to Curtis we are trying to get a spectrum of a Nova.  A 
#buddy of his let us know about a really bright one 4.4 in V so we are going to look for both continuum and H I emission at 808.  Fingers crossed.
#

#808 cm-1 in medium mode
#used narrow water line in middle of tripplet in the middle of the setting. 808.036
wno0=808.351
pal.7581

wno0=808.429
sumspec=nova.808
nova.7582
nova.7583
nova.7584
nova.7585
storesum

#trying now at 884 cm-1
#used strong line which is water at 887.221
wno0=887.053
pal.7586

wno0=887.107
sumspec=nova.884
nova.7587
nova.7588
nova.7589
nova.7590
nova.7591
nova.7592
nova.7593
nova.7594
nova.7595
storesum

end