Scott Virtes: PMDO Survey: Target Variables

Scott Virtes: Astronomy : PMDO Survey Target Variables

Here is a list of variables I've attempted to observe in the PMDO images & data. I am still going through the last few variable star Name Lists, and I keep finding more targets to add. Meanwhile, I've split this list into two parts: Target Variables (period >5 days) and Short Period Variables (period <5 days). The short period ones are listed only because they may show up at different brightnesses on different plates, but with one data point per night, no real study of them is possible.

This list is sorted by Right Ascension.

391 Rows found.
Showing 0 to 49.

ID	Name	GSC	Type	Range	Period	Data	Red Mag.	Notes
FIRST -- previous 50 -- next 50 -- LAST
001V1	RR Psc	none	M	12.1-16	270.6	A/-/F
002V1	DV Psc	0008-0324	E/RS	10.6-11.1	-	-/C/N
003V1	V Psc	0009-0487	UV:	11-12 V	-	-/-/-
004V1	CD Psc	0009-0521	SRD:	9.8-10	-	-/C+/N
-	NSV 15113	0016-1423	E:	5.7-9 V	-	-/-/-
010V1	UY Psc	0026-0257	SRD	8.8-9.2	80	-/-/-
011V1	AR Psc	0027-0157	XI+RS	8.2-9.1	-	-/-/D
013V1	AY Psc	none	nova-like	15.2-16.6 p	irreg	-/-/-
-	AA Psc	0033-0605	LB	10.9-11.2 V	-	-/-/-	9.8	low range, and at S edge of images
-	TT Psc	0043-0934	SRB	10.9-13 p	144.8	-/-/-	10.4
017VS09	CGCS 313	0043-0025	-	---	-	-/C/-	11.1
-	DX Cet	0052-1490	DSCT	7-7.2	-	-/C/-
-	BR Cet	U2:0900-00611781	flare	14.3-16.4 p	-	-/-/N	16.4
-	EF Cet	0053-1224	LB:	12.1-12.5 Hp	-	-/N/N
023V1	IRAS 02568+0547	0054-0555	-	---	-	B/C/-	11.7
-	EK Cet	0062-1248	BY:	11.6-12 Hp	-	-/-/N
-	CGCS 6064	U2:0900-00850364	-	---	-	-/-/-	12.2
029V1	V1083 Tau	none	M	6-7.4	-	B/B/F
-	V1191 Tau	0071-0544	M	11.1-16 V	-	-/B/N
032V1	XY Tau	0079-0253	M	12.4-16	206	C/-/D
034V1	EV Tau	none	M	12-16	-	-/-/A
-	CGCS 657	0080-0035	-	---	-	-/B-/-	10.3
-	V1145 Tau	0081-1820	SRC:	6.9-7.1 Hp	-	-/C/N
035V1	BW Tau	none	galaxy	13.7-16.4	-	-/-/D		Seyfert galaxy 3C 120
-	V1152 Tau	0095-0944	SRB:	8.7-9.2 Hp	-	-/B+/N
-	BY Tau	none	I	14.1-15 p	-	-/-/N		IRAS 04389+0450
036V1	BZ Tau	0095-0070	SR	13.7-15.8 p	400	C/C/C
-	NSV 16181	0096-0602	UV:	13-13.7 p	-	-/-/-
-	GO Ori	none	RR	14.2-15.4 p	-	-/-/-
038V1	-	0097-0955	-	13.2--	-	A/C/-
039V1	DG Ori	none	M	13-16	450	C/-/C
-	CGCS 859	0106-0126	-	---	-	-/C/-	11
-	V1367 Ori	0108-2419	LB	8.6-8.8 Hp	-	-/C/N
041V1	-	0108-0868	-	---	-	A/-/-
-	V1368 Ori	0112-1704	SRA	9.7-10 Hp	-	-/C/N
042V1	V0435 Ori	0113-1060	SRA	12.5-14.5 p	188	A/B/C
-	V1015 Ori	none	RR:	14-15 p	-	-/N/-
043V1	RT Ori	0126-0161	SRB	9.7-11.8 p	321	-/C/D		CGCS 988
043V2	BN Ori	0126-0781	INSB	8.8-13.9 p	-	-/C/D
044V3	-	0127-1011	-	13.3--	-	C/C/-
044V2	V0520 Ori	0127-0715	LB	11.7-13.3 p	-	A/-/C
044V1	FQ Ori	none	M	12-16 p	276	A/-/A
-	CGCS 1040	0123-0805	-	---	-	-/B/-	10.6
-	V0661 Ori	U2:0900-01935986	IS:	15-16.5 p	-	-/-/N	13.3
-	CGCS 1064	0124-0611	-	---	-	-/C/-	12	Pos from Aladin, CGCS off a bit
-	V1623 Ori	0128-1121	SRA	11.7-12.5 V	-	-/C/N
046V1	alpha Ori	0129-1873	SRC	0-1.3 V	2335	-/F/N
046V2	V1201 Ori	none	*	13-14.1 V	-	-/-/N
-	CGCS 1145	0142-0358	-	---	-	-/N/-	9.5	Pos from Aladin
047V1	V1259 Ori	none	M	6.04-8.27 K	-	-/-/F
FIRST -- previous 50 -- next 50 -- LAST

About the columns:

ID: I give stars from each survey I work with a unique ID. Since I'm in the middle of adding a ton of new targets, these numbers are a mess right now.
GSC: usually the Guide Star Catalog (1.2) identifier; may also have a USNO A2.0 (U2) or USNO B1.0 (UB) identifier here.
Red mag: the red magnitude. I've found that the PMDO camera's color response is similar to the USNO A2.0 red magnitudes, so these are given here.
Data: this is a ranking of the types and quality of data I've found. It is in 3 parts: Image/Curve/PCurve, where:
- Image: If I have tried to get a time-series image, I rate its quality here (A to F)
- Curve: If I have tried to graph a light curve from PMDO data, I rate its quality here (A to F)
- PCurve: If Steve has a light curve on the PMDO website, I rate its quality here (A to F), or N for stars not on his list yet

Now, the curve ratings are subjective, but here's my guideline:

A = good density of points, at least one full cycle clearly shown
B = good density of points, most of a cycle shown
B- = most of a cycle shown, needs more points
C = a scatter with a suggestion of variation
D = too few points
F = no data at all - this can happen if the GSC entry is listed as a non-star, or for other reasons

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The text contents of this page are Copyright 2003-2004 by Scott Virtes.
The data is generated by the PMDO Survey, Steve Chambers.