Search and Retrieval

Q: How to retrieve all of the objects mentioned in a given paper?
A: Any of the search options will return a list of papers. Click on the reference code for the paper in question. This will open a new screen with the title and abstract text (if available), and a link to Retrieve NNN NED Objects ("NNN" is the number of NED objects included in the reference). This will give you a list of all NED objects mentioned in the selected paper.

Q: How to find all of the papers written by a given author?
A: If the author is among the first 20 or so listed for an extragalactic paper, select the Author Name option in the "Literature" menu. This option will open the Search for Abstracts by Author Name screen. Submit the query using the author's last name as input parameter.

Only the first 160 ASCII characters of the author list and article title can be searched or displayed on the results page. Long author lists and long titles are not completely displayed, and author searches will not return papers when the name is not included in the first 160 characters of the author list. Note, however, that NED's abstracts include the full title and author list, so you may use a Text Search to find authors in long author lists.

Q: How can I find QSO 2251+113 without doing a position search?
A: You may use the IAU Format option from the "Objects" menu. This option will open the Search for Object for Given IAU Name screen. You may then submit the query using an IAU-style name as the input parameter.

Q: In the Advanced All-Sky Search page, is it possible to add a filter for the V magnitude of the target?
A: Yes. In the "Photometric Constraints" section of the page, you may choose many different passbands, including Johnson V. These constraints use NED's "Photometry Data Frames". If an object does not yet have photometry available through the Photometry option in the "Data" menu on the home page, it will not be included in a search depending on photometric constraints.

Q: Is there any way to retrieve data concerning velocity dispersions within galaxies, so I can get, for example, the velocity distributions of stars as a function of galaxy morphology?
A: NED does not yet list velocity dispersions for its galaxies. However, you may use the Text Search option to scan NED's titles and abstracts, and LEVEL 5, for papers that contain velocity dispersions.

Q: How to get measured fluxes for my objects using NED?
A: For single objects, you may search NED's photometric database using the Photometry option in the "Data" menu on the home page.

Q: Is there a way to perform a NED search for objects based only on spectroscopic redshifts, and not on redshifts from colors or magnitudes?
A: We adopt spectroscopic redshifts whenever they are available. Sometimes, however, only a photometric redshift is available for an object, or the source of a redshift is not clearly stated in the published paper. In those cases, we flag the redshifts if we know that they are not from spectroscopy. It is still possible, however, for photometric redshifts to slip in unflagged. In cases of doubt, we urge you to go back to the published paper to check the source of the redshifts.

Q: When I use the search for References from the "Literature" menu on NED's home page, why do I sometimes get results referring to papers that are not related to my intended object?
A: The default for this type of search is to return all "related" objects, that is, all objects with the same root name. For example, if you search for NGC 1614, you will also get references for NGC 1614A, NGC 1614:SN 1996D, etc. If you want just the references for a specific object, set the Related object name search? option to No.

Q: Why does a search for M51 return the wrong position?
A: "M51" refers to the pair of galaxies, NGC 5194 and NGC 5195, not just to the larger spiral NGC 5194. The position that NED adopts for M51 is therefore the mean position of the two galaxies. We treat other pairs, triplets, groups, and clusters listed in NED the same way: we adopt mean positions for all the galaxies rather than for just the brightest or for the most centrally-located. Many pairs and triplets in NED have position errors that -- rather than representing the 95% confidence ellipse -- represent half the separation of the objects. The "error ellipse" therefore encloses both/all positions for the member galaxies.

Q: Why doesn't NED provide simple text files containing basic data such as preferred coordinates and redshifts for all objects with available redshifts?
A: The database is updated frequently, thus any such files would be quickly out-of-date, and would no longer represent the current state of knowledge available in NED. In addition to new objects and data that are continuously being integrated into the database, the cross-identifications of incoming sources with existing objects in NED, as well as the selection of the most reliable ("preferred") positions, redshifts and other quantities that appear by default in object queries when there are multiple measurements available, are constantly being refined with improving algorithms and scientific vetting procedures. Also, the NED team is working on database restructuring and a new search engine that will enable users to select what fields are contained in query output tables, for example particular photometric bands from large surveys and derived quantities. (This will be an extension of NED functionality currently available in the service to search for objects by classifications/attributes.) Stay tuned!

Q: What is the difference between Strict and Liberal in the IAU-format search?
A: The IAU names are in the form HHMMSS.d+DDMMd where H = hours of RA D = degrees of DEC M = minutes of RA or DEC S = seconds of RA or DEC + = + or - declination d = decimal numbers.

For example: 2214+3307 would represent: 22h14m +33deg 07' 2214+337 would represent: 22h14m +33.7 deg

The Strict convention understands the input as a truncated version of the coordinates and adds a half decimal to the last digit given in RA and Dec, then searches for all objects within a radius equal to the larger of the half decimal suffixes.

For example: Input: 2214+3307
→ 22h 14m +33deg 7'

Since the range in position is up to 22h 15m +33deg 8' the center position is determined by adding half a decimal to the input position 22h 14.5m +33deg 7.5'
22h 14m 30s +33deg 7' 30"

This position becomes the center of the search circle. Since the center is within 30 sec and 30 arcsec from the input position, the radius of the search should cover the largest distance, in this case 30 seconds of time.

The Liberal convention assumes that the last digit could be either truncated or rounded, and considers the resulting possibilities. NED then searches for all objects within the largest circle containing all the possibilities.

For example: Input: 22142+332 could be:
221420+3320 → 221429+3329
22h14m20s +33deg 20' → 22h14m29s +33deg 29'
221412+3312 → 221418+3318
22h14m12s +33deg 12' → 22h14m18s +33deg 18'

So, the search is between the extremes of these positions: 22h14m12s +33deg 12' → 22h14m29s +33deg 29' which would make the center at: 22h14m20.5s +33deg 20' 30" The search radius which encompasses all possible interpretations of the IAU name is then: 10.7' = 10' 42"