DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | HESSJ1507-622_CENTER | 226.7316 | -62.3464 | 225.708755 | -62.153708 | 244.337801 | -42.703137 | 317.95199358 | -3.49348671 | 301.8082 | 56181.4881712963 | 2012-09-11 11:42:58 | 56183.9549189815 | 2012-09-13 22:55:05 | 507025010 | 79.8869 | 80 | 79.8949 | 79.9029 | 0 | 79.8869 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 74.1958 | 74.1958 | 213.1037 | 1 | PROCESSED | 57607.0557986111 | 2016-08-07 01:20:21 | 56582 | 2013-10-17 00:00:00 | 56212.7347337963 | 2012-10-12 17:38:01 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070033 | HESS J1507-622 is one of the unidentified TeV-gamma-ray sources discovered in the H.E.S.S. Galactic plane survey. The object is unique in the sense of the location, off the Galactic plane. There are no counterparts in radio, infrared, X-ray bands and thus the origin is still mystery, but the object represents several hints; X-ray source like pulsar wind nebula exists near the object, and the location is at the edge of the large molecular cloud near a radio supernova remnant. The main purpose of the Suzaku observation with the best use of high sensitive capability in diffuse X-rays and of a unique low galactic-absorption feature of the object is to determine the origin of TeV emission, such as old supernova remnant with molecular cloud, pulsar-wind driven radiations, or darkest accelerator. | GALACTIC DIFFUSE EMISSION | 5 | B | YUKIKATSU TERADA | HIRONORI MATSUMOTO | JAP | 7 | AO7 | SUZAKU OBSERVATION OF HESS J1507-622; A UNIQUE TEV UNIDENTIFIED SOURCE OFF THE GALACTIC PLANE | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/507025010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '507025010'
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