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 | HESS J1427-608 | 216.9609 | -60.8505 | 216.024633 | -60.626609 | 237.709544 | -43.214788 | 314.40487303 | -0.14444396 | 90.5578 | 55209.5761458333 | 2010-01-13 13:49:39 | 55212.1891666667 | 2010-01-16 04:32:24 | 504034010 | 104.1379 | 100 | 104.1379 | 104.1379 | 0 | 104.1379 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 71.2611 | 71.2611 | 225.7378 | 1 | PROCESSED | 57550.2389930556 | 2016-06-11 05:44:09 | 55594 | 2011-02-02 00:00:00 | 55225.4958449074 | 2010-01-29 11:54:01 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 040066 | Pulsar wind nebula (PWN) has began to be recognized as the best candidate of a large fraction of the HESS-unidentified (unID) sources. It could be true for some sources like HESS J1825-137, while other PWN candidates are sometimes listed simply because they satisfy one or two of the necessary conditions (e.g., there is an energetic pulsar nearby). We then propose a Suzaku observation of HESS J1427-608, which is the most ``unlike'' HESS-unID source to be a PWN. The advantage that we can safely exclude a PWN for its candidate allows us to identify the emission mechanism/origin of HESS J1427-608 more unambiguously compared to other unID sources. We request a 150 ks exposure to constrain the ratio between X-ray and TeV fluxes, which is a good measure of the emission mechanism of TeV sources. | GALACTIC DIFFUSE EMISSION | 5 | C | KOJI MORI | JAP | 4 | AO4 | A SUZAKU OBSERVATION OF HESS J1427-608 | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/504034010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '504034010'
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