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 | WESTERLUND1_3 | 252.0931 | -46.1953 | 251.177246 | -46.107555 | 256.5618 | -23.584825 | 339.43313351 | -0.79934014 | 282.1087 | 55462.25625 | 2010-09-23 06:09:00 | 55463.3946296296 | 2010-09-24 09:28:16 | 505051010 | 50.2046 | 50 | 50.2046 | 50.2046 | 0 | 50.2046 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 40.7966 | 40.7966 | 98.3438 | 1 | PROCESSED | 57553.5465162037 | 2016-06-14 13:06:59 | 55840 | 2011-10-06 00:00:00 | 55474.0771180556 | 2010-10-05 01:51:03 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 050078 | TeV emission surrounding Westerlund 1, the only super star cluster in our Galaxy, has been discovered. Molecular clouds associated with the TeV emission have been also discovered. This coincidence between the TeV emission and the molecular clouds suggests the proton origin of the TeV emission. However, the TeV emission should include the contribution from high-energy electrons. We observe Westerlund 1 with Suzaku to clarify the electron distribution and to examine the proton acceleration in the star cluster. | GALACTIC DIFFUSE EMISSION | 5 | A | HIRONORI MATSUMOTO | JAP | 5 | AO5 | IS THE SUPER STAR CLUSTER WESTERLUND 1 ACCERELATING PROTONS? | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/505051010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '505051010'
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