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 | CTB1_NE | 0.2869 | 62.6043 | 359.6465 | 62.325973 | 37.675416 | 54.459267 | 117.18345572 | 0.29518062 | 253.7193 | 55923.0281134259 | 2011-12-28 00:40:29 | 55924.1251736111 | 2011-12-29 03:00:15 | 506035010 | 52.666 | 50 | 52.666 | 52.666 | 0 | 52.666 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 48.3108 | 48.3108 | 94.7759 | 3 | PROCESSED | 57604.2722569444 | 2016-08-04 06:32:03 | 56313 | 2013-01-21 00:00:00 | 55972.6734490741 | 2012-02-15 16:09:46 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 060086 | CTB 1 is an old (9 - 44 thousand years) galactic supernova remnant (SNR). The ASCA observation of CTB 1 suggested a hard X-ray emission in the 3 - 10 keV band. The hard emission may be originated in synchrotron radiation (non-thermal) or in thermal bremsstrahlung (kT ~ 3 keV). In the case of the non-thermal origin, the old SNR still accelerate electrons up to 100 TeV. On the other hand, the thermal origin indicates that very hot plasma is still kept in such an old SNR. In order to clean up the nature of the hard emission which would give a large impact for the mechanism of particle acceleration and SNR evolution, we propose the Suzaku observation of CTB 1. | GALACTIC DIFFUSE EMISSION | 5 | C | SHINYA NAKASHIMA | JAP | 6 | AO6 | NON-THERMAL EMISSION FROM THE MOST ANCIENT SUPERNOVA REMNANT | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/506035010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '506035010'
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