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 | N23_DEML71 | 76.4544 | -67.9572 | 76.483575 | -68.02238 | 338.831134 | -84.597327 | 278.75688601 | -34.83345845 | 297.0986 | 56021.0207986111 | 2012-04-04 00:29:57 | 56023.6043402778 | 2012-04-06 14:30:15 | 807008010 | 101.9614 | 100 | 101.9614 | 101.9614 | 0 | 101.9614 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 99.0031 | 99.0031 | 223.204 | 1 | PROCESSED | 57605.1620023148 | 2016-08-05 03:53:17 | 56401 | 2013-04-19 00:00:00 | 56034.2910069444 | 2012-04-17 06:59:03 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 070036 | Recently, we discovered recombining plasma (RP) from several mixed-morphology (MM) SNRs in our galaxy, which provides us a new insight into the evolution of SNRs. On the other hand, the RP has not been detected yet from extragalactic SNRs, while many MM-SNRs exist also in extra galaxies. We investigated all the X-ray spectra obtained from previous observations with Suzaku, XMM-Newton and Chandra and found a clear signal of the RP from three LMC SNRs (N49, N23 and DEM L71). Long-time observations with Suzaku XIS will provide us a first evidence of RP from extra galaxies. We propose 2-pointing observations of three SNRs for 290ks. | EXTRAGALACTIC DIFFUSE SOURCES | 8 | A | HIROYUKI UCHIDA | JAP | 7 | AO7 | FIRST INVESTIGATION OF RECOMBINING PLASMA FROM EXTRAGALACTIC SNRS | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/807008010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '807008010'
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