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 | EV LAC | 341.7127 | 44.3232 | 341.158134 | 44.059332 | 6.045133 | 46.919235 | 100.60502245 | -13.08073089 | 256.1601 | 54432.9692013889 | 2007-11-28 23:15:39 | 54434.4655208333 | 2007-11-30 11:10:21 | 402032010 | 68.9493 | 100 | 68.9493 | 69.1333 | 0 | 69.1275 | 2 | 1 | 0 | 2 | 1 | 0 | 0 | 65.0113 | 65.0113 | 129.2328 | 2 | PROCESSED | 57540.7939236111 | 2016-06-01 19:03:15 | 54808 | 2008-12-08 00:00:00 | 54441.0876851852 | 2007-12-07 02:06:16 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021013 | We propose a 100 ks Suzaku XIS observation of the dMe flare star EV Lac to measure coronal element abundances during quiescence and flares of different sizes. EV Lac undergoes frequent small flares, and is known to have undergone a very large flare at ~300 times the quiescent count rate in 2000. Coronal abundance changes shed light on the process of chromospheric evaporation under conditions different to those on the Sun. Depending on the size and spectrum of the flare, we may also be able to detect a hard burst of emission that would serve as a time marker for particle acceleration during the flare. | GALACTIC POINT SOURCES | 4 | C | UNA HWANG | USA | 2 | AO2 | FLARE AND QUIESENT CONORAL ELEMENT ABUNDANCES IN EV LAC | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402032010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402032010'
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