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 | ETA CARINAE | 161.2181 | -59.7282 | 160.732192 | -59.464935 | 202.181916 | -58.969104 | 287.59637986 | -0.67920855 | 289.0006 | 54274.2459259259 | 2007-06-23 05:54:08 | 54275.9015509259 | 2007-06-24 21:38:14 | 402039010 | 58.3961 | 50 | 58.4041 | 58.3961 | 0 | 58.4041 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 51.552 | 51.552 | 143.0099 | 1 | PROCESSED | 57539.0368981482 | 2016-05-31 00:53:08 | 54695 | 2008-08-17 00:00:00 | 54322.5140856482 | 2007-08-10 12:20:17 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021026 | XMM-Newton observations in 2003 suggest that X-ray emission from Eta Carinae has a hard X-ray component above 10 keV in addition to the thermal emission with kT ~3-5 keV. The excess is apparently strongest near the 2-10 keV X-ray maximum, and possibly produced by very hot plasma or 1st-order Fermi acceleration of particles which then inverse Compton-upscatter UV seed photons from the stellar photospheres. We propose a 50 ksec observation of Eta Carinae with the Suzaku telescope during AO2, compare the X-ray spectrum with earlier observations and determine the level of emission at E >9 keV. | GALACTIC POINT SOURCES | 4 | B | KENJI HAMAGUCHI | USA | 2 | AO2 | HARD X-RAY EMISSION FROM ETA CARINAE | HXD | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/402039010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '402039010'
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