DARTS Astro
total 1
Show the used SQL Download WgetScript
No. | target_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 | proposal_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 | hxd_burst_num | processing_status | processing_end_time_mjd | processing_end_time | public_date_mjd | public_date | distribute_start_date_mjd | distribute_start_date | processing_version | processing_quantity | processing_software | proposal_id | proposal_abstract | proposal_category | proposal_category_code | proposal_priority | pi_name | co_pi_name | proposal_affiliated_country | proposal_cycle_count | observation_type | proposal_title | main_detector | xis_injection_flag | data_access_url | ql_access_url | ql_image_url |
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1 | BD +30 3639 | 293.6887 | 30.5051 | 293.198078 | 30.394341 | 303.540216 | 51.224252 | 64.77556877 | 5.01383279 | 277.8713 | 53634.3814930556 | 2005-09-21 09:09:21 | 53635.2473842593 | 2005-09-22 05:56:14 | 100025010 | 35.2146 | 40 | 35.2306 | 35.2306 | 35.2146 | 35.2226 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 33.3728 | 33.3728 | 74.8039 | 1 | PROCESSED | 57527.3931597222 | 2016-05-19 09:26:09 | 54247 | 2007-05-27 00:00:00 | 54035.4664583333 | 2006-10-27 11:11:42 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 000025 | The proposed target, BD +30 3639, is a prototypical planetary nebula which emit diffuse X-rays; planetary nebulae represent the final evolutionary stage of low mass stars, and contain very rich information on the stellar nucleosynthesis. The Chandra ACIS spectrum of BD +30 3639 bears an amazingly strong Ne-K line, most certainly because the X-ray emitting material directly reflect the "onion-like structure" of elements insied evolved stars. However, the ACIS was not able to resolve C, N, O lines, which are of vital importance. The XMM RGS and Chandra LETG could do, but we need very long exposure. Using the Suzaku XIS-BI with the excellent low-energy performance, we can for the first time measure the C/N/O/Mg abundance ratios of this important object in a short time. | CALIBRATION | 1 | A | SWG | JAP | 0 | SWG | Observation of planetary nebula BD +30 3639 | N | https://darts.isas.jaxa.jp/pub/suzaku/ver3.0/100025010/ | Quick Look | ![]() |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '100025010'
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